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Partial Differential Equations

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Pure Mathematics·Captain: korbonits

Formalize Navier-StokesOpen Problem

Motivation

The incompressible Navier–Stokes equations are the standard model for the motion of a viscous fluid such as water or air, used daily in engineering, meteorology and oceanography. Yet the most basic mathematical question about them is open: starting from smooth initial data in three dimensions, does a smooth solution exist for all time? This is one of the seven Millennium Prize Problems of the Clay Mathematics Institute. Its official formulation is Charles Fefferman's problem description, Existence and smoothness of the Navier–Stokes equation (2000), which offers a prize for a proof of any one of four statements: global existence and smoothness on R3\mathbb{R}^3R3 (statement (A)) or on the torus R3/Z3\mathbb{R}^3/\mathbb{Z}^3R3/Z3 (statement (B)), or a counterexample to either (statements (C) and (D)). This mission formalizes statement (A), together with the classical partial results that Fefferman lists as known.

Timeline.

  • 1822–1845: Navier and Stokes write down the equations of a viscous incompressible fluid.
  • 1934: Jean Leray, Sur le mouvement d'un liquide visqueux emplissant l'espace (Acta Math. 63), proves on R3\mathbb{R}^3R3 that smooth solutions exist for a positive time depending on the data, that they exist for all time when the data is small compared with the viscosity, and that global weak solutions with finite energy always exist. Their smoothness and uniqueness are left open.
  • 1933–1969: the two-dimensional problem is settled (Leray for the plane; Olga Ladyzhenskaya's monograph The Mathematical Theory of Viscous Incompressible Flow, 2nd ed. 1969, for bounded domains): smooth solutions exist for all time and are unique.
  • 1984: Tosio Kato, Strong LpL^pLp-solutions of the Navier–Stokes equation in Rm\mathbb{R}^mRm (Math. Z. 187), gives global solutions for initial data small in L3(R3)L^3(\mathbb{R}^3)L3(R3).
  • 1976–1998: partial regularity. Scheffer, then Caffarelli, Kohn and Nirenberg (Comm. Pure Appl. Math. 35, 1982), show that the singular set of a suitable weak solution has one-dimensional parabolic Hausdorff measure zero.
  • 2000: the Clay Mathematics Institute adopts Fefferman's formulation as a Millennium Prize Problem. It remains open.

Setting

Fix a dimension n≥1n \ge 1n≥1 and write Rn\mathbb{R}^nRn for Euclidean nnn-space with its Euclidean norm ∣x∣|x|∣x∣; in Lean this is NavierStokes.Vec n. A velocity field assigns to each time t∈Rt \in \mathbb{R}t∈R and point x∈Rnx \in \mathbb{R}^nx∈Rn a vector u(x,t)∈Rnu(x,t) \in \mathbb{R}^nu(x,t)∈Rn; in Lean u tu\,tut is the field at time ttt and u t xu\,t\,xutx is Fefferman's u(x,t)u(x,t)u(x,t). A pressure is a real function p(x,t)p(x,t)p(x,t). The viscosity ν\nuν is a positive constant. The external force of Fefferman's equation (1) is identically zero throughout, as in statement (A).

For a vector field v:Rn→Rnv : \mathbb{R}^n \to \mathbb{R}^nv:Rn→Rn the divergence is

div⁡v=∑i=1n∂vi∂xi,\operatorname{div} v = \sum_{i=1}^n \frac{\partial v_i}{\partial x_i},divv=i=1∑n​∂xi​∂vi​​,

in Lean NavierStokes.div, computed from the Fréchet derivative Dv(x)Dv(x)Dv(x) as ∑i(Dv(x) ei)i\sum_i (Dv(x)\,e_i)_i∑i​(Dv(x)ei​)i​. The Laplacian Δv=∑i∂2v/∂xi2\Delta v = \sum_i \partial^2 v/\partial x_i^2Δv=∑i​∂2v/∂xi2​ acts componentwise (Mathlib's Laplacian on inner product spaces). The gradient ∇p\nabla p∇p is Mathlib's gradient. The convective term ∑juj ∂u/∂xj\sum_j u_j\,\partial u/\partial x_j∑j​uj​∂u/∂xj​ is the derivative of u(⋅,t)u(\cdot,t)u(⋅,t) at xxx in the direction u(x,t)u(x,t)u(x,t). Finally ∣∇v∣2=∑i,j(∂vi/∂xj)2|\nabla v|^2 = \sum_{i,j} (\partial v_i/\partial x_j)^2∣∇v∣2=∑i,j​(∂vi​/∂xj​)2 is NavierStokes.gradNormSq.

Admissible initial data (Fefferman's condition (4), NavierStokes.IsInitialData): a C∞C^\inftyC∞, divergence-free vector field u0u^0u0 that decays together with all its derivatives faster than any power,

∣∂xαu0(x)∣≤CαK (1+∣x∣)−Kon Rn, for every α and K.|\partial_x^\alpha u^0(x)| \le C_{\alpha K}\,(1+|x|)^{-K} \quad \text{on } \mathbb{R}^n, \text{ for every } \alpha \text{ and } K.∣∂xα​u0(x)∣≤CαK​(1+∣x∣)−Kon Rn, for every α and K.

In Lean the bound is (1+∣x∣)K ∥Dku0(x)∥≤CkK(1+|x|)^K\,\|D^k u^0(x)\| \le C_{kK}(1+∣x∣)K∥Dku0(x)∥≤CkK​ on the kkk-th Fréchet derivative, an equivalent family of conditions. These are exactly the divergence-free Schwartz functions.

A physically reasonable solution on a set SSS of times (NavierStokes.IsSolutionOn; S=[0,∞)S = [0,\infty)S=[0,∞) for NavierStokes.IsSolution) is a pair (u,p)(u,p)(u,p) such that

  1. (Fefferman (6)) uuu and ppp are C∞C^\inftyC∞ on S×RnS \times \mathbb{R}^nS×Rn, up to the boundary of SSS;
  2. (Fefferman (1), f≡0f \equiv 0f≡0) for every t∈St \in St∈S with t>0t > 0t>0 and every xxx,
∂u∂t+∑j=1nuj∂u∂xj=ν Δu−∇p;\frac{\partial u}{\partial t} + \sum_{j=1}^n u_j \frac{\partial u}{\partial x_j} = \nu\,\Delta u - \nabla p;∂t∂u​+j=1∑n​uj​∂xj​∂u​=νΔu−∇p;
  1. (Fefferman (2)) div⁡u(⋅,t)=0\operatorname{div} u(\cdot,t) = 0divu(⋅,t)=0 for every t∈St \in St∈S;
  2. (Fefferman (3)) u(x,0)=u0(x)u(x,0) = u^0(x)u(x,0)=u0(x);
  3. (Fefferman (7), bounded energy) ∫Rn∣u(x,t)∣2 dx<C\int_{\mathbb{R}^n} |u(x,t)|^2\,dx < C∫Rn​∣u(x,t)∣2dx<C for all t∈St \in St∈S, for some constant CCC.

Formalization targets

Goal: Fefferman's statement (A)

Take ν>0\nu > 0ν>0 and n=3n = 3n=3. For every admissible initial datum u0u^0u0 there exist a velocity field uuu and a pressure ppp forming a physically reasonable solution on R3×[0,∞)\mathbb{R}^3 \times [0,\infty)R3×[0,∞):

∀ ν>0, ∀ u0 satisfying (4), ∃ (u,p) satisfying (1), (2), (3), (6), (7) on R3×[0,∞).\forall\, \nu > 0,\ \forall\, u^0 \text{ satisfying (4)},\ \exists\, (u,p) \text{ satisfying (1), (2), (3), (6), (7) on } \mathbb{R}^3 \times [0,\infty).∀ν>0, ∀u0 satisfying (4), ∃(u,p) satisfying (1), (2), (3), (6), (7) on R3×[0,∞).

This is NavierStokes.existence_and_smoothness_R3. It is open; a proof would settle the Millennium Prize Problem in the affirmative.

Milestones: what Fefferman lists as known

  1. Local existence (NavierStokes.local_existence_R3): for n=3n = 3n=3 and every admissible u0u^0u0 there are T>0T > 0T>0 and a physically reasonable solution on R3×[0,T)\mathbb{R}^3 \times [0,T)R3×[0,T). Fefferman: "(A) and (B) hold ... if the time interval [0,∞)[0,\infty)[0,∞) is replaced by a small time interval [0,T)[0,T)[0,T), with TTT depending on the initial data."
  2. Global existence for small data (NavierStokes.small_data_global_existence_R3): there is an absolute constant c>0c > 0c>0 such that, for n=3n = 3n=3, (A) holds for every admissible u0u^0u0 with
∥u0∥L22 ∥∇u0∥L22≤c ν4.\|u^0\|_{L^2}^2\,\|\nabla u^0\|_{L^2}^2 \le c\,\nu^4.∥u0∥L22​∥∇u0∥L22​≤cν4.

Fefferman: "(A) and (B) hold provided the initial velocity u0u^0u0 satisfies a smallness condition." The scale-invariant product is Leray's form of the condition; it implies smallness of ∥u0∥L3/ν\|u^0\|_{L^3}/\nu∥u0∥L3​/ν, so Kato's theorem also applies. 3. The two-dimensional case (NavierStokes.existence_and_smoothness_R2): statement (A) with n=2n = 2n=2. Fefferman: "In two dimensions, the analogues of assertions (A) and (B) have been known for a long time (Ladyzhenskaya)."

A bridging lemma, NavierStokes.isInitialData_iff_schwartz, identifies the admissible data with the divergence-free elements of Mathlib's Schwartz space.

Significance

The result itself. Statement (A) asks whether the basic model of viscous flow is well posed in the classical sense, i.e. whether smooth finite-energy flows can develop singularities in finite time. A positive answer shows the equations never leave the classical regime; a negative one shows the model predicts its own breakdown. Fefferman: "since we don't even know whether these solutions exist, our understanding is at a very primitive level."

Formalizing it. None of the results in this mission has a machine-checked proof, and Mathlib contains no theory of the Navier–Stokes or Euler equations. The milestones are all proved in the literature; formalizing them requires building, on Mathlib's calculus, measure theory and Schwartz space, the heat semigroup on Rn\mathbb{R}^nRn, the pressure equation Δp=−∑i,j∂i∂j(uiuj)\Delta p = -\sum_{i,j} \partial_i\partial_j(u_i u_j)Δp=−∑i,j​∂i​∂j​(ui​uj​) or the Leray projection, energy estimates, and a fixed-point construction of solutions, most of which is reusable for other evolution equations. The goal is open and expected to remain so; its role is to fix in Lean the exact statement the prize asks for, so partial results are formalized against it.

Difficulty

The energy identity ddt∫∣u∣2=−2ν∫∣∇u∣2\frac{d}{dt}\int|u|^2 = -2\nu\int|\nabla u|^2dtd​∫∣u∣2=−2ν∫∣∇u∣2 controls uuu in L2L^2L2 and ∇u\nabla u∇u in Lt,x2L^2_{t,x}Lt,x2​, but in three dimensions this control is supercritical: under the scaling uλ(x,t)=λu(λx,λ2t)u_\lambda(x,t) = \lambda u(\lambda x, \lambda^2 t)uλ​(x,t)=λu(λx,λ2t) that preserves the equations, the energy of uλu_\lambdauλ​ shrinks as λ→∞\lambda \to \inftyλ→∞, so bounded energy does not prevent concentration at small scales. Every known continuation criterion (Leray, Prodi–Serrin, Beale–Kato–Majda, Escauriaza–Seregin–Šverák) needs a quantity at or above critical scaling, none of which the energy controls. The obvious first idea, an ordinary differential inequality for ∥∇u(t)∥L2\|\nabla u(t)\|_{L^2}∥∇u(t)∥L2​, gives ddt∥∇u∥L22≤Cν−3∥∇u∥L26\frac{d}{dt}\|\nabla u\|_{L^2}^2 \le C\nu^{-3}\|\nabla u\|_{L^2}^6dtd​∥∇u∥L22​≤Cν−3∥∇u∥L26​, which closes only for small data or short time. That is exactly why milestones 1 and 2 are theorems and the goal is not.

The formalization adds a second difficulty: the solutions of the literature live in Sobolev or Besov spaces, with pointwise smoothness of uuu and ppp recovered afterwards by regularity theory, and Mathlib has neither Sobolev spaces on Rn\mathbb{R}^nRn nor the heat semigroup in usable form.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n) with Lebesgue measure; the dimension is a parameter, the goal fixes n=3n = 3n=3 and the 2D milestone n=2n = 2n=2.
  • A velocity field is a function of all real times, but every condition is imposed only on the time set SSS; values at negative times are unconstrained.
  • Smoothness on Rn×[0,∞)\mathbb{R}^n \times [0,\infty)Rn×[0,∞) is Mathlib's ContDiffOn of the uncurried map on the closed half-space, i.e. all derivatives extend continuously to t=0t = 0t=0. The momentum equation is imposed at interior times t>0t > 0t>0 with two-sided derivatives; by continuity of the derivatives this is equivalent to Fefferman's "t≥0t \ge 0t≥0".
  • Derivatives are Mathlib's total functions (fderiv, deriv, iteratedFDeriv, gradient, Laplacian) with junk value 000 at non-differentiable points; the smoothness hypotheses make every derivative in the statements honest.
  • The energy is a Lebesgue integral in [0,∞][0,\infty][0,∞], equal to ∞\infty∞ when u(⋅,t)∉L2u(\cdot,t) \notin L^2u(⋅,t)∈/L2, so bounded energy cannot hold vacuously. The L2L^2L2 norms in the small-data hypothesis are Bochner integrals, genuine for Schwartz data.
  • No normalization is imposed on the pressure, as in Fefferman's text.

No trivializing formalization. The zero field solves the equations only for u0=0u^0 = 0u0=0; for any other admissible u0u^0u0 the initial condition, smoothness, the equation on t>0t > 0t>0 and bounded energy must all hold.

Infrastructure needed and welcome contributions. The heat kernel on Rn\mathbb{R}^nRn with Schwartz bounds; the Riesz-transform representation of the pressure or the Leray projection; energy identities for smooth decaying solutions; local existence by Picard iteration; the two-dimensional vorticity equation and its maximum principle. Theorems in the NavierStokes namespace, decompositions of the milestones, and Mathlib lemmas about ContDiffOn on half-spaces are all welcome. Statements (B), (C), (D) and the Euler equations (ν=0\nu = 0ν=0) are out of scope.

Selected references

  • C. L. Fefferman, Existence and smoothness of the Navier–Stokes equation, Clay Mathematics Institute Millennium Prize Problem description, 2000. https://www.claymath.org/wp-content/uploads/2022/06/navierstokes.pdf
  • J. Leray, Sur le mouvement d'un liquide visqueux emplissant l'espace, Acta Mathematica 63 (1934), 193–248. https://doi.org/10.1007/BF02547354
  • O. A. Ladyzhenskaya, The Mathematical Theory of Viscous Incompressible Flow, 2nd ed., Gordon and Breach, 1969. https://archive.org/details/mathematicaltheo0000lady
  • T. Kato, Strong LpL^pLp-solutions of the Navier–Stokes equation in Rm\mathbb{R}^mRm, with applications to weak solutions, Mathematische Zeitschrift 187 (1984), 471–480. https://doi.org/10.1007/BF01174182
  • L. Caffarelli, R. Kohn, L. Nirenberg, Partial regularity of suitable weak solutions of the Navier–Stokes equations, Communications on Pure and Applied Mathematics 35 (1982), 771–831. https://doi.org/10.1002/cpa.3160350604
  • A. J. Majda, A. L. Bertozzi, Vorticity and Incompressible Flow, Cambridge University Press, 2002. https://doi.org/10.1017/CBO9780511613203
  • J. C. Robinson, J. L. Rodrigo, W. Sadowski, The Three-Dimensional Navier–Stokes Equations: Classical Theory, Cambridge University Press, 2016. https://doi.org/10.1017/CBO9781139095143
20 thms4 active usersReviewed
Symplectic Geometry·Captain: Mazecto

Lectures on Symplectic Field Theory VII: Finite-Energy Pseudoholomorphic Curves in SymplectizationsTextbook

Motivation

Let S⊂R2n+2S\subset\mathbb{R}^{2n+2}S⊂R2n+2 be a hypersurface that is strictly star-shaped about the origin. The standard Liouville form restricts to a contact form on SSS, and its Reeb vector field RRR is a reparametrization of the Hamiltonian flow of any function with SSS as a regular level. Weinstein conjectured in 1978, motivated by results of Rabinowitz, that Reeb flows on closed contact manifolds have periodic orbits; H. Hofer established this for the three-sphere and further three-dimensional cases in 1993 (Invent. Math. 114), with finite-energy pseudoholomorphic curves in the symplectization R×S\mathbb{R}\times SR×S as the central objects. Since then these curves have been the main source of periodic orbits, global surfaces of section and invariants of Reeb flows, for example in U. Hryniewicz's characterization of the Reeb orbits that bound disk-like global surfaces of section (arXiv:1105.2077).

The basic fact about these curves is their behaviour near a puncture: a finite-energy curve on a punctured disk either extends over the puncture or approaches a periodic Reeb orbit there. This mission formalizes that statement for the symplectization of a strictly star-shaped level in R2n+2\mathbb{R}^{2n+2}R2n+2, following C. Wendl, Lectures on Symplectic Field Theory, Lecture 9 (arXiv:1612.01009), together with the results on planes, cylinders and energy concentration that accompany it in Hofer's and Hryniewicz's papers. It is the seventh mission in a series on symplectic field theory and builds on the sixth, which defines almost complex structures and pseudoholomorphic maps on open subsets of a vector space.

Setting

  • Linear data. V=R2n+2V=\mathbb{R}^{2n+2}V=R2n+2 with coordinates (q1,p1,…,qn+1,pn+1)(q_1,p_1,\dots,q_{n+1},p_{n+1})(q1​,p1​,…,qn+1​,pn+1​), the complex structure j0j_0j0​ (multiplication by iii on qk+ipkq_k+ip_kqk​+ipk​), ω0=∑kdqk∧dpk\omega_0=\sum_kdq_k\wedge dp_kω0​=∑k​dqk​∧dpk​ and λ0=12∑k(qk dpk−pk dqk)\lambda_0=\tfrac12\sum_k(q_k\,dp_k-p_k\,dq_k)λ0​=21​∑k​(qk​dpk​−pk​dqk​).
  • The level. H:V→RH:V\to\mathbb{R}H:V→R is smooth, every ray from 000 meets S=H−1(1)S=H^{-1}(1)S=H−1(1) exactly once, and dH(x)x>0dH(x)x>0dH(x)x>0 on SSS. The Reeb field is R=XH/λ0(XH)R=X_H/\lambda_0(X_H)R=XH​/λ0​(XH​) with XH=j0∇HX_H=j_0\nabla HXH​=j0​∇H, and ξx=ker⁡λ0(x)∩ker⁡dH(x)\xi_x=\ker\lambda_0(x)\cap\ker dH(x)ξx​=kerλ0​(x)∩kerdH(x) is the contact plane.
  • Symplectization. R×S\mathbb{R}\times SR×S is identified with V∖{0}V\setminus\{0\}V∖{0} by (a,x)↦e2ax(a,x)\mapsto e^{2a}x(a,x)↦e2ax. A smooth JJJ that is a dλ0d\lambda_0dλ0​-compatible complex structure on each ξx\xi_xξx​ determines the almost complex structure J~\tilde JJ~ on V∖{0}V\setminus\{0\}V∖{0} with ∂a↦R\partial_a\mapsto R∂a​↦R, R↦−∂aR\mapsto-\partial_aR↦−∂a​, and JJJ on ξ\xiξ.
  • Energy. For a map uuu from an open U⊆CU\subseteq\mathbb{C}U⊆C, with aaa and w=proj∘uw=\mathrm{proj}\circ uw=proj∘u its two components, Hofer's energy is E(u)=sup⁡φ∫Uu∗d(φ(a)λ0)E(u)=\sup_\varphi\int_Uu^*d(\varphi(a)\lambda_0)E(u)=supφ​∫U​u∗d(φ(a)λ0​) over smooth nondecreasing φ:R→[0,1]\varphi:\mathbb{R}\to[0,1]φ:R→[0,1], and the dλd\lambdadλ-energy is ∫Uw∗dλ0\int_Uw^*d\lambda_0∫U​w∗dλ0​.
  • Finite-energy curves. Smooth maps u:U→V∖{0}u:U\to V\setminus\{0\}u:U→V∖{0} with ∂su+J~(u)∂tu=0\partial_su+\tilde J(u)\partial_tu=0∂s​u+J~(u)∂t​u=0 and E(u)<∞E(u)<\inftyE(u)<∞.
  • Periodic Reeb orbits P=(x,T)P=(x,T)P=(x,T), T>0T>0T>0 not necessarily minimal, the trivial cylinder FP(e2π(s+it))=e2Tsx(Tt)F_P(e^{2\pi(s+it)})=e^{2Ts}x(Tt)FP​(e2π(s+it))=e2Tsx(Tt), and the charge of a puncture: the limit of the actions ∫λ0\int\lambda_0∫λ0​ of the image loops of small clockwise circles around it.

Formalization targets

Goal: asymptotics of finite-energy punctured disks

Let uuu be a finite-energy J~\tilde JJ~-holomorphic curve on the punctured unit disk D∖{0}D\setminus\{0\}D∖{0}. Then either uuu extends smoothly and J~\tilde JJ~-holomorphically over 000 with values in V∖{0}V\setminus\{0\}V∖{0}, or the charge QQQ at 000 exists and is nonzero, a(u(z))→±∞a(u(z))\to\pm\inftya(u(z))→±∞ as z→0z\to0z→0 with the sign of QQQ, and for every sequence ρk→0+\rho_k\to0^+ρk​→0+ a subsequence of the loops t↦proj u(ρke−2πit)t\mapsto\mathrm{proj}\,u(\rho_ke^{-2\pi it})t↦proju(ρk​e−2πit) converges in C∞C^\inftyC∞ to t↦x(Qt+c)t\mapsto x(Qt+c)t↦x(Qt+c) for a periodic Reeb orbit (x,∣Q∣)(x,|Q|)(x,∣Q∣) (Wendl, Theorem 9.8, without the nondegenerate and Morse–Bott clause and without the linear asymptotics of aaa along the end).

Milestones

  1. Structure of the symplectization. J~\tilde JJ~ is a smooth almost complex structure on V∖{0}V\setminus\{0\}V∖{0}, invariant under y↦cyy\mapsto cyy↦cy; the radial coordinates are smooth (Hryniewicz § 2.2).
  2. Reeb field. λ0(R)=1\lambda_0(R)=1λ0​(R)=1 and ω0(R,⋅)=0\omega_0(R,\cdot)=0ω0​(R,⋅)=0 on TSTSTS (Hofer § 1).
  3. Compatibility. ω0\omega_0ω0​ is compatible with J~(y)\tilde J(y)J~(y) for every y≠0y\ne0y=0.
  4. Energy densities. The energy integrands of finite-energy curves are nonnegative, ∫u∗dλ≤E(u)\int u^*d\lambda\le E(u)∫u∗dλ≤E(u), and E(u)=0E(u)=0E(u)=0 forces a constant map on a connected domain (Hryniewicz (17)).
  5. Periods. The periods of periodic Reeb orbits on SSS have a positive lower bound.
  6. Hofer's lemma for continuous nonnegative functions on complete metric spaces (Wendl, Lemma 9.4).
  7. Monotonicity. For JJJ on an open subset of a finite-dimensional space and KKK compact, proper JJJ-holomorphic maps into a small ball Br(p)B_r(p)Br​(p), p∈Kp\in Kp∈K, passing through ppp, have ∫∥Du∥2≥cr2\int\|Du\|^2\ge cr^2∫∥Du∥2≥cr2 (Zinger, Proposition 3.12).
  8. Removal of singularities for JJJ-holomorphic punctured disks of finite energy with values in a compact set (Wendl, Theorem 9.2).
  9. Zero dλd\lambdadλ-energy, negative punctures. Such curves on C∖Γ\mathbb{C}\setminus\GammaC∖Γ are FP∘pF_P\circ pFP​∘p for a polynomial ppp (Hryniewicz, Theorem 2.18).
  10. Planes. Nonconstant finite-energy planes have positive dλd\lambdadλ-energy (Hryniewicz, Corollary 2.19).
  11. Cylinders. A nonconstant finite-energy cylinder with zero dλd\lambdadλ-energy is z↦FP(czk)z\mapsto F_P(cz^k)z↦FP​(czk) (Wendl, Lemma 9.9).
  12. Bubbling-off points. Gradient blow-up of curves with bounded energy concentrates dλd\lambdadλ-energy at least the period of some Reeb orbit of period ≤\le≤ the energy bound (Hryniewicz, Lemma 2.20).
  13. Isolated orbits. If loops at a nonremovable puncture converge along one sequence of radii to an isolated orbit, they converge to it up to phase for all small radii (Wendl, Lemma 9.18).
  14. Asymptotics of planes. A nonconstant finite-energy plane has a positive puncture at ∞\infty∞ with charge equal to its dλd\lambdadλ-energy (Hofer, Theorem 31).
  15. Bridge to R4\mathbb{R}^4R4. For n=1n=1n=1, star-shapedness and periodic orbits agree with the HryniewiczCriterion setting, with period equal to action.

Significance

The results. The goal is the local half of SFT compactness and of the Fredholm theory of punctured curves: it says every finite-energy end is cylindrical over a Reeb orbit, which is what makes asymptotic operators, Conley–Zehnder indices and the index formula of the earlier missions applicable to actual curves. Milestones 9–14 (from Hofer, Hryniewicz and Wendl) describe planes, cylinders and bubbling in the form in which they enter Hofer's work on the Weinstein conjecture for S3S^3S3 and Hryniewicz's work on global surfaces of section; milestone 15 connects them to the open HryniewiczCriterion mission. Milestones 6–8 are general results about pseudoholomorphic maps into any finite-dimensional space.

Formalizing them. All results are classical and proved in the cited sources. None of them has been formalized in a proof assistant, as far as a literature search shows; Mathlib has no symplectizations, no Hofer energy and no Reeb dynamics. The mission produces these objects in general dimension 2n+22n+22n+2, with the energies as lower Lebesgue integrals.

Difficulty

The target V∖{0}V\setminus\{0\}V∖{0} is not compact and J~\tilde JJ~ is not the standard structure, so the curves can escape to 000 or to infinity; the goal has to decide which happens and produce a limit orbit, though the limit orbit is not assumed nondegenerate and may depend on the chosen sequence of radii. Hofer's energy is a supremum over a family of integrands rather than a single integral, and its finiteness does not bound the Euclidean area of the curve. The Euclidean size of the derivative grows with e2ae^{2a}e2a, so all scale-sensitive statements are made with the size ∥D(a∘u)∥+∥D(proj∘u)∥\|D(a\circ u)\|+\|D(\mathrm{proj}\circ u)\|∥D(a∘u)∥+∥D(proj∘u)∥, which is invariant under y↦cyy\mapsto cyy↦cy. Milestones 7–8 hold for an arbitrary norm on the target and an almost complex structure defined only on an open set.

Formalization scope

  • Namespace FiniteEnergyPlane; the definition module FiniteEnergyPlane_Setting imports JHolomorphic_Setting (the sixth mission) for IsAlmostComplexOn and IsJHolomorphicOn. The bridge item also imports HryniewiczCriterion_Basic.
  • Space. VVV is Fin (2 * (n + 1)) → ℝ with interleaved coordinates; n=1n=1n=1 matches HryniewiczCriterion.R4. Its default norm is the sup norm.
  • Radial coordinates. scaleToS H y is the r>0r>0r>0 with H(ry)=1H(ry)=1H(ry)=1 (default 111, used only at y=0y=0y=0), proj H y = scaleToS H y • y, aCoord H y = -½ log (scaleToS H y).
  • Energies are ℝ≥0∞-valued lower integrals of ENNReal.ofReal of the integrands, so E(u)<∞E(u)<\inftyE(u)<∞ is a genuine restriction (a Bochner integral would return 000 on non-integrable integrands and make it vacuous).
  • Punctures and loops. All finite punctures use clockwise loops t↦z0+ρe−2πitt\mapsto z_0+\rho e^{-2\pi it}t↦z0​+ρe−2πit, and ∞\infty∞ uses counterclockwise loops t↦Re2πitt\mapsto Re^{2\pi it}t↦Re2πit; at a negative puncture the limit x(Qt+c)x(Qt+c)x(Qt+c) with Q<0Q<0Q<0 therefore runs the orbit backward. Removability requires an extension that avoids 000.
  • Not included. The statement in Wendl's Theorem 9.8 that a∓∣Q∣sa\mp|Q|sa∓∣Q∣s converges in C∞C^\inftyC∞ along the end, convergence for all radii at nondegenerate or Morse–Bott orbits, exponential convergence and the asymptotic eigenvector are left to a later mission.

Contributions welcome: general lemmas on lower integrals over planar domains and on radial projections to star-shaped hypersurfaces.

Selected references

  • C. Wendl, Lectures on Symplectic Field Theory, arXiv:1612.01009 (2016), Lecture 9. https://arxiv.org/abs/1612.01009
  • H. Hofer, Pseudoholomorphic curves in symplectizations with applications to the Weinstein conjecture in dimension three, Invent. Math. 114 (1993), 515–563. https://doi.org/10.1007/BF01232679
  • U. Hryniewicz, Systems of global surfaces of section for dynamically convex Reeb flows on the 3-sphere, J. Symplectic Geom. 12 (2014), § 2.2. https://arxiv.org/abs/1105.2077
  • A. Zinger, Notes on J-holomorphic maps, arXiv:1706.00331 (2017), §§ 3.3 and 5.1. https://arxiv.org/abs/1706.00331
  • H. Hofer, K. Wysocki, E. Zehnder, Properties of pseudoholomorphic curves in symplectisations I: Asymptotics, Ann. Inst. H. Poincaré Anal. Non Linéaire 13 (1996), 337–379. https://doi.org/10.1016/S0294-1449(16)30108-1
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Control TheoryProbability·Captain: mikedeng1

Nonconcave Utility Maximization with Portfolio Bounds: The Value Function Is the Unique Viscosity Solution of the HJB Equation under the New Terminal Asymptotic ConditionResearch Paper

Motivation

An investor may care about reaching a target, avoiding a loss, or crossing an aspiration level rather than maximizing a concave function of final wealth. A target reward can jump from zero to one at a specified wealth. Such nonconcave utility is a natural model for goal-reaching portfolios, but its discontinuity changes what the associated Hamilton–Jacobi–Bellman equation can say at maturity. Portfolio bounds make the distinction sharper: an investor with finite leverage and short-sale limits cannot instantaneously smooth a jump in the payoff. Dai, Kou, Qian and Wan analyze this combination of nonconcavity, portfolio constraints, and a liquidation floor in their 2022 paper.

The paper proves a comparison principle and identifies the control value as the unique viscosity solution under a special terminal asymptotic condition. These are known mathematical results; this mission asks for their Lean proofs. The source is the authors' accepted manuscript, whose main theorem is Theorem 4.2 on printed page 12. The e-companion supplies boundary and terminal results supporting that theorem.

Setting

The market contains one risky stock and one riskless bond. After the paper's forward-wealth normalization, wealth WsW_sWs​ started from Wt=wW_t=wWt​=w follows

dWs=Wsπs(η ds+σ dBs),t≤s≤T.dW_s=W_s\pi_s(\eta\,ds+\sigma\,d\mathcal B_s),\qquad t\le s\le T.dWs​=Ws​πs​(ηds+σdBs​),t≤s≤T.

Here η\etaη is the excess stock return, σ>0\sigma>0σ>0 is volatility, B\mathcal BB is Brownian motion, and πs\pi_sπs​ is the fraction of wealth invested in the stock. Portfolio weights satisfy d≤πs≤ud\le\pi_s\le ud≤πs​≤u, with d≤0≤ud\le0\le ud≤0≤u; either endpoint may be infinite. Wealth remains above the liquidation floor B≥0B\ge0B≥0. For utility UUU, the value function is

V(t,w)=sup⁡π admissibleE[U(WT)∣Wt=w].V(t,w)=\sup_{\pi\text{ admissible}}\mathbb E[U(W_T)\mid W_t=w].V(t,w)=π admissiblesup​E[U(WT​)∣Wt​=w].

Assumption 3.1 permits utility to be nondecreasing and right-continuous without being concave or continuous. For some 0<p^<10<\hat p<10<p^​<1, it eventually satisfies U(w)≤wp^U(w)\le w^{\hat p}U(w)≤wp^​. At w=Bw=Bw=B it either has a finite value or, when B=0B=0B=0, has the paper's CRRA form near zero. The second case includes logarithmic utility. These alternatives lead to different liquidation boundary conditions.

The formalized Hamiltonian is

H(w,p,A)=sup⁡d≤π≤u{12π2w2σ2A+πwηp},H(w,p,A)=\sup_{d\le\pi\le u}\left\{\frac12\pi^2w^2\sigma^2A+\pi w\eta p\right\},H(w,p,A)=d≤π≤usup​{21​π2w2σ2A+πwηp},

and the HJB equation is −Vt−H(w,Vw,Vww)=0-V_t-H(w,V_w,V_{ww})=0−Vt​−H(w,Vw​,Vww​)=0 for t<Tt<Tt<T and w>Bw>Bw>B. Definition A.1 tests upper and lower semicontinuous envelopes of candidate solutions against smooth functions and uses the corresponding envelopes H∗H^*H∗ and H∗H_*H∗​. It also imposes the liquidation boundary condition and a terminal asymptotic condition. For bounded portfolio weights the terminal condition retains the jump of UUU through the normal distribution function Φ\PhiΦ and L=σmax⁡{u,−d}L=\sigma\max\{u,-d\}L=σmax{u,−d}. For unbounded weights its target is the concave envelope U^\hat UU^.

Formalization targets

Value-function characterization

The goal is Theorem 4.2: for both bounded and unbounded portfolio intervals, the control value satisfies Definition A.1 and is continuous on [0,T)×(B,∞)[0,T)\times(B,\infty)[0,T)×(B,∞). In the growth class used by Theorem 4.1, every other viscosity solution agrees with it:

V′(t,w)=V(t,w),0<t<T,w>B.V'(t,w)=V(t,w),\qquad 0<t<T,\quad w>B.V′(t,w)=V(t,w),0<t<T,w>B.

The goal keeps the actual stochastic-control supremum as VVV and quantifies over competing solutions V′V'V′. It does not select a particular numerical method or a preferred proof. Theorem 4.1 gives comparison in this class. Proposition EC.3.2 gives the liquidation boundary behavior. Proposition EC.3.3 gives two terminal regimes, and Lemma EC.3.3 supplies the power-majorant statement used in the unbounded regime. The milestone list follows these stated results, specialized to the one-stock constant-coefficient model of the main theorem.

Significance

The characterization connects a portfolio optimization problem to an HJB equation even when the terminal utility jumps. It specifies the terminal behavior that distinguishes the bounded and unbounded portfolio regimes. In the bounded case a discontinuity can persist in the approach to maturity; in the unbounded case the limiting target is the concave envelope. The comparison statement then makes the characterization unique within the stated growth class. These conclusions are the analytical basis for the paper's later discussion of numerical schemes, although the numerical convergence theorem is outside this mission's scope (Dai et al., 2022, §§4 and EC.3).

A complete formalization would produce reusable definitions of the constrained control value, the extended-real Hamiltonian and its envelopes, and terminal limits for discontinuous payoffs. The paper's results are proved on paper but have no machine-checked proof in this proposal. The declarations here are compiled statements awaiting proofs. Independent work on the comparison theorem, boundary behavior, terminal asymptotics, and supporting real analysis can proceed against the same definition layer.

Difficulty

The usual terminal condition V(T,w)=U(w)V(T,w)=U(w)V(T,w)=U(w) does not describe the limit of V(t,ζ)V(t,\zeta)V(t,ζ) as (t,ζ)(t,\zeta)(t,ζ) approaches (T,w)(T,w)(T,w) when UUU jumps. Replacing the limit by U(w)U(w)U(w) would erase the singular behavior that the paper studies. The bounded-portfolio condition instead depends on the left limit U(w−)U(w-)U(w−), the size of the jump, and the scaled quantity log⁡(ζ/w)/T−t\log(\zeta/w)/\sqrt{T-t}log(ζ/w)/T−t​. A viscosity comparison argument must handle this terminal profile while the Hamiltonian itself can be infinite or discontinuous in the unbounded portfolio regime. The liquidation boundary has a separate CRRA asymptotic when utility diverges at zero. Each of these clauses is part of the solution concept and must remain compatible with the value function.

Formalization scope

The Lean market stores η,σ,T,B\eta,\sigma,T,Bη,σ,T,B as real numbers and d,ud,ud,u as extended real endpoints. It assumes σ>0\sigma>0σ>0, T>0T>0T>0, B≥0B\ge0B≥0, d≤0≤ud\le0\le ud≤0≤u, and at least one nonzero admissible weight. The last three inequalities include the paper's standing bounds and exclude L=0L=0L=0. Admissible controls are progressively measurable, obey the bounds and liquidation floor, satisfy the integral wealth equation through a Brownian Itô integral, and have integrable terminal utility. The supremum of their expectations is extended real so an infinite value is preserved; the goal explicitly proves finiteness before converting it to a real value. Brownian motions are quantified over filtered probability spaces and have independent future increments relative to their filtration.

The PDE domain is D=[0,T)×(B,∞)D=[0,T)\times(B,\infty)D=[0,T)×(B,∞). Semicontinuous envelopes and boundary and terminal limits approach within DDD. Smooth tests are C∞C^\inftyC∞ real functions. The Hamiltonian and its envelopes are extended real; finite-width expressions involving LLL are used only under bounded portfolio endpoints. The terminal point w=Bw=Bw=B is included only for the finite-utility boundary branch, where the source defines U(B−)=U(B)U(B-)=U(B)U(B−)=U(B). The CRRA formula uses a logarithmic branch at zero power, avoiding division by zero. These commitments rule out a vacuous solution notion or a value function defined as an arbitrary viscosity solution. Proving the control value finite, nontrivial comparison, and both terminal limits remains part of the mission. The e-companion's multivariate statements are included only in the one-stock constant-coefficient specialization used by Theorems 4.1–4.2.

Selected references

  • M. Dai, S. Kou, S. Qian and X. Wan, Nonconcave utility maximization with portfolio bounds, Management Science 68(11), 8368–8385, 2022. DOI: 10.1287/mnsc.2021.4228. This mission cites the authors' accepted manuscript, including its e-companion.
9 thms2 active usersReviewed
AnalysisMathematical Physics·Captain: wurtle

Nonuniqueness for the periodic hard-sphere Boltzmann equationResearch Paper

Motivation: uniqueness of weak Boltzmann solutions

The Boltzmann equation describes a dilute gas through a density F(t,x,v)F(t,x,v)F(t,x,v) of particles at position xxx with velocity vvv, evolving by free transport and binary collisions. For hard spheres, the collision rate is proportional to the normal relative speed. In 1989 DiPerna and Lions constructed global renormalized solutions for all initial data with finite mass, energy and entropy, and weak stability holds at the same level. Existence and stability do not give uniqueness, though: the physical bounds do not even make the quadratic collision term locally integrable, and the uniqueness of general renormalized solutions is a basic question in kinetic theory (Silvestre 2022, §2). Uniqueness is known only under much stronger assumptions, such as Maxwellian upper bounds or closeness to equilibrium.

Timeline

  • 1974 — Ukai: global existence and uniqueness near a Maxwellian for periodic cutoff hard potentials (Proc. Japan Acad. 1974).
  • 1978 — Kaniel and Shinbrot: uniqueness and local existence under Maxwellian upper bounds (CMP 1978).
  • 1988 — Golse, Lions, Perthame and Sentis: velocity averaging lemmas (JFA 1988).
  • 1989 — DiPerna and Lions: global renormalized solutions and weak stability (Ann. of Math. 1989); the entropy inequality follows in 1991 (ARMA 1991).
  • 1999 — For the spatially homogeneous hard-sphere equation, Mischler and Wennberg prove uniqueness among conservative solutions with finite mass and energy (Ann. IHP C 1999); Wennberg gives homogeneous nonuniqueness examples in which the energy increases (J. Stat. Phys. 1999).
  • 2010 — Levermore and Masmoudi give a periodic formulation of renormalized solutions relative to a Maxwellian (ARMA 2010).
  • 2024–2026 — Ill-posedness results: Chen–Holmer for the constant kernel (Ann. PDE 2024), Chen–Guo–Shen–Zhang for hard spheres in Gaussian-weighted Lv2HxsL^2_vH^s_xLv2​Hxs​ (arXiv:2606.01331). Gismondi, Golding and Novack conjecture nonuniqueness of renormalized inhomogeneous Landau and Boltzmann solutions for a dense class of data (arXiv:2608.13758).
  • 2026 — An OpenAI preprint, Nonuniqueness for the periodic hard-sphere Boltzmann equation (OpenAI Math Release, September 23, 2026), claims a single finite-entropy datum on T3×R3\mathbb T^3\times\mathbb R^3T3×R3 with two distinct admissible solutions. It has not been peer reviewed, and the claim has not been formally verified.

Setting

Phase space is Ω=Tx3×Rv3\Omega=\mathbb T^3_x\times\mathbb R^3_vΩ=Tx3​×Rv3​, with T3=R3/Z3\mathbb T^3=\mathbb R^3/\mathbb Z^3T3=R3/Z3. For incoming velocities v,v∗v,v_*v,v∗​ and a collision normal ω∈S2\omega\in S^2ω∈S2, put a=(v−v∗)⋅ωa=(v-v_*)\cdot\omegaa=(v−v∗​)⋅ω, v′=v−aωv'=v-a\omegav′=v−aω, v∗′=v∗+aωv_*'=v_*+a\omegav∗′​=v∗​+aω. The hard-sphere collision operator is

Q(F,F)(v)=∫R3×S2∣a∣ (F(v′)F(v∗′)−F(v)F(v∗)) dv∗ dω,Q(F,F)(v)=\int_{\mathbb R^3\times S^2}|a|\,\big(F(v')F(v_*')-F(v)F(v_*)\big)\,dv_*\,d\omega ,Q(F,F)(v)=∫R3×S2​∣a∣(F(v′)F(v∗′​)−F(v)F(v∗​))dv∗​dω,

with ordinary surface measure on S2S^2S2; the two terms are the gain and the loss. The Cauchy problem is (∂t+v⋅∇x)F=Q(F,F)(\partial_t+v\cdot\nabla_x)F=Q(F,F)(∂t​+v⋅∇x​)F=Q(F,F), F(0)=F0F(0)=F_0F(0)=F0​. An initial datum has finite entropy if it is nonnegative and ∫ΩF0(1+∣v∣2+∣log⁡F0∣)<∞\int_\Omega F_0(1+|v|^2+|\log F_0|)<\infty∫Ω​F0​(1+∣v∣2+∣logF0​∣)<∞.

A solution is admissible (Definition 2.1 of the source) if, with M(v)=(2π)−3/2e−∣v∣2/2M(v)=(2\pi)^{-3/2}e^{-|v|^2/2}M(v)=(2π)−3/2e−∣v∣2/2:

  • it is renormalized: the equation holds weakly for Mβ(F/M)M\beta(F/M)Mβ(F/M) for every C1C^1C1 β\betaβ with β(0)=0\beta(0)=0β(0)=0 and ∣β′(z)∣≤Cβ/(1+z)|\beta'(z)|\le C_\beta/(1+z)∣β′(z)∣≤Cβ​/(1+z), and the separately renormalized gain and loss are integrable on bounded time intervals;
  • it is weakly continuous in L1L^1L1 against every bounded measurable test and takes the initial value F0F_0F0​;
  • mass, energy and absolute entropy stay bounded on bounded time intervals;
  • it conserves local mass and total momentum, and satisfies the energy inequality and the relative-entropy inequality with the full entropy dissipation at every time.

Formalization targets

Goal: two admissible solutions from one datum (Theorem 1.1)

There is a nonnegative finite-entropy datum F0F_0F0​ with bounded velocity support, two admissible global solutions F,GF,GF,G with initial datum F0F_0F0​, and a time T>0T>0T>0 such that

F,G∈C([0,T];L1(Ω)),Q±(F), Q±(G)∈L1([0,T]×Ω),F(t)≠G(t) in L1 for some t∈[0,T].F,G\in C([0,T];L^1(\Omega)),\qquad Q^\pm(F),\,Q^\pm(G)\in L^1([0,T]\times\Omega),\qquad F(t)\neq G(t)\ \text{in } L^1 \text{ for some } t\in[0,T].F,G∈C([0,T];L1(Ω)),Q±(F),Q±(G)∈L1([0,T]×Ω),F(t)=G(t) in L1 for some t∈[0,T].

This is Theorem 1.1 of the source (p. 3), with the difference placed in the common interval of strong continuity, which is where the source establishes it. The goal is published on the platform with status Open: no machine-checked proof exists yet.

Significance

The result itself. If the source's proof is correct, the theorem shows that the DiPerna–Lions framework, even with local mass conservation, momentum conservation and the energy and entropy inequalities retained, does not determine the evolution uniquely. The example is spatially inhomogeneous and periodic, and the two solutions start from exactly the same datum, unlike ill-posedness results that compare nearby data. On the interval where they differ, both solutions satisfy the unrenormalized equation. The datum has bounded velocities but unbounded amplitudes concentrated at smaller and smaller spatial scales, which points to the kind of extra control a uniqueness theorem has to impose.

Formalizing it. The statement fixes a long list of admissibility conditions. Its definitions are a useful contribution in their own right: renormalized solutions, entropy dissipation and kinetic test functions on the torus are not in Mathlib. The 65-page proof (colored decompositions, Carleman representation, velocity averaging, a dilation limit and a branching analysis) is a long-term target. Its propositions are natural milestones.

Difficulty

Constructing two different weak limits is not the hard part: approximations with and without a small "hot seed" give two candidate solutions. The difficulty is to show that they really differ. A vanishing seed can produce a hit on the a priori cap that carries arbitrarily little mass, and weak compactness can erase it in the limit. The source must rule out this loss of information uniformly as the cold velocity distributions collapse onto an axis, where the weight controlling the hot density is singular. At the same time every admissibility condition, including the entropy-dissipation inequality and local mass conservation, has to survive the limits. Energy-increasing constructions (Wennberg) and homogeneous examples do not meet these constraints.

Formalization scope

  • Velocities live in EuclideanSpace ℝ (Fin 3), positions in Fin 3 → AddCircle 1, and densities are real functions on phase space. The sphere carries (volume).toSphere, which is ordinary surface area, not a probability measure.
  • gain and loss are Bochner integrals. To prevent them from silently returning 000 on non-integrable fibers, AdmissibleGlobal requires fiberwise integrability and space-time integrability of the renormalized gain and loss.
  • AdmissibleGlobal f₀ F encodes Definition 2.1: finite entropy at each time, a.e. initial value, weak continuity against bounded measurable tests, uniform moment bounds, the renormalized equation for all Renormalization β\betaβ and all smooth periodic KineticTest φ\varphiφ, local mass conservation against MassTest, total momentum conservation, the energy inequality, and the entropy inequality in ℝ≥0∞ with the lower semicontinuous extension of (A−B)log⁡(A/B)(A-B)\log(A/B)(A−B)log(A/B).
  • StrongEarly T F adds T>0T>0T>0, strong L1L^1L1 continuity on [0,T][0,T][0,T] via eLpNorm, and integrability of gain and loss on [0,T][0,T][0,T]. Distinctness is ¬ (F t =ᵐ G t) for some t∈[0,T]t\in[0,T]t∈[0,T].
  • Infrastructure needed: averaging lemmas, renormalized-solution compactness, the Carleman representation, and estimates on free transport on the torus. Contributions to any of these are welcome.

Selected references

  • R. J. DiPerna and P.-L. Lions, On the Cauchy problem for Boltzmann equations: global existence and weak stability, Ann. of Math. 130 (1989), 321–366. https://doi.org/10.2307/1971423
  • R. J. DiPerna and P.-L. Lions, Global solutions of Boltzmann's equation and the entropy inequality, Arch. Ration. Mech. Anal. 114 (1991), 47–55. https://doi.org/10.1007/BF00375684
  • C. D. Levermore and N. Masmoudi, From the Boltzmann equation to an incompressible Navier–Stokes–Fourier system, Arch. Ration. Mech. Anal. 196 (2010), 753–809. https://doi.org/10.1007/s00205-009-0254-5
  • L. Silvestre, Regularity estimates and open problems in kinetic equations, arXiv:2204.06401 (2022). https://doi.org/10.48550/arXiv.2204.06401
  • S. Kaniel and M. Shinbrot, The Boltzmann equation. I. Uniqueness and local existence, Comm. Math. Phys. 58 (1978), 65–84. https://doi.org/10.1007/BF01624788
  • S. Ukai, On the existence of global solutions of mixed problem for non-linear Boltzmann equation, Proc. Japan Acad. 50 (1974), 179–184. https://doi.org/10.3792/pja/1195519027
  • S. Mischler and B. Wennberg, On the spatially homogeneous Boltzmann equation, Ann. Inst. H. Poincaré C 16 (1999), 467–501. https://doi.org/10.1016/S0294-1449(99)80025-0
  • B. Wennberg, An example of nonuniqueness for solutions to the homogeneous Boltzmann equation, J. Stat. Phys. 95 (1999), 469–477. https://doi.org/10.1023/A:1004546031908
  • F. Golse, P.-L. Lions, B. Perthame and R. Sentis, Regularity of the moments of the solution of a transport equation, J. Funct. Anal. 76 (1988), 110–125. https://doi.org/10.1016/0022-1236(88)90051-1
  • X. Chen and J. Holmer, Well/ill-posedness bifurcation for the Boltzmann equation with constant collision kernel, Ann. PDE 10 (2024), Art. 14. https://doi.org/10.1007/s40818-024-00177-w
  • X. Chen, Y. Guo, S. Shen and Z. Zhang, Sharp HxsH^s_xHxs​ ill-posedness of the hard-sphere Boltzmann equation, arXiv:2606.01331 (2026). https://doi.org/10.48550/arXiv.2606.01331
  • N. Gismondi, W. Golding and M. Novack, A sharp rigidity/flexibility threshold for the isotropic Landau equation, arXiv:2608.13758 (2026). https://doi.org/10.48550/arXiv.2608.13758
  • OpenAI, Nonuniqueness for the periodic hard-sphere Boltzmann equation, OpenAI Math Release preprint, September 23, 2026 (Theorem 1.1, p. 3; Definition 2.1, p. 8). https://github.com/openai/math/blob/adc7f1241b42e322a6451854ab7e4b4c146bf78a/preprints/Nonuniqueness-for-the-periodic-hard-sphere-Boltzmann-equation-September-23-2026/paper.pdf
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Differential GeometryOptimal Transport·Captain: wurtle

Global Support and Convex Injectivity Domains under Weak MTWResearch Paper

Motivation: curvature conditions in optimal transport on manifolds

In optimal transport on a Riemannian manifold with the quadratic cost c(x,y)=d(x,y)2/2c(x,y)=d(x,y)^2/2c(x,y)=d(x,y)2/2, the regularity of optimal maps is governed by a fourth-order curvature quantity of the cost, the Ma–Trudinger–Wang (MTW) tensor. Its nonnegativity on orthogonal pairs, the weak MTW condition (A3w), is necessary for continuity of optimal maps, and together with convexity of the tangent injectivity domains it yields the global geometric "supporting" properties used in regularity theory. Whether weak MTW by itself forces those injectivity domains to be convex was proposed by Villani and proved previously only under a nonfocality assumption, which excludes cut points that are also conjugate points.

Background

  • 2005 — Ma, Trudinger and Wang introduce a strictly positive curvature condition for regularity of transport potentials (MTW 2005).
  • 2009 — Trudinger and Wang treat the degenerate nonnegative form A3w (TW 2009); Loeper proves necessity for continuity and the supporting-mountain principle (Loeper 2009).
  • 2010 — Loeper and Villani connect MTW to cut-locus geometry, proving convexity under strong MTW and nonfocality (Loeper–Villani 2010); Kim and McCann give a geometric formulation and a double-mountain principle (Kim–McCann 2010); Figalli's Bourbaki survey (Astérisque 332, 2010).
  • 2011 — Figalli, Rifford and Villani derive the global supporting principle from weak MTW plus convex injectivity domains (FRV 2011); Villani proposes that weak MTW alone should force convexity of every tangent injectivity domain (Villani 2011, §4.2).
  • 2015 — Figalli, Gallouët and Rifford prove that implication on nonfocal manifolds (FGR 2015, Thm 1.7).
  • 2026 — An OpenAI preprint, Global Support and Convex Injectivity Domains under Weak MTW (OpenAI Math Release, September 25, 2026), claims the implication on every smooth compact connected Riemannian manifold of dimension n≥2n\ge2n≥2, with conjugate cut points allowed. It has not been peer reviewed and its theorems are not formally verified.

Setting

Let (M,g)(M,g)(M,g) be a smooth, connected, compact Riemannian manifold without boundary, of dimension n≥2n\ge2n≥2, with geodesic distance ddd and exponential map exp⁡x:TxM→M\exp_x:T_xM\to Mexpx​:Tx​M→M. The open tangent injectivity domain at xxx is

I(x)={v∈TxM: d(x,exp⁡x(av))=a∣v∣x for some a>1},I(x)=\{v\in T_xM:\ d(x,\exp_x(av))=a|v|_x\ \text{for some } a>1\},I(x)={v∈Tx​M: d(x,expx​(av))=a∣v∣x​ for some a>1},

the set of velocities whose geodesic is still minimizing slightly beyond time one. With c(x,y)=d(x,y)2/2c(x,y)=d(x,y)^2/2c(x,y)=d(x,y)2/2, the MTW quantity at v∈I(x)v\in I(x)v∈I(x) is

S(x,v)(ξ,η)=−32 ∂4∂s2 ∂t2 c(exp⁡x(tξ),exp⁡x(v+sη))∣s=t=0,\mathfrak S_{(x,v)}(\xi,\eta)=-\frac32\,\frac{\partial^4}{\partial s^2\,\partial t^2}\,c\big(\exp_x(t\xi),\exp_x(v+s\eta)\big)\Big|_{s=t=0},S(x,v)​(ξ,η)=−23​∂s2∂t2∂4​c(expx​(tξ),expx​(v+sη))​s=t=0​,

and weak MTW means S(x,v)(ξ,η)≥0\mathfrak S_{(x,v)}(\xi,\eta)\ge0S(x,v)​(ξ,η)≥0 whenever ⟨ξ,η⟩x=0\langle\xi,\eta\rangle_x=0⟨ξ,η⟩x​=0, for all xxx and v∈I(x)v\in I(x)v∈I(x). No nonfocality, strict positivity, or prior convexity is assumed.

In Lean, MMM is a Mathlib Riemannian manifold modelled on EuclideanSpace ℝ (Fin n) (so without boundary), with CompactSpace, ConnectedSpace and IsRiemannianManifold linking the metric-space distance to the Riemannian metric. exp x v is the time-one point of a smooth curve with initial point xxx, initial velocity vvv, and locally constant-speed distance-realizing behaviour; mtw is the iterated one-variable derivative formula above.

Formalization targets

Goal: convexity of injectivity domains

If (M,g)(M,g)(M,g) satisfies weak MTW, then for every x∈Mx\in Mx∈M, every v0,v1∈I(x)v_0,v_1\in I(x)v0​,v1​∈I(x) and θ∈[0,1]\theta\in[0,1]θ∈[0,1],

(1−θ)v0+θv1∈I(x),(1-\theta)v_0+\theta v_1\in I(x),(1−θ)v0​+θv1​∈I(x),

i.e. I(x)I(x)I(x) is convex. This is Theorem 1.1 of the source. The goal is published on the platform with status Open.

Significance

The result itself. Combined with the Figalli–Rifford–Villani supporting principle, convexity of injectivity domains under weak MTW alone removes an extra geometric hypothesis from the regularity theory of optimal transport on compact manifolds, and covers focal manifolds where minimizing geodesics may reach conjugate cut points. The source also proves a global supporting property, convexity of lifted gap sections, and uniform C1,1C^{1,1}C1,1 intermediate-time geometry (Theorem 1.2), which feed the companion preprint on bi-Hölder regularity of transport maps.

Formalizing it. The statement uses only geodesics, distance and a four-fold derivative of the squared distance, so it can be phrased with current Mathlib Riemannian infrastructure. A proof needs nonsmooth analysis of the distance function near the cut locus, semiconvex potentials and their subdifferentials, and a continuity (degree) argument; this layer would be reusable for other cut-locus results.

Difficulty

The cost ccc is smooth only before the cut locus, while convexity of I(x)I(x)I(x) concerns segments whose interior points might a priori leave the region where S\mathfrak SS is defined. Weak MTW controls the cost Hessian only in directions perpendicular to a velocity segment and gives no strict inequality. Smooth-cost concavity arguments therefore cannot be applied beyond their domain, and nonfocality — the assumption that cut points are reached strictly before conjugate points — is exactly what earlier proofs used to keep the cost smooth along the segment.

Formalization scope

  • exp is defined through complete geodesics with prescribed initial data (ContMDiff curve, mfderiv at 000 equal to vvv, locally d(γs,γr)=∣v∣ ∣s−r∣d(\gamma s,\gamma r)=|v|\,|s-r|d(γs,γr)=∣v∣∣s−r∣); on a compact manifold such a geodesic exists and is unique, so the Classical.choose fallback is never used.
  • injectivityDomain matches I(x)I(x)I(x) exactly; mtw uses iterated deriv, which is the true fourth derivative wherever the cost is smooth (the case v∈I(x)v\in I(x)v∈I(x), near s=t=0s=t=0s=t=0).
  • The hypothesis quantifies over all xxx, all v∈I(x)v\in I(x)v∈I(x), and all gxg_xgx​-orthogonal ξ,η\xi,\etaξ,η; the conclusion is Convex ℝ (injectivityDomain x) for every xxx.
  • Dimension n≥2n\ge2n≥2, compactness and connectedness are explicit hypotheses; boundaryless-ness comes from the Euclidean model.
  • Needed infrastructure: Hopf–Rinow and uniqueness of geodesics, first and second variation, semiconcavity of the distance squared, cut and conjugate locus theory.

Selected references

  • X.-N. Ma, N. S. Trudinger and X.-J. Wang, Regularity of potential functions of the optimal transportation problem, Arch. Ration. Mech. Anal. 177 (2005), 151–183. https://doi.org/10.1007/s00205-005-0362-9
  • N. S. Trudinger and X.-J. Wang, On the second boundary value problem for Monge–Ampère type equations and optimal transportation, Ann. Sc. Norm. Super. Pisa 8 (2009), 143–174. https://doi.org/10.2422/2036-2145.2009.1.07
  • G. Loeper, On the regularity of solutions of optimal transportation problems, Acta Math. 202 (2009), 241–283. https://doi.org/10.1007/s11511-009-0037-8
  • G. Loeper and C. Villani, Regularity of optimal transport in curved geometry: the nonfocal case, Duke Math. J. 151 (2010), 431–485. https://doi.org/10.1215/00127094-2010-003
  • Y.-H. Kim and R. J. McCann, Continuity, curvature, and the general covariance of optimal transportation, J. Eur. Math. Soc. 12 (2010), 1009–1040. https://doi.org/10.4171/JEMS/221
  • A. Figalli, Regularity of optimal transport maps [after Ma–Trudinger–Wang and Loeper], Séminaire Bourbaki 2008/2009, Astérisque 332 (2010), 341–368.
  • A. Figalli, L. Rifford and C. Villani, Necessary and sufficient conditions for continuity of optimal transport maps on Riemannian manifolds, Tohoku Math. J. 63 (2011), 855–876. https://doi.org/10.2748/tmj/1325886291
  • C. Villani, Regularity of optimal transport and cut locus: from nonsmooth analysis to geometry to smooth analysis, Discrete Contin. Dyn. Syst. 30 (2011), 559–571. https://doi.org/10.3934/dcds.2011.30.559
  • A. Figalli, T. O. Gallouët and L. Rifford, On the convexity of injectivity domains on nonfocal manifolds, SIAM J. Math. Anal. 47 (2015), 969–1000. https://doi.org/10.1137/140961821
  • OpenAI, Global Support and Convex Injectivity Domains under Weak MTW, OpenAI Math Release preprint, September 25, 2026 (Theorem 1.1, p. 2). https://github.com/openai/math/blob/adc7f1241b42e322a6451854ab7e4b4c146bf78a/preprints/Global-Support-and-Convex-Injectivity-Domains-under-Weak-MTW-September-25-2026/paper.pdf
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Mathematical PhysicsOptimizationProbability·Captain: mikedeng1

Optimization of Mean-field Spin Glasses I: Every Minimizer of the Extended Parisi Functional Has Full SupportResearch Paper

Motivation

The Ising mixed ppp-spin model assigns to each configuration σ∈{−1,+1}N\sigma \in \{-1,+1\}^Nσ∈{−1,+1}N the energy of a random polynomial whose covariance is E{HN(σ)HN(σ′)}=Nξ(⟨σ,σ′⟩/N)\mathbb E\{H_N(\sigma)H_N(\sigma')\} = N\xi(\langle\sigma,\sigma'\rangle/N)E{HN​(σ)HN​(σ′)}=Nξ(⟨σ,σ′⟩/N). Its ground-state energy max⁡σHN(σ)/N\max_\sigma H_N(\sigma)/Nmaxσ​HN​(σ)/N converges to the value of a variational problem, the zero-temperature Parisi formula (Auffinger–Chen 2017), in which a functional P\mathsf PP is minimized over non-decreasing order parameters γ\gammaγ. El Alaoui, Montanari and Sellke (arXiv:2001.00904v1) ask how close a polynomial-time algorithm can get to this maximum. Their answer is an extended variational principle: the best value reachable by incremental approximate message passing is inf⁡γ∈LP(γ)\inf_{\gamma\in\mathscr L}\mathsf P(\gamma)infγ∈L​P(γ), where the space L\mathscr LL drops the monotonicity constraint.

The algorithm that reaches this value is built from a minimizer γ∗\gamma_*γ∗​ of P\mathsf PP over L\mathscr LL, and it runs along the set of times where γ∗\gamma_*γ∗​ is positive. Theorem 5 of the paper (p. 30) shows that this set is dense: a minimizer has full support. This mission formalizes that theorem and the first- and second-order optimality conditions it rests on (Section 6.1, pp. 22–31).

Timeline. Parisi proposed the variational formula in 1979. Talagrand (2006) and Panchenko (2013) proved it at positive temperature. Auffinger and Chen (2017) established the zero-temperature version with Φ(1,x)=∣x∣\Phi(1,x)=|x|Φ(1,x)=∣x∣ and proved that a minimizer over the monotone space exists. Jagannath and Tobasco (2016) developed the PDE and SDE tools for the Parisi functional that Section 6.1 of the present paper adapts to non-monotone order parameters. Montanari (2019) gave the first message passing algorithm for the Sherrington–Kirkpatrick case; the present paper (2020) extended it to general mixtures and introduced L\mathscr LL.

Setting

A mixture is ξ(t)=∑k≥2ck2tk\xi(t) = \sum_{k\ge2} c_k^2 t^kξ(t)=∑k≥2​ck2​tk with ξ(1+ε)<∞\xi(1+\varepsilon) < \inftyξ(1+ε)<∞ for some ε>0\varepsilon > 0ε>0; its derivatives ξ′\xi'ξ′, ξ′′\xi''ξ′′ are the termwise differentiated power series, non-negative and non-decreasing on [0,1][0,1][0,1].

An order parameter is a function γ:[0,1)→R≥0\gamma : [0,1) \to \mathbb R_{\ge0}γ:[0,1)→R≥0​. The extended space is

L={γ:[0,1)→R≥0:∥ξ′′γ∥TV[0,t]<∞ ∀t∈[0,1), ∫01ξ′′(t)γ(t) dt<∞},\mathscr L = \Bigl\{\gamma : [0,1)\to\mathbb R_{\ge0} : \|\xi''\gamma\|_{\mathrm{TV}[0,t]}<\infty\ \forall t\in[0,1),\ \int_0^1\xi''(t)\gamma(t)\,dt<\infty\Bigr\},L={γ:[0,1)→R≥0​:∥ξ′′γ∥TV[0,t]​<∞ ∀t∈[0,1), ∫01​ξ′′(t)γ(t)dt<∞},

with the weighted distance ∥γ1−γ2∥1,ξ′′=∫01ξ′′(t)∣γ1(t)−γ2(t)∣ dt\|\gamma_1-\gamma_2\|_{1,\xi''} = \int_0^1\xi''(t)|\gamma_1(t)-\gamma_2(t)|\,dt∥γ1​−γ2​∥1,ξ′′​=∫01​ξ′′(t)∣γ1​(t)−γ2​(t)∣dt. The non-negative step functions SF+\mathsf{SF}_+SF+​ are the finite sums ∑iaiI[ti−1,ti)\sum_i a_i\mathbb I_{[t_{i-1},t_i)}∑i​ai​I[ti−1​,ti​)​ with 0=t0<⋯<tm=10=t_0<\dots<t_m=10=t0​<⋯<tm​=1 and ai≥0a_i\ge0ai​≥0.

For a terminal condition f0f_0f0​ (convex, continuous, even, non-negative, differentiable off 000 with 0≤f0′≤10\le f_0'\le10≤f0′​≤1 on (0,∞)(0,\infty)(0,∞)) and γ∈SF+\gamma\in\mathsf{SF}_+γ∈SF+​, the Parisi PDE

∂tΦ+12ξ′′(t)(∂x2Φ+γ(t)(∂xΦ)2)=0,Φ(1,x)=f0(x),\partial_t\Phi + \tfrac12\xi''(t)\bigl(\partial_x^2\Phi + \gamma(t)(\partial_x\Phi)^2\bigr) = 0,\qquad \Phi(1,x) = f_0(x),∂t​Φ+21​ξ′′(t)(∂x2​Φ+γ(t)(∂x​Φ)2)=0,Φ(1,x)=f0​(x),

has the explicit Cole–Hopf solution Φγ\Phi^\gammaΦγ: on [ti−1,ti)[t_{i-1},t_i)[ti−1​,ti​), Φ(t,x)=γi−1log⁡Eexp⁡{γiΦ(ti,x+ξ′(ti)−ξ′(t) G)}\Phi(t,x) = \gamma_i^{-1}\log\mathbb E\exp\{\gamma_i\Phi(t_i, x+\sqrt{\xi'(t_i)-\xi'(t)}\,G)\}Φ(t,x)=γi−1​logEexp{γi​Φ(ti​,x+ξ′(ti​)−ξ′(t)​G)} with G∼N(0,1)G\sim\mathsf N(0,1)G∼N(0,1). For γ∈L\gamma\in\mathscr Lγ∈L, Φγ\Phi^\gammaΦγ is the limit of Φγn\Phi^{\gamma_n}Φγn​ along step functions γn→γ\gamma_n\to\gammaγn​→γ in the weighted distance. The Parisi functional is

P(γ)=Φγ(0,0)−12∫01t ξ′′(t)γ(t) dt.\mathsf P(\gamma) = \Phi^\gamma(0,0) - \frac12\int_0^1 t\,\xi''(t)\gamma(t)\,dt .P(γ)=Φγ(0,0)−21​∫01​tξ′′(t)γ(t)dt.

Given a Brownian motion BBB, the process XXX solves dXt=ξ′′(t)γ(t) ∂xΦγ(t,Xt) dt+ξ′′(t) dBtdX_t = \xi''(t)\gamma(t)\,\partial_x\Phi^\gamma(t,X_t)\,dt + \sqrt{\xi''(t)}\,dB_tdXt​=ξ′′(t)γ(t)∂x​Φγ(t,Xt​)dt+ξ′′(t)​dBt​, X0=0X_0 = 0X0​=0. The support of γ\gammaγ is S(γ)={t∈[0,1):γ(t)>0}S(\gamma) = \{t\in[0,1):\gamma(t)>0\}S(γ)={t∈[0,1):γ(t)>0}, and S‾(γ)\overline S(\gamma)S(γ) is its closure in [0,1)[0,1)[0,1).

Formalization targets

Goal: Theorem 5

With f0(x)=∣x∣f_0(x) = |x|f0​(x)=∣x∣, if γ∗∈L\gamma_*\in\mathscr Lγ∗​∈L satisfies P(γ∗)=inf⁡γ∈LP(γ)\mathsf P(\gamma_*) = \inf_{\gamma\in\mathscr L}\mathsf P(\gamma)P(γ∗​)=infγ∈L​P(γ), then

S‾(γ∗)=[0,1).\overline S(\gamma_*) = [0,1).S(γ∗​)=[0,1).

Milestones

The path to the goal, in attack order:

  • Proposition 6.1(b),(c): on step functions, ∂xΦ\partial_x\Phi∂x​Φ is non-decreasing with ∣∂xΦ∣≤1|\partial_x\Phi|\le1∣∂x​Φ∣≤1, and ∥Φγ1−Φγ2∥∞≤∥ξ′′(γ1−γ2)∥1\|\Phi^{\gamma_1}-\Phi^{\gamma_2}\|_\infty\le\|\xi''(\gamma_1-\gamma_2)\|_1∥Φγ1​−Φγ2​∥∞​≤∥ξ′′(γ1​−γ2​)∥1​.
  • Lemma 6.2: these properties pass to γ∈L\gamma\in\mathscr Lγ∈L.
  • Lemma 6.5: the SDE has a unique strong solution on [0,1][0,1][0,1].
  • Corollary 6.6: E{∂xΦ(t2,Xt2)2}−E{∂xΦ(t1,Xt1)2}=∫t1t2ξ′′(s) E{(∂x2Φ(s,Xs))2} ds\mathbb E\{\partial_x\Phi(t_2,X_{t_2})^2\}-\mathbb E\{\partial_x\Phi(t_1,X_{t_1})^2\}=\int_{t_1}^{t_2}\xi''(s)\,\mathbb E\{(\partial_x^2\Phi(s,X_s))^2\}\,dsE{∂x​Φ(t2​,Xt2​​)2}−E{∂x​Φ(t1​,Xt1​​)2}=∫t1​t2​​ξ′′(s)E{(∂x2​Φ(s,Xs​))2}ds.
  • Lemma 6.7: the map t↦E{∂x2Φ(t,Xt)2}t\mapsto\mathbb E\{\partial_x^2\Phi(t,X_t)^2\}t↦E{∂x2​Φ(t,Xt​)2} is continuous on [0,1)[0,1)[0,1).
  • Proposition 6.8: the first variation ddsP(γ+sδ)∣s=0+=12∫01ξ′′δ (E{∂xΦ(t,Xt)2}−t) dt\frac{d}{ds}\mathsf P(\gamma+s\delta)|_{s=0+}=\frac12\int_0^1\xi''\delta\,(\mathbb E\{\partial_x\Phi(t,X_t)^2\}-t)\,dtdsd​P(γ+sδ)∣s=0+​=21​∫01​ξ′′δ(E{∂x​Φ(t,Xt​)2}−t)dt.
  • Lemma 6.9: S(γ)S(\gamma)S(γ) is a countable disjoint union of intervals.
  • Corollary 6.10: E{∂xΦγ∗(t,Xt)2}=t\mathbb E\{\partial_x\Phi^{\gamma_*}(t,X_t)^2\}=tE{∂x​Φγ∗​(t,Xt​)2}=t on S‾(γ∗)\overline S(\gamma_*)S(γ∗​) and ≥t\ge t≥t off it.
  • Corollary 6.11: ξ′′(t) E{∂x2Φγ∗(t,Xt)2}=1\xi''(t)\,\mathbb E\{\partial_x^2\Phi^{\gamma_*}(t,X_t)^2\}=1ξ′′(t)E{∂x2​Φγ∗​(t,Xt​)2}=1 on S‾(γ∗)\overline S(\gamma_*)S(γ∗​).
  • Lemma 6.12: the law of XtX_tXt​ has a density, bounded below on compact sets, once γ\gammaγ vanishes.

Significance

The result. Full support identifies the extended variational principle as one whose minimizers are "nowhere flat". The algorithm of Theorem 3 in the paper follows γ∗\gamma_*γ∗​ through incremental steps whose size is set by γ∗\gamma_*γ∗​, and it needs no special treatment of gaps where γ∗=0\gamma_* = 0γ∗​=0. The stationarity conditions (Corollaries 6.10–6.11) also characterize minimizers over L\mathscr LL the way the Auffinger–Chen conditions characterize minimizers over the monotone space. They are the starting point for comparing inf⁡LP\inf_{\mathscr L}\mathsf PinfL​P with the Parisi value.

Formalizing it. The theorem is proved in the paper; nothing here is open mathematics. The paper's proofs rely on cited PDE regularity (Jagannath–Tobasco 2016) and on standard SDE theory, often in one line. The mission produces a machine-checked chain from the explicit Cole–Hopf formula to the support theorem. Along the way it builds the Parisi PDE solution on a non-monotone class, a first-variation formula, and stationarity conditions, none of which have a formal counterpart. No formal statement of the Parisi functional or the Parisi PDE exists on Prove2Me (index search, 2026-10-03).

Difficulty

Two steps resist a direct argument. The first is the first variation (Proposition 6.8): differentiating Φγ(0,0)\Phi^\gamma(0,0)Φγ(0,0) in γ\gammaγ requires comparing the SDE for γ\gammaγ with the SDE for the perturbed parameter and controlling their difference uniformly, which needs bounds on ∂x2Φ\partial_x^2\Phi∂x2​Φ that degenerate as t→1t\to1t→1. The second is the exclusion of gaps: on an interval where γ∗=0\gamma_*=0γ∗​=0 the PDE is a time-changed heat equation, and the contradiction comes from a strict inequality, which requires the law of XtX_tXt​ to charge every interval (Lemma 6.12). The obvious idea of perturbing γ∗\gamma_*γ∗​ upward on a gap only yields the inequality (6.14), which is consistent with a gap; the second-order identity at the gap's endpoints is what closes the argument.

Formalization scope

Conventions committed to in Lean:

  • The mixture is a coefficient sequence ccc with c0=c1=0c_0=c_1=0c0​=c1​=0; ξ,ξ′,ξ′′\xi,\xi',\xi''ξ,ξ′,ξ′′ are explicit series.
  • Order parameters are functions R→R\mathbb R\to\mathbb RR→R read only on [0,1)[0,1)[0,1). Membership in L\mathscr LL uses eVariationOn for the total variation and IntegrableOn for the integral; the latter includes the a.e.-measurability that the paper takes for granted.
  • Φγ\Phi^\gammaΦγ for step functions is the Cole–Hopf recursion (7.3). For a piece with γi=0\gamma_i = 0γi​=0 the formula's limit, the heat semigroup, is used instead of a division by zero. E\mathbb EE over GGG is integration against gaussianReal 0 1. For γ∈L\gamma\in\mathscr Lγ∈L, Φγ\Phi^\gammaΦγ is a limit along the filter of step functions converging in the weighted L1L^1L1 distance; it is never "some solution of the PDE".
  • ∂xΦ\partial_x\Phi∂x​Φ and ∂x2Φ\partial_x^2\Phi∂x2​Φ are iterated derivs in xxx. Lemma 6.2's weak-derivative claim is stated as "convex and 1-Lipschitz", its equivalent.
  • The SDE uses the published strong-solution concept EthierKurtz.SolvesBrownianSDE in dimension one, with coefficients extended by zero after time 111. The driver is assumed to be a standard Brownian motion (IsBrownianReal). Statements about XXX hold for every strong solution, which by Lemma 6.5 is unique.
  • Section 6.1's results are stated for every admissible f0f_0f0​; P\mathsf PP is parametrized by f0f_0f0​, and Theorem 5 fixes f0=∣⋅∣f_0=|\cdot|f0​=∣⋅∣.
  • Minimality is "P(γ∗)≤P(γ)\mathsf P(\gamma_*)\le\mathsf P(\gamma)P(γ∗​)≤P(γ) for all γ∈L\gamma\in\mathscr Lγ∈L", never a real infimum. S‾(γ)\overline S(\gamma)S(γ) is closure (S γ) ∩ Ico 0 1. Right-continuity of γ∗\gamma_*γ∗​, the paper's convention from p. 28, is a hypothesis.
  • Disclosed hypothesis ξ≢0\xi\not\equiv0ξ≡0 (some ck≠0c_k\neq0ck​=0) on Theorem 5, Corollaries 6.10–6.11 and Lemma 6.12. For ξ≡0\xi\equiv0ξ≡0 every γ\gammaγ minimizes P\mathsf PP and X≡0X\equiv0X≡0, so γ∗≡0\gamma_*\equiv0γ∗​≡0 has empty support and each of those statements fails. When c2=0c_2=0c2​=0 no minimizer exists (Corollary 6.11 at t=0t=0t=0), and Theorem 5 is vacuous, as in the paper.
  • Lemma 6.12's density bound is stated without choosing density versions: ε Leb(A)≤P(Xt∈A)\varepsilon\,\mathrm{Leb}(A)\le\mathbb P(X_t\in A)εLeb(A)≤P(Xt​∈A) for measurable A⊆[−M,M]A\subseteq[-M,M]A⊆[−M,M].

A trivializing formalization is excluded: Φγ\Phi^\gammaΦγ and XXX are the paper's objects, built from the data, so the goal cannot be met by choosing a convenient solution, and minimality over L\mathscr LL cannot be satisfied by a junk infimum.

Not formalized: the weak formulation (6.4) of Lemma 6.2, printed with a wrong boundary term; the stochastic-integral identity (6.7) of Lemma 6.5; the regularity Lemmas 6.3–6.4; Proposition 6.1(a). The paper's algorithmic Theorems 2–4 are out of scope, because they concern algorithms in an informal model of computation and an AMP state-evolution theory that is not part of this mission.

Useful infrastructure beyond this mission: the Cole–Hopf solution and its Lipschitz dependence on γ\gammaγ, the Parisi functional on L\mathscr LL, and the SDE (6.3). Contributions that formalize Itô's formula for these processes or the regularity of Φγ\Phi^\gammaΦγ are welcome as supporting lemmas.

Selected references

  • A. El Alaoui, A. Montanari, M. Sellke, Optimization of Mean-field Spin Glasses, arXiv:2001.00904v1, 2020. https://arxiv.org/abs/2001.00904
  • A. Auffinger, W.-K. Chen, Parisi formula for the ground state energy in the mixed p-spin model, Annals of Probability, 2017. https://arxiv.org/abs/1606.05335
  • A. Jagannath, I. Tobasco, A dynamic programming approach to the Parisi functional, Proceedings of the AMS, 2016. https://arxiv.org/abs/1502.04398
  • A. Montanari, Optimization of the Sherrington–Kirkpatrick Hamiltonian, FOCS 2019. https://arxiv.org/abs/1812.10897
  • M. Talagrand, The Parisi formula, Annals of Mathematics 163(1), 2006. https://doi.org/10.4007/annals.2006.163.221
  • D. Panchenko, The Parisi ultrametricity conjecture, Annals of Mathematics 177(1), 2013. https://doi.org/10.4007/annals.2013.177.1.8
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AnalysisControl Theory·Captain: mikedeng1

Stability and Instability Results of the Wave Equation with a Delay Term in the Boundary or Internal Feedbacks IV: Arbitrarily Small Destabilizing Delays for Internal DampingResearch Paper

Motivation

Feedback laws in engineering are applied with a lag: sensors, actuators and communication channels introduce a time delay τ\tauτ between the measurement of a state and the control that reacts to it. For finite-dimensional systems small delays are usually harmless. For distributed systems such as the wave equation they need not be: Datko, Lagnese and Polis (SIAM J. Control Optim. 24, 1986) and Datko (SIAM J. Control Optim. 26, 1988) showed, for one-dimensional examples, that an arbitrarily small delay in a stabilizing feedback can destroy stability. The question matters to anyone who designs boundary or internal controllers for vibrating structures and wants to know whether a stabilizing law is robust to delay.

Nicaise and Pignotti (SIAM J. Control Optim. 45 (2006)) study the wave equation on a bounded domain of Rn\mathbb R^nRn with a damping term that combines an instantaneous and a delayed velocity feedback, with coefficients μ1\mu_1μ1​ and μ2\mu_2μ2​. They show that the system is exponentially stable when μ2<μ1\mu_2 < \mu_1μ2​<μ1​ (Theorems 1.1 and 1.3), and that when μ2≥μ1\mu_2 \ge \mu_1μ2​≥μ1​ stability can fail (Theorems 1.2 and 1.4). This mission is Theorem 1.4, the internal-damping instability result, in the case the paper proves.

  • 1986–1988: Datko, Lagnese and Polis; Datko — destabilization by small delays in one-dimensional boundary-damped wave equations.
  • 2006: Nicaise and Pignotti — the multi-dimensional dichotomy μ2<μ1\mu_2 < \mu_1μ2​<μ1​ (stability) versus μ2≥μ1\mu_2 \ge \mu_1μ2​≥μ1​ (instability for some delays), for boundary and internal feedback.

Setting

Let n≥1n \ge 1n≥1 and let Ω⊂Rn\Omega \subset \mathbb R^nΩ⊂Rn be a bounded open set with boundary Γ\GammaΓ of class C2C^2C2, split as Γ=ΓD∪ΓN\Gamma = \Gamma_D \cup \Gamma_NΓ=ΓD​∪ΓN​ with ΓD‾∩ΓN‾=∅\overline{\Gamma_D} \cap \overline{\Gamma_N} = \emptysetΓD​​∩ΓN​​=∅ and ΓD≠∅\Gamma_D \neq \emptysetΓD​=∅. Write ν\nuν for the outer unit normal and ∂u/∂ν\partial u/\partial\nu∂u/∂ν for the normal derivative. Let μ1>0\mu_1 > 0μ1​>0, μ2>0\mu_2 > 0μ2​>0 and let τ>0\tau > 0τ>0 be the delay. With damping coefficient a≡1a \equiv 1a≡1 the problem is

utt(x,t)−Δu(x,t)+μ1ut(x,t)+μ2ut(x,t−τ)=0in Ω×(0,∞),u_{tt}(x,t) - \Delta u(x,t) + \mu_1 u_t(x,t) + \mu_2 u_t(x,t-\tau) = 0 \quad \text{in } \Omega \times (0,\infty),utt​(x,t)−Δu(x,t)+μ1​ut​(x,t)+μ2​ut​(x,t−τ)=0in Ω×(0,∞), u=0  on ΓD×(0,∞),∂u∂ν=0  on ΓN×(0,∞),u = 0 \ \text{ on } \Gamma_D \times (0,\infty), \qquad \frac{\partial u}{\partial\nu} = 0 \ \text{ on } \Gamma_N \times (0,\infty),u=0  on ΓD​×(0,∞),∂ν∂u​=0  on ΓN​×(0,∞),

with initial data u(⋅,0)=u0u(\cdot,0) = u_0u(⋅,0)=u0​, ut(⋅,0)=u1u_t(\cdot,0) = u_1ut​(⋅,0)=u1​ and a history ut=g0u_t = g_0ut​=g0​ on Ω×(−τ,0)\Omega \times (-\tau, 0)Ω×(−τ,0). The standard energy of a solution is

E(t)=12∫Ω{∣ut(x,t)∣2+∣∇u(x,t)∣2} dx.\mathcal E(t) = \frac12 \int_\Omega \big\{ |u_t(x,t)|^2 + |\nabla u(x,t)|^2 \big\}\,dx .E(t)=21​∫Ω​{∣ut​(x,t)∣2+∣∇u(x,t)∣2}dx.

The condition μ2<μ1\mu_2 < \mu_1μ2​<μ1​ is the paper's assumption (1.8). The paper's problem (1.12)–(1.16) carries a general coefficient a∈L∞(Ω)a \in L^\infty(\Omega)a∈L∞(Ω) with a≥0a \ge 0a≥0 and a>a0>0a > a_0 > 0a>a0​>0 near ΓN\Gamma_NΓN​; a≡1a \equiv 1a≡1 is one such coefficient.

Formalization targets

Goal: Theorem 1.4 for a≡1a \equiv 1a≡1

If (1.8) fails, i.e. 0<μ1≤μ20 < \mu_1 \le \mu_20<μ1​≤μ2​, then

∀ε>0 ∃τ∈(0,ε) ∃u solving the problem with delay τ:  E(t)↛0 (t→∞),\forall \varepsilon > 0\ \exists \tau \in (0,\varepsilon)\ \exists u \text{ solving the problem with delay } \tau:\ \ \mathcal E(t) \not\to 0 \ (t \to \infty),∀ε>0 ∃τ∈(0,ε) ∃u solving the problem with delay τ:  E(t)→0 (t→∞),

and the same holds with "τ∈(0,ε)\tau \in (0,\varepsilon)τ∈(0,ε)" replaced by "τ>M\tau > Mτ>M", for every MMM. The goal asserts only non-decay, not a rate of growth or the value of the energy, so it survives any sharpening of the examples.

Milestones

  1. (5.21)–(5.23): if φ\varphiφ is an eigenfunction of the mixed Dirichlet–Neumann Laplacian, Δφ=−Λ2φ\Delta\varphi = -\Lambda^2\varphiΔφ=−Λ2φ, and λ∈C\lambda \in \mathbb Cλ∈C solves λ2+(μ1+μ2e−λτ)λ=−Λ2\lambda^2 + (\mu_1 + \mu_2 e^{-\lambda\tau})\lambda = -\Lambda^2λ2+(μ1​+μ2​e−λτ)λ=−Λ2, then eλtφ(x)e^{\lambda t}\varphi(x)eλtφ(x) is a solution.
  2. (5.24)–(5.25): with λ=α+iβ\lambda = \alpha + i\betaλ=α+iβ and βτ=(2l+1)π\beta\tau = (2l+1)\piβτ=(2l+1)π, that equation is equivalent to α2+β2=Λ2\alpha^2 + \beta^2 = \Lambda^2α2+β2=Λ2, μ2e−ατ=2α+μ1\mu_2 e^{-\alpha\tau} = 2\alpha + \mu_1μ2​e−ατ=2α+μ1​.
  3. Case (a), μ1=μ2\mu_1 = \mu_2μ1​=μ2​: the system forces α=0\alpha = 0α=0 and β2=Λ2\beta^2 = \Lambda^2β2=Λ2.
  4. Case (b), μ2>μ1\mu_2 > \mu_1μ2​>μ1​, (5.26)–(5.27): for every Λ>0\Lambda > 0Λ>0 and lll there is α∈(0,(μ2−μ1)/2)\alpha \in (0, (\mu_2-\mu_1)/2)α∈(0,(μ2​−μ1​)/2) with τ(α)=α−1ln⁡(μ2/(μ1+2α))>0\tau(\alpha) = \alpha^{-1}\ln(\mu_2/(\mu_1+2\alpha)) > 0τ(α)=α−1ln(μ2​/(μ1​+2α))>0 solving the system.
  5. Energy of separated solutions (p. 1584): E(t)=e2 Re(λ)t E(0)\mathcal E(t) = e^{2\,\mathrm{Re}(\lambda)t}\,\mathcal E(0)E(t)=e2Re(λ)tE(0) with E(0)>0\mathcal E(0) > 0E(0)>0.
  6. Delay bounds (p. 1585, corrected): (2l+1)π/Λ<τ<(2l+1)π/Λ2−(μ2−μ1)2/4(2l+1)\pi/\Lambda < \tau < (2l+1)\pi/\sqrt{\Lambda^2 - (\mu_2-\mu_1)^2/4}(2l+1)π/Λ<τ<(2l+1)π/Λ2−(μ2​−μ1​)2/4​, the second when Λ2>(μ2−μ1)2/4\Lambda^2 > (\mu_2-\mu_1)^2/4Λ2>(μ2​−μ1​)2/4.

Significance

The result shows that the stability threshold μ2<μ1\mu_2 < \mu_1μ2​<μ1​ of Theorem 1.3 is sharp in the sense that matters for design: at or beyond the threshold there is no delay margin, since delays as small as desired already produce solutions whose energy does not decay. Together with Theorem 1.3 it gives a complete dichotomy in the coefficients (μ1,μ2)(\mu_1,\mu_2)(μ1​,μ2​) for the internally damped wave equation with delay, in any dimension, and it identifies the mechanism (roots of the characteristic equation on or to the right of the imaginary axis) that later work on delayed stabilization has had to avoid.

The result is proved in the paper; to the best of current knowledge it has not been machine-checked. The mission's product is a formal proof of the a≡1a \equiv 1a≡1 case together with its algebraic core: the reduction of the transcendental characteristic equation, the analysis of both cases, and the two-sided bounds on the delays. The spectral input it needs, an unbounded sequence of eigenvalues of the mixed Dirichlet–Neumann Laplacian with regular eigenfunctions, is reusable well beyond this paper.

Difficulty

The scalar part is elementary. The difficulty is the spectral input. The small delays come from τn,l≈(2l+1)π/Λn\tau_{n,l} \approx (2l+1)\pi/\Lambda_nτn,l​≈(2l+1)π/Λn​ with Λn→∞\Lambda_n \to \inftyΛn​→∞, so the proof needs infinitely many eigenvalues Λn2→∞\Lambda_n^2 \to \inftyΛn2​→∞ of the Laplacian with mixed Dirichlet–Neumann conditions on a C2C^2C2 domain, with eigenfunctions that are C2C^2C2 inside and C1C^1C1 up to the boundary. This requires compactness of the embedding HΓD1(Ω)↪L2(Ω)H^1_{\Gamma_D}(\Omega) \hookrightarrow L^2(\Omega)HΓD​1​(Ω)↪L2(Ω), the spectral theorem for compact self-adjoint operators, and elliptic regularity for a mixed problem, none of which is available in Mathlib for domains in Rn\mathbb R^nRn. A single eigenpair gives only the large delays (letting l→∞l \to \inftyl→∞); it does not give the small ones.

A second point: the paper's own bound (2l+1)2π2/τn,l2≤Λn2(2l+1)^2\pi^2/\tau_{n,l}^2 \le \Lambda_n^2(2l+1)2π2/τn,l2​≤Λn2​ bounds τn,l\tau_{n,l}τn,l​ only from below, so it does not by itself give τn,l→0\tau_{n,l} \to 0τn,l​→0; the upper bound of milestone 6 is needed.

Formalization scope

  • Space: Rn\mathbb R^nRn is EuclideanSpace ℝ (Fin n) with n≥1n \ge 1n≥1. The C2C^2C2 boundary is given by a global C2C^2C2 defining function ψ\psiψ (Ω={ψ<0}\Omega = \{\psi < 0\}Ω={ψ<0}, ∂Ω={ψ=0}\partial\Omega = \{\psi = 0\}∂Ω={ψ=0}, ∇ψ≠0\nabla\psi \ne 0∇ψ=0 on ∂Ω\partial\Omega∂Ω); ν=∇ψ/∣∇ψ∣\nu = \nabla\psi/|\nabla\psi|ν=∇ψ/∣∇ψ∣; the surface measure is pinned by the Gauss–Green formula for all C1C^1C1 fields.
  • Solutions are complex valued functions u(x,t)u(x,t)u(x,t) defined for all t∈Rt \in \mathbb Rt∈R, C2C^2C2 on Ω×R\Omega \times \mathbb RΩ×R and C1C^1C1 on Ω‾×R\overline\Omega \times \mathbb RΩ×R; the equation and boundary conditions hold for t>0t > 0t>0; initial data and history are the traces of uuu. The Neumann condition uses the derivative within Ω‾\overline\OmegaΩ. ∣∇u∣2|\nabla u|^2∣∇u∣2 is the sum of the squared moduli of the partial derivatives.
  • Corrected scope: Theorem 1.4 is printed for a general aaa satisfying (1.17)–(1.18); §5.2 proves it only for a≡1a \equiv 1a≡1, which is what is stated.
  • Corrected slips: (5.22) prints Δφ=−μ2φ\Delta\varphi = -\mu^2\varphiΔφ=−μ2φ for −Λ2φ-\Lambda^2\varphi−Λ2φ; p. 1584 prints eα+iβφ(x)e^{\alpha+i\beta}\varphi(x)eα+iβφ(x) for e(α+iβ)tφ(x)e^{(\alpha+i\beta)t}\varphi(x)e(α+iβ)tφ(x); the p. 1585 bound is supplemented by the upper bound of milestone 6. Milestone texts are quoted verbatim, including the slips.
  • The standing hypotheses (1.6)–(1.7) and the constant ξ\xiξ of (1.10) are not used by §5.2 and are omitted, which strengthens the statements.
  • A trivializing formalization is ruled out: the goal's conclusion E↛0\mathcal E \not\to 0E→0 excludes u≡0u \equiv 0u≡0, the energy integrand is continuous on the compact Ω‾\overline\OmegaΩ so the integral is genuine, and the normal derivative is taken within Ω‾\overline\OmegaΩ so the Neumann condition is not satisfied by a junk value.
  • No statement assumes the existence of eigenvalues; supplying the spectral theory of the mixed Laplacian is part of the goal. Contributions welcome: the spectral theorem for the mixed Dirichlet–Neumann Laplacian on a bounded C2C^2C2 domain, boundary regularity of its eigenfunctions, and the energy identity for separated solutions.

Selected references

  • S. Nicaise, C. Pignotti, Stability and instability results of the wave equation with a delay term in the boundary or internal feedbacks, SIAM J. Control Optim. 45(5):1561–1585, 2006. https://doi.org/10.1137/060648891
  • R. Datko, Not all feedback stabilized hyperbolic systems are robust with respect to small time delays in their feedbacks, SIAM J. Control Optim. 26:697–713, 1988.
  • R. Datko, J. Lagnese, M. P. Polis, An example on the effect of time delays in boundary feedback stabilization of wave equations, SIAM J. Control Optim. 24:152–156, 1986.
  • P. Grisvard, Elliptic Problems in Nonsmooth Domains, Pitman, 1985 (regularity of mixed boundary value problems).
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AnalysisControl Theory·Captain: mikedeng1

Stability and Instability Results of the Wave Equation with a Delay Term in the Boundary or Internal Feedbacks III: Destabilizing Delays for Boundary FeedbackResearch Paper

Motivation

Boundary feedback stabilization of the wave equation asks whether a damping term placed on part of the boundary drives the energy of every solution to zero. Without delay the answer is classical: the feedback ∂u/∂ν=−μ1ut\partial u/\partial\nu = -\mu_1 u_t∂u/∂ν=−μ1​ut​ on a part ΓN\Gamma_NΓN​ of the boundary gives exponential energy decay under geometric conditions (Chen, Lagnese, Lasiecka–Triggiani, Komornik–Zuazua). In practice a feedback is applied with a lag, and a small lag can destroy stability. Datko, Lagnese and Polis (doi:10.1137/0324007) and Datko (doi:10.1137/0326040) showed, in one space dimension, that a purely delayed boundary feedback destabilizes the system for arbitrarily small delays.

Nicaise and Pignotti (doi:10.1137/060648891) study a feedback made of an instantaneous part and a delayed part, with weights μ1\mu_1μ1​ and μ2\mu_2μ2​, in any space dimension. Their Theorem 1.1 gives exponential decay when μ2<μ1\mu_2 < \mu_1μ2​<μ1​. This mission formalizes the converse, Theorem 1.2: when μ2≥μ1\mu_2 \ge \mu_1μ2​≥μ1​, some delays admit solutions whose energy does not decay at all.

Timeline.

  • 1986: Datko, Lagnese and Polis, a one-dimensional wave equation whose delayed boundary feedback is unstable.
  • 1988: Datko, instability under arbitrarily small delays for a class of hyperbolic systems.
  • 2006: Xu, Yung and Li (doi:10.1051/cocv:2006021), one space dimension, by spectral analysis: stability for μ2<μ1\mu_2 < \mu_1μ2​<μ1​, instability for μ2>μ1\mu_2 > \mu_1μ2​>μ1​, possible instabilities for μ1=μ2\mu_1 = \mu_2μ1​=μ2​.
  • 2006: Nicaise and Pignotti, the same dichotomy in any dimension nnn, with explicit destabilizing delays built from eigenfunctions (§5.1).

Setting

Let n≥1n \ge 1n≥1 and let Ω⊂Rn\Omega \subset \mathbb R^nΩ⊂Rn be a bounded open set with boundary Γ\GammaΓ of class C2C^2C2. The boundary is split as Γ=ΓD∪ΓN\Gamma = \Gamma_D \cup \Gamma_NΓ=ΓD​∪ΓN​, with ΓD‾∩ΓN‾=∅\overline{\Gamma_D} \cap \overline{\Gamma_N} = \emptysetΓD​​∩ΓN​​=∅ and ΓD≠∅\Gamma_D \neq \emptysetΓD​=∅. Write ν\nuν for the outer unit normal and dΓd\GammadΓ for the surface measure. Together these data form a mixed domain (MixedDomain n in Lean).

Fix μ1,μ2>0\mu_1, \mu_2 > 0μ1​,μ2​>0 and a delay τ>0\tau > 0τ>0. The problem (1.1)–(1.3) is

{utt(x,t)−Δu(x,t)=0in Ω×(0,+∞),u(x,t)=0on ΓD×(0,+∞),∂u∂ν(x,t)=−μ1ut(x,t)−μ2ut(x,t−τ)on ΓN×(0,+∞),\begin{cases} u_{tt}(x,t) - \Delta u(x,t) = 0 & \text{in } \Omega \times (0,+\infty),\\ u(x,t) = 0 & \text{on } \Gamma_D \times (0,+\infty),\\ \dfrac{\partial u}{\partial\nu}(x,t) = -\mu_1 u_t(x,t) - \mu_2 u_t(x,t-\tau) & \text{on } \Gamma_N \times (0,+\infty), \end{cases}⎩⎨⎧​utt​(x,t)−Δu(x,t)=0u(x,t)=0∂ν∂u​(x,t)=−μ1​ut​(x,t)−μ2​ut​(x,t−τ)​in Ω×(0,+∞),on ΓD​×(0,+∞),on ΓN​×(0,+∞),​

with initial data u(⋅,0)u(\cdot,0)u(⋅,0), ut(⋅,0)u_t(\cdot,0)ut​(⋅,0) and a history utu_tut​ on ΓN×(−τ,0)\Gamma_N \times (-\tau,0)ΓN​×(−τ,0) (1.4)–(1.5). The standard energy of a solution is (3.7)

E(t)=12∫Ω(∣ut(x,t)∣2+∣∇u(x,t)∣2) dx.\mathcal E(t) = \frac12\int_\Omega \big(|u_t(x,t)|^2 + |\nabla u(x,t)|^2\big)\,dx .E(t)=21​∫Ω​(∣ut​(x,t)∣2+∣∇u(x,t)∣2)dx.

Condition (1.8) of the paper is μ2<μ1\mu_2 < \mu_1μ2​<μ1​. This mission concerns the complementary case μ2≥μ1\mu_2 \ge \mu_1μ2​≥μ1​.

For real functions www on Ω\OmegaΩ, (5.11) defines q0(w)=∫ΓN∣w∣2 dΓq_0(w) = \int_{\Gamma_N} |w|^2\,d\Gammaq0​(w)=∫ΓN​​∣w∣2dΓ and q1(w)=∫Ω∣∇w∣2 dxq_1(w) = \int_\Omega |\nabla w|^2\,dxq1​(w)=∫Ω​∣∇w∣2dx.

Formalization targets

Goal: Theorem 1.2 (p. 1563)

If μ2≥μ1\mu_2 \ge \mu_1μ2​≥μ1​, there exist delays 0<τ0<τ1<⋯0 < \tau_0 < \tau_1 < \cdots0<τ0​<τ1​<⋯ and, for each kkk, a classical solution uku_kuk​ of (1.1)–(1.3) with delay τk\tau_kτk​ and a constant ck>0c_k > 0ck​>0 such that

Ek(t)=ckfor all t≥0.\mathcal E_k(t) = c_k \qquad \text{for all } t \ge 0 .Ek​(t)=ck​for all t≥0.

The statement fixes no formula for the delays and no value of the energy. It asserts only the existence of infinitely many delays for which the energy does not decay.

Milestones

  1. (5.1)–(5.2), pp. 1579–1580. If λ∈C\lambda \in \mathbb Cλ∈C and φ\varphiφ solves −Δφ+λ2φ=0-\Delta\varphi + \lambda^2\varphi = 0−Δφ+λ2φ=0 in Ω\OmegaΩ, φ=0\varphi = 0φ=0 on ΓD\Gamma_DΓD​ and ∂φ/∂ν=−(μ1+μ2e−λτ)λφ\partial\varphi/\partial\nu = -(\mu_1 + \mu_2 e^{-\lambda\tau})\lambda\varphi∂φ/∂ν=−(μ1​+μ2​e−λτ)λφ on ΓN\Gamma_NΓN​, then u=eλtφu = e^{\lambda t}\varphiu=eλtφ solves (1.1)–(1.3).
  2. (5.5)–(5.7), pp. 1580 and 1582. For b>0b > 0b>0, l∈Nl \in \mathbb Nl∈N and bτ=arccos⁡(−μ1/μ2)+2lπb\tau = \arccos(-\mu_1/\mu_2) + 2l\pibτ=arccos(−μ1​/μ2​)+2lπ:
cos⁡(bτ)=−μ1/μ2,μ2sin⁡(bτ)=μ22−μ12,(μ1+μ2e−ibτ) ib=bμ22−μ12.\cos(b\tau) = -\mu_1/\mu_2,\qquad \mu_2\sin(b\tau) = \sqrt{\mu_2^2-\mu_1^2},\qquad (\mu_1 + \mu_2e^{-ib\tau})\,ib = b\sqrt{\mu_2^2-\mu_1^2}.cos(bτ)=−μ1​/μ2​,μ2​sin(bτ)=μ22​−μ12​​,(μ1​+μ2​e−ibτ)ib=bμ22​−μ12​​.
  1. Case (a), μ1=μ2\mu_1 = \mu_2μ1​=μ2​, p. 1581. For a normalized mixed Dirichlet–Neumann eigenfunction φ\varphiφ with −Δφ=b2φ-\Delta\varphi = b^2\varphi−Δφ=b2φ and τ=(2l+1)π/b\tau = (2l+1)\pi/bτ=(2l+1)π/b, the function u=eibtφu = e^{ibt}\varphiu=eibtφ is a solution and
∫Ω(∣∇u∣2+∣ut∣2) dx=2b2(t≥0).\int_\Omega(|\nabla u|^2 + |u_t|^2)\,dx = 2b^2 \quad (t \ge 0).∫Ω​(∣∇u∣2+∣ut​∣2)dx=2b2(t≥0).
  1. Case (b), μ2>μ1\mu_2 > \mu_1μ2​>μ1​, pp. 1581–1582. A normalized minimizer φ\varphiφ of s q0(w)+s2q0(w)2+4q1(w)s\,q_0(w) + \sqrt{s^2q_0(w)^2 + 4q_1(w)}sq0​(w)+s2q0​(w)2+4q1​(w)​, where s=μ22−μ12s = \sqrt{\mu_2^2-\mu_1^2}s=μ22​−μ12​​, solves the variational problem (5.7) with 2b2b2b equal to the minimum value.

Significance

The result. Theorem 1.2 shows that the threshold μ2<μ1\mu_2 < \mu_1μ2​<μ1​ of Theorem 1.1 is sharp in the following sense: once the delayed weight reaches the instantaneous one, no geometric assumption restores asymptotic stability for every delay. Together, Theorems 1.1 and 1.2 separate robust from non-robust boundary feedbacks by a single inequality between the two gains. The explicit delays of case (a), τn,l=(2l+1)π/bn\tau_{n,l} = (2l+1)\pi/b_nτn,l​=(2l+1)π/bn​, become arbitrarily small or large. So even an arbitrarily short lag in an equally weighted feedback can remove decay.

The formalization. The paper proves the result. It has not been formalized, and Mathlib has no wave equation on domains, no mixed eigenvalue problems and no Sobolev spaces on domains. This mission produces:

  • a machine-checked statement of the instability half of the paper's dichotomy;
  • the reduction to a spectral problem as separate, checkable steps;
  • a precise record of what the paper leaves implicit. In case (b) the existence of the minimizer is assumed ("if the minimum … is attained"), and in case (a) the existence of Dirichlet–Neumann eigenfunctions is quoted.

Difficulty

Milestones 1 and 2 are calculus and trigonometry. The difficulty sits in producing φ\varphiφ. The goal needs a nonzero function φ\varphiφ that is C2C^2C2 in Ω\OmegaΩ and C1C^1C1 up to the boundary and solves an eigenvalue problem with mixed Dirichlet and Neumann (case (a)) or Dirichlet and Robin-type (case (b)) boundary conditions. Existence requires compactness of HΓD1(Ω)↪L2(Ω)H^1_{\Gamma_D}(\Omega) \hookrightarrow L^2(\Omega)HΓD​1​(Ω)↪L2(Ω) and of the trace into L2(ΓN)L^2(\Gamma_N)L2(ΓN​), followed by elliptic regularity up to a C2C^2C2 boundary. None of these is in Mathlib.

A shortcut does not work: in case (b) the frequency bbb enters the boundary condition, so φ\varphiφ is not an eigenfunction of a fixed self-adjoint operator. The page instead minimizes a non-quadratic functional, and its first-variation computation (5.18)–(5.19) needs care: the functional is not 2-homogeneous, so the normalization by 1+ε2∥v∥21 + \varepsilon^2\|v\|^21+ε2∥v∥2 does not literally give g(ε)≥g(0)g(\varepsilon) \ge g(0)g(ε)≥g(0), although the first-order condition is right.

Taking real parts does not give a real-valued solution with constant energy: in case (b) the energy of cos⁡(bt)φ\cos(bt)\varphicos(bt)φ oscillates.

Formalization scope

  • Solutions are complex-valued, u:Rn×R→Cu : \mathbb R^n \times \mathbb R \to \mathbb Cu:Rn×R→C, as the page's eλtφe^{\lambda t}\varphieλtφ with λ∈C\lambda \in \mathbb Cλ∈C are. ∣ut∣2|u_t|^2∣ut​∣2 and ∣∇u∣2=∑i∣∂iu∣2|\nabla u|^2 = \sum_i |\partial_i u|^2∣∇u∣2=∑i​∣∂i​u∣2 are squared moduli.
  • Classical solutions. A solution is C2C^2C2 on Ω×R\Omega \times \mathbb RΩ×R and C1C^1C1 on Ω‾×R\overline\Omega \times \mathbb RΩ×R. It solves the equations for t>0t > 0t>0, and its values at t≤0t \le 0t≤0 are the initial data and history. The normal derivative is the derivative within Ω‾\overline\OmegaΩ applied to ν\nuν. C2C^2C2 regularity up to the boundary is not required, because eigenfunctions of mixed problems generally lack it.
  • The domain. The C2C^2C2 boundary is given by a global defining function ψ\psiψ with Ω={ψ<0}\Omega = \{\psi < 0\}Ω={ψ<0}. The surface measure is pinned down by the Gauss–Green formula for all C1C^1C1 vector fields, which determines it uniquely.
  • Dropped hypotheses. The geometric hypotheses (1.6)–(1.7) and the parameter ξ\xiξ of (1.10) are not used in §5.1 and are omitted. This strengthens the statements.
  • Sobolev spaces. HΓD1(Ω)H^1_{\Gamma_D}(\Omega)HΓD​1​(Ω) is replaced in milestone 4 by the class of real functions that are C2C^2C2 in Ω\OmegaΩ, C1C^1C1 on Ω‾\overline\OmegaΩ and zero on ΓD\Gamma_DΓD​, both as the minimization class and as the test class.
  • Non-triviality. The goal requires the constant energy to be positive and the delays to be strictly increasing. Without positivity, the zero solution would satisfy "constant energy". Without strict monotonicity, one delay repeated would count as a sequence.

A complete development needs the following:

  • Green's first identity on C2C^2C2 domains for functions that are C1C^1C1 up to the boundary;
  • existence and regularity of eigenfunctions of the Laplacian with mixed boundary conditions;
  • in case (b), existence of the minimizer (Rellich compactness and the trace theorem).

These pieces are reusable well beyond this mission. Contributions of any of them, or of an alternative route to a φ\varphiφ with the required properties, are welcome.

Selected references

  • S. Nicaise, C. Pignotti, Stability and instability results of the wave equation with a delay term in the boundary or internal feedbacks, SIAM J. Control Optim. 45(5):1561–1585, 2006. https://doi.org/10.1137/060648891
  • R. Datko, J. Lagnese, M. P. Polis, An example on the effect of time delays in boundary feedback stabilization of wave equations, SIAM J. Control Optim. 24:152–156, 1986. https://doi.org/10.1137/0324007
  • R. Datko, Not all feedback stabilized hyperbolic systems are robust with respect to small time delays in their feedbacks, SIAM J. Control Optim. 26:697–713, 1988. https://doi.org/10.1137/0326040
  • G. Q. Xu, S. P. Yung, L. K. Li, Stabilization of wave systems with input delay in the boundary control, ESAIM Control Optim. Calc. Var. 12:770–785, 2006. https://doi.org/10.1051/cocv:2006021
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AnalysisFunctional AnalysisMathematical Physics·Captain: mikedeng1

Mathematical Methods in Quantum Mechanics XII: Self-Adjointness and Essential Spectrum of One-Particle Schrödinger OperatorsTextbook

Motivation

The Hamiltonian of a single nonrelativistic particle in Rn\mathbb R^nRn moving in a potential VVV is the Schrödinger operator H=−Δ+VH = -\Delta + VH=−Δ+V acting in L2(Rn)L^2(\mathbb R^n)L2(Rn). Before anything can be said about the dynamics or the energy levels of such a particle, one must know that HHH is a genuine observable: a self-adjoint operator on a specified domain. For potentials that decay at infinity one also wants the coarse structure of the spectrum, namely that it is bounded below and that everything below the continuum threshold 000 consists of isolated eigenvalues of finite multiplicity. The hydrogen atom, with the Coulomb potential −γ/∣x∣-\gamma/|x|−γ/∣x∣ in three dimensions, is the central example.

The self-adjointness results go back to T. Kato's 1951 paper on the Hamiltonians of atoms; the identification of the essential spectrum through relatively compact perturbations is due to H. Weyl's theorem and its later extensions. This mission follows Chapter 10 of G. Teschl, Mathematical Methods in Quantum Mechanics (AMS GSM 99, 2009), Sections 10.1, 10.2, 10.4 and 10.5.

Setting

L2(Rn)L^2(\mathbb R^n)L2(Rn) is the complex Hilbert space of square integrable functions with respect to Lebesgue measure. The free Schrödinger operator is H0=−ΔH_0 = -\DeltaH0​=−Δ with domain the Sobolev space H2(Rn)={f∈L2∣∣p∣2f^(p)∈L2}H^2(\mathbb R^n) = \{ f \in L^2 \mid |p|^2 \hat f(p) \in L^2 \}H2(Rn)={f∈L2∣∣p∣2f^​(p)∈L2}; equivalently, H0H_0H0​ is the inverse Fourier transform of the maximally defined multiplication by p2p^2p2. Units are ℏ=1\hbar = 1ℏ=1 and mass m=1/2m = 1/2m=1/2.

A real function VVV acts by the multiplication operator (Vf)(x)=V(x)f(x)(Vf)(x) = V(x) f(x)(Vf)(x)=V(x)f(x) on its maximal domain {f∈L2∣Vf∈L2}\{f \in L^2 \mid Vf \in L^2\}{f∈L2∣Vf∈L2}. The sum H0+VH_0 + VH0​+V is defined on D(H0)∩D(V)\mathfrak D(H_0) \cap \mathfrak D(V)D(H0​)∩D(V). L∞∞(Rn)L^\infty_\infty(\mathbb R^n)L∞∞​(Rn) denotes the bounded Borel functions vanishing at infinity, and Cc∞(Rn)C_c^\infty(\mathbb R^n)Cc∞​(Rn) the smooth compactly supported functions.

For a linear operator AAA, the resolvent RA(z)=(A−z)−1R_A(z) = (A - z)^{-1}RA​(z)=(A−z)−1 exists when A−zA - zA−z maps D(A)\mathfrak D(A)D(A) bijectively onto L2L^2L2 with bounded inverse; the resolvent set ρ(A)\rho(A)ρ(A) collects such zzz and σ(A)=C∖ρ(A)\sigma(A) = \mathbb C \setminus \rho(A)σ(A)=C∖ρ(A). The point spectrum σp(A)\sigma_p(A)σp​(A) is the set of eigenvalues; the discrete spectrum σd(A)\sigma_d(A)σd​(A) consists of the eigenvalues that are isolated in σ(A)\sigma(A)σ(A) and have finite-dimensional eigenspace; the essential spectrum is σess(A)=σ(A)∖σd(A)\sigma_{ess}(A) = \sigma(A) \setminus \sigma_d(A)σess​(A)=σ(A)∖σd​(A). An operator KKK is relatively compact with respect to AAA if D(A)⊆D(K)\mathfrak D(A) \subseteq \mathfrak D(K)D(A)⊆D(K) and KRA(z)K R_A(z)KRA​(z) is compact for one z∈ρ(A)z \in \rho(A)z∈ρ(A). AAA is bounded from below if ⟨ψ,Aψ⟩≥γ∥ψ∥2\langle \psi, A\psi\rangle \ge \gamma\|\psi\|^2⟨ψ,Aψ⟩≥γ∥ψ∥2 on D(A)\mathfrak D(A)D(A) for some real γ\gammaγ, and a subspace is a core of a closed operator if the closure of the restriction to it is the operator itself.

The hydrogen Hamiltonian is H(1)=−Δ−γ/∣x∣H^{(1)} = -\Delta - \gamma/|x|H(1)=−Δ−γ/∣x∣ on L2(R3)L^2(\mathbb R^3)L2(R3). A function in L2(Rn)L^2(\mathbb R^n)L2(Rn) is positive if it is ≥0\ge 0≥0 a.e. and not a.e. zero, and strictly positive if it is >0> 0>0 a.e.; a bounded operator is positivity improving if it maps positive functions to strictly positive ones.

Formalization targets

Goal: self-adjointness and essential spectrum (Theorem 10.2)

Let n≥1n \ge 1n≥1 and VVV real with V∈L∞∞(Rn)V \in L^\infty_\infty(\mathbb R^n)V∈L∞∞​(Rn) if n>3n > 3n>3 and V∈L∞∞(Rn)+L2(Rn)V \in L^\infty_\infty(\mathbb R^n) + L^2(\mathbb R^n)V∈L∞∞​(Rn)+L2(Rn) if n≤3n \le 3n≤3. Then VVV is relatively compact with respect to H0H_0H0​, and H=H0+VH = H_0 + VH=H0​+V has domain H2(Rn)H^2(\mathbb R^n)H2(Rn), is self-adjoint and bounded from below, satisfies

σess(H)=[0,∞),\sigma_{ess}(H) = [0,\infty),σess​(H)=[0,∞),

and has Cc∞(Rn)C_c^\infty(\mathbb R^n)Cc∞​(Rn) as a core.

Milestones

  • Sobolev bound (Lemma 10.1). For n≤3n \le 3n≤3, every ψ∈H2(Rn)\psi \in H^2(\mathbb R^n)ψ∈H2(Rn) is continuous and vanishes at infinity, and for every a>0a > 0a>0 there is b>0b > 0b>0 with ∥ψ∥∞≤a∥H0ψ∥+b∥ψ∥\|\psi\|_\infty \le a\|H_0\psi\| + b\|\psi\|∥ψ∥∞​≤a∥H0​ψ∥+b∥ψ∥ on H2(Rn)H^2(\mathbb R^n)H2(Rn).
  • Virial theorem (Theorem 10.3). If VVV is homogeneous of degree −1-1−1 under dilations, every normalized eigenfunction of H0+VH_0 + VH0​+V with eigenvalue λ\lambdaλ satisfies λ=−⟨ψ,H0ψ⟩=12⟨ψ,Vψ⟩\lambda = -\langle\psi, H_0\psi\rangle = \frac12\langle\psi, V\psi\rangleλ=−⟨ψ,H0​ψ⟩=21​⟨ψ,Vψ⟩; in particular λ<0\lambda < 0λ<0.
  • Hydrogen spectrum (Corollary 10.4). For γ>0\gamma > 0γ>0, σp(H(1))=σd(H(1))\sigma_p(H^{(1)}) = \sigma_d(H^{(1)})σp​(H(1))=σd​(H(1)) is a strictly increasing sequence of negative numbers converging to 000.
  • Hydrogen eigenvalues (Theorem 10.9, eigenvalue part). For γ>0\gamma > 0γ>0 the eigenvalues of H(1)H^{(1)}H(1) are En=−(γ/(2(n+1)))2E_n = -(\gamma/(2(n+1)))^2En​=−(γ/(2(n+1)))2, n∈N0n \in \mathbb N_0n∈N0​.
  • Perron–Frobenius for positivity improving operators (Theorem 10.11). If AAA is bounded, self-adjoint, real and positivity improving and ∥A∥\|A\|∥A∥ is an eigenvalue, it is simple with a strictly positive eigenfunction.
  • Nondegenerate ground state (Theorem 10.12). If H0+VH_0 + VH0​+V is self-adjoint, bounded below, has Cc∞C_c^\inftyCc∞​ as a core, and E0=min⁡σ(H)E_0 = \min\sigma(H)E0​=minσ(H) is an eigenvalue, then E0E_0E0​ is simple with a strictly positive eigenfunction.

Significance

The result. Theorem 10.2 is the existence theorem for one-particle quantum mechanics with decaying potentials. It makes H0+VH_0 + VH0​+V an observable on the natural domain H2H^2H2, guarantees a lowest energy, and places the continuum exactly at [0,∞)[0,\infty)[0,∞), so that all spectral information below zero is carried by bound states. Its three-dimensional case covers the Coulomb potential, and the same scheme (relative boundedness, Kato–Rellich, relative compactness, Weyl) is the template for the NNN-body HVZ theorem. The virial theorem, the qualitative and the explicit hydrogen spectrum, and the nondegeneracy of ground states are the standard first applications.

Formalizing it. None of these statements is formalized. Mathlib has the L2L^2L2 Fourier transform, tempered distributions and Sobolev spaces on the distribution side, and LinearPMap with adjoints and closures, but no free Schrödinger operator as an unbounded operator on L2L^2L2, no resolvent set or essential spectrum for unbounded operators, and no self-adjointness theorem for −Δ+V-\Delta + V−Δ+V. The mission asks for proofs of Teschl's statements and, with them, a reusable definition of H0H_0H0​ on H2(Rn)H^2(\mathbb R^n)H2(Rn) and of maximally defined multiplication operators.

Difficulty

The goal combines several chapters of the book. A proof needs self-adjointness of H0H_0H0​ on H2H^2H2 via the Fourier transform, the Sobolev bound of Lemma 10.1 to get D(H0)⊆D(V)\mathfrak D(H_0) \subseteq \mathfrak D(V)D(H0​)⊆D(V) with relative bound zero, the Kato–Rellich theorem, compactness of operators of the form g(x)f(p)g(x)f(p)g(x)f(p) (Lemma 7.11) to obtain relative compactness, Weyl's theorem on the invariance of the essential spectrum, σ(H0)=[0,∞)\sigma(H_0) = [0,\infty)σ(H0​)=[0,∞) with no eigenvalues, and the fact that Cc∞C_c^\inftyCc∞​ is a core for H0H_0H0​. None of these intermediate results is in Mathlib for unbounded operators.

The milestones add their own difficulties: the virial theorem requires the dilation group and a derivative argument on domains; Corollary 10.4 requires a variational argument producing infinitely many negative eigenvalues; Theorem 10.9 requires separation of variables in spherical coordinates and the Laguerre polynomials; and Theorem 10.12 uses the Trotter product formula and strong resolvent convergence to transfer positivity from e−tH0e^{-tH_0}e−tH0​ to e−tHe^{-tH}e−tH.

Formalization scope

Rn\mathbb R^nRn is EuclideanSpace ℝ (Fin n) with Lebesgue measure and L2(Rn)L^2(\mathbb R^n)L2(Rn) is Mathlib's Lp ℂ 2 volume, a separable complex Hilbert space. Unbounded operators are Mathlib LinearPMaps, sums of unbounded operators are LinearPMap sums on the intersection of domains, self-adjointness is Mathlib's IsSelfAdjoint, and "core" is LinearPMap.HasCore. The resolvent is the bounded two-sided inverse of A−zA - zA−z; ρ(A)\rho(A)ρ(A), σ(A)\sigma(A)σ(A), σp\sigma_pσp​, σd\sigma_dσd​ and σess\sigma_{ess}σess​ are defined from it, and Mathlib's Banach-algebra spectrum is not used. Compactness is IsCompactOperator.

The Fourier transform is Mathlib's unitary L2L^2L2 transform with kernel e−2πi⟨x,ξ⟩e^{-2\pi i\langle x,\xi\rangle}e−2πi⟨x,ξ⟩, not Teschl's (2π)−n/2e−ipx(2\pi)^{-n/2}e^{-ipx}(2π)−n/2e−ipx. H0H_0H0​ is defined as F−1(2π∣ξ∣)2F\mathcal F^{-1}(2\pi|\xi|)^2\mathcal FF−1(2π∣ξ∣)2F and H2H^2H2 as {f∣(2π∣ξ∣)2Ff∈L2}\{f \mid (2\pi|\xi|)^2 \mathcal F f \in L^2\}{f∣(2π∣ξ∣)2Ff∈L2}; both coincide with the book's objects, independently of the normalization. No projection-valued measure or functional calculus is taken as data. C∞(Rn)C_\infty(\mathbb R^n)C∞​(Rn) is Mathlib's space of continuous functions vanishing at infinity, and positivity of complex values is taken in ComplexOrder.

The virial hypothesis U(−s)VU(s)=e−sVU(-s)VU(s) = e^{-s}VU(−s)VU(s)=e−sV is stated as V(esx)=e−sV(x)V(e^s x) = e^{-s}V(x)V(esx)=e−sV(x) for almost every xxx, for every sss, which is what the operator identity means for a multiplication operator. Corollary 10.4's index set {Ej−1}j∈N0\{E_{j-1}\}_{j\in\mathbb N_0}{Ej−1​}j∈N0​​ is read as the sequence E0,E1,…E_0, E_1, \dotsE0​,E1​,…. Only the eigenvalue formula of Theorem 10.9 is included, not its explicit eigenbasis.

A trivializing formalization is ruled out: the only hypotheses of the goal are the function-space conditions on VVV and n≥1n \ge 1n≥1. Neither D(H0)⊆D(V)\mathfrak D(H_0) \subseteq \mathfrak D(V)D(H0​)⊆D(V), a relative bound below one, nor closedness of H0+VH_0 + VH0​+V is assumed; the equality of the domain with H2(Rn)H^2(\mathbb R^n)H2(Rn) and the relative compactness of VVV are conclusions. The essential spectrum requires all three of "eigenvalue", "isolated" and "finite multiplicity" in its complement, so [0,∞)[0,\infty)[0,∞) is a genuine identification.

Selected references

  • G. Teschl, Mathematical Methods in Quantum Mechanics, With Applications to Schrödinger Operators, Graduate Studies in Mathematics 99, AMS, 2009, Chapter 10. https://doi.org/10.1090/gsm/099
  • T. Kato, Fundamental properties of Hamiltonian operators of Schrödinger type, Transactions of the AMS 70 (1951), 195–211. https://doi.org/10.1090/S0002-9947-1951-0041010-X
  • M. Reed and B. Simon, Methods of Modern Mathematical Physics II: Fourier Analysis, Self-Adjointness (Section X.2) and IV: Analysis of Operators (Sections XIII.4, XIII.12), Academic Press, 1975, 1978.
  • H. L. Cycon, R. G. Froese, W. Kirsch and B. Simon, Schrödinger Operators, Springer, 1987.
20 thms2 active usersReviewed
AnalysisDifferential GeometryPure Mathematics·Captain: mikedeng1

Tasty Bits of Several Complex Variables V: CR Functions and Severi's Extension TheoremTextbook

Motivation

A holomorphic function on an open set of Cn\mathbb{C}^nCn restricts to a real hypersurface MMM as a function that satisfies the tangential Cauchy–Riemann equations: it is annihilated by every antiholomorphic vector tangent to MMM. Functions on MMM with this property are called CR functions, and they are the boundary values that several complex variables studies whenever a domain is approached through its boundary. The basic question is the converse: when is a CR function locally the restriction of a holomorphic function? For smooth data the answer is "not always" (the book's Example 3.2.7 gives a smooth CR function on the hyperplane Im⁡z2=0\operatorname{Im} z_2 = 0Imz2​=0 that is no such restriction). For real-analytic data the answer is "always", and that is Severi's theorem, the goal of this mission.

The mission follows Chapter 3 of Jiří Lebl's open textbook Tasty Bits of Several Complex Variables (version 4.4, 2026), where Severi's theorem is proved by complexification: a real-analytic function of zzz and zˉ\bar zzˉ is treated as a holomorphic function of two independent variables (z,ζ)(z, \zeta)(z,ζ) restricted to the diagonal ζ=zˉ\zeta = \bar zζ=zˉ. The milestones are the steps of that route: uniqueness on totally real slices, the two complexification propositions, the fact that restrictions of holomorphic functions are CR, and the normal form wˉ=Φ(z,zˉ,w)\bar w = \Phi(z, \bar z, w)wˉ=Φ(z,zˉ,w) of a real-analytic hypersurface.

Setting

Write Cn≅R2n\mathbb{C}^n \cong \mathbb{R}^{2n}Cn≅R2n with zk=xk+iykz_k = x_k + i y_kzk​=xk​+iyk​. A function on an open subset of RN\mathbb{R}^NRN is real-analytic if near each point it equals a convergent power series in the real coordinates. A set M⊂CnM \subset \mathbb{C}^nM⊂Cn is a real-analytic hypersurface if near each of its points, after choosing one real coordinate yyy among the 2n2n2n and collecting the other 2n−12n-12n−1 as xxx, it is the graph y=φ(x)y = \varphi(x)y=φ(x) of a real-analytic function φ\varphiφ.

A function fff on an arbitrary set X⊂CnX \subset \mathbb{C}^nX⊂Cn is smooth (respectively real-analytic) if near each point of XXX it agrees on XXX with a smooth (respectively real-analytic) function FFF defined on an open neighbourhood. A defining function of MMM at ppp is a smooth real function rrr on an open V∋pV \ni pV∋p with nonvanishing derivative and M∩V={r=0}M \cap V = \{r = 0\}M∩V={r=0}; MMM is a smooth real hypersurface if it has one at every point.

With the Wirtinger derivative ∂/∂zˉk=12(∂/∂xk+i ∂/∂yk)\partial/\partial\bar z_k = \tfrac12(\partial/\partial x_k + i\,\partial/\partial y_k)∂/∂zˉk​=21​(∂/∂xk​+i∂/∂yk​), the space of antiholomorphic tangent vectors of MMM at ppp is

Tp(0,1)M={∑kak∂∂zˉk∣p:∑kak∂r∂zˉk(p)=0}.T^{(0,1)}_p M = \Big\{ \textstyle\sum_{k} a_k \frac{\partial}{\partial \bar z_k}\big|_p : \sum_k a_k \frac{\partial r}{\partial \bar z_k}(p) = 0 \Big\}.Tp(0,1)​M={∑k​ak​∂zˉk​∂​​p​:∑k​ak​∂zˉk​∂r​(p)=0}.

A smooth f:M→Cf : M \to \mathbb{C}f:M→C is a CR function if Xpf=0X_p f = 0Xp​f=0 for all p∈Mp \in Mp∈M and Xp∈Tp(0,1)MX_p \in T^{(0,1)}_pMXp​∈Tp(0,1)​M, where XpfX_p fXp​f is computed on any smooth local extension of fff. A real-analytic CR function is a CR function that is real-analytic on MMM.

In Lean, Cn\mathbb{C}^nCn is Fin n → ℂ, and these notions are the definitions IsRealAnalyticOn, IsRealAnalyticHypersurface, IsSmoothHypersurface, IsSmoothOnSet / IsRealAnalyticOnSet, antiholTangent and IsSmoothCRFunction / IsRealAnalyticCRFunction of the namespace LeblSCV.CR.

Formalization targets

Goal: Severi's theorem (Theorem 3.2.9)

Let M⊂CnM \subset \mathbb{C}^nM⊂Cn be a real-analytic hypersurface, p∈Mp \in Mp∈M, and f:M→Cf : M \to \mathbb{C}f:M→C a real-analytic CR function. Then there are an open neighbourhood UUU of ppp and F∈O(U)F \in \mathcal{O}(U)F∈O(U) with

F(q)=f(q)for all q∈M∩U.F(q) = f(q) \qquad \text{for all } q \in M \cap U.F(q)=f(q)for all q∈M∩U.

Milestones

  1. Lemma 3.1.2. Holomorphic functions on a domain V⊂CnV \subset \mathbb{C}^nV⊂Cn that agree on V∩Rn≠∅V \cap \mathbb{R}^n \neq \emptysetV∩Rn=∅ agree on VVV.
  2. Proposition 3.1.3. A real-analytic function on a domain U⊂RnU \subset \mathbb{R}^nU⊂Rn extends to a unique holomorphic function on some domain V⊃UV \supset UV⊃U of Cn\mathbb{C}^nCn.
  3. Lemma 3.1.4. Holomorphic functions on a domain V⊂Cn×CnV \subset \mathbb{C}^n \times \mathbb{C}^nV⊂Cn×Cn that agree on V∩{ζ=zˉ}≠∅V \cap \{\zeta = \bar z\} \neq \emptysetV∩{ζ=zˉ}=∅ agree on VVV.
  4. Proposition 3.1.5. A real-analytic fff on a domain U⊂CnU \subset \mathbb{C}^nU⊂Cn has a unique holomorphic FFF on a domain V⊃{(z,zˉ):z∈U}V \supset \{(z, \bar z) : z \in U\}V⊃{(z,zˉ):z∈U} with F(z,zˉ)=f(z)F(z, \bar z) = f(z)F(z,zˉ)=f(z).
  5. Proposition 3.2.6. The restriction of a holomorphic function to a smooth (respectively real-analytic) hypersurface is a smooth (respectively real-analytic) CR function.
  6. Proposition 3.2.8. After a translation and a unitary rotation taking ppp to 000, a real-analytic hypersurface is locally wˉ=Φ(z,zˉ,w)\bar w = \Phi(z, \bar z, w)wˉ=Φ(z,zˉ,w) with Φ\PhiΦ holomorphic, Φ\PhiΦ, ∂Φ/∂zk\partial\Phi/\partial z_k∂Φ/∂zk​, ∂Φ/∂ζk\partial\Phi/\partial\zeta_k∂Φ/∂ζk​ vanishing at 000, and w=Φˉ(ζ,z,Φ(z,ζ,w))w = \bar\Phi(\zeta, z, \Phi(z, \zeta, w))w=Φˉ(ζ,z,Φ(z,ζ,w)).

Significance

Severi's theorem identifies the real-analytic CR functions on a real-analytic hypersurface with the local traces of holomorphic functions. Together with Proposition 3.2.6 it shows that, in the real-analytic category, the tangential Cauchy–Riemann equations are exactly the obstruction to holomorphic extension. It is the model for the later extension theorems of the chapter: the Baouendi–Trèves approximation theorem (Theorem 3.3.1) and the Lewy extension theorem (Theorem 3.4.1), which replace real-analyticity with smoothness and pay for it with one-sided extension or approximation. Complexification (Propositions 3.1.3 and 3.1.5) is also a tool in its own right, used for the composition of real-analytic maps (Proposition 3.1.10) and for pluriharmonic functions.

All results here are classical and proved in the book; none of them is formalized in Lean or Mathlib as far as a search of the Prove2Me corpus and Mathlib shows. Mathlib has real and complex analyticity (AnalyticOnNhd), the one-variable and several-variable identity theorems for analytic functions, and the holomorphic implicit function theorem is within reach, but it has no notion of real hypersurface, CR vector or CR function. The mission produces that layer and a checked proof of the first extension theorem for CR functions.

Difficulty

The obvious idea is to take a real-analytic extension of fff, complexify it to a holomorphic function f(z,w,ζ,ω)f(z, w, \zeta, \omega)f(z,w,ζ,ω) of 2n2n2n variables, and substitute ω=Φ(z,ζ,w)\omega = \Phi(z, \zeta, w)ω=Φ(z,ζ,w) to remove wˉ\bar wwˉ. That produces a holomorphic function of (z,w,ζ)(z, w, \zeta)(z,w,ζ), not of (z,w)(z, w)(z,w); showing that it does not depend on ζ\zetaζ requires transporting the CR equations, which hold only on MMM, to the whole complexified hypersurface. That transport is a uniqueness statement for the complexification, and it rests on the normal form of Proposition 3.2.8, itself an application of the holomorphic implicit function theorem to the complexified defining function together with its reality symmetry. On the Lean side, the diagonal {ζ=zˉ}\{\zeta = \bar z\}{ζ=zˉ} is not a complex submanifold, so identity theorems along it (Lemmas 3.1.2 and 3.1.4) do not follow from the standard identity theorem for open sets.

Formalization scope

  • Cn\mathbb{C}^nCn is Fin n → ℂ, with 0-based indices; Cn×Cn\mathbb{C}^n \times \mathbb{C}^nCn×Cn is the product type. The sup norm of Fin n → ℂ never enters a statement: no ball, norm or distance occurs.
  • Holomorphic on an open set is DifferentiableOn ℂ, which is equivalent to the book's Definition 1.1.2 there. A domain is an open connected (hence nonempty) set.
  • Real-analytic is Mathlib's AnalyticOnNhd ℝ on an open set, applied to Cn\mathbb{C}^nCn as a real vector space, which is the book's power series in x,yx, yx,y (equivalently in z,zˉz, \bar zz,zˉ).
  • A real-analytic hypersurface is a local graph over one of the 2n2n2n real coordinates (Definition 3.1.9), not the zero set of a real-analytic function.
  • Functions on MMM are functions on Cn\mathbb{C}^nCn of which only the values on MMM are read. "Smooth on MMM" means locally the restriction of a C∞C^\inftyC∞ function (Definition 3.2.1). The CR condition is imposed for every defining function and every smooth local extension, which is equivalent to one choice because both are independent of the choice.
  • Proposition 3.2.8 is stated for n=m+1n = m + 1n=m+1, with the unitary change of coordinates q↦U(q−p)q \mapsto U(q - p)q↦U(q−p) and every "near the origin" made an explicit open set. Only its displayed statement is a target; the remarks that follow it on the page are not.
  • The goal cannot be satisfied by an empty hypothesis: real-analytic hypersurfaces exist (a sorry-free check shows {Im⁡z1=0}\{\operatorname{Im} z_1 = 0\}{Imz1​=0} qualifies), and by Proposition 3.2.6 every restriction of a holomorphic function is a real-analytic CR function. The CR condition is the intrinsic one on Tp(0,1)MT^{(0,1)}_pMTp(0,1)​M; replacing it with "restriction of a holomorphic function" would make the goal a tautology and is ruled out.
  • Needed infrastructure: the several-variable identity theorem, holomorphic implicit functions, power series in 2n2n2n variables, and the chain rule for Wirtinger derivatives. The definitions of real-analytic hypersurface and CR function are reusable by the later extension theorems of Chapter 3. Contributions of any milestone, of a proof that Tp(0,1)MT^{(0,1)}_pMTp(0,1)​M is independent of the defining function, or of Exercise 3.2.3 (independence of the extension) are welcome.

Selected references

  • J. Lebl, Tasty Bits of Several Complex Variables, version 4.4, 2026, Chapter 3. https://www.jirka.org/scv/
  • Mathlib documentation, Mathlib.Analysis.Analytic.Basic (analytic functions, AnalyticOnNhd). https://leanprover-community.github.io/mathlib4_docs/Mathlib/Analysis/Analytic/Basic.html
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AnalysisHarmonic Analysis·Captain: mikedeng1

Notes on Partial Differential Equations VII: The Heat Kernel and the Linear Heat and Schrödinger EquationsTextbook

Motivation

The heat equation ut=Δuu_t = \Delta uut​=Δu and the free Schrödinger equation iut=−Δui u_t = -\Delta uiut​=−Δu are the two model evolution equations of linear PDE on Rn\mathbb{R}^nRn. The first describes diffusion and is the prototype of every parabolic equation; the second describes a free quantum particle and is the prototype of dispersive wave equations. Both are solved explicitly by the Fourier transform and by convolution with a Gaussian-type kernel, and the estimates obtained from these formulas (smoothing, L2L^2L2 and HsH^sHs energy bounds, L1→L∞L^1 \to L^\inftyL1→L∞ decay) are the tools later used for nonlinear problems: semilinear heat equations, nonlinear Schrödinger equations, Galerkin constructions for general parabolic PDE, and Strichartz estimates.

This mission formalizes Chapter 5, §§5.1–5.3, of J. K. Hunter's Notes on Partial Differential Equations (UC Davis lecture notes, revised 6/18/2014, author's copy), which follows the presentation of Taylor's Partial Differential Equations (Taylor, vol. I, Ch. 3). The classical material goes back to Fourier (1822) for the heat kernel and to the analysis of dispersion for the Schrödinger group in the twentieth century; the goal and milestones are textbook results with complete proofs in the literature.

Setting

Write Rn\mathbb{R}^nRn for Euclidean space with Lebesgue measure, ∣x∣|x|∣x∣ for the Euclidean norm and Δ=∑i∂i2\Delta = \sum_i \partial_i^2Δ=∑i​∂i2​ for the Laplacian. The heat kernel is

Γ(x,t)=1(4πt)n/2 e−∣x∣2/4t,x∈Rn, t>0,\Gamma(x,t) = \frac{1}{(4\pi t)^{n/2}}\, e^{-|x|^2/4t}, \qquad x \in \mathbb{R}^n,\ t > 0,Γ(x,t)=(4πt)n/21​e−∣x∣2/4t,x∈Rn, t>0,

and for data fff the heat convolution is u(x,t)=∫RnΓ(x−y,t)f(y) dyu(x,t) = \int_{\mathbb{R}^n} \Gamma(x-y,t) f(y)\,dyu(x,t)=∫Rn​Γ(x−y,t)f(y)dy.

The Schwartz space S(Rn)\mathcal S(\mathbb{R}^n)S(Rn) consists of smooth functions all of whose derivatives decay faster than every power of ∣x∣|x|∣x∣, with the Fréchet topology of the seminorms sup⁡∣xα∂βf∣\sup |x^\alpha \partial^\beta f|sup∣xα∂βf∣. A curve u:I→Su : I \to \mathcal Su:I→S on a time interval III has a strong derivative vvv at ttt if the difference quotients (u(t+h)−u(t))/h(u(t+h)-u(t))/h(u(t+h)−u(t))/h converge to vvv in S\mathcal SS; Ck(I;S)C^k(I;\mathcal S)Ck(I;S) and C∞(I;S)C^\infty(I;\mathcal S)C∞(I;S) are defined with continuous strong derivatives. A Schwartz solution of the heat problem with data f∈Sf \in \mathcal Sf∈S is a curve u∈C([0,∞);S)∩C1(0,∞;S)u \in C([0,\infty);\mathcal S) \cap C^1(0,\infty;\mathcal S)u∈C([0,∞);S)∩C1(0,∞;S) with u(0)=fu(0) = fu(0)=f and ut(t)=Δu(t)u_t(t) = \Delta u(t)ut​(t)=Δu(t) for t>0t > 0t>0; a Schwartz solution of the Schrödinger problem is u∈C1(R;S)u \in C^1(\mathbb{R};\mathcal S)u∈C1(R;S) with u(0)=fu(0) = fu(0)=f and iut=−Δui u_t = -\Delta uiut​=−Δu for all ttt.

The Fourier transform is used in the book's normalization,

f^(k)=1(2π)n∫Rnf(x) e−ik⋅x dx,\hat f(k) = \frac{1}{(2\pi)^n}\int_{\mathbb{R}^n} f(x)\, e^{-ik\cdot x}\,dx,f^​(k)=(2π)n1​∫Rn​f(x)e−ik⋅xdx,

and, with ⟨k⟩=(1+∣k∣2)1/2\langle k\rangle = (1+|k|^2)^{1/2}⟨k⟩=(1+∣k∣2)1/2, the Sobolev norm is ∥f∥Hs=((2π)n∫⟨k⟩2s∣f^(k)∣2 dk)1/2\|f\|_{H^s} = \big((2\pi)^n\int \langle k\rangle^{2s}|\hat f(k)|^2\,dk\big)^{1/2}∥f∥Hs​=((2π)n∫⟨k⟩2s∣f^​(k)∣2dk)1/2 for s∈Rs \in \mathbb{R}s∈R.

Formalization targets

Goal: smoothing by the heat kernel (Theorem 5.5)

Let 1≤p≤∞1 \le p \le \infty1≤p≤∞ and f∈Lp(Rn)f \in L^p(\mathbb{R}^n)f∈Lp(Rn). Then the heat convolution converges absolutely for t>0t>0t>0, uuu is C∞C^\inftyC∞ on Rn×(0,∞)\mathbb{R}^n \times (0,\infty)Rn×(0,∞), and

ut=Δu(t>0).u_t = \Delta u \quad (t > 0).ut​=Δu(t>0).

If p<∞p < \inftyp<∞, every derivative of uuu tends to zero as ∣x∣→∞|x| \to \infty∣x∣→∞ at each fixed t>0t > 0t>0, and

u(⋅,t)→f  in Lp as t→0+.u(\cdot,t) \to f \ \text{ in } L^p \text{ as } t \to 0^+.u(⋅,t)→f  in Lp as t→0+.

This is the chapter's statement that rough data are instantly smoothed while the initial condition is attained in the LpL^pLp sense; it involves no Fourier transform.

Milestones

  1. Eq. (5.9): Γ\GammaΓ is C∞C^\inftyC∞ on Rn×(0,∞)\mathbb{R}^n \times (0,\infty)Rn×(0,∞) and Γt=ΔΓ\Gamma_t = \Delta\GammaΓt​=ΔΓ.
  2. Theorem 5.4: for f∈Sf \in \mathcal Sf∈S the heat problem has a unique Schwartz solution; it lies in C∞([0,∞);S)C^\infty([0,\infty);\mathcal S)C∞([0,∞);S), satisfies u^(k,t)=f^(k)e−t∣k∣2\hat u(k,t) = \hat f(k) e^{-t|k|^2}u^(k,t)=f^​(k)e−t∣k∣2, and equals the heat convolution for t>0t > 0t>0.
  3. Theorem 5.8: ∥u(t)∥L2≤∥f∥L2\|u(t)\|_{L^2} \le \|f\|_{L^2}∥u(t)∥L2​≤∥f∥L2​ and ∥u(t)∥L∞≤(4πt)−n/2∥f∥L1\|u(t)\|_{L^\infty} \le (4\pi t)^{-n/2}\|f\|_{L^1}∥u(t)∥L∞​≤(4πt)−n/2∥f∥L1​.
  4. Theorem 5.9: ∥u(t)∥Hs≤∥f∥Hs\|u(t)\|_{H^s} \le \|f\|_{H^s}∥u(t)∥Hs​≤∥f∥Hs​ for all s∈Rs \in \mathbb{R}s∈R, t≥0t \ge 0t≥0.
  5. Theorem 5.10: on [0,T][0,T][0,T], max⁡t∥u(t)∥Hs≤∥f∥Hs\max_t \|u(t)\|_{H^s} \le \|f\|_{H^s}maxt​∥u(t)∥Hs​≤∥f∥Hs​ and ∥Du∥L2([0,T];Hs)≤12∥f∥Hs\|Du\|_{L^2([0,T];H^s)} \le \tfrac{1}{\sqrt 2}\|f\|_{H^s}∥Du∥L2([0,T];Hs)​≤2​1​∥f∥Hs​.
  6. Theorem 5.15: for f∈Sf \in \mathcal Sf∈S the Schrödinger problem has a unique solution in C∞(R;S)C^\infty(\mathbb{R};\mathcal S)C∞(R;S), with u^(k,t)=e−it∣k∣2f^(k)\hat u(k,t) = e^{-it|k|^2}\hat f(k)u^(k,t)=e−it∣k∣2f^​(k) and u(⋅,t)=ΓS(⋅,t)∗fu(\cdot,t) = \Gamma_S(\cdot,t) * fu(⋅,t)=ΓS​(⋅,t)∗f for t≠0t \ne 0t=0, ΓS(x,t)=(4πit)−n/2ei∣x∣2/4t\Gamma_S(x,t) = (4\pi i t)^{-n/2} e^{i|x|^2/4t}ΓS​(x,t)=(4πit)−n/2ei∣x∣2/4t.
  7. Theorem 5.16: ∥u(t)∥L2≤∥f∥L2\|u(t)\|_{L^2} \le \|f\|_{L^2}∥u(t)∥L2​≤∥f∥L2​, ∥u(t)∥L∞≤(4π∣t∣)−n/2∥f∥L1\|u(t)\|_{L^\infty} \le (4\pi|t|)^{-n/2}\|f\|_{L^1}∥u(t)∥L∞​≤(4π∣t∣)−n/2∥f∥L1​ and, for 2<p<∞2<p<\infty2<p<∞, ∥u(t)∥Lp≤(4π∣t∣)−n(1/2−1/p)∥f∥Lp′\|u(t)\|_{L^p} \le (4\pi|t|)^{-n(1/2-1/p)}\|f\|_{L^{p'}}∥u(t)∥Lp​≤(4π∣t∣)−n(1/2−1/p)∥f∥Lp′​.
  8. Theorem 5.17: ∥u(t)∥Hs=∥f∥Hs\|u(t)\|_{H^s} = \|f\|_{H^s}∥u(t)∥Hs​=∥f∥Hs​ for all sss and ttt.

A further item, not a milestone, records that ∫Γ(x,t) dx=1\int \Gamma(x,t)\,dx = 1∫Γ(x,t)dx=1 for t>0t > 0t>0 (p. 131).

Significance

The result itself. Theorem 5.5 is the statement that the heat semigroup maps LpL^pLp into smooth functions decaying with all derivatives, and that it is strongly continuous on LpL^pLp for p<∞p < \inftyp<∞. It is used whenever a parabolic problem with rough data is solved by the Duhamel formula, in particular for the semilinear heat equation in the next part of the chapter. Theorem 5.4 and the energy estimates 5.9–5.10 are the input for generalized HsH^sHs solutions (Theorem 5.12) and for Galerkin existence for parabolic PDE in Chapter 6. The Schrödinger estimates 5.16–5.17 are the linear input of the local theory of nonlinear Schrödinger equations and of Strichartz estimates.

Formalizing it. All results are classical and fully proved on paper. Mathlib has Schwartz functions, its own Fourier transform on S\mathcal SS with Plancherel, Gaussian integrals and Fourier transforms of Gaussians, convolution and approximate identities for compactly supported kernels, and the Laplacian on inner-product spaces. It does not have the heat kernel on Rn\mathbb{R}^nRn as a solution operator, the differentiation of Schwartz-valued curves, the HsH^sHs energy estimates, or the dispersive estimates for the Schrödinger group. A platform development of the heat kernel exists only on R3\mathbb{R}^3R3 with a viscosity parameter (the Navier–Stokes mission), and the platform's Plancherel theorem is in Mathlib's normalization. The remaining work is to formalize the known proofs in the book's normalization and dimension.

Difficulty

For the goal, the obvious argument is "differentiate under the integral sign and apply the mollifier theorem". Both steps need care in Lean. Differentiation in (x,t)(x,t)(x,t) requires domination of every derivative of Γ\GammaΓ uniformly on neighbourhoods of (x,t)(x,t)(x,t), paired by Hölder's inequality with an arbitrary f∈Lpf \in L^pf∈Lp. The approximation-of-identity result in Mathlib and in the book (Theorem 1.28) is stated for compactly supported mollifiers, whereas Γ(⋅,t)\Gamma(\cdot,t)Γ(⋅,t) has full support, so the LpL^pLp convergence needs the Gaussian version with a tail estimate. The decay of all derivatives as ∣x∣→∞|x| \to \infty∣x∣→∞ relies on p<∞p < \inftyp<∞. For the Schwartz-space results the difficulty is the calculus of S\mathcal SS-valued curves: strong differentiability is convergence of difference quotients in every Schwartz seminorm, and uniqueness requires passing from the strong equation to the pointwise ODE for u^(k,t)\hat u(k,t)u^(k,t). The Lp′→LpL^{p'} \to L^pLp′→Lp bound (5.16) rests on Riesz–Thorin interpolation, which Mathlib does not have.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n) with volume; coordinates are 0-based (i : Fin n). Δ\DeltaΔ is Mathlib's Laplacian: on functions for the goal and (5.9), and Δ:S→S\Delta : \mathcal S \to \mathcal SΔ:S→S for the Schwartz solutions. Smoothness is ContDiff/ContDiffOn ℝ ∞.
  • S\mathcal SS is Mathlib's SchwartzMap with its Fréchet topology, the same as the book's. Real-valued for the heat equation, complex-valued for Schrödinger. Strong derivatives, C∞(I;S)C^\infty(I;\mathcal S)C∞(I;S) and the two solution predicates are defined in HunterPDE.HeatFourier.SchwartzCurve. Uniqueness in Theorem 5.4 is agreement for t≥0t \ge 0t≥0.
  • The Fourier transform is the book's (2π)−n∫fe−ik⋅x(2\pi)^{-n}\int f e^{-ik\cdot x}(2π)−n∫fe−ik⋅x, defined explicitly; Mathlib's 𝓕 is not used. The HsH^sHs norm is [0,∞][0,\infty][0,∞]-valued and is the norm of the book's HsH^sHs inner product, ((2π)n∫⟨k⟩2s∣f^∣2)1/2\big((2\pi)^n\int\langle k\rangle^{2s}|\hat f|^2\big)^{1/2}((2π)n∫⟨k⟩2s∣f^​∣2)1/2; the norm formula printed with Definition 5.74 places (2π)n(2\pi)^n(2π)n outside the square root, which differs by the constant (2π)n/2(2\pi)^{n/2}(2π)n/2 and does not affect any statement here, since every HsH^sHs inequality and identity has an HsH^sHs norm on both sides. LpL^pLp norms are eLpNorm in [0,∞][0,\infty][0,∞], and the factors 1/(4π∣t∣)…1/(4\pi|t|)^{\dots}1/(4π∣t∣)… in Theorem 5.16 are divisions in [0,∞][0,\infty][0,∞], so t=0t = 0t=0 gives the trivial bound ∞\infty∞.
  • Corrections of the page. (i) The book states u∈C0∞(Rn×(0,∞))u \in C_0^\infty(\mathbb{R}^n \times (0,\infty))u∈C0∞​(Rn×(0,∞)) in Theorem 5.5 for every p≤∞p \le \inftyp≤∞. For p=∞p = \inftyp=∞ this fails (f≡1f \equiv 1f≡1), so the decay of derivatives is stated for p<∞p < \inftyp<∞, which is the case its proof covers. "C0∞C_0^\inftyC0∞​" is read as the proof explains it: every derivative tends to zero as ∣x∣→∞|x| \to \infty∣x∣→∞ at fixed t>0t > 0t>0. (ii) The Schrödinger kernel is printed as (4πit)−n/2e−i∣x∣2/4t(4\pi i t)^{-n/2}e^{-i|x|^2/4t}(4πit)−n/2e−i∣x∣2/4t. The sign of the exponent contradicts the book's (5.15), so the corrected e+i∣x∣2/4te^{+i|x|^2/4t}e+i∣x∣2/4t is used, with the principal-branch power.
  • Theorems 5.9 and 5.10 assume the solution property of Theorem 5.4 rather than C∞C^\inftyC∞ regularity in time. By Theorem 5.4 this is the same solution. The absolute convergence of (5.5) is part of the goal's conclusion.
  • Ruling out trivializations. The goal is not the statement "uuu is smooth": the heat equation, the decay of every derivative and the LpL^pLp convergence are all required. No hypothesis restricts fff beyond f∈Lpf \in L^pf∈Lp. The solution predicates are satisfiable (the zero curve solves the problem with zero data), and existence in Theorems 5.4 and 5.15 is asserted, not assumed.
  • Not included: generalized HsH^sHs solutions (Definition 5.11, Theorem 5.12), the heat Lp′→LpL^{p'}\to L^pLp′→Lp bound (5.10), and the Fourier-transform background of Appendix 5.B (Theorems 5.66–5.73). Contributions welcome: a Gaussian approximate-identity theorem in LpL^pLp, the S\mathcal SS-valued calculus of Proposition 5.3, and a conversion lemma between the book's and Mathlib's Fourier normalizations. All three are reusable across this series (semigroups, the semilinear heat equation, NLS).

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, Chapter 5. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • M. E. Taylor, Partial Differential Equations I: Basic Theory, 2nd ed., Springer, 2011. https://doi.org/10.1007/978-1-4419-7055-8
  • L. C. Evans, Partial Differential Equations, 2nd ed., AMS Graduate Studies in Mathematics 19, 2010, §2.3 and §4.3. https://doi.org/10.1090/gsm/019
  • T. Cazenave, Semilinear Schrödinger Equations, Courant Lecture Notes 10, AMS, 2003, Ch. 2. https://doi.org/10.1090/cln/010
12 thms2 active usersReviewed
AnalysisProbability·Captain: Lucas

Hairer: A Theory of Regularity Structures I — The Reconstruction TheoremResearch Paper

Motivation

Several equations of mathematical physics are written down formally but have no classical meaning as stated. The dynamical Φ34\Phi^4_3Φ34​ model ∂tu=Δu−u3+ξ\partial_t u = \Delta u - u^3 + \xi∂t​u=Δu−u3+ξ on the three-dimensional torus, the KPZ equation ∂th=∂x2h+(∂xh)2−∞+ξ\partial_t h = \partial_x^2 h + (\partial_x h)^2 - \infty + \xi∂t​h=∂x2​h+(∂x​h)2−∞+ξ, and the parabolic Anderson model ∂tu=Δu+u ξ\partial_t u = \Delta u + u\,\xi∂t​u=Δu+uξ all require multiplying a distribution of negative regularity by itself, an operation that Schwartz distribution theory does not provide. Martin Hairer's A theory of regularity structures (Invent. Math. 198 (2014) 269–504, arXiv:1303.5113) develops a calculus in which such products, and the resulting fixed-point problems, become well posed.

The line of work leading to it is short and well documented: rough path theory (Lyons, 1998) solved the analogous problem for controlled ordinary differential equations driven by irregular signals; Gubinelli's controlled paths (2004) and branched rough paths (2010) reorganised it around local expansions; Hairer's theory extends that idea from paths to fields on Rd\mathbb{R}^dRd with anisotropic (e.g. parabolic) scaling. Paracontrolled distributions (Gubinelli–Imkeller–Perkowski, 2015) give an alternative route to some of the same equations. The algebraic and probabilistic infrastructure around regularity structures has since been systematised (Bruned–Hairer–Zambotti, 2019; Chandra–Hairer, 2016), but the analytic core is still the 2014 paper.

Setting

Fix a dimension ddd and a scaling s=(s1,…,sd)s = (s_1,\dots,s_d)s=(s1​,…,sd​) of positive integers, with ∣s∣=∑isi|s| = \sum_i s_i∣s∣=∑i​si​, and put ∥x∥s=max⁡i∣xi∣1/si\|x\|_s = \max_i |x_i|^{1/s_i}∥x∥s​=maxi​∣xi​∣1/si​. For δ>0\delta > 0δ>0, a point x∈Rdx \in \mathbb{R}^dx∈Rd and a test function φ\varphiφ, the rescaled test function is

(Ss,xδφ)(y)=δ−∣s∣ φ ⁣(y1−x1δs1,…,yd−xdδsd).(S^{\delta}_{s,x}\varphi)(y) = \delta^{-|s|}\,\varphi\!\left(\frac{y_1-x_1}{\delta^{s_1}},\dots,\frac{y_d-x_d}{\delta^{s_d}}\right).(Ss,xδ​φ)(y)=δ−∣s∣φ(δs1​y1​−x1​​,…,δsd​yd​−xd​​).

Write Bs,0r\mathcal{B}^r_{s,0}Bs,0r​ for the set of test functions supported in {∥y∥s≤1}\{\|y\|_s \le 1\}{∥y∥s​≤1} whose derivatives up to order rrr are bounded by 111. For α<0\alpha<0α<0, a distribution ξ\xiξ belongs to the Hölder–Besov space Csα\mathcal{C}^\alpha_sCsα​ if, on every compact set KKK, ∣⟨ξ,Ss,xδη⟩∣≤Cδα|\langle \xi, S^{\delta}_{s,x}\eta\rangle| \le C\delta^{\alpha}∣⟨ξ,Ss,xδ​η⟩∣≤Cδα uniformly over x∈Kx\in Kx∈K, δ∈(0,1]\delta \in (0,1]δ∈(0,1] and η∈Bs,0r\eta \in \mathcal{B}^r_{s,0}η∈Bs,0r​ with r=−⌊α⌋r=-\lfloor\alpha\rfloorr=−⌊α⌋.

A regularity structure (A,T,G)(A,T,G)(A,T,G) consists of an index set A⊆RA \subseteq \mathbb{R}A⊆R containing 000, bounded below and locally finite; a graded vector space T=⨁α∈ATαT = \bigoplus_{\alpha\in A} T_\alphaT=⨁α∈A​Tα​ with T0≅RT_0 \cong \mathbb{R}T0​≅R spanned by a unit 1\mathbf{1}1; and a group GGG of linear operators on TTT with Γa−a∈⨁β<αTβ\Gamma a - a \in \bigoplus_{\beta<\alpha}T_\betaΓa−a∈⨁β<α​Tβ​ for a∈Tαa \in T_\alphaa∈Tα​, and Γ1=1\Gamma\mathbf{1} = \mathbf{1}Γ1=1. Elements of TαT_\alphaTα​ are "homogeneous of order α\alphaα": they are placeholders for objects whose size at scale ε\varepsilonε is εα\varepsilon^{\alpha}εα.

A model (Π,Γ)(\Pi,\Gamma)(Π,Γ) assigns to each point xxx a linear map Πx:T→D′(Rd)\Pi_x : T \to \mathcal{D}'(\mathbb{R}^d)Πx​:T→D′(Rd) and to each pair (x,y)(x,y)(x,y) an element Γxy∈G\Gamma_{xy}\in GΓxy​∈G, subject to Γxx=id\Gamma_{xx}=\mathrm{id}Γxx​=id, ΓxyΓyz=Γxz\Gamma_{xy}\Gamma_{yz}=\Gamma_{xz}Γxy​Γyz​=Γxz​, Πy=Πx∘Γxy\Pi_y = \Pi_x\circ\Gamma_{xy}Πy​=Πx​∘Γxy​ and, locally uniformly, the analytic bounds

∣(Πxa)(Ss,xδφ)∣≲∥a∥ℓ δℓ,∥Γxya∥m≲∥a∥ℓ ∥x−y∥sℓ−m,a∈Tℓ,  m<ℓ.|(\Pi_x a)(S^{\delta}_{s,x}\varphi)| \lesssim \|a\|_\ell\,\delta^{\ell}, \qquad \|\Gamma_{xy}a\|_m \lesssim \|a\|_\ell\,\|x-y\|_s^{\ell-m}, \qquad a \in T_\ell,\; m<\ell.∣(Πx​a)(Ss,xδ​φ)∣≲∥a∥ℓ​δℓ,∥Γxy​a∥m​≲∥a∥ℓ​∥x−y∥sℓ−m​,a∈Tℓ​,m<ℓ.

A modelled distribution of order γ\gammaγ is a function f:Rd→T<γf : \mathbb{R}^d \to T_{<\gamma}f:Rd→T<γ​ such that on every compact KKK

∣∣∣f∣∣∣γ;K=sup⁡x∈K, β<γ∥f(x)∥β+sup⁡x,y∈K, ∥x−y∥s≤1β<γ∥f(x)−Γxyf(y)∥β∥x−y∥sγ−β<∞;|||f|||_{\gamma;K} = \sup_{x\in K,\ \beta<\gamma}\|f(x)\|_\beta + \sup_{\substack{x,y \in K,\ \|x-y\|_s\le 1 \\ \beta<\gamma}} \frac{\|f(x)-\Gamma_{xy}f(y)\|_\beta}{\|x-y\|_s^{\gamma-\beta}} < \infty;∣∣∣f∣∣∣γ;K​=x∈K, β<γsup​∥f(x)∥β​+x,y∈K, ∥x−y∥s​≤1β<γ​sup​∥x−y∥sγ−β​∥f(x)−Γxy​f(y)∥β​​<∞;

the space of these is Dγ\mathcal{D}^\gammaDγ, and Dγ(V)\mathcal{D}^\gamma(V)Dγ(V) if fff takes values in a sector VVV, that is, a graded GGG-invariant subspace vanishing in degrees below its regularity.

Formalization targets

Goal — reconstruction theorem, Theorem 3.10 for γ>0\gamma>0γ>0

With α=min⁡A<0\alpha = \min A < 0α=minA<0 and rrr the order attached to AAA, for every f∈Dγf \in \mathcal{D}^\gammaf∈Dγ with γ>0\gamma>0γ>0 there is a unique distribution Rf∈Csα\mathcal{R}f \in \mathcal{C}^\alpha_sRf∈Csα​ with

∣(Rf−Πxf(x))(Ss,xδη)∣≲δγ(x∈K, δ∈(0,1], η∈Bs,0r).\big|(\mathcal{R}f - \Pi_x f(x))(S^{\delta}_{s,x}\eta)\big| \lesssim \delta^{\gamma} \qquad (x \in K,\ \delta\in(0,1],\ \eta\in\mathcal{B}^r_{s,0}).​(Rf−Πx​f(x))(Ss,xδ​η)​≲δγ(x∈K, δ∈(0,1], η∈Bs,0r​).

The statement asserts only the shape of the estimate — a constant per compact set — and so is insensitive to any later sharpening of constants.

Milestone level — the calculus around the reconstruction operator

The uniqueness clause of Theorem 3.10 in isolation; the existence of a linear reconstruction operator for arbitrary γ∈R\gamma \in \mathbb{R}γ∈R (for γ≤0\gamma\le 0γ≤0 the bound no longer pins it down); Corollary 3.16, improving the regularity of Rf\mathcal{R}fRf to Csβ\mathcal{C}^\beta_sCsβ​ when fff takes values in a sector of regularity β\betaβ; Proposition 3.31, that for ν>0\nu>0ν>0 the action of Π\PiΠ on TνT_\nuTν​ is determined by Γ\GammaΓ and by Π\PiΠ in lower homogeneities; and Theorem 4.7, that the truncated pointwise product of f1∈Dγ1(V)f_1 \in \mathcal{D}^{\gamma_1}(V)f1​∈Dγ1​(V) and f2∈Dγ2(W)f_2\in\mathcal{D}^{\gamma_2}(W)f2​∈Dγ2​(W) lies in Dγ\mathcal{D}^{\gamma}Dγ with γ=(γ1+α2)∧(γ2+α1)\gamma = (\gamma_1+\alpha_2)\wedge(\gamma_2+\alpha_1)γ=(γ1​+α2​)∧(γ2​+α1​).

Significance

The reconstruction theorem is what turns a book-keeping device into analysis: it says that a coherent family of local expansions, indexed by base point, glues to a single genuine distribution, with an error controlled by the order of the expansion. Every subsequent operation in the theory — multiplication (Theorem 4.7), composition with smooth functions (Theorem 4.16), the multi-level Schauder estimate (Theorem 5.12), and the fixed-point theorem for singular SPDEs (Theorem 7.8) — is stated and used through it. Without it, the abstract spaces Dγ\mathcal{D}^\gammaDγ carry no information about actual distributions.

Regularity structures are not currently available in Mathlib, and neither are the anisotropic Hölder–Besov spaces Csα\mathcal{C}^\alpha_sCsα​ that the theory is phrased in. The result itself is proved in the literature; the work this mission asks for is a machine-checked proof of the known argument, together with the reusable definitions it needs. The formal development is a prerequisite for anything downstream — Schauder estimates, the fixed-point theory, or the Φ34\Phi^4_3Φ34​ and PAM convergence results of §10 — which are natural follow-on missions rather than part of this one.

Difficulty

The naive construction fails: setting Rf:=Πxf(x)\mathcal{R}f := \Pi_x f(x)Rf:=Πx​f(x) for a fixed xxx is wrong away from xxx, and the pointwise limit lim⁡δ→0\lim_{\delta\to0}limδ→0​ of localisations of Πxf(x)\Pi_x f(x)Πx​f(x) around each xxx does not obviously exist, because the objects being glued are distributions of negative order, not functions, so there is no value to take and no partition-of-unity argument that respects the scaling. Hairer's proof goes through a wavelet multiresolution analysis adapted to the scaling sss: one defines the candidate on each dyadic level by pairing with wavelets centred at grid points, and shows the resulting sequence is Cauchy using the Dγ\mathcal{D}^\gammaDγ bound level by level. A formalization therefore needs either a scaled wavelet basis with Daubechies-type regularity (Theorem 3.17 in the paper) or a substitute for it; this, and the uniform-in-scale bookkeeping, is where the effort lies. Uniqueness for γ>0\gamma>0γ>0 is by contrast short, and is listed as a separate milestone.

Formalization scope

The development commits to the following conventions, fixed in the mission's definition files. Points of Rd\mathbb{R}^dRd are Fin d → ℝ. Test functions are smooth and compactly supported, forming a submodule of all real-valued functions, and a distribution is a linear functional on that submodule; the pairing is extended by 000 to non-test functions, and a lemma in the definition file certifies that rescaling maps test functions to test functions, so no statement is vacuous for that reason. Hairer's Bs,0r\mathcal{B}^r_{s,0}Bs,0r​ consists of CrC^rCr functions; here it consists of smooth ones, which defines the same spaces Csα\mathcal{C}^\alpha_sCsα​. The model space is the algebraic direct sum ⨁a∈ATa\bigoplus_{a\in A} T_a⨁a∈A​Ta​ over the index set, each TaT_aTa​ a real normed space, with QaQ_aQa​ the corresponding projection; the structure group is a subgroup of the linear automorphisms of that direct sum. Sectors are families of subspaces Va⊆TaV_a \subseteq T_aVa​⊆Ta​; Hairer's requirement that each VaV_aVa​ admit a complement is automatic in this algebraic setting. The integer rrr appearing in the model bounds is the smallest one with ℓ>−r\ell > -rℓ>−r for all ℓ∈A\ell \in Aℓ∈A, which is part of the definition of a model rather than a free parameter. All statements quantify over an arbitrary regularity structure, an arbitrary model, and an arbitrary compact set, so they are not satisfiable by a degenerate choice; the goal in particular claims existence, membership in Csα\mathcal{C}^\alpha_sCsα​, and uniqueness simultaneously.

Infrastructure that a complete proof will need, and which is reusable beyond this mission: scaled wavelet bases on Rd\mathbb{R}^dRd, the elementary theory of Csα\mathcal{C}^\alpha_sCsα​ (including the positive-regularity case), and basic operations on compactly supported test functions under anisotropic rescaling. Contributions of any of these as separate lemmas are welcome, as are reductions that decompose the goal into wavelet-level estimates.

Selected references

  • M. Hairer, A theory of regularity structures, Inventiones Mathematicae 198 (2014) 269–504. arXiv:1303.5113, DOI:10.1007/s00222-014-0505-4
  • T. Lyons, Differential equations driven by rough signals, Revista Matemática Iberoamericana 14 (1998) 215–310. DOI:10.4171/RMI/240
  • M. Gubinelli, Controlling rough paths, Journal of Functional Analysis 216 (2004) 86–140. arXiv:math/0306433
  • M. Gubinelli, P. Imkeller, N. Perkowski, Paracontrolled distributions and singular PDEs, Forum of Mathematics Pi 3 (2015) e6. arXiv:1210.2684
  • Y. Bruned, M. Hairer, L. Zambotti, Algebraic renormalisation of regularity structures, Inventiones Mathematicae 215 (2019) 1039–1156. arXiv:1610.08468
13 thms2 active usersReviewed
Functional AnalysisSymplectic Geometry·Captain: Mazecto

Lectures on Symplectic Field Theory VI: Elliptic Regularity and Compactness of Pseudoholomorphic MapsTextbook

Motivation

A pseudoholomorphic map from a planar domain U⊆CU\subseteq\mathbb{C}U⊆C into an almost complex manifold solves the nonlinear Cauchy–Riemann equation

∂ˉJu=∂su+J(u) ∂tu=0,z=s+it.\bar\partial_Ju=\partial_su+J(u)\,\partial_tu=0,\qquad z=s+it.∂ˉJ​u=∂s​u+J(u)∂t​u=0,z=s+it.

These maps are the basic objects of Gromov's theory of holomorphic curves, of Floer homology and of symplectic field theory. Two analytic facts about them are used everywhere: solutions of low regularity are automatically smooth, and families with a uniform bound on the first derivative are precompact in Cloc∞C^\infty_{\mathrm{loc}}Cloc∞​. A third fact, unique continuation, says that a solution is determined near a point by its derivatives there.

This mission formalizes these results locally, for maps from discs into a finite-dimensional real vector space with an almost complex structure defined on an open subset, following C. Wendl, Lectures on Symplectic Field Theory, Lecture 2 (§ 2.4–2.5) and Proposition 9.1. Mathlib has no Sobolev spaces of weakly differentiable maps, no almost complex structures and no pseudoholomorphic maps. The definitions build on the Wk,pW^{k,p}Wk,p norm of the DbarRegularity mission.

Setting

  • Target. EEE is a finite-dimensional real vector space and O⊆EO\subseteq EO⊆E is open. A smooth almost complex structure on OOO is a C∞C^\inftyC∞ map J:O→End⁡R(E)J:O\to\operatorname{End}_{\mathbb{R}}(E)J:O→EndR​(E) with J(x)2=−IdJ(x)^2=-\mathrm{Id}J(x)2=−Id. Allowing an open subset rather than all of EEE covers, for example, symplectizations of contact-type hypersurfaces.
  • Domain. U⊆CU\subseteq\mathbb{C}U⊆C is open, usually the open unit disc DDD; ∂su\partial_su∂s​u and ∂tu\partial_tu∂t​u are the derivatives in the directions 111 and iii.
  • JJJ-holomorphic maps. uuu is JJJ-holomorphic on UUU if it is differentiable there with ∂su+J(u)∂tu=0\partial_su+J(u)\partial_tu=0∂s​u+J(u)∂t​u=0.
  • Weak solutions. uuu is a Wloc1,pW^{1,p}_{\mathrm{loc}}Wloc1,p​ solution if it is continuous with values in OOO, has weak partial derivatives that lie with uuu in LpL^pLp of every compact subset of UUU, and satisfies the equation almost everywhere.
  • Convergence. Cloc∞C^\infty_{\mathrm{loc}}Cloc∞​ convergence on an open set means uniform convergence of all derivatives on every compact subset.

Formalization targets

Goal: compactness of pseudoholomorphic discs

Let Jν→JJ_\nu\to JJν​→J in Cloc∞C^\infty_{\mathrm{loc}}Cloc∞​ be smooth almost complex structures on OOO and let K0⊆OK_0\subseteq OK0​⊆O be compact. Every sequence of JνJ_\nuJν​-holomorphic C1C^1C1 maps uν:D→K0u_\nu:D\to K_0uν​:D→K0​ with sup⁡νsup⁡D∥Duν∥<∞\sup_\nu\sup_D\|Du_\nu\|<\inftysupν​supD​∥Duν​∥<∞ has a subsequence converging in Cloc∞C^\infty_{\mathrm{loc}}Cloc∞​ on DDD to a smooth JJJ-holomorphic map D→K0D\to K_0D→K0​ (Wendl, Proposition 9.1).

Milestones

  1. Regularity of weak solutions. For p>2p>2p>2, a continuous Wloc1,pW^{1,p}_{\mathrm{loc}}Wloc1,p​ solution of ∂su+J(u)∂tu=0\partial_su+J(u)\partial_tu=0∂s​u+J(u)∂t​u=0 on an open UUU is C∞C^\inftyC∞ on UUU (Theorem 2.22 (1)).
  2. Uniform interior bounds. For p>2p>2p>2, smooth JνJ_\nuJν​-holomorphic discs with values in K0K_0K0​ and uniformly bounded W1,pW^{1,p}W1,p norm have derivatives of every order bounded on compact subsets of DDD, uniformly in ν\nuν (Theorem 2.22 (2a)).
  3. Convergence. For p>2p>2p>2, if such discs converge in W1,pW^{1,p}W1,p to a smooth map, they converge to it in Cloc∞C^\infty_{\mathrm{loc}}Cloc∞​ (Theorem 2.22 (2b)).
  4. Weakly holomorphic functions. An L1L^1L1 function on DDD with ∂su+i∂tu=0\partial_su+i\partial_tu=0∂s​u+i∂t​u=0 in the sense of distributions agrees almost everywhere with a holomorphic function (Lemma 2.19).
  5. Local solutions with prescribed value. For 2<p<∞2<p<\infty2<p<∞ and A∈Lp(D,End⁡R(Cn))A\in L^p(D,\operatorname{End}_{\mathbb{R}}(\mathbb{C}^n))A∈Lp(D,EndR​(Cn)), the equation ∂su+i∂tu+Au=0\partial_su+i\partial_tu+Au=0∂s​u+i∂t​u+Au=0 has, on every sufficiently small disc, a continuous W1,pW^{1,p}W1,p solution with any prescribed value at 000 (Lemma 2.24).
  6. Local holomorphic factorization. A smooth solution of ∂sh+Jˉ(z)∂th+A(z)h=0\partial_sh+\bar J(z)\partial_th+A(z)h=0∂s​h+Jˉ(z)∂t​h+A(z)h=0, with Jˉ(z)\bar J(z)Jˉ(z) a smooth family of complex structures on EEE, is locally of the form h=Φfh=\Phi fh=Φf, where Φ(z):Cn→E\Phi(z):\mathbb{C}^n\to EΦ(z):Cn→E is a continuous family of real-linear bijections with Φ(z)∘i=Jˉ(z)∘Φ(z)\Phi(z)\circ i=\bar J(z)\circ\Phi(z)Φ(z)∘i=Jˉ(z)∘Φ(z) and fff is holomorphic (Theorem 2.26).
  7. Unique continuation. Two smooth JJJ-holomorphic discs whose derivatives of all orders agree at 000 coincide near 000 (Proposition 2.28).

Significance

The results. Regularity and Cloc∞C^\infty_{\mathrm{loc}}Cloc∞​ compactness are the local half of Gromov compactness: once a moduli space of holomorphic curves has a uniform C1C^1C1 bound, it is precompact in the smooth topology. Unique continuation is the local input for the structure theory of holomorphic curves, such as the decomposition of a curve into a simple curve and a branched cover.

Formalizing them. The mission introduces almost complex structures, pseudoholomorphic maps, weak derivatives and Wloc1,pW^{1,p}_{\mathrm{loc}}Wloc1,p​ solutions of a nonlinear first-order system, in a form that applies to any finite-dimensional target and to structures defined on an open subset. These are foundations for finite-energy holomorphic curves in symplectizations, the next stage of this series. Milestones 4 and 5 are statements about linear first-order elliptic equations in the plane, and milestone 6 is a normal form for real-linear Cauchy–Riemann equations; all three are of independent use in complex analysis.

Difficulty

The equation is nonlinear in uuu and the structures JνJ_\nuJν​ vary with ν\nuν; the statements about sequences are uniform in ν\nuν, with all constants chosen before the index. The weak formulation involves maps that are not assumed differentiable, and the conclusion of milestone 1 is classical smoothness of the given continuous map, not of a representative. The almost complex structure is only defined on an open subset of the target, so every statement keeps track of where the maps take their values. In milestone 6 the complex structure on the target varies with the point of the domain.

Formalization scope

  • Namespace JHolomorphic. The definition module JHolomorphic_Setting defines IsAlmostComplexOn, dbarJ, IsJHolomorphicOn, HasWeakPartialsOn, IsWeakJHolomorphicOn and TendstoCInftyLocOn. It imports the DbarRegularity setting for sobolevNorm (the Wk,p(U)W^{k,p}(U)Wk,p(U) norm ∑j≤k∥Djφ∥Lp(U)\sum_{j\le k}\|D^j\varphi\|_{L^p(U)}∑j≤k​∥Djφ∥Lp(U)​).
  • Spaces. EEE is a real normed space with [FiniteDimensional ℝ E], without an inner product. Cn\mathbb{C}^nCn is EuclideanSpace ℂ (Fin n). Almost complex structures have type E → E →L[ℝ] E.
  • Exponents. ppp is a real number with p>2p>2p>2, used as ENNReal.ofReal p.
  • Smoothness. Smoothness is ContDiffOn ℝ ∞ (C∞C^\inftyC∞, not analytic); derivatives of order mmm are iteratedFDeriv ℝ m.
  • Generality. Wendl states the nonlinear results for E=CnE=\mathbb{C}^nE=Cn with the normalization J(0)=iJ(0)=iJ(0)=i, u(0)=0u(0)=0u(0)=0; the statements here drop the normalization, allow an open domain of definition OOO for JJJ, and require images in a fixed compact subset of OOO in the statements about sequences.

Contributions welcome: general lemmas on weak derivatives and on LpL^pLp spaces over planar domains.

Selected references

  • C. Wendl, Lectures on Symplectic Field Theory, arXiv:1612.01009, Lecture 2 and Lecture 9. https://arxiv.org/abs/1612.01009
  • D. McDuff, D. Salamon, J-holomorphic Curves and Symplectic Topology, 2nd ed., AMS Colloquium Publications 52 (2012), Chapter 2 and Appendix B.
  • C. Abbas, H. Hofer, Holomorphic Curves and Global Questions in Contact Geometry, Birkhäuser (2019).
23 thms1 active userReviewed
Algorithmic Game TheoryOperations ResearchProbability·Captain: mikedeng1

Finite State Mean Field Games with Wright–Fisher Common Noise as Limits of N-Player Weighted Games: Normalized N-Player Equilibrium Values Converge to the Master Equation at a Polynomial RateResearch Paper

Motivation

Mean field games describe Nash equilibria of games with very many symmetric players by a single limiting object. Whether, and how fast, the equilibria of the NNN-player game converge to that limit is the convergence problem. For games with common noise, a source of randomness shared by all players, the standard route goes through the master equation, a PDE on the space of probability measures whose solution UUU gives the equilibrium value of a representative player as a function of the population's distribution (Cardaliaguet, Delarue, Lasry and Lions, 2019, arXiv:1509.02505).

For finite state spaces the distribution is a point of the simplex. Bayraktar, Cecchin, Cohen and Delarue (J. Math. Pures Appl. 147, 2021) introduced a common noise of Wright–Fisher type, the noise of population genetics, which keeps the distribution in the simplex and makes the master equation uniquely solvable. Its NNN-player counterpart is not obvious, because the Wright–Fisher diffusion is the limit of a resampling of the population, not of independent player noises. The paper behind this mission (Bayraktar, Cecchin, Cohen and Delarue, Mathematics of Operations Research, 2022, arXiv:2012.04845) builds such a game, in which players carry weights that are resampled at random times, and proves that its normalized equilibrium values converge to UUU at a polynomial rate.

Setting

There are d≥1d \ge 1d≥1 states [ ⁣[d] ⁣]={1,…,d}[\![d]\!] = \{1,\dots,d\}[[d]]={1,…,d} and N≥1N \ge 1N≥1 players. Player lll is at a state xlx^lxl and carries a weight yl≥0y^l \ge 0yl≥0; the weights are rational and sum to NNN, and the set of such weight tuples is Y\mathbb YY. The players interact through the weighted empirical measure

μx,yN[i]=1N∑lyl1{xl=i},\mu^N_{x,y}[i] = \frac1N\sum_{l} y^l \mathbb 1_{\{x^l = i\}},μx,yN​[i]=N1​l∑​yl1{xl=i}​,

a point of the simplex Sd−1={p∈Rd:pi≥0,∑ipi=1}\mathcal S_{d-1} = \{p \in \mathbb R^d : p_i \ge 0, \sum_i p_i = 1\}Sd−1​={p∈Rd:pi​≥0,∑i​pi​=1}.

Each player controls the rates at which it jumps between states, at quadratic cost. A drift φ(μ[j])\varphi(\mu[j])φ(μ[j]) pushes players towards nearly empty states, where φ\varphiφ is non-increasing and Lipschitz, equal to κ\kappaκ on [0,δ][0,\delta][0,δ] and to 000 beyond 2δ2\delta2δ. At rate εN\varepsilon NεN the common noise draws S∼Multinomial(N,μx,yN)S \sim \mathrm{Multinomial}(N, \mu^N_{x,y})S∼Multinomial(N,μx,yN​) and replaces every weight yly^lyl by ylS[xl]/(Nμx,yN[xl])y^l S[x^l]/(N\mu^N_{x,y}[x^l])ylS[xl]/(Nμx,yN​[xl]). Players pay ylf(xl,μ)y^l f(x^l, \mu)ylf(xl,μ) per unit time and ylg(xl,μT)y^l g(x^l,\mu_T)ylg(xl,μT​) at time TTT.

The equilibrium values divided by the weights, wN,l(t,x,y)w^{N,l}(t,x,y)wN,l(t,x,y), solve the normalized Nash system: a countable family of ordinary differential equations in ttt, indexed by (l,x,y)(l, x, y)(l,x,y), with the Hamiltonian H(i,u)=−12∑j≠i(ui−uj)+2H(i,u) = -\frac12\sum_{j\ne i}(u^i - u^j)_+^2H(i,u)=−21​∑j=i​(ui−uj)+2​ and the terminal condition wN,l(T,x,y)=g(xl,μx,yN)w^{N,l}(T,x,y) = g(x^l, \mu^N_{x,y})wN,l(T,x,y)=g(xl,μx,yN​).

The limit object is U=(U1,…,Ud)U = (U^1,\dots,U^d)U=(U1,…,Ud) on [0,T]×Sd−1[0,T]\times\mathcal S_{d-1}[0,T]×Sd−1​, solving the master equation

∂tUi+H(i,U)+fi+∑jφ(pj)(Uj−Ui)+∑j,kpk[φ(pj)+(Uk−Uj)+](djUi−dkUi)+ε∑j≠ipj(diUi−djUi)+ε2∑j,k(pjδjk−pjpk)dj,k2Ui=0\partial_tU^i + H(i, U) + f^i + \sum_j\varphi(p_j)(U^j - U^i) + \sum_{j,k}p_k[\varphi(p_j) + (U^k - U^j)_+](\mathfrak d_jU^i - \mathfrak d_kU^i) + \varepsilon\sum_{j\ne i}p_j(\mathfrak d_iU^i - \mathfrak d_jU^i) + \frac\varepsilon2\sum_{j,k}(p_j\delta_{jk} - p_jp_k)\mathfrak d^2_{j,k}U^i = 0∂t​Ui+H(i,U)+fi+j∑​φ(pj​)(Uj−Ui)+j,k∑​pk​[φ(pj​)+(Uk−Uj)+​](dj​Ui−dk​Ui)+εj=i∑​pj​(di​Ui−dj​Ui)+2ε​j,k∑​(pj​δjk​−pj​pk​)dj,k2​Ui=0

with Ui(T,⋅)=giU^i(T,\cdot) = g^iUi(T,⋅)=gi. Here di\mathfrak d_idi​ are the intrinsic derivatives on the simplex, dih(p)=1d∑m∂ei−emh(p)\mathfrak d_ih(p) = \frac1d\sum_m\partial_{e_i - e_m}h(p)di​h(p)=d1​∑m​∂ei​−em​​h(p), and the last term is the Kimura operator of Wright–Fisher diffusions. The mean-field prediction for player lll is zN,l(t,x,y)=Uxl(t,μx,yN)z^{N,l}(t,x,y) = U^{x^l}(t,\mu^N_{x,y})zN,l(t,x,y)=Uxl(t,μx,yN​).

Formalization targets

Goal: Theorem 2.4

For κ\kappaκ large enough, there are χ>0\chi > 0χ>0 and CCC such that for every NNN, lll, ttt, xxx and y∈Yy \in \mathbb Yy∈Y,

∣(zN,l−wN,l)(t,x,y)∣≤CN−χ(∏i1N−1/8+μx,yN[i])1/(2d)(1N∑m∣ym∣3)1/2.\big|(z^{N,l} - w^{N,l})(t,x,y)\big| \le CN^{-\chi}\Big(\prod_{i}\frac{1}{N^{-1/8} + \mu^N_{x,y}[i]}\Big)^{1/(2d)}\Big(\frac1N\sum_m|y^m|^3\Big)^{1/2}.​(zN,l−wN,l)(t,x,y)​≤CN−χ(i∏​N−1/8+μx,yN​[i]1​)1/(2d)(N1​m∑​∣ym∣3)1/2.

The exponent χ\chiχ is existential, so an improvement of the rate does not invalidate the target.

Milestones

  1. Proposition 3.1: the normalized Nash system has a unique bounded solution.
  2. Proposition 3.2: that solution is bounded by T∥f∥∞+∥g∥∞T\|f\|_\infty + \|g\|_\inftyT∥f∥∞​+∥g∥∞​, uniformly in NNN.
  3. Lemma 4.5: moment and deviation bounds for (Sμ[i]/(Nμ[i]))ℓ−1(S_\mu[i]/(N\mu[i]))^\ell - 1(Sμ​[i]/(Nμ[i]))ℓ−1.
  4. Lemmas 4.8–4.11: the common-noise, discrete-gradient, drift and Hamiltonian terms of the Nash system along zN,lz^{N,l}zN,l against those of the master equation.
  5. Proposition 4.6 with Remark 4.7: zN,lz^{N,l}zN,l solves the Nash system up to a rest O(N−η)O(N^{-\eta})O(N−η) on the set TN\mathcal T_NTN​ where min⁡iμx,yN[i]≥N−ϵ\min_i\mu^N_{x,y}[i] \ge N^{-\epsilon}mini​μx,yN​[i]≥N−ϵ and max⁡lyl≤12N1−ϵ\max_l y^l \le \frac12N^{1-\epsilon}maxl​yl≤21​N1−ϵ.

Significance

Theorem 2.4 gives a convergence rate for a finite-state mean field game whose common noise keeps the population on the simplex. It shows that the master equation of the earlier paper is the right limit of a concrete finite game, and with a diffusion-approximation argument it yields the paper's second main result, the weak convergence of the equilibrium empirical measure to the Wright–Fisher-type SDE (Theorem 2.6). The bound is not uniform in (x,y)(x,y)(x,y): it degenerates near the boundary of the simplex and for spread-out weights, which reflects the singular coefficient 1/μ[xl]1/\mu[x^l]1/μ[xl] in the resampling.

None of these results has a machine-checked proof. The mission produces a formal statement of the convergence problem for a game with weighted players, a formal Nash system on a countable state space, intrinsic derivatives on the simplex, and multinomial moment estimates.

Difficulty

The usual proof of convergence plugs zN,lz^{N,l}zN,l into the Nash system, controls the rest, and closes with a Gronwall argument along the NNN-player dynamics. Here the rest is small only on TN\mathcal T_NTN​, away from the boundary of the simplex and for moderate weights; the second derivatives of UUU may blow up at the boundary, and the resampling ratio S[i]/(Nμ[i])S[i]/(N\mu[i])S[i]/(Nμ[i]) is unbounded as μ[i]→0\mu[i] \to 0μ[i]→0. A uniform estimate of sup⁡x,y∣zN,l−wN,l∣\sup_{x,y}|z^{N,l} - w^{N,l}|supx,y​∣zN,l−wN,l∣ is therefore not available, and the comparison must be weighted by functions of (x,y)(x,y)(x,y) whose expectations along the dynamics can be controlled. The weights are unbounded and enter through their moments.

Formalization scope

States are Fin d and players Fin N, with d≥1d \ge 1d≥1 and N≥1N \ge 1N≥1 (no N≥2N \ge 2N≥2). Weights are rational, and every equation and conclusion is required only for y∈Yy \in \mathbb Yy∈Y and t∈[0,T]t \in [0,T]t∈[0,T]. The simplex is Mathlib's stdSimplex. Intrinsic derivatives use lineDeriv; multinomial expectations are finite sums over Finset.Nat.antidiagonalTuple. The resampling ratio is 111 when μ[xl]=0\mu[x^l] = 0μ[xl]=0, as in the paper. Solutions of the Nash system and of the master equation are classical in ttt, with one-sided derivatives at 000 and TTT. The Nash system is solved by any bounded classical solution; Proposition 3.1 says there is exactly one.

The formalization commits to the following readings of the source.

  • ε\varepsilonε for ε2\varepsilon^2ε2. The master equation carries ε\varepsilonε and ε/2\varepsilon/2ε/2 in front of the common-noise terms where (2.3) prints ε2\varepsilon^2ε2 and ε2/2\varepsilon^2/2ε2/2. The NNN-player noise rings at rate εN\varepsilon NεN, and the limit SDE (2.4) has intensity ε\sqrt\varepsilonε​; with ε2\varepsilon^2ε2, Proposition 4.6 and Theorem 2.4 would be false.
  • Regularity class. The Wright–Fisher Hölder space of Proposition 2.1, which the paper only describes, is replaced by an explicit class: UUU continuous on [0,T]×Sd−1[0,T]\times\mathcal S_{d-1}[0,T]×Sd−1​, differentiable along the simplex in the interior together with dU\mathfrak dUdU, with UUU and dU\mathfrak dUdU bounded, and dU\mathfrak dUdU and pjpk dj,k2U\sqrt{p_jp_k}\,\mathfrak d^2_{j,k}Upj​pk​​dj,k2​U bounded and γ′/2\gamma'/2γ′/2-Hölder. These are the properties §7 says the proofs use. The Hölder assumptions on f,gf, gf,g are replaced by boundedness.
  • Constants. χ\chiχ is chosen after ddd and γ′\gamma'γ′, the threshold κˉ0\bar\kappa_0κˉ0​ after d,ε,Td, \varepsilon, Td,ε,T and the bounds of f,gf, gf,g, and CCC after all model data and UUU, before NNN and the point.
  • Remark 4.7. Lemmas 4.9–4.11 and Proposition 4.6 are stated for zN,lz^{N,l}zN,l, so no division by a vanishing weight occurs.
  • Two printed slips. Lemma 4.9's (4.28) uses dUj\mathfrak dU^jdUj, not dUxl\mathfrak dU^{x^l}dUxl, and Lemma 4.5's (4.19) assumes Nμ[i]≥1N\mu[i] \ge 1Nμ[i]≥1, without which it fails.

The bound is not trivial. Since ∣z−w∣≤2(T∥f∥∞+∥g∥∞)|z - w| \le 2(T\|f\|_\infty + \|g\|_\infty)∣z−w∣≤2(T∥f∥∞​+∥g∥∞​) and the right side is at least of order CN−χCN^{-\chi}CN−χ, a constant CCC chosen after NNN would make the theorem empty; CCC precedes NNN. The functions www and UUU enter only through the Nash system and the master equation, and the class of UUU is not empty: for d=1d = 1d=1 the function U1(t)=g1+(T−t)f1U^1(t) = g^1 + (T - t)f^1U1(t)=g1+(T−t)f1 is in it.

The mission takes UUU as given. Its existence for d≥2d \ge 2d≥2 is Theorems 3.2 and 3.4 of Bayraktar, Cecchin, Cohen and Delarue (2021), quoted as Proposition 2.1, which is not a target. Also outside the mission are the NNN-player game itself (Propositions 2.2–2.3), Theorem 2.6, and the process estimates of §4.1 (Theorem 4.1, Remark 4.2, Propositions 4.3–4.4), which need a continuous-time Markov chain with a martingale-problem characterization. Contributions are welcome on every milestone; the multinomial estimates and the simplex calculus are reusable elsewhere.

Selected references

  • E. Bayraktar, A. Cecchin, A. Cohen, F. Delarue, Finite state mean field games with Wright–Fisher common noise as limits of N-player weighted games, Mathematics of Operations Research, 2022. arXiv:2012.04845v2
  • E. Bayraktar, A. Cecchin, A. Cohen, F. Delarue, Finite state mean field games with Wright–Fisher common noise, Journal de Mathématiques Pures et Appliquées 147:98–162, 2021. search
  • P. Cardaliaguet, F. Delarue, J.-M. Lasry, P.-L. Lions, The Master Equation and the Convergence Problem in Mean Field Games, Annals of Mathematics Studies 201, Princeton University Press, 2019. arXiv:1509.02505
  • C. L. Epstein, R. Mazzeo, Degenerate Diffusion Operators Arising in Population Biology, Annals of Mathematics Studies 185, Princeton University Press, 2013. search
  • S. N. Ethier, T. G. Kurtz, Markov Processes: Characterization and Convergence, Wiley, 1986. doi:10.1002/9780470316658
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Dynamic Optimal Reinsurance and Dividend Payout in Finite Time Horizon I: The HJB Variational Inequality Has a Unique Classical Solution with v_x ≥ 1, v_xx ≤ 0 and λv_x + v_xx ≥ 0Research Paper

Dividends, reinsurance and a finite horizon

An insurer that pays dividends to its shareholders faces a trade-off studied since de Finetti (1957): paying out surplus early raises the discounted payout but brings ruin closer. Reinsurance changes the trade-off, because ceding part of each claim lowers the volatility of the surplus at the price of a reinsurance premium. When the insurer may choose both the dividend stream and, at every moment, an arbitrary reinsurance contract, the problem becomes a mixed singular–classical stochastic control problem. Most of the literature treats it on an infinite horizon, where the value function solves an ordinary differential equation. On a finite horizon TTT the value function also depends on time to maturity, the Hamilton–Jacobi–Bellman (HJB) equation becomes a parabolic variational inequality with a gradient constraint, and neither its solvability nor the regularity of its solution is classical.

Guan, Xu and Zhou (arXiv:2008.00391v3, Mathematics of Operations Research, 2023) show by PDE methods that this variational inequality has a classical solution, identify it with the value function, and read the optimal reinsurance contract and dividend barrier off its derivatives. This mission formalizes the PDE part: Theorem 3.1 and the steps of Appendix A that lead to it.

Setting

Claims are nonnegative random variables with common distribution function FFF, F(0−)=0F(0-)=0F(0−)=0, possibly discontinuous. The paper assumes the tail condition

z3 (1−F(z)) is bounded on [0,∞),(3.3)z^3\,(1-F(z))\ \text{is bounded on }[0,\infty), \tag{3.3}z3(1−F(z)) is bounded on [0,∞),(3.3)

so the moments μ1=∫0∞z dF(z)\mu_1=\int_0^\infty z\,dF(z)μ1​=∫0∞​zdF(z) and μ2=∫0∞z2 dF(z)\mu_2=\int_0^\infty z^2\,dF(z)μ2​=∫0∞​z2dF(z) are finite. The other data are the net reinsurance loading γ>0\gamma>0γ>0, the discount factor c>0c>0c>0 and the horizon T>0T>0T>0; the mission assumes γ<μ1\gamma<\mu_1γ<μ1​ throughout.

A reinsurance contract is described by the retained loss H(z)H(z)H(z) the insurer keeps out of a claim of size zzz, with 0≤H(z)≤z0\le H(z)\le z0≤H(z)≤z; H\mathcal HH is the set of such functions. For a function v(x,t)v(x,t)v(x,t) of the surplus xxx and the time to maturity ttt the operator

Lv=sup⁡H∈H(vxx2∫0∞H(z)2 dF(z)+vx∫0∞H(z) dF(z))−γvx−cv(3.2)\mathcal Lv=\sup_{H\in\mathcal H}\Big(\frac{v_{xx}}2\int_0^\infty H(z)^2\,dF(z)+v_x\int_0^\infty H(z)\,dF(z)\Big)-\gamma v_x-cv \tag{3.2}Lv=H∈Hsup​(2vxx​​∫0∞​H(z)2dF(z)+vx​∫0∞​H(z)dF(z))−γvx​−cv(3.2)

is the generator of the controlled diffusion approximation of the surplus. The HJB equation is the variational inequality, on QT=(0,∞)×(0,T]\mathcal Q_T=(0,\infty)\times(0,T]QT​=(0,∞)×(0,T],

min⁡{vt−Lv, vx−1}=0,v(0,t)=0,v(x,0)=x.(3.1)\min\{v_t-\mathcal Lv,\ v_x-1\}=0,\qquad v(0,t)=0,\qquad v(x,0)=x. \tag{3.1}min{vt​−Lv, vx​−1}=0,v(0,t)=0,v(x,0)=x.(3.1)

The functions

A(y)=∫01/yz(1−F(z)) dz,B(y)=∫01/y(1−F(z)) dz(y>0),A(y)=\int_0^{1/y}z(1-F(z))\,dz,\qquad B(y)=\int_0^{1/y}(1-F(z))\,dz\qquad(y>0),A(y)=∫01/y​z(1−F(z))dz,B(y)=∫01/y​(1−F(z))dz(y>0),

with A=μ2/2A=\mu_2/2A=μ2​/2 and B=μ1B=\mu_1B=μ1​ for y≤0y\le0y≤0, compute the supremum in (3.2), and f(y)=−yA(y)+B(y)−γf(y)=-yA(y)+B(y)-\gammaf(y)=−yA(y)+B(y)−γ has a unique root λ>0\lambda>0λ>0. The penalized gradient problem (A.17) on QL,T=(0,L)×(0,T]\mathcal Q_{L,T}=(0,L)\times(0,T]QL,T​=(0,L)×(0,T] is

ut−Tu+βε(u−1)=0,(λu+ux)(0,t)=fε(t),u(L,t)=1,u(x,0)=1,u_t-\mathcal Tu+\beta_\varepsilon(u-1)=0,\quad (\lambda u+u_x)(0,t)=f_\varepsilon(t),\quad u(L,t)=1,\quad u(x,0)=1,ut​−Tu+βε​(u−1)=0,(λu+ux​)(0,t)=fε​(t),u(L,t)=1,u(x,0)=1,

with Tu=A(−ux/u)uxx+B(−ux/u)ux−γux−cu\mathcal Tu=A(-u_x/u)u_{xx}+B(-u_x/u)u_x-\gamma u_x-cuTu=A(−ux​/u)uxx​+B(−ux​/u)ux​−γux​−cu, a penalty function βε\beta_\varepsilonβε​ and a boundary datum fεf_\varepsilonfε​ that ramps from λ\lambdaλ down to 000 on [0,ε][0,\varepsilon][0,ε].

Formalization targets

Goal: Theorem 3.1

There is a unique v∈C2,1(Q‾T∖{(0,0)})∩C(Q‾T)v\in C^{2,1}(\overline{\mathcal Q}_T\setminus\{(0,0)\})\cap C(\overline{\mathcal Q}_T)v∈C2,1(Q​T​∖{(0,0)})∩C(Q​T​) that solves (3.1) and satisfies

vx≥1,vt≥0,vxx≤0,vxxx≥0 (weakly),vxt≥0,λvx+vxx≥0.v_x\ge1,\quad v_t\ge0,\quad v_{xx}\le0,\quad v_{xxx}\ge0\ \text{(weakly)},\quad v_{xt}\ge0,\quad \lambda v_x+v_{xx}\ge0 .vx​≥1,vt​≥0,vxx​≤0,vxxx​≥0 (weakly),vxt​≥0,λvx​+vxx​≥0.

Uniqueness is among solutions in the same class with the same six properties, as equality on Q‾T\overline{\mathcal Q}_TQ​T​.

Milestones

  1. (A.7)–(A.9): AAA, BBB are non-increasing, Lipschitz, bounded by 12min⁡{y−2,μ2}\tfrac12\min\{y^{-2},\mu_2\}21​min{y−2,μ2​} and min⁡{y−1,μ1}\min\{y^{-1},\mu_1\}min{y−1,μ1​}, with y3A′=y2B′=F(1/y)−1y^3A'=y^2B'=F(1/y)-1y3A′=y2B′=F(1/y)−1.
  2. (A.10): Lv=A(−vxx/vx)vxx+B(−vxx/vx)vx−γvx−cv\mathcal Lv=A(-v_{xx}/v_x)v_{xx}+B(-v_{xx}/v_x)v_x-\gamma v_x-cvLv=A(−vxx​/vx​)vxx​+B(−vxx​/vx​)vx​−γvx​−cv when vx>0v_x>0vx​>0.
  3. (A.12)–(A.13): f′=−A<0f'=-A<0f′=−A<0 everywhere, and fff has a unique root, which is positive.
  4. Lemma A.1: A(−y/z)A(-y/z)A(−y/z) and B(−y/z)B(-y/z)B(−y/z) are Lipschitz on R×[1,∞)\mathbb R\times[1,\infty)R×[1,∞).
  5. Lemma A.2: a comparison principle for (A.17) between functions ≥1\ge1≥1.
  6. Lemma A.3: (A.17) has a C2,1C^{2,1}C2,1 solution, and 1≤uε≤KeΛt/(x+1/λ)1\le u^\varepsilon\le Ke^{\Lambda t}/(x+1/\lambda)1≤uε≤KeΛt/(x+1/λ) for small ε\varepsilonε, with K=L+1/λ+1K=L+1/\lambda+1K=L+1/λ+1, Λ=μ2/γ2+γλ\Lambda=\mu_2/\gamma^2+\gamma\lambdaΛ=μ2​/γ2+γλ.
  7. Lemmas A.4–A.6: utε≥0u^\varepsilon_t\ge0utε​≥0, uxε≤0u^\varepsilon_x\le0uxε​≤0, λuε+uxε≥0\lambda u^\varepsilon+u^\varepsilon_x\ge0λuε+uxε​≥0, uxxε≥0u^\varepsilon_{xx}\ge0uxxε​≥0.

Significance

Theorem 3.1 is the analytic core of the paper. The verification theorem (Theorem 3.2) needs a classical solution that is increasing and concave in xxx, which Theorem 3.1 provides, and Section 4 derives the shape of the optimal policy from (3.4)–(3.9): the optimal retained loss is min⁡{z, −vx/vxx}\min\{z,\,-v_x/v_{xx}\}min{z,−vx​/vxx​}, and (3.9) bounds the reinsurance barrier away from zero. Without the existence of a classical solution, the HJB equation could only be interpreted in the viscosity sense, whose uniqueness theory for this mixed singular–classical problem is not available, and the strategies would not be well defined.

The result is proved in the paper; nothing in it has been machine-checked. A formal development would produce, beyond the theorem, a reusable formal treatment of a parabolic obstacle problem with a Robin boundary condition through penalization, comparison principles for quasilinear parabolic equations, and the explicit reduction of a supremum over reinsurance contracts against an arbitrary claim distribution. The appendix lemmas (A.7)–(A.13) and Lemma A.1 are elementary real analysis and are self-contained targets.

Difficulty

The supremum in L\mathcal LL is over a function space and FFF may have atoms, so even the closed form (A.10) and the everywhere-differentiability of fff require care with one-sided derivatives at the jumps of FFF. The operator is fully nonlinear and degenerates as −vxx/vx→∞-v_{xx}/v_x\to\infty−vxx​/vx​→∞, since A(y)→0A(y)\to0A(y)→0. The inequality carries a gradient constraint vx≥1v_x\ge1vx​≥1 rather than an obstacle, and the left boundary condition (λu+ux)(0,t)=0(\lambda u+u_x)(0,t)=0(λu+ux​)(0,t)=0 is incompatible with the initial condition at the corner (0,0)(0,0)(0,0), which is why the solution is only claimed to be C2,1C^{2,1}C2,1 away from that corner. The obvious route, solving (3.1) directly by a fixed-point argument, does not control vxxv_{xx}vxx​; the paper differentiates in xxx and works with the gradient u=vxu=v_xu=vx​, which turns the gradient constraint into an obstacle but introduces the Robin condition with the wrong sign for a direct maximum principle. The passage ε→0\varepsilon\to0ε→0 needs Wp2,1W^{2,1}_pWp2,1​ and Hölder estimates uniform in ε\varepsilonε, which are not in Mathlib.

Formalization scope

  • Functions of (x,t)(x,t)(x,t) are ℝ → ℝ → ℝ; ttt is time to maturity. Partial derivatives are explicit functions vx,vxx,vtv_x, v_{xx}, v_tvx​,vxx​,vt​ tied to vvv by HasDerivAt on sections at interior points (x>0x>0x>0, 0<t<T0<t<T0<t<T) and continuous on Q‾T∖{(0,0)}\overline{\mathcal Q}_T\setminus\{(0,0)\}Q​T​∖{(0,0)}; boundary values are these continuous extensions, and (3.1) holds at t=Tt=Tt=T through them.
  • The claim law is a probability measure on R\mathbb RR with no mass on (−∞,0)(-\infty,0)(−∞,0), and F(z)=μ((−∞,z])F(z)=\mu((-\infty,z])F(z)=μ((−∞,z]); no density is assumed. H\mathcal HH consists of measurable HHH with 0≤H(z)≤z0\le H(z)\le z0≤H(z)≤z for z≥0z\ge0z≥0, and L\mathcal LL is defined by the supremum (3.2), not by (A.10).
  • 0<γ<μ10<\gamma<\mu_10<γ<μ1​ is a standing hypothesis (the paper imposes it from Section 4; without it fff has no positive root and (3.9) is undefined).
  • (3.7) is read as monotonicity of x↦vxx(x,t)x\mapsto v_{xx}(x,t)x↦vxx​(x,t), (3.8) as monotonicity of t↦vx(x,t)t\mapsto v_x(x,t)t↦vx​(x,t), (3.9) for every positive root of fff.
  • Uniqueness is equality on Q‾T\overline{\mathcal Q}_TQ​T​ within the class of solutions with (3.4)–(3.9). Uniqueness among all classical solutions is not posed: the paper's argument on an unbounded domain uses no growth condition.
  • Penalty data are taken at one fixed ε\varepsilonε; the limit ε→0\varepsilon\to0ε→0 of βε\beta_\varepsilonβε​ is not part of the data. "Sufficiently small ε\varepsilonε" is an ε0>0\varepsilon_0>0ε0​>0 depending on the model and LLL.
  • A formalization in which L\mathcal LL is given by its closed form, the derivatives are deriv evaluated at boundary points, or uniqueness is stated as equality of functions on all of R2\mathbb R^2R2, would trivialize or falsify the goal; the statements avoid all three.

Needed infrastructure: interval integrals of monotone functions and their one-sided derivatives, maximum and comparison principles for linear and quasilinear parabolic equations in one space dimension, existence for quasilinear parabolic problems (Leray–Schauder with Schauder estimates), and compactness in Hölder and Sobolev spaces. The parabolic comparison principle and the penalization scheme are reusable well beyond this mission. Proofs of individual milestones, in particular the elementary ones (A.7)–(A.13) and Lemma A.1, are welcome independently.

Selected references

  • C. Guan, Z. Q. Xu, R. Zhou, Dynamic optimal reinsurance and dividend-payout in finite time horizon, Mathematics of Operations Research, 2023; preprint arXiv:2008.00391v3. https://arxiv.org/abs/2008.00391
  • B. de Finetti, Su un'impostazione alternativa della teoria collettiva del rischio, Transactions of the XVth International Congress of Actuaries, 1957.
  • G. M. Lieberman, Second Order Parabolic Differential Equations, World Scientific, 1996. https://doi.org/10.1142/3302
  • L. C. Evans, Partial Differential Equations, 2nd ed., American Mathematical Society, 2010. https://doi.org/10.1090/gsm/019
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Dynamic Optimal Reinsurance and Dividend Payout in Finite Time Horizon II: For Discrete Claims the Reinsurance Boundaries Are C¹, Start at 0 and Are Spaced Less Than (z_j − z_{j−1})/2c ApartResearch Paper

Motivation

An insurance company pays out dividends to its shareholders and buys reinsurance to limit its exposure to large claims. Both decisions are dynamic: the right amount to cede and the right moment to pay depend on the current surplus and on the time left until a fixed maturity TTT. Guan, Xu and Zhou (2023) solve the combined problem for a diffusion-approximated surplus with a general claim distribution, a general reinsurance contract (any retained-loss function 0≤H(z)≤z0\le H(z)\le z0≤H(z)≤z), and a finite horizon. Their main structural output is a description of the optimal strategy by free boundaries in the surplus–time plane: a dividend barrier d(τ)d(\tau)d(τ), and for each claim size zzz a reinsurance barrier K(z,τ)K(z,\tau)K(z,τ).

A companion mission formalizes the existence and uniqueness of the classical solution of the HJB variational inequality (Theorem 3.1 of the paper). This mission takes that solution as given and formalizes the shape of the boundaries (Section 4 of the paper), culminating in the description of the reinsurance boundaries for discrete claim distributions (Theorem 4.5).

Setting

Claims are i.i.d. copies of a nonnegative random variable Z1Z_1Z1​ with distribution function FFF, satisfying the tail condition that z3(1−F(z))z^3(1-F(z))z3(1−F(z)) is bounded on [0,∞)[0,\infty)[0,∞). Write μ1=∫0∞z dF(z)\mu_1=\int_0^\infty z\,dF(z)μ1​=∫0∞​zdF(z) and μ2=∫0∞z2 dF(z)\mu_2=\int_0^\infty z^2\,dF(z)μ2​=∫0∞​z2dF(z). The reinsurance loading is γ>0\gamma>0γ>0, the discount rate c>0c>0c>0, the horizon T>0T>0T>0, and throughout 0<γ<μ10<\gamma<\mu_10<γ<μ1​ (for γ≥μ1\gamma\ge\mu_1γ≥μ1​ the problem is trivial).

The value function v(x,τ)v(x,\tau)v(x,τ), with x≥0x\ge0x≥0 the surplus and τ∈[0,T]\tau\in[0,T]τ∈[0,T] the time to maturity, is the solution of the variational inequality

min⁡{vτ−Lv, vx−1}=0 on (0,∞)×(0,T],v(0,τ)=0,v(x,0)=x,\min\{v_\tau-\mathcal Lv,\ v_x-1\}=0\ \text{on }(0,\infty)\times(0,T],\qquad v(0,\tau)=0,\qquad v(x,0)=x,min{vτ​−Lv, vx​−1}=0 on (0,∞)×(0,T],v(0,τ)=0,v(x,0)=x,

where

Lv=sup⁡0≤H(z)≤z(vxx2∫0∞H2 dF+vx∫0∞H dF)−γvx−cv.\mathcal Lv=\sup_{0\le H(z)\le z}\Bigl(\frac{v_{xx}}{2}\int_0^\infty H^2\,dF+v_x\int_0^\infty H\,dF\Bigr)-\gamma v_x-cv .Lv=0≤H(z)≤zsup​(2vxx​​∫0∞​H2dF+vx​∫0∞​HdF)−γvx​−cv.

It is the unique function of class C2,1([0,∞)×[0,T]∖{(0,0)})∩C([0,∞)×[0,T])C^{2,1}([0,\infty)\times[0,T]\setminus\{(0,0)\})\cap C([0,\infty)\times[0,T])C2,1([0,∞)×[0,T]∖{(0,0)})∩C([0,∞)×[0,T]) that solves this inequality and satisfies vx≥1v_x\ge1vx​≥1, vτ≥0v_\tau\ge0vτ​≥0, vxx≤0v_{xx}\le0vxx​≤0, vxxv_{xx}vxx​ nondecreasing in xxx, vxv_xvx​ nondecreasing in τ\tauτ, and λvx+vxx≥0\lambda v_x+v_{xx}\ge0λvx​+vxx​≥0. Here λ\lambdaλ is the unique positive root of

f(y)=−yA(y)+B(y)−γ,A(y)=∫01/yz(1−F(z)) dz,B(y)=∫01/y(1−F(z)) dz(y>0).f(y)=-yA(y)+B(y)-\gamma,\qquad A(y)=\int_0^{1/y}z(1-F(z))\,dz,\quad B(y)=\int_0^{1/y}(1-F(z))\,dz\quad(y>0).f(y)=−yA(y)+B(y)−γ,A(y)=∫01/y​z(1−F(z))dz,B(y)=∫01/y​(1−F(z))dz(y>0).

The no-dividend region is ND={(x,τ):vx(x,τ)>1}\mathcal{ND}=\{(x,\tau): v_x(x,\tau)>1\}ND={(x,τ):vx​(x,τ)>1}, and the dividend boundary is

d(τ)=inf⁡{x≥0:vx(x,τ)=1}.d(\tau)=\inf\{x\ge0: v_x(x,\tau)=1\}.d(τ)=inf{x≥0:vx​(x,τ)=1}.

For a claim of size zzz the optimal retained loss is −vx/vxx-v_x/v_{xx}−vx​/vxx​ if −vxx/vx>1/z-v_{xx}/v_x>1/z−vxx​/vx​>1/z and zzz otherwise, and the ceded loss I^(z,x,τ)\hat I(z,x,\tau)I^(z,x,τ) is the difference from zzz. The reinsurance boundary is K(z,τ)=sup⁡{x>0:−vxx/vx(x,τ)>1/z}K(z,\tau)=\sup\{x>0: -v_{xx}/v_x(x,\tau)>1/z\}K(z,τ)=sup{x>0:−vxx​/vx​(x,τ)>1/z}. For a discrete law P(Z1=zj)=pj>0\mathbb P(Z_1=z_j)=p_j>0P(Z1​=zj​)=pj​>0 with 0<z1<⋯<zN0<z_1<\dots<z_N0<z1​<⋯<zN​, the jjj-th reinsurance boundary is

Kj(τ)=inf⁡{x>0:−vxxvx(x,τ)≤1zj}.K_j(\tau)=\inf\Bigl\{x>0: -\frac{v_{xx}}{v_x}(x,\tau)\le\frac1{z_j}\Bigr\}.Kj​(τ)=inf{x>0:−vx​vxx​​(x,τ)≤zj​1​}.

Formalization targets

Goal: Theorem 4.5

For a discrete claim law, every KjK_jKj​ is continuously differentiable on (0,T](0,T](0,T], and for every τ∈(0,T]\tau\in(0,T]τ∈(0,T]:

Kj(τ)=0  if zj≤1λ;0<Ki0(τ)<zi0−1/λ2c;0<Kj(τ)−Kj−1(τ)<zj−zj−12c  (j>i0);lim⁡τ→0+Kj(τ)=0,K_j(\tau)=0\ \text{ if }z_j\le\tfrac1\lambda;\qquad 0<K_{i_0}(\tau)<\frac{z_{i_0}-1/\lambda}{2c};\qquad 0<K_j(\tau)-K_{j-1}(\tau)<\frac{z_j-z_{j-1}}{2c}\ \ (j>i_0);\qquad \lim_{\tau\to0+}K_j(\tau)=0,Kj​(τ)=0  if zj​≤λ1​;0<Ki0​​(τ)<2czi0​​−1/λ​;0<Kj​(τ)−Kj−1​(τ)<2czj​−zj−1​​  (j>i0​);τ→0+lim​Kj​(τ)=0,

where zi0z_{i_0}zi0​​ is the smallest atom above 1/λ1/\lambda1/λ.

Milestones

  1. Theorem 4.2: ddd is continuous and nondecreasing on (0,T](0,T](0,T], and d(0+)=0<d(τ)≤(μ1+cγ)(cμ2+γ2)/(γc3)d(0+)=0<d(\tau)\le\sqrt{(\mu_1+c\gamma)(c\mu_2+\gamma^2)/(\gamma c^3)}d(0+)=0<d(τ)≤(μ1​+cγ)(cμ2​+γ2)/(γc3)​.
  2. Lemma 4.3: vx,vτ∈C2,1v_x,v_\tau\in C^{2,1}vx​,vτ​∈C2,1 in ND\mathcal{ND}ND, vxx<0v_{xx}<0vxx​<0 in ND\mathcal{ND}ND, and I^(z,x,τ)=max⁡{z+vx/vxx,0}\hat I(z,x,\tau)=\max\{z+v_x/v_{xx},0\}I^(z,x,τ)=max{z+vx​/vxx​,0} there.
  3. Lemma 4.4: −vx/vxx=1/λ-v_x/v_{xx}=1/\lambda−vx​/vxx​=1/λ at x=0x=0x=0, −vx/vxx>1/λ-v_x/v_{xx}>1/\lambda−vx​/vxx​>1/λ in ND\mathcal{ND}ND, and ∂x(−vx/vxx)≥2c\partial_x(-v_x/v_{xx})\ge2c∂x​(−vx​/vxx​)≥2c in ND\mathcal{ND}ND.
  4. Section 4.2, p. 18: for z>1/λz>1/\lambdaz>1/λ, K(z,τ)≤z/(2c)−1/(2cλ)K(z,\tau)\le z/(2c)-1/(2c\lambda)K(z,τ)≤z/(2c)−1/(2cλ).

Significance

The theorems turn an existence result for a fully nonlinear variational inequality into a usable description of the optimal policy. Claims below 1/λ1/\lambda1/λ are never reinsured; a claim of size z>1/λz>1/\lambdaz>1/λ is partly ceded only when the surplus lies below a barrier that starts at the origin at maturity, stays below z/(2c)−1/(2cλ)z/(2c)-1/(2c\lambda)z/(2c)−1/(2cλ), and stays below the dividend barrier, which is itself bounded by an explicit constant independent of the horizon. For discrete claims the barriers are smooth, ordered, and separated by gaps of at most (zj−zj−1)/(2c)(z_j-z_{j-1})/(2c)(zj​−zj−1​)/(2c). The quantity −vx/vxx-v_x/v_{xx}−vx​/vxx​, the optimal retention level, is shown to grow at rate at least 2c2c2c in the surplus; this single monotonicity estimate is what makes the regions of the surplus–time plane ordered and nonoverlapping.

The results are proved in the paper; none of them, nor Theorem 3.1 on which they rest, has a machine-checked proof. Formalizing them requires the parabolic regularity statements of Lemma 4.3 (the paper's proof invokes interior Schauder estimates) and the implicit function theorem in a form that gives one-variable C1C^1C1 dependence of a level set. Statements of the boundary properties in this mission are posed for any function with the properties of Theorem 3.1, so they can be proved independently of the companion mission.

Difficulty

Most of the elementary statements reduce to a sign or a monotonicity property of −vx/vxx-v_x/v_{xx}−vx​/vxx​, and the first idea is to differentiate the equation. That requires vxxxv_{xxx}vxxx​ and vxτv_{x\tau}vxτ​ to exist as classical derivatives in ND\mathcal{ND}ND, which the class of Theorem 3.1 does not provide: it gives only two xxx-derivatives and one τ\tauτ-derivative, and a weak monotonicity of vxxv_{xx}vxx​. Lemma 4.3's interior regularity is therefore not a formality but the gateway to Lemma 4.4, and its proof uses Hölder estimates for linear parabolic equations, which are not available in Mathlib.

The positivity d(τ)>0d(\tau)>0d(τ)>0 and the limit d(0+)=0d(0+)=0d(0+)=0 are statements about the free boundary itself, not about vvv at fixed points, and need the uniqueness part of Theorem 3.1 or a comparison argument. The strict inequalities in (4.13)–(4.14) need more than the bound ∂x(−vx/vxx)≥2c\partial_x(-v_x/v_{xx})\ge2c∂x​(−vx​/vxx​)≥2c as stated.

Formalization scope

All objects live in the namespace DynReinsDiv.Barriers. Conventions:

  • The claim law is a probability measure μ on R\mathbb RR with μ((−∞,0))=0\mu((-\infty,0))=0μ((−∞,0))=0; F(z)=μ((−∞,z])F(z)=\mu((-\infty,z])F(z)=μ((−∞,z]); no density is assumed. μ1,μ2\mu_1,\mu_2μ1​,μ2​ are Bochner integrals, finite under the tail condition. The standing hypothesis 0<γ<μ10<\gamma<\mu_10<γ<μ1​ is a field of the model.
  • v:R→R→Rv:\mathbb R\to\mathbb R\to\mathbb Rv:R→R→R takes (x,τ)(x,\tau)(x,τ), and the derivatives vx vxx vt are explicit functions: they are HasDerivAt derivatives of the sections at interior points (x>0x>0x>0, 0<τ<T0<\tau<T0<τ<T) and continuous on [0,∞)×[0,T]∖{(0,0)}[0,\infty)\times[0,T]\setminus\{(0,0)\}[0,∞)×[0,T]∖{(0,0)}; boundary values (at x=0x=0x=0 and τ=T\tau=Tτ=T) are the continuous extensions. "vxxx≥0v_{xxx}\ge0vxxx​≥0 in the weak sense" is monotonicity of vxxv_{xx}vxx​ in xxx, "vxτ≥0v_{x\tau}\ge0vxτ​≥0" is monotonicity of vxv_xvx​ in τ\tauτ.
  • The only hypothesis on vvv is the conclusion of Theorem 3.1, bundled as IsTheorem31Solution. The milestone conclusions (vxx<0v_{xx}<0vxx​<0, the bounds on −vx/vxx-v_x/v_{xx}−vx​/vxx​, d(0+)=0d(0+)=0d(0+)=0) are never hypotheses; with them as hypotheses Theorem 4.5 would be a short mean-value argument.
  • L\mathcal LL is the supremum over measurable retained-loss functions, not its closed form.
  • Infima and suprema of empty sets are 000 in Lean. Theorem 4.2 concludes that {x≥0:vx=1}\{x\ge0: v_x=1\}{x≥0:vx​=1} is nonempty; K(z,τ)K(z,\tau)K(z,τ) uses 000 for the empty set, as the paper does.
  • Atoms are indexed by Fin N from 000. The paper's index i0i_0i0​ is replaced by conditions on zjz_jzj​ and zj−1z_{j-1}zj−1​, which also cover laws whose atoms all lie below 1/λ1/\lambda1/λ.
  • Not formalized: d(∞)d(\infty)d(∞) (the horizon is finite; d(τ)≤x2d(\tau)\le x_2d(τ)≤x2​ for every τ≤T\tau\le Tτ≤T and every TTT carries the same content), the C∞C^\inftyC∞ regularity of ddd for bounded claims (only sketched in the paper), and the Verification Theorem 3.2.

Contributions welcome: the interior regularity of Lemma 4.3, the monotonicity estimate (4.10), and the derivation of Theorem 4.5 from the milestones.

Selected references

  • Chonghu Guan, Zuo Quan Xu, Rui Zhou, Dynamic optimal reinsurance and dividend-payout in a finite time horizon, Mathematics of Operations Research, 2023; read as arXiv:2008.00391v3 (2022). https://arxiv.org/abs/2008.00391
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Control TheoryEconomicsProbability·Captain: mikedeng1

A Dynamic Principal Agent Problem with One-sided Commitment: The Principal's Value Function Is the Minimal Continuous Viscosity Solution of the Type-Indexed HJB SystemResearch Paper

Motivation

In a principal–agent problem with moral hazard, a principal (an employer) pays an agent whose effort she cannot observe; she sees only an output process whose drift the effort controls. Continuous-time versions of the problem, starting with Holmström–Milgrom (1987) and Sannikov (2008), are solved by turning the agent's continuation utility into a state variable and writing a Hamilton–Jacobi–Bellman (HJB) equation for the principal's value.

Most of this literature assumes two-sided commitment: the agent cannot leave. In labour markets the agent can quit whenever an outside offer beats his continuation utility, and the principal must then hire someone else. Zhang and Zhu (arXiv:2208.06473; Mathematics of Operations Research, 2025) study this one-sided commitment: the principal is committed to the contract, the agent is free to quit at a stopping time of his choice, and after each quitting the principal pays a cost and hires a new agent, possibly of another type. The principal's value then depends on every future hire, and the paper characterises it by a coupled system of HJB equations.

Setting

Fix a horizon T>0T>0T>0 and a payment cap C0>0C_0>0C0​>0. A standard Brownian motion BBB on (Ω,F,P)(\Omega,\mathcal F,\mathbb P)(Ω,F,P) is the output. Agents have types θ∈Θ\theta\in\Thetaθ∈Θ. An agent of type θ\thetaθ receiving a payment rate η≤C0\eta\le C_0η≤C0​ and exerting effort α\alphaα has running utility f(θ;s,η)f(\theta;s,\eta)f(θ;s,η) and running cost h(θ;s,α)h(\theta;s,\alpha)h(θ;s,α); fff is increasing and concave in η\etaη, hhh is convex in α\alphaα (Assumption 2.2). Effort shifts the drift of BBB through the Girsanov measure Pα\mathbb P^\alphaPα (weak formulation). The agent's optimal effort against a sensitivity process ZZZ is α=Ih(θ;⋅,Z)\alpha=I^h(\theta;\cdot,Z)α=Ih(θ;⋅,Z), the inverse of ∂αh\partial_\alpha h∂α​h, and Eθ,Z\mathbb E^{\theta,Z}Eθ,Z denotes expectation under the corresponding measure.

A contract started at time ttt is described in forward form by (η,Z)(\eta,Z)(η,Z): the agent's continuation utility is

Xsθ;t,x,η,Z=x−∫ts[f(θ;r,ηr)+H(θ;r,Zr)]dr+∫tsZr dBr,\mathcal X^{\theta;t,x,\eta,Z}_s=x-\int_t^s\big[f(\theta;r,\eta_r)+H(\theta;r,Z_r)\big]dr+\int_t^sZ_r\,dB_r,Xsθ;t,x,η,Z​=x−∫ts​[f(θ;r,ηr​)+H(θ;r,Zr​)]dr+∫ts​Zr​dBr​,

with H(θ;s,z)=sup⁡α[αz−h(θ;s,α)]H(\theta;s,z)=\sup_\alpha[\alpha z-h(\theta;s,\alpha)]H(θ;s,z)=supα​[αz−h(θ;s,α)] and the constraint XT=0\mathcal X_T=0XT​=0. The agent's utility is capped by the upper barrier L‾tθ=∫tTf(θ;s,C0) ds\overline L^\theta_t=\int_t^Tf(\theta;s,C_0)\,dsLtθ​=∫tT​f(θ;s,C0​)ds. He quits at the first time X\mathcal XX reaches the lower barrier L‾tθ=Rtθ−ctθ\underline L^\theta_t=R^\theta_t-c^\theta_tL​tθ​=Rtθ​−ctθ​, where RθR^\thetaRθ is his market value and cθ≥1/Λ0c^\theta\ge1/\Lambda_0cθ≥1/Λ0​ his quitting cost (Assumptions 2.7, 3.1). The relevant domain is

Dθ={(t,x):0≤t<T, L‾tθ<x≤L‾tθ}.D_\theta=\{(t,x):0\le t<T,\ \underline L^\theta_t<x\le\overline L^\theta_t\}.Dθ​={(t,x):0≤t<T, L​tθ​<x≤Ltθ​}.

When the iii-th agent quits at τi<T\tau_i<Tτi​<T, the principal pays cτiPc^P_{\tau_i}cτi​P​ and hires an agent of type ζτi\zeta_{\tau_i}ζτi​​ at utility RτiζτiR^{\zeta_{\tau_i}}_{\tau_i}Rτi​ζτi​​​ (the quitting sequence (5.8)). The principal's value is

u∞(θ;t,x)=sup⁡(η,Z,ζ)Eζ,Z[∫tT[Ih(ζs;s,Zs)−ηs]ds−∑i≥1cτiP1{τi<T}],u_\infty(\theta;t,x)=\sup_{(\eta,Z,\zeta)}\mathbb E^{\zeta,Z}\Big[\int_t^T\big[I^h(\zeta_s;s,Z_s)-\eta_s\big]ds-\sum_{i\ge1}c^P_{\tau_i}\mathbf 1_{\{\tau_i<T\}}\Big],u∞​(θ;t,x)=(η,Z,ζ)sup​Eζ,Z[∫tT​[Ih(ζs​;s,Zs​)−ηs​]ds−i≥1∑​cτi​P​1{τi​<T}​],

and the value of the best new hire at time ttt is u‾∞(t)=sup⁡θu∞(θ;t,Rtθ)−ctP\overline u_\infty(t)=\sup_\theta u_\infty(\theta;t,R^\theta_t)-c^P_tu∞​(t)=supθ​u∞​(θ;t,Rtθ​)−ctP​.

Formalization targets

Goal: Theorem 6.3

The family {u∞(θ;⋅,⋅)}θ∈Θ\{u_\infty(\theta;\cdot,\cdot)\}_{\theta\in\Theta}{u∞​(θ;⋅,⋅)}θ∈Θ​ is the minimal continuous viscosity solution of

∂tu+sup⁡η≤C0, z∈R[12∣z∣2∂xxu−[f(θ;t,η)+H~(θ;t,z)]∂xu+Ih(θ;t,z)−η]=0on Dθ, θ∈Θ,\partial_tu+\sup_{\eta\le C_0,\ z\in\mathbb R}\Big[\tfrac12|z|^2\partial_{xx}u-\big[f(\theta;t,\eta)+\tilde H(\theta;t,z)\big]\partial_xu+I^h(\theta;t,z)-\eta\Big]=0\quad\text{on }D_\theta,\ \theta\in\Theta,∂t​u+η≤C0​, z∈Rsup​[21​∣z∣2∂xx​u−[f(θ;t,η)+H~(θ;t,z)]∂x​u+Ih(θ;t,z)−η]=0on Dθ​, θ∈Θ,

with boundary conditions

u(θ;t,L‾tθ)=−C0(T−t),u(θ;T−,x)=0,u(θ;t,L‾tθ+)≥sup⁡θ′u(θ′;t,Rtθ′)−ctP.u(\theta;t,\overline L^\theta_t)=-C_0(T-t),\qquad u(\theta;T-,x)=0,\qquad u(\theta;t,\underline L^\theta_t+)\ge\sup_{\theta'}u(\theta';t,R^{\theta'}_t)-c^P_t.u(θ;t,Ltθ​)=−C0​(T−t),u(θ;T−,x)=0,u(θ;t,L​tθ​+)≥θ′sup​u(θ′;t,Rtθ′​)−ctP​.

The last condition couples the equations for different types. The goal also asserts that the value sets in (6.1) are nonempty and bounded above, so that u∞u_\inftyu∞​ is a genuine real-valued function.

Milestones

  1. Lemma 3.4: explicit contracts with ∫tT[C0−ηs]ds≤δ\int_t^T[C_0-\eta_s]ds\le\delta∫tT​[C0​−ηs​]ds≤δ under which the agent never quits.
  2. Lemma 2.5 (2.20): a priori estimates for admissible contracts.
  3. Proposition 2.8 and Lemma 3.6: the self-enforcing value V0PV^P_0V0P​ and the new-hire value u‾0\overline u_0u0​ are uniformly continuous with modulus CρC\sqrt\rhoCρ​.
  4. Theorem 4.5: with at most one quitting, u1u_1u1​ is the minimal continuous viscosity solution of the same equation with boundary datum u‾0\overline u_0u0​.
  5. Proposition 5.4: a non-recursive representation of unu_nun​ (at most nnn quittings).
  6. Proposition 6.1: Pζ,Z(τn<T)≤C/n\mathbb P^{\zeta,Z}(\tau_n<T)\le C/nPζ,Z(τn​<T)≤C/n, and ∣un−u∞∣≤C/n|u_n-u_\infty|\le C/n∣un​−u∞​∣≤C/n.
  7. Proposition 6.2: monotonicity and uniform continuity of u∞u_\inftyu∞​, regularity of u‾∞\overline u_\inftyu∞​, and the boundary conditions.
  8. (6.7): the dynamic programming principle for u∞u_\inftyu∞​.

Significance

The theorem identifies the principal's value under one-sided commitment as a PDE object, which makes it computable and comparable with other contracting regimes. Along the way the paper shows that the principal sees only finitely many quittings (Proposition 6.1) and that tolerating more quittings never lowers her value, so contracts that prevent quitting altogether (self-enforcing contracts) are in general suboptimal. The coupling through u‾∞\overline u_\inftyu∞​ turns the problem into an infinite system of HJB equations indexed by agent types, a structure that also appears in switching and re-hiring problems.

The result is proved in the paper; none of it is formalized. A formalization would add to the platform a continuous-time moral-hazard model in the weak formulation, hitting-time stopping driven by an Itô integral, a quitting sequence with random restarts and type switching, and a viscosity-solution notion for a fully nonlinear HJB equation on a time-dependent domain. The paper's own proof leaves several steps to the reader (the dynamic programming principle, the viscosity property, comparison for a truncated equation), so a complete development would also supply these.

Difficulty

The obvious route is "dynamic programming principle, then viscosity property, then comparison". Each step is harder here than in a textbook control problem. The control zzz is unbounded, so the Hamiltonian can be +∞+\infty+∞ and the viscosity property must be derived without a finite Hamiltonian. The process is stopped at a hitting time of a moving barrier and restarted at a random level with a new type, so the dynamic programming principle must handle restarts. Minimality cannot come from a standard comparison principle, because the boundary datum at L‾θ\underline L^\thetaL​θ depends on the competitor itself and no growth condition is imposed on competitors; the paper argues through approximation by unu_nun​ and Theorem 4.5 instead.

Formalization scope

All objects are defined in the namespace DynPrincipalAgent.HJB. Process time is R≥0\mathbb R_{\ge0}R≥0​; deterministic data are functions of real time. The Itô integral is the published Peng1990.SMP.IsItoIntegral, with a continuous version required wherever hitting times read paths. Controls started at ttt are progressively measurable for the filtration Ft\mathbb F^tFt of Bs−BtB_s-B_tBs​−Bt​. Value functions are real suprema of value sets that record an expectation only when it is genuine (integrable payoffs, almost surely integrable drifts and running rewards, summable quitting costs); these conditions hold for every admissible control.

Pinned readings, all disclosed in the items: viscosity solutions are the standard Crandall–Ishii–Lions notion with C2C^2C2 test functions on R2\mathbb R^2R2, tested on the interior of DθD_\thetaDθ​, with the supremum in the HJB operator never formed; the boundary condition at L‾θ\underline L^\thetaL​θ requires a real right limit compared against every u(θ′;t,Rtθ′)−ctPu(\theta';t,R^{\theta'}_t)-c^P_tu(θ′;t,Rtθ′​)−ctP​; Θ\ThetaΘ carries a σ-algebra and fff, hhh, ∂αh\partial_\alpha h∂α​h are jointly measurable; Assumption 2.7 (ii) is read as ∣Rsθ−Rs′θ∣≤ρ(∣s−s′∣)|R^\theta_s-R^\theta_{s'}|\le\rho(|s-s'|)∣Rsθ​−Rs′θ​∣≤ρ(∣s−s′∣); a modulus of continuity is nondecreasing, vanishes at 0+0^+0+ and satisfies ρ(δ)≥δ\rho(\delta)\ge\deltaρ(δ)≥δ; generic constants depend only on (T,C0,Λ0,Λ1)(T,C_0,\Lambda_0,\Lambda_1)(T,C0​,Λ0​,Λ1​) and are fixed before the model; HHH and H~\tilde HH~ take the closed forms of (2.11)–(2.12). The agent's BSDE and reflected BSDE (Propositions 2.3, 3.2), §7's standard contracts and the economic interpretation of RθR^\thetaRθ, cθc^\thetacθ, cPc^PcP are out of scope.

A formalization in which a value function equals a junk value (an empty or unbounded real supremum, a Bochner integral of a non-integrable payoff, a hitting time of an empty set) or in which the viscosity notion is vacuous does not count: the goal states that the value sets are nonempty and bounded, and the definitions avoid junk by construction. Competitors in the minimality clause satisfy exactly the printed boundary conditions, with no added growth bound.

Reusable infrastructure: Girsanov measures for BMO drifts, forward utility processes, hitting times of continuous semimartingales, and viscosity solutions of HJB equations on non-cylindrical domains. Contributions on any milestone, and on general lemmas such as the dynamic programming principle for controlled diffusions stopped at hitting times, are welcome.

Selected references

  • J. Zhang, Z. Zhu, A Dynamic Principal Agent Problem with One-sided Commitment, Mathematics of Operations Research, 2025. Preprint arXiv:2208.06473v3. https://arxiv.org/abs/2208.06473
  • Y. Sannikov, A Continuous-Time Version of the Principal–Agent Problem, Review of Economic Studies 75 (2008). https://doi.org/10.1111/j.1467-937X.2008.00486.x
  • B. Holmström, P. Milgrom, Aggregation and Linearity in the Provision of Intertemporal Incentives, Econometrica 55 (1987). https://doi.org/10.2307/1913238
  • M. G. Crandall, H. Ishii, P.-L. Lions, User's guide to viscosity solutions of second order partial differential equations, Bull. AMS 27 (1992). https://doi.org/10.1090/S0273-0979-1992-00266-5
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Control TheoryStochastic Systems·Captain: mikedeng1

Stochastic Control Problems with State Reflections Arising from Relaxed Benchmark Tracking: Verification Theorem for the Optimal Feedback Investment-Consumption StrategyResearch Paper

Motivation

A fund manager who tracks a benchmark (a stock index, a price index, the cost of higher education) wants the managed wealth to stay above the benchmark at all times. Under a strict floor constraint Vt≥MtV_t\ge M_tVt​≥Mt​ the set of admissible strategies can be empty when the benchmark is random. Bo, Huang and Yu (arXiv:2302.08302, Math. Oper. Res.) relax the constraint: the manager may inject capital AtA_tAt​ so that Vt+At≥MtV_t+A_t\ge M_tVt​+At​≥Mt​, and pays β>0\beta>0β>0 per unit injected. The problem becomes a consumption–investment problem with a running-maximum cost, of the type studied with viscosity methods by Barron–Ishii (1989) and Bokanowski et al. (2015). The paper obtains instead a classical solution of the associated HJB equation and an explicit optimal feedback control. The reduction from the constrained problem to the auxiliary problem below is due to Bo, Liao and Yu (2021) and is not part of this mission.

Setting

A market has ddd risky assets with return vector μ≠0\mu\ne0μ=0 and invertible volatility matrix σ\sigmaσ; the riskless rate is 000. On a filtered probability space satisfying the usual conditions with a ddd-dimensional Brownian motion WWW, write Wγ=∑jγjWjW^\gamma=\sum_j\gamma_jW^jWγ=∑j​γj​Wj and Wη=∑jηjWjW^\eta=\sum_j\eta_jW^jWη=∑j​ηj​Wj with ∣γ∣=∣η∣=1|\gamma|=|\eta|=1∣γ∣=∣η∣=1. The benchmark is Mt=mt+ZtM_t=m_t+Z_tMt​=mt​+Zt​, where ZZZ is a geometric Brownian motion with drift μZ\mu_ZμZ​ and volatility σZ≥0\sigma_Z\ge0σZ​≥0 driven by WηW^\etaWη, and mtm_tmt​ is the running maximum of Bt=b+μBt+σBWtγB_t=b+\mu_Bt+\sigma_BW^\gamma_tBt​=b+μB​t+σB​Wtγ​, σB≥0\sigma_B\ge0σB​≥0.

A strategy (θ,c)(\theta,c)(θ,c) invests θt∈Rd\theta_t\in\mathbb R^dθt​∈Rd and consumes at rate ct≥0c_t\ge0ct​≥0; the class Ur\mathbb U^rUr consists of progressively measurable pairs for which the wealth equation is well defined on every bounded interval. The auxiliary states are the reflected wealth surplus X≥0X\ge0X≥0, started at xxx,

Xt=x+∫0tθs⊤μ ds+∫0tθs⊤σ dWs−∫0tcs ds−(Zt−z)−(mt−m0)+LtX,X_t=x+\int_0^t\theta_s^\top\mu\,ds+\int_0^t\theta_s^\top\sigma\,dW_s-\int_0^tc_s\,ds-(Z_t-z)-(m_t-m_0)+L^X_t,Xt​=x+∫0t​θs⊤​μds+∫0t​θs⊤​σdWs​−∫0t​cs​ds−(Zt​−z)−(mt​−m0​)+LtX​,

where LXL^XLX is the minimal nondecreasing process keeping X≥0X\ge0X≥0 (the injected capital), and the reflected distance It=mt−Bt≥0I_t=m_t-B_t\ge0It​=mt​−Bt​≥0 started at hhh. With power utility U(c)=cp/pU(c)=c^p/pU(c)=cp/p, p∈(−∞,0)∪(0,1)p\in(-\infty,0)\cup(0,1)p∈(−∞,0)∪(0,1), and discount rate ρ>0\rho>0ρ>0, the objective is

J(x,h,z;θ,c)=E[∫0∞e−ρtU(ct) dt−β∫0∞e−ρtdLtX].J(x,h,z;\theta,c)=\mathbb E\Big[\int_0^\infty e^{-\rho t}U(c_t)\,dt-\beta\int_0^\infty e^{-\rho t}dL^X_t\Big].J(x,h,z;θ,c)=E[∫0∞​e−ρtU(ct​)dt−β∫0∞​e−ρtdLtX​].

The candidate value function is built from a probabilistic representation. On a space with independent Brownian motions B0,B1,B2B^0,B^1,B^2B0,B1,B2, let RrR^rRr be a reflected drifted Brownian motion r+(α2/2−ρ)t+αBt1+Ltr≥0r+(\alpha^2/2-\rho)t+\alpha B^1_t+L^r_t\ge0r+(α2/2−ρ)t+αBt1​+Ltr​≥0, let HhH^hHh be a correlated one with local time KhK^hKh, and let NzN^zNz be a geometric Brownian motion. With the coefficients α,κ1,κ2,ϱ1,ϱ2\alpha,\kappa_1,\kappa_2,\varrho_1,\varrho_2α,κ1​,κ2​,ϱ1​,ϱ2​ of (2.9) and (3.4),

v(r,h,z)=1−ppβ−p1−pE[∫0∞e−ρs+p1−pRsrds]+β(κ2−μZ)E[∫0∞e−ρs−RsrNszds]−βE[∫0∞e−ρs−RsrdKsh],v(r,h,z)=\tfrac{1-p}p\beta^{-\frac p{1-p}}\mathbb E\Big[\int_0^\infty e^{-\rho s+\frac p{1-p}R^r_s}ds\Big]+\beta(\kappa_2-\mu_Z)\mathbb E\Big[\int_0^\infty e^{-\rho s-R^r_s}N^z_sds\Big]-\beta\mathbb E\Big[\int_0^\infty e^{-\rho s-R^r_s}dK^h_s\Big],v(r,h,z)=p1−p​β−1−pp​E[∫0∞​e−ρs+1−pp​Rsr​ds]+β(κ2​−μZ​)E[∫0∞​e−ρs−Rsr​Nsz​ds]−βE[∫0∞​e−ρs−Rsr​dKsh​],

u^(y,h,z)=v(−ln⁡(y/β),h,z)\hat u(y,h,z)=v(-\ln(y/\beta),h,z)u^(y,h,z)=v(−ln(y/β),h,z) for y∈(0,β]y\in(0,\beta]y∈(0,β], and

u(x,h,z)=inf⁡y∈(0,β]{u^(y,h,z)+yx}.u(x,h,z)=\inf_{y\in(0,\beta]}\{\hat u(y,h,z)+yx\}.u(x,h,z)=y∈(0,β]inf​{u^(y,h,z)+yx}.

Formalization targets

Goal: Theorem 4.1 (verification theorem)

For model parameters with μZ>κ2\mu_Z>\kappa_2μZ​>κ2​ and σB≠0\sigma_B\ne0σB​=0 there is ρ0>0\rho_0>0ρ0​>0 such that for every ρ>ρ0\rho>\rho_0ρ>ρ0​: (i) uuu is a classical solution of the HJB equation (4.2) with the Neumann conditions ux(0,h,z)=βu_x(0,h,z)=\betaux​(0,h,z)=β and uh(x,0,z)=ux(x,0,z)u_h(x,0,z)=u_x(x,0,z)uh​(x,0,z)=ux​(x,0,z), with ux>0u_x>0ux​>0 and uxx<0u_{xx}<0uxx​<0; (ii) for every admissible strategy and every (x,h,z)∈R+3(x,h,z)\in\mathbb R^3_+(x,h,z)∈R+3​,

J(x,h,z;θ,c)≤u(x,h,z),J(x,h,z;\theta,c)\le u(x,h,z),J(x,h,z;θ,c)≤u(x,h,z),

with equality for the feedback strategy θ∗=−(σσ⊤)−1μux−σBσγuxh+σZσηz(uxx−uxz)uxx\theta^*=-(\sigma\sigma^\top)^{-1}\frac{\mu u_x-\sigma_B\sigma\gamma u_{xh}+\sigma_Z\sigma\eta z(u_{xx}-u_{xz})}{u_{xx}}θ∗=−(σσ⊤)−1uxx​μux​−σB​σγuxh​+σZ​σηz(uxx​−uxz​)​, c∗=ux1/(p−1)c^*=u_x^{1/(p-1)}c∗=ux1/(p−1)​ along a solution of the reflected feedback system (4.4). The threshold ρ0\rho_0ρ0​ is asserted to exist, not fixed: the paper's formula (4.45) for it depends on ρ\rhoρ and is not self-contained.

Milestones, in the order of the proof

  1. Lemma 3.2. The first two terms l(r,z)l(r,z)l(r,z) of vvv solve the Neumann problem (3.8) and equal the explicit form (3.9).
  2. Lemma 3.4. For σB≠0\sigma_B\ne0σB​=0, φ(r,h)=−βE[∫0∞e−ρs−RsrdGsh]\varphi(r,h)=-\beta\mathbb E[\int_0^\infty e^{-\rho s-R^r_s}dG^h_s]φ(r,h)=−βE[∫0∞​e−ρs−Rsr​dGsh​] is C2C^2C2 on R+2\mathbb R^2_+R+2​, where GhG^hGh is the local time of a reflected Brownian motion independent of RrR^rRr.
  3. Lemma 3.3. GhG^hGh and RrR^rRr are independent and φ\varphiφ solves the Neumann problem (3.15).
  4. Proposition 3.5. ψ=φ+ξ\psi=\varphi+\xiψ=φ+ξ solves (3.38), and every bounded classical solution of (3.38) equals the last term of vvv.
  5. Remark 3.6. ψr+ψrr>0\psi_r+\psi_{rr}>0ψr​+ψrr​>0.
  6. Theorem 3.1. u^\hat uu^ is strictly convex in yyy and solves the dual PDE (2.8) with (2.10), (2.11).
  7. Theorem 4.1(i) and (4.7): the linear growth ∣θ∗∣≤Co(1+x+z)|\theta^*|\le C_o(1+x+z)∣θ∗∣≤Co​(1+x+z), ∣c∗∣≤Cq(1+x)|c^*|\le C_q(1+x)∣c∗∣≤Cq​(1+x).

Significance

The theorem settles two questions about the relaxed tracking formulation: the optimal portfolio–consumption pair exists in feedback form, and the value function is a classical (not only viscosity) solution of an HJB equation with two Neumann boundary conditions. Together with the paper's Lemma 4.4, it shows that the expected discounted capital injection of the optimal strategy is finite, so the relaxed problem is well posed. The dual representation also gives the value in a separated form, three expectations of functionals of reflected Brownian motions, which is what makes the derivatives and the feedback explicit.

The result is proved in the paper; nothing here is open. No part of it is formalized. A formal proof would need Itô's formula for reflected processes, the smoothness of expectations of local-time functionals, and the duality argument; any of the milestones on its own is a self-contained target.

Difficulty

The last term of vvv couples the reflected process RrR^rRr with the local time KhK^hKh of a second reflected process correlated with it through ϱ1\varrho_1ϱ1​. Differentiating E[∫e−ρs−RsrdKsh]\mathbb E[\int e^{-\rho s-R^r_s}dK^h_s]E[∫e−ρs−Rsr​dKsh​] in (r,h)(r,h)(r,h) directly fails: the local time is not differentiable in its starting point in any pathwise sense, and the correlation prevents conditioning one process on the other. The paper first treats the independent case (Lemmas 3.3–3.4), where the expectation factors through the law of GhG^hGh, and then removes the correlation by a homogenization of the Neumann conditions (Proposition 3.5). A second difficulty is the verification step itself: the admissible class is unbounded and the state reflects at two boundaries, so the local martingale terms must be controlled by moment bounds that depend on the growth (4.7) of the feedback.

Formalization scope

  • Parameters. One structure holds μ,σ,μZ,σZ,μB,σB,γ,η,β,p\mu,\sigma,\mu_Z,\sigma_Z,\mu_B,\sigma_B,\gamma,\eta,\beta,pμ,σ,μZ​,σZ​,μB​,σB​,γ,η,β,p; the standing assumptions are d≥1d\ge1d≥1, det⁡σ≠0\det\sigma\ne0detσ=0, μ≠0\mu\ne0μ=0, σZ,σB≥0\sigma_Z,\sigma_B\ge0σZ​,σB​≥0, γ⋅γ=η⋅η=1\gamma\cdot\gamma=\eta\cdot\eta=1γ⋅γ=η⋅η=1, β>0\beta>0β>0, p<1p<1p<1, p≠0p\ne0p=0. All coefficients (α,κ1,κ2,ϱ1,ϱ2,C1,C2,ℓ\alpha,\kappa_1,\kappa_2,\varrho_1,\varrho_2,C_1,C_2,\ellα,κ1​,κ2​,ϱ1​,ϱ2​,C1​,C2​,ℓ) are definitions.
  • Carriers. vvv, u^\hat uu^, uuu are defined on any probability space with a standard 3-dimensional Brownian motion (published EthierKurtz.IsStandardBrownian), and every statement holds for every such space. The control problem lives on any filtered space satisfying the usual conditions with an F\mathbb FF-Brownian motion (published RankBasedSDI.LoadBalancing.UsualConditions, IsFBrownian).
  • Processes in closed form. Rr,Hh,Kh,Lr,GhR^r,H^h,K^h,L^r,G^hRr,Hh,Kh,Lr,Gh are given by Skorokhod formulas (published skorokhodReg), ZZZ and NzN^zNz as explicit exponentials. The only stochastic integral is ∫θ⊤σ dW\int\theta^\top\sigma\,dW∫θ⊤σdW, through the published EthierKurtz.HasBrownianItoIntegral with a continuous version required.
  • Expectations and objective. Expectations of nonnegative integrands are lintegrals; statements about vvv assert their finiteness. Stieltjes integrals use the Lebesgue–Stieltjes measure of the path. The objective is compared in the extended reals as utility≤u+β⋅cost\text{utility}\le u+\beta\cdot\text{cost}utility≤u+β⋅cost, which agrees with J≤uJ\le uJ≤u whenever JJJ is defined and never produces ∞−∞\infty-\infty∞−∞; cpc^pcp is computed in [0,∞][0,\infty][0,∞] so that 0p=∞0^p=\infty0p=∞ for p<0p<0p<0.
  • Classical solutions. C2C^2C2 on the closed domain (ContDiffOn ℝ 2), the PDE on the open set the paper names, Neumann conditions pointwise on the faces; derivatives are taken within the closed coordinate domains. The suprema in (4.2) are least upper bounds (IsLUB), the consumption supremum over c>0c>0c>0.
  • Added hypotheses. μZ>κ2\mu_Z>\kappa_2μZ​>κ2​ and σB≠0\sigma_B\ne0σB​=0 in Theorem 4.1 and σB≠0\sigma_B\ne0σB​=0, ρ>α2∣p∣/(2(1−p))+μZ\rho>\alpha^2|p|/(2(1-p))+\mu_Zρ>α2∣p∣/(2(1−p))+μZ​ in Theorem 3.1 are used by the proofs but not printed in the statements; they are added. Lemma 3.2 and the milestone Theorem 4.1(i) also carry Theorem 3.1's ρ>α2p/(2(1−p))\rho>\alpha^2p/(2(1-p))ρ>α2p/(2(1−p)): when μZ<0\mu_Z<0μZ​<0 Lemma 3.2's printed condition does not imply it, and without it the first expectation in vvv is infinite.
  • Ruled out. Defining uuu as the supremum of JJJ would make (ii) circular, and specializing to d=1d=1d=1, σB=0\sigma_B=0σB​=0, ϱ1=0\varrho_1=0ϱ1​=0 or a fixed ρ\rhoρ changes the theorem; none of these is used. A statement "for every solution of (4.4)" would be vacuous if (4.4) had no solution, so the optimal pair is asserted to exist.

The definitions of reflected processes, Stieltjes integrals against local times, and classical Neumann solutions are reusable beyond this mission. Proofs of any milestone, and of the deterministic facts (0<ℓ<10<\ell<10<ℓ<1, ∣ϱi∣≤1|\varrho_i|\le1∣ϱi​∣≤1, (3.9) solving (3.8)), are welcome.

Selected references

  • G. Bo, Y. Huang, X. Yu, Stochastic control problems with state-reflections arising from relaxed benchmark tracking, arXiv:2302.08302v4 (Math. Oper. Res.). https://arxiv.org/abs/2302.08302
  • L. Bo, H. Liao, X. Yu, Optimal tracking portfolio with a ratcheting capital benchmark, SIAM J. Control Optim. 59(3), 2346–2380, 2021.
  • J. M. Harrison, Brownian Motion and Stochastic Flow Systems, Wiley, New York, 1985.
  • W. Łaukajtys, L. Słomiński, Penalization methods for the Skorokhod problem and reflecting SDEs with jumps, Bernoulli 19(5A), 1750–1775, 2013.
  • E. N. Barron, H. Ishii, The Bellman equation for minimizing the maximum cost, Nonlinear Anal. TMA 13(9), 1067–1090, 1989.
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Functional AnalysisOperations ResearchOptimization·Captain: mikedeng1

Optimality Conditions in Control Problems with Random State Constraints in Probabilistic or Almost Sure Form IV: Radon-Measure Optimality Conditions for Robust State ConstraintsResearch Paper

Motivation

Optimal control problems governed by partial differential equations (PDEs) often carry uncertainty in their data, for example a random source term. When the state must stay below a threshold, there are several ways to impose the constraint: with high probability (chance constraints), almost surely, or for every value in a fixed uncertainty set (robust constraints). C. Geiersbach and R. Henrion (arXiv:2306.03965v2, Math. Oper. Res. 2025) derive first-order optimality conditions for all three models for the same elliptic model problem. This mission covers the robust model of §3.2 (pp. 23–25). Its Karush–Kuhn–Tucker (KKT) system has a Radon measure as multiplier, and it is related to the semi-infinite programming view of the same problem.

Robust state constraints are also the limiting case of the almost-sure model: by Lemma 3.4 of the paper (p. 19), an almost-sure constraint and the constraint for every parameter in the support of the distribution coincide when the constraint function is lower semicontinuous in the parameter. The robust multipliers live in C(Dˉ×Ξ)∗C(\bar D\times\Xi)^*C(Dˉ×Ξ)∗, which is a space of measures, whereas the almost-sure multipliers of §3.1 contain singular functionals with no such representation.

Setting

Let D⊆RdD\subseteq\mathbb R^dD⊆Rd, d∈{1,2,3}d\in\{1,2,3\}d∈{1,2,3}, be open, bounded and of class S: there are γ∈(0,1)\gamma\in(0,1)γ∈(0,1) and r0>0r_0>0r0​>0 such that meas⁡(Br(x)∖D)≥γmeas⁡(Br(x))\operatorname{meas}(B_r(x)\setminus D)\ge\gamma\operatorname{meas}(B_r(x))meas(Br​(x)∖D)≥γmeas(Br​(x)) for all x∈∂Dx\in\partial Dx∈∂D and 0<r<r00<r<r_00<r<r0​. Let Ξ⊂Rm\Xi\subset\mathbb R^mΞ⊂Rm be compact, let f0,φ1,…,φm∈L2(D)f_0,\varphi_1,\dots,\varphi_m\in L^2(D)f0​,φ1​,…,φm​∈L2(D), and set f(x,z)=f0(x)+∑i=1mziφi(x)f(x,z)=f_0(x)+\sum_{i=1}^m z_i\varphi_i(x)f(x,z)=f0​(x)+∑i=1m​zi​φi​(x) (Assumption 1.1, eq. (3)). The solution operator A−1:L2(D)→C(Dˉ)A^{-1}:L^2(D)\to C(\bar D)A−1:L2(D)→C(Dˉ) maps FFF to the unique weak solution y∈H01(D)∩C(Dˉ)y\in H^1_0(D)\cap C(\bar D)y∈H01​(D)∩C(Dˉ) of −Δy=F-\Delta y=F−Δy=F in DDD, y=0y=0y=0 on ∂D\partial D∂D.

For a control u∈L2(D)u\in L^2(D)u∈L2(D), a cost F:L2(D)→RF:L^2(D)\to\mathbb RF:L2(D)→R and a threshold α∈R\alpha\in\mathbb Rα∈R, the robust problem (63) is

min⁡u∈L2(D)F(u)s.t.−Δy^(⋅,z)=u+f(⋅,z) in D,y^(⋅,z)=0 on ∂D,y^(x,z)≤α  ∀(x,z)∈D×Ξ.\min_{u\in L^2(D)}F(u)\quad\text{s.t.}\quad -\Delta\hat y(\cdot,z)=u+f(\cdot,z)\ \text{in }D,\quad \hat y(\cdot,z)=0\ \text{on }\partial D,\quad \hat y(x,z)\le\alpha\ \ \forall (x,z)\in D\times\Xi.u∈L2(D)min​F(u)s.t.−Δy^​(⋅,z)=u+f(⋅,z) in D,y^​(⋅,z)=0 on ∂D,y^​(x,z)≤α  ∀(x,z)∈D×Ξ.

The state is S^(u)∈C(Dˉ×Ξ)\hat{\mathcal S}(u)\in C(\bar D\times\Xi)S^(u)∈C(Dˉ×Ξ), [S^(u)](x,z)=[A−1(u+f(⋅,z))](x)[\hat{\mathcal S}(u)](x,z)=[A^{-1}(u+f(\cdot,z))](x)[S^(u)](x,z)=[A−1(u+f(⋅,z))](x), and G^(u)=S^(u)−α\hat{\mathcal G}(u)=\hat{\mathcal S}(u)-\alphaG^​(u)=S^(u)−α. The cone is K^={y∈C(Dˉ×Ξ):y≤0}\hat{\mathcal K}=\{y\in C(\bar D\times\Xi):y\le0\}K^={y∈C(Dˉ×Ξ):y≤0} and its polar cone is K^−={y∗∈C(Dˉ×Ξ)∗:⟨y∗,y⟩≤0 ∀y∈K^}\hat{\mathcal K}^-=\{y^*\in C(\bar D\times\Xi)^*:\langle y^*,y\rangle\le0\ \forall y\in\hat{\mathcal K}\}K^−={y∗∈C(Dˉ×Ξ)∗:⟨y∗,y⟩≤0 ∀y∈K^}. The linear part of the state is [A^−1B^h](x,z)=[A−1h](x)[\hat{\mathcal A}^{-1}\hat{\mathcal B}h](x,z)=[A^{-1}h](x)[A^−1B^h](x,z)=[A−1h](x). The active set is M(u)={(x,z)∈Dˉ×Ξ:[S^(u)](x,z)=max⁡Dˉ×ΞS^(u)}M(u)=\{(x,z)\in\bar D\times\Xi:[\hat{\mathcal S}(u)](x,z)=\max_{\bar D\times\Xi}\hat{\mathcal S}(u)\}M(u)={(x,z)∈Dˉ×Ξ:[S^(u)](x,z)=maxDˉ×Ξ​S^(u)}.

Formalization targets

Goal: Lemma 3.14 refined to (66), pp. 23–24

Let FFF be convex and continuously Fréchet differentiable, and assume the constraint qualification 0∈int⁡{G^(L2(D))−K^}0\in\operatorname{int}\{\hat{\mathcal G}(L^2(D))-\hat{\mathcal K}\}0∈int{G^​(L2(D))−K^}. Then u∗u^*u∗ is a solution of (63) if and only if there is a nonnegative finite Borel measure μ∗\mu^*μ∗ on Dˉ×Ξ\bar D\times\XiDˉ×Ξ with, for y∗=S^(u∗)y^*=\hat{\mathcal S}(u^*)y∗=S^(u∗),

⟨DF(u∗),h⟩+∫Dˉ×Ξ[A−1h](x) dμ∗(x,z)=0∀h∈L2(D),\langle DF(u^*),h\rangle+\int_{\bar D\times\Xi}[A^{-1}h](x)\,d\mu^*(x,z)=0\quad\forall h\in L^2(D),⟨DF(u∗),h⟩+∫Dˉ×Ξ​[A−1h](x)dμ∗(x,z)=0∀h∈L2(D), y∗≤α on Dˉ×Ξ,∫Dˉ×Ξ(y∗−α) dμ∗=0.y^*\le\alpha\ \text{on }\bar D\times\Xi,\qquad\int_{\bar D\times\Xi}(y^*-\alpha)\,d\mu^*=0.y∗≤α on Dˉ×Ξ,∫Dˉ×Ξ​(y∗−α)dμ∗=0.

The page derives (66) from the abstract system (65) of Lemma 3.14 (necessity). Sufficiency is the converse direction of Lemma 3.14, since a nonnegative measure defines a multiplier in K^−\hat{\mathcal K}^-K^− by integration. Both directions are part of the goal.

Milestones

  1. Lemma 3.13: unique solvability of (63b)–(63c) in C(Dˉ×Ξ)C(\bar D\times\Xi)C(Dˉ×Ξ) with the bound (64).
  2. Lemma 3.14: the abstract KKT system (65) with λ∗∈C(Dˉ×Ξ)∗\lambda^*\in C(\bar D\times\Xi)^*λ∗∈C(Dˉ×Ξ)∗.
  3. The identification C(Dˉ×Ξ)∗≅M(Dˉ×Ξ)C(\bar D\times\Xi)^*\cong\mathcal M(\bar D\times\Xi)C(Dˉ×Ξ)∗≅M(Dˉ×Ξ) (p. 23): every λ∗\lambda^*λ∗ is integration against a signed measure.
  4. Nonnegativity (p. 24): λ∗∈K^−\lambda^*\in\hat{\mathcal K}^-λ∗∈K^− gives a nonnegative μ∗\mu^*μ∗.
  5. Lemma 3.15: (66) is equivalent to the scalar-multiplier form (67): λ∗≥0\lambda^*\ge0λ∗≥0 and a probability measure μ~\tilde\muμ~​ on M(u∗)M(u^*)M(u∗) with ⟨DF(u∗),h⟩+λ∗∫[A−1h](x) dμ~=0\langle DF(u^*),h\rangle+\lambda^*\int[A^{-1}h](x)\,d\tilde\mu=0⟨DF(u∗),h⟩+λ∗∫[A−1h](x)dμ~​=0, max⁡y∗≤α\max y^*\le\alphamaxy∗≤α, λ∗(max⁡y∗−α)=0\lambda^*(\max y^*-\alpha)=0λ∗(maxy∗−α)=0.
  6. Lemma 3.16: the convex-hull condition (68) is equivalent to the existence of such a μ~\tilde\muμ~​.
  7. Lemma 3.4: for lower semicontinuous hhh, h(ξ)≤0h(\xi)\le0h(ξ)≤0 almost surely if and only if h≤0h\le0h≤0 on the support of the law of ξ\xiξ.

Significance

The goal gives the robust problem a KKT system whose multiplier is a nonnegative measure on Dˉ×Ξ\bar D\times\XiDˉ×Ξ that is carried by the points where the constraint is active. Lemmas 3.15 and 3.16 turn this into a scalar multiplier times a probability measure on the active set, and into a convex-hull condition. These are the forms used by semi-infinite programming algorithms and by discretizations that approximate the measure by finitely many atoms. Together with Lemma 3.4, they say when the KKT system of the almost-sure model (§3.1, with its singular multipliers) can be replaced by the measure-valued system of the robust model.

All statements of the mission are proved in the paper, some by reference: Lemma 3.14's proof refers to the argument of Lemma 3.7, and Lemma 3.16 relies on Phelps's barycenter theorem. None of them is formalized. A formal development would also check two points that the page leaves implicit. Lemma 3.15's proof divides by the total mass of μ∗\mu^*μ∗ and does not treat μ∗=0\mu^*=0μ∗=0. Condition (68) is printed per direction hhh, while (67a) needs one measure for all hhh.

Difficulty

The necessity direction of the goal needs a Lagrange multiplier theorem in a Banach space whose constraint cone K^\hat{\mathcal K}K^ has nonempty interior. The multiplier is a priori only an element of C(Dˉ×Ξ)∗C(\bar D\times\Xi)^*C(Dˉ×Ξ)∗, and the Riesz–Markov–Kakutani theorem on the compact space Dˉ×Ξ\bar D\times\XiDˉ×Ξ turns it into a measure. The state S^(u)\hat{\mathcal S}(u)S^(u) must also be shown to lie in C(Dˉ×Ξ)C(\bar D\times\Xi)C(Dˉ×Ξ). Continuity of each slice in xxx is the regularity of Lemma 1.2 (continuity of H01H^1_0H01​ solutions up to the boundary for class-S domains, from Kinderlehrer–Stampacchia), and joint continuity needs the bound (64), uniform in zzz. Working pointwise in zzz does not give these: a family of continuous slices need not be jointly continuous without an estimate that is uniform in the parameter.

Formalization scope

Dˉ\bar DDˉ and Ξ\XiΞ are subtypes of Euclidean spaces with CompactSpace instances, so C(Dˉ×Ξ)C(\bar D\times\Xi)C(Dˉ×Ξ) carries its sup norm. Measures on Dˉ×Ξ\bar D\times\XiDˉ×Ξ are Borel measures; on this compact metric space every finite Borel measure is regular, so "regular Borel (Radon) measure" is IsFiniteMeasure, and nonnegativity (66c) is built into Lean's Measure type. The solution operator is a hypothesis: a bounded linear map L2(D)→C(Dˉ)L^2(D)\to C(\bar D)L2(D)→C(Dˉ) such that A−1FA^{-1}FA−1F is, for every FFF, the weak solution in H01(D)∩C(Dˉ)H^1_0(D)\cap C(\bar D)H01​(D)∩C(Dˉ), encoded with the published weak-derivative definitions HunterPDE.Shared.WeakDeriv. The page's "≤0\le0≤0 in D×ΞD\times\XiD×Ξ" is encoded on Dˉ×Ξ\bar D\times\XiDˉ×Ξ, the same condition for continuous functions. "Solution" means global minimizer over the feasible set. L2(D)∗L^2(D)^*L2(D)∗ is identified with L2(D)L^2(D)L2(D) through the Riesz map. In Lemma 3.16 the clco of (68) is the norm closure of the convex hull, which equals the weak closure.

Added hypotheses: DDD and Ξ\XiΞ nonempty in Lemmas 3.15 and 3.16 (no probability measure exists on an empty set). Pinned reading: (68) is posed as one inclusion 0∈DF(u∗)+λ∗ co⁡‾{ux:(x,z)∈M(u∗)}0\in DF(u^*)+\lambda^*\,\overline{\operatorname{co}}\{u_x:(x,z)\in M(u^*)\}0∈DF(u∗)+λ∗co{ux​:(x,z)∈M(u∗)} in L2(D)L^2(D)L2(D), where uxu_xux​ represents h↦[A−1h](x)h\mapsto[A^{-1}h](x)h↦[A−1h](x). The page derives (68) from exactly this inclusion. The closed hull is kept because the page's remark that "co" suffices is not proved in infinite dimension.

Several trivializing formalizations are ruled out. The state operator is tied to the PDE and is never an arbitrary map into C(Dˉ×Ξ)C(\bar D\times\Xi)C(Dˉ×Ξ). The multiplier carries its sign (a nonnegative measure, or λ∗∈K^−\lambda^*\in\hat{\mathcal K}^-λ∗∈K^−) together with complementarity. Optimality is global minimality, not a stationarity condition. All integrands are continuous functions on a compact space against finite measures, so no integral takes a junk value.

A complete development needs elliptic regularity in C(Dˉ)C(\bar D)C(Dˉ) for class-S domains, a Banach-space Lagrange multiplier theorem under a Robinson-type constraint qualification, the Riesz–Markov–Kakutani theorem for C(K)∗C(K)^*C(K)∗ with signed measures (the platform's FamousTheorems.riesz_markov_kakutani covers positive functionals on CcC_cCc​), and barycenters of probability measures on compact convex sets. The last three are reusable beyond this mission. Contributions of proofs for any of them are welcome.

Selected references

  • C. Geiersbach, R. Henrion, Optimality conditions in control problems with random state constraints in probabilistic or almost-sure form, arXiv:2306.03965v2, 2024; Math. Oper. Res., 2025. https://arxiv.org/abs/2306.03965
  • F. Clarke, Optimization and Nonsmooth Analysis, Wiley, 1983. https://doi.org/10.1137/1.9781611971309
  • D. Kinderlehrer, G. Stampacchia, An Introduction to Variational Inequalities and Their Applications, Academic Press, 1980 (SIAM reprint 2000). https://doi.org/10.1137/1.9780898719451
  • R. R. Phelps, Lectures on Choquet's Theorem, 2nd ed., Lecture Notes in Mathematics 1757, Springer, 2001. https://doi.org/10.1007/b76887
  • H. W. Alt, Lineare Funktionalanalysis, Springer, 2012. https://doi.org/10.1007/978-3-662-08386-4
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Functional AnalysisOperations ResearchOptimization+1·Captain: mikedeng1

Optimality Conditions in Control Problems with Random State Constraints in Probabilistic or Almost Sure Form III: Absolutely Continuous and Singular Multipliers for Almost Sure State ConstraintsResearch Paper

Motivation

Optimal control of partial differential equations under uncertainty asks for a single deterministic control uuu that performs well when the data of the PDE are random. When a constraint on the state must hold, the modeller has to decide how strictly: with high probability (a probabilistic constraint), for almost every realization (an almost-sure constraint), or for every realization in a support set (a robust constraint). C. Geiersbach and R. Henrion (arXiv:2306.03965v2, Math. Oper. Res. 2025) derive optimality conditions for all three forms on a common model problem. This mission covers §3.1 of that paper, the almost-sure case.

Almost-sure state constraints are the natural model when a bound (a temperature, a stress, a concentration) must never be violated, and they appear throughout risk-averse PDE-constrained optimization (Geiersbach and Wollner, SIAM J. Optim. 2021; Geiersbach and Hintermüller, ESAIM:COCV 2022). Their difficulty is functional-analytic: the constraint lives in LP∞(Ω,C(Dˉ))L^\infty_{\mathbb P}(\Omega,\mathcal C(\bar D))LP∞​(Ω,C(Dˉ)), a space whose dual is not a function space, so Lagrange multipliers are a priori only finitely additive objects.

Setting

Let D⊆RdD\subseteq\mathbb R^dD⊆Rd, d∈{1,2,3}d\in\{1,2,3\}d∈{1,2,3}, be open, bounded and of class S: there are γ∈(0,1)\gamma\in(0,1)γ∈(0,1) and r0>0r_0>0r0​>0 with meas⁡(Br(x)∖D)≥γmeas⁡(Br(x))\operatorname{meas}(B_r(x)\setminus D)\ge\gamma\operatorname{meas}(B_r(x))meas(Br​(x)∖D)≥γmeas(Br​(x)) for all x∈∂Dx\in\partial Dx∈∂D and 0<r<r00<r<r_00<r<r0​. For F∈L2(D)F\in L^2(D)F∈L2(D) the Dirichlet problem −Δy=F-\Delta y=F−Δy=F in DDD, y=0y=0y=0 on ∂D\partial D∂D has a unique weak solution y∈H01(D)∩C(Dˉ)y\in H^1_0(D)\cap\mathcal C(\bar D)y∈H01​(D)∩C(Dˉ); the solution map is a continuous linear operator A−1:L2(D)→C(Dˉ)A^{-1}:L^2(D)\to\mathcal C(\bar D)A−1:L2(D)→C(Dˉ).

Let (Ω,F,P)(\Omega,\mathcal F,\mathbb P)(Ω,F,P) be a probability space and f~∈LP∞(Ω,L2(D))\tilde f\in L^\infty_{\mathbb P}(\Omega,L^2(D))f~​∈LP∞​(Ω,L2(D)) a random source. For a control u∈L2(D)u\in L^2(D)u∈L2(D) the random state y(⋅,ω)y(\cdot,\omega)y(⋅,ω) solves −Δy(⋅,ω)=u+f~(⋅,ω)-\Delta y(\cdot,\omega)=u+\tilde f(\cdot,\omega)−Δy(⋅,ω)=u+f~​(⋅,ω), y(⋅,ω)=0y(\cdot,\omega)=0y(⋅,ω)=0 on ∂D\partial D∂D. With B\mathcal BB the embedding of L2(D)L^2(D)L2(D) into constant elements of LP∞(Ω,L2(D))L^\infty_{\mathbb P}(\Omega,L^2(D))LP∞​(Ω,L2(D)) and [A−1y](ω)=A−1y(⋅,ω)[\mathcal A^{-1}y](\omega)=A^{-1}y(\cdot,\omega)[A−1y](ω)=A−1y(⋅,ω), the control-to-state operator is S(u)=A−1(Bu+f~)\mathcal S(u)=\mathcal A^{-1}(\mathcal Bu+\tilde f)S(u)=A−1(Bu+f~​) and the constraint map is G(u)=S(u)−α\mathcal G(u)=\mathcal S(u)-\boldsymbol\alphaG(u)=S(u)−α, where α\boldsymbol\alphaα is the constant function α∈R\alpha\in\mathbb Rα∈R. The problem is

min⁡u∈L2(D)F(u)s.t.G(u)∈K,(51)\min_{u\in L^2(D)}F(u)\quad\text{s.t.}\quad\mathcal G(u)\in\mathcal K,\qquad(51)u∈L2(D)min​F(u)s.t.G(u)∈K,(51)

with the cone K={y∈LP∞(Ω,C(Dˉ)):y(x,ω)≤0 on Dˉ, P-a.s.}\mathcal K=\{y\in L^\infty_{\mathbb P}(\Omega,\mathcal C(\bar D)):y(x,\omega)\le0\text{ on }\bar D,\ \mathbb P\text{-a.s.}\}K={y∈LP∞​(Ω,C(Dˉ)):y(x,ω)≤0 on Dˉ, P-a.s.} and its polar K−⊆(LP∞(Ω,C(Dˉ)))∗\mathcal K^-\subseteq(L^\infty_{\mathbb P}(\Omega,\mathcal C(\bar D)))^*K−⊆(LP∞​(Ω,C(Dˉ)))∗. The cost FFF is convex and continuously Fréchet differentiable.

For a separable Banach space XXX, a functional v∈(LP∞(Ω,X))∗v\in(L^\infty_{\mathbb P}(\Omega,X))^*v∈(LP∞​(Ω,X))∗ is absolutely continuous if ⟨v,x⟩=∫Ω⟨x∗(ω),x(ω)⟩ dP\langle v,x\rangle=\int_\Omega\langle x^*(\omega),x(\omega)\rangle\,d\mathbb P⟨v,x⟩=∫Ω​⟨x∗(ω),x(ω)⟩dP for a weakly measurable x∗:Ω→X∗x^*:\Omega\to X^*x∗:Ω→X∗ with ∫∥x∗∥ dP<∞\int\|x^*\|\,d\mathbb P<\infty∫∥x∗∥dP<∞ (the set Λ1(X∗)\Lambda_1(X^*)Λ1​(X∗) of such x∗x^*x∗), and singular if it vanishes on every xxx that vanishes on some FnF_nFn​, for a decreasing sequence of events with P(Fn)→0\mathbb P(F_n)\to0P(Fn​)→0 (the set Λ∘(X∗)\Lambda_\circ(X^*)Λ∘​(X∗)).

Formalization targets

Goal: Theorem 3.10

Under the constraint qualification 0∈int⁡{G(L2(D))−K}0\in\operatorname{int}\{\mathcal G(L^2(D))-\mathcal K\}0∈int{G(L2(D))−K}, u∗u^*u∗ solves (51) if and only if there are λ∈Λ1(C(Dˉ)∗)\lambda\in\Lambda_1(\mathcal C(\bar D)^*)λ∈Λ1​(C(Dˉ)∗), λ∘∈Λ∘(C(Dˉ)∗)\lambda^\circ\in\Lambda_\circ(\mathcal C(\bar D)^*)λ∘∈Λ∘​(C(Dˉ)∗) and a state y∗y^*y∗ with

DF(u∗)+E[A−∗λ]+B∗A−∗λ∘=0,Ay∗(⋅,ω)=u∗+f~(⋅,ω),DF(u^*)+\mathbb E[A^{-*}\lambda]+\mathcal B^*\mathcal A^{-*}\lambda^\circ=0,\qquad Ay^*(\cdot,\omega)=u^*+\tilde f(\cdot,\omega),DF(u∗)+E[A−∗λ]+B∗A−∗λ∘=0,Ay∗(⋅,ω)=u∗+f~​(⋅,ω), y∗(⋅,ω)≤α,λ(⋅,ω)≥0,⟨λ(⋅,ω),y∗(⋅,ω)−α⟩=0  P-a.s.,λ∘∈K−,⟨λ∘,y∗−α⟩=0.y^*(\cdot,\omega)\le\alpha,\quad\lambda(\cdot,\omega)\ge0,\quad\langle\lambda(\cdot,\omega),y^*(\cdot,\omega)-\boldsymbol\alpha\rangle=0\ \ \mathbb P\text{-a.s.},\qquad\lambda^\circ\in\mathcal K^-,\quad\langle\lambda^\circ,y^*-\boldsymbol\alpha\rangle=0.y∗(⋅,ω)≤α,λ(⋅,ω)≥0,⟨λ(⋅,ω),y∗(⋅,ω)−α⟩=0  P-a.s.,λ∘∈K−,⟨λ∘,y∗−α⟩=0.

Milestones

  1. Lemma 3.6: the random state exists, is a.s. unique, lies in LP∞(Ω,C(Dˉ))L^\infty_{\mathbb P}(\Omega,\mathcal C(\bar D))LP∞​(Ω,C(Dˉ)), and obeys the bound (52).
  2. Lemma 3.7: the abstract KKT system (53) with a multiplier λ∗∈(LP∞(Ω,C(Dˉ)))∗\lambda^*\in(L^\infty_{\mathbb P}(\Omega,\mathcal C(\bar D)))^*λ∗∈(LP∞​(Ω,C(Dˉ)))∗.
  3. Theorem 3.9 (Ioffe–Levin): every v∗∈(LP∞(Ω,X))∗v^*\in(L^\infty_{\mathbb P}(\Omega,X))^*v∗∈(LP∞​(Ω,X))∗ splits uniquely as va+v∘v^a+v^\circva+v∘ with ∥v∗∥=∥va∥+∥v∘∥\|v^*\|=\|v^a\|+\|v^\circ\|∥v∗∥=∥va∥+∥v∘∥.
  4. The splitting ⟨λ∗,A−1Bh⟩=E[⟨λ,A−1h⟩]+⟨λ∘,A−1Bh⟩\langle\lambda^*,\mathcal A^{-1}\mathcal Bh\rangle=\mathbb E[\langle\lambda,A^{-1}h\rangle]+\langle\lambda^\circ,\mathcal A^{-1}\mathcal Bh\rangle⟨λ∗,A−1Bh⟩=E[⟨λ,A−1h⟩]+⟨λ∘,A−1Bh⟩.
  5. (57): λ∗∈K−\lambda^*\in\mathcal K^-λ∗∈K− passes to both parts.
  6. (59) and pointwise complementarity: λ(ω)≥0\lambda(\omega)\ge0λ(ω)≥0 and ⟨λ(ω),y∗(ω)−α⟩=0\langle\lambda(\omega),y^*(\omega)-\boldsymbol\alpha\rangle=0⟨λ(ω),y∗(ω)−α⟩=0 almost surely.

Significance

The result. Lemma 3.7 gives a multiplier in the dual of L∞L^\inftyL∞, which cannot be evaluated scenario by scenario. Theorem 3.10 shows that, for this problem, the multiplier consists of an honest random variable λ(ω)∈C(Dˉ)∗\lambda(\omega)\in\mathcal C(\bar D)^*λ(ω)∈C(Dˉ)∗ (a random signed measure on Dˉ\bar DDˉ) satisfying sign and complementarity conditions for almost every realization, plus a singular remainder. This is the form needed to write adjoint equations and to design discretizations and algorithms (Proposition 3.12 of the paper). As Remark 3.11 notes, the derivation does not require reflexivity of the state space, unlike earlier work on LP∞(Ω,X)L^\infty_{\mathbb P}(\Omega,X)LP∞​(Ω,X)-constraints.

Formalizing it. The paper's argument is complete, but it rests on two cited results: the regularity theory behind Lemma 1.2/3.6 (Stampacchia-type continuity of weak solutions on class-S domains, Kinderlehrer–Stampacchia) and the Ioffe–Levin decomposition of (LP∞(Ω,X))∗(L^\infty_{\mathbb P}(\Omega,X))^*(LP∞​(Ω,X))∗ (Ioffe–Levin, Appendix 1, Theorem 3, and Levin 1974). Neither is in Mathlib. A formal development produces machine-checked versions of both, of a Robinson-type KKT theorem in Banach spaces, and of the multiplier refinement itself. None of these results has a machine-checked proof as far as the platform's catalog shows.

Difficulty

The obvious route is to apply the Riesz representation pointwise in ω\omegaω. It fails: (LP∞(Ω,C(Dˉ)))∗(L^\infty_{\mathbb P}(\Omega,\mathcal C(\bar D)))^*(LP∞​(Ω,C(Dˉ)))∗ contains purely finitely additive functionals that are not given by any integrand, so λ∗\lambda^*λ∗ has no density in general. The decomposition theorem isolates them, and the proof of Theorem 3.10 must then show that the sign condition λ∗∈K−\lambda^*\in\mathcal K^-λ∗∈K− and the complementarity condition pass to each part separately. The step from E[⟨λ,y⟩]≤0\mathbb E[\langle\lambda,y\rangle]\le0E[⟨λ,y⟩]≤0 for all y∈Ky\in\mathcal Ky∈K to "λ(ω)≥0\lambda(\omega)\ge0λ(ω)≥0 for almost every ω\omegaω, simultaneously for all nonnegative test functions" requires the separability of C(Dˉ)\mathcal C(\bar D)C(Dˉ); a version with a null set depending on the test function is weaker and is not the statement. Lemma 3.6 needs C(Dˉ)\mathcal C(\bar D)C(Dˉ)-regularity of weak solutions, which is where class S and d≤3d\le3d≤3 enter.

Formalization scope

Rd\mathbb R^dRd is EuclideanSpace ℝ (Fin d). L2(D)L^2(D)L2(D) is Lp ℝ 2 (volume.restrict D) and LP∞(Ω,X)L^\infty_{\mathbb P}(\Omega,X)LP∞​(Ω,X) is Lp X ⊤ P; their elements are a.e. classes, so every pointwise statement in ω\omegaω is stated P\mathbb PP-a.s. C(Dˉ)\mathcal C(\bar D)C(Dˉ) is C(closure D, ℝ) with [CompactSpace (closure D)] as an instance argument (implied by boundedness). Weak derivatives use the published HunterPDE.Shared.HasWeakDeriv; a weak solution in H01(D)∩C(Dˉ)H^1_0(D)\cap\mathcal C(\bar D)H01​(D)∩C(Dˉ) is encoded as continuity on Dˉ\bar DDˉ, zero boundary values, L2L^2L2 weak gradient and the weak form. A−1A^{-1}A−1 is a hypothesis: a continuous linear map L2(D)→C(Dˉ)L^2(D)\to\mathcal C(\bar D)L2(D)→C(Dˉ) whose values are weak solutions. "≤0\le0≤0 a.e. in DDD" for a function continuous on Dˉ\bar DDˉ is read as "≤0\le0≤0 on Dˉ\bar DDˉ"; "λ(⋅,ω)≥0\lambda(\cdot,\omega)\ge0λ(⋅,ω)≥0" as positivity of the functional. "Solution of (51)" is a global minimizer. (56a) is stated applied to every direction hhh.

Trivializing formalizations are ruled out: the state operator is tied to the PDE, not an arbitrary bounded operator; the multipliers carry their sign and complementarity conditions; absolutely continuous functionals require a weakly measurable, integrable density; singular functionals are concentrated on a decreasing sequence of events of vanishing probability, not merely "not absolutely continuous"; optimality is global.

Needed infrastructure: Lax–Milgram on H01(D)H^1_0(D)H01​(D) and continuity of weak solutions (Lemma 3.6); a KKT theorem under Robinson's constraint qualification (Lemma 3.7); the Yosida–Hewitt decomposition for finitely additive measures and a weak*-measurable representation of L1(Ω,X)∗L^1(\Omega,X)^*L1(Ω,X)∗ (Theorem 3.9). The decomposition theorem is reusable far beyond this mission; contributions toward any of these are welcome.

Selected references

  • C. Geiersbach, R. Henrion, Optimality conditions in control problems with random state constraints in probabilistic or almost-sure form, arXiv:2306.03965v2, 2024; Math. Oper. Res. 2025. https://arxiv.org/abs/2306.03965
  • A. D. Ioffe, V. L. Levin, Subdifferentials of convex functions, Trudy Moskov. Mat. Obshch. 26, 3–73, 1972 (Appendix 1, Theorem 3).
  • V. L. Levin, The Lebesgue decomposition for functionals on the vector-function space LX∞L^\infty_XLX∞​, Funct. Anal. Appl. 8(4), 314–317, 1974. https://doi.org/10.1007/bf01075488
  • K. Yosida, E. Hewitt, Finitely additive measures, Trans. Amer. Math. Soc. 72, 1952. https://doi.org/10.1090/S0002-9947-1952-0045194-X
  • J. F. Bonnans, A. Shapiro, Perturbation Analysis of Optimization Problems, Springer, 2000. https://doi.org/10.1007/978-1-4612-1394-9
  • C. Geiersbach, W. Wollner, Optimality conditions for convex stochastic optimization problems in Banach spaces with almost sure state constraints, SIAM J. Optim. 31(4), 2455–2480, 2021.
  • C. Geiersbach, M. Hintermüller, Optimality conditions and Moreau–Yosida regularization for almost sure state constraints, ESAIM: COCV 28, Paper No. 80, 2022. https://doi.org/10.1051/cocv/2022070
  • D. Kinderlehrer, G. Stampacchia, An Introduction to Variational Inequalities and Their Applications, Academic Press, 1980 (Chapter II, Appendices B and C). https://doi.org/10.1137/1.9780898719451
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Operations ResearchOptimizationProbability·Captain: mikedeng1

Optimality Conditions in Control Problems with Random State Constraints in Probabilistic or Almost Sure Form II: Explicit Optimality Conditions for Probabilistic Elliptic PDE State ConstraintsResearch Paper

Motivation

Optimal control of partial differential equations under uncertainty arises whenever a physical system is steered by a control while its sources, coefficients or loads are only known in distribution. A typical requirement is a state constraint: the state (a temperature, a concentration, a displacement) must stay below a threshold everywhere in the domain. When the source term is random, demanding this for every realization is often impossible or too conservative, and the natural relaxation is a probabilistic (chance) constraint: the state must stay below the threshold uniformly on the domain with probability at least ppp.

Probabilistic constraints are classical in operations research (Prékopa, Stochastic Programming, 1995), but in a PDE setting the constraint is an infinite family of random inequalities, one per point of the domain, and the probability function is not differentiable in general. C. Geiersbach and R. Henrion (arXiv:2306.03965v2, Math. Oper. Res. 2025) derive optimality conditions for such problems in terms of the Clarke subdifferential, building on the spherical-radial decomposition of Gaussian vectors developed by Hantoute, Henrion and Pérez-Aros (Math. Program. 2019) and van Ackooij and Henrion. This mission formalizes the PDE half of §2 of that paper: explicit formulas for the subdifferential of the probability function and the resulting optimality conditions.

Setting

Let D⊆RdD\subseteq\mathbb R^dD⊆Rd, d∈{1,2,3}d\in\{1,2,3\}d∈{1,2,3}, be a nonempty, open, bounded set of class S: there are γ∈(0,1)\gamma\in(0,1)γ∈(0,1) and r0>0r_0>0r0​>0 with meas⁡(Br(x)∖D)≥γmeas⁡(Br(x))\operatorname{meas}(B_r(x)\setminus D)\ge\gamma\operatorname{meas}(B_r(x))meas(Br​(x)∖D)≥γmeas(Br​(x)) for all x∈∂Dx\in\partial Dx∈∂D and 0<r<r00<r<r_00<r<r0​. For F∈L2(D)F\in L^2(D)F∈L2(D) the Dirichlet problem −Δy=F-\Delta y=F−Δy=F in DDD, y=0y=0y=0 on ∂D\partial D∂D has a unique weak solution in H01(D)∩C(Dˉ)H^1_0(D)\cap C(\bar D)H01​(D)∩C(Dˉ); the solution operator A−1:L2(D)→C(Dˉ)A^{-1}:L^2(D)\to C(\bar D)A−1:L2(D)→C(Dˉ) is linear and continuous.

Fix f0,φ1,…,φm∈L2(D)f_0,\varphi_1,\dots,\varphi_m\in L^2(D)f0​,φ1​,…,φm​∈L2(D) and a threshold α∈R\alpha\in\mathbb Rα∈R. The control-to-state operator is

S(u,z)=A−1(u+f0+∑i=1mziφi)=P(u,z)+y0,P(u,z)=A−1u+∑iziA−1φi, y0=A−1f0.S(u,z)=A^{-1}\Big(u+f_0+\sum_{i=1}^m z_i\varphi_i\Big)=P(u,z)+y_0,\qquad P(u,z)=A^{-1}u+\sum_i z_iA^{-1}\varphi_i,\ y_0=A^{-1}f_0.S(u,z)=A−1(u+f0​+i=1∑m​zi​φi​)=P(u,z)+y0​,P(u,z)=A−1u+i∑​zi​A−1φi​, y0​=A−1f0​.

The random vector ξ\xiξ on a probability space (Ω,F,P)(\Omega,\mathcal F,\mathbb P)(Ω,F,P) is Gaussian N(0,Σ)\mathcal N(0,\Sigma)N(0,Σ) with Σ\SigmaΣ positive definite, and y(⋅,ω)=S(u,ξ(ω))y(\cdot,\omega)=S(u,\xi(\omega))y(⋅,ω)=S(u,ξ(ω)) is the random state. With g(u,z)=max⁡x∈Dˉ[S(u,z)](x)−αg(u,z)=\max_{x\in\bar D}[S(u,z)](x)-\alphag(u,z)=maxx∈Dˉ​[S(u,z)](x)−α and the probability function φ(u)=P(ω∣g(u,ξ(ω))≤0)\varphi(u)=\mathbb P(\omega\mid g(u,\xi(\omega))\le0)φ(u)=P(ω∣g(u,ξ(ω))≤0), the problem is

min⁡u∈L2(D)F(u)s.t.φ(u)=P(y(x,ω)≤α  ∀x∈D)≥p,(24)\min_{u\in L^2(D)}F(u)\quad\text{s.t.}\quad \varphi(u)=\mathbb P\big(y(x,\omega)\le\alpha\ \ \forall x\in D\big)\ge p,\tag{24}u∈L2(D)min​F(u)s.t.φ(u)=P(y(x,ω)≤α  ∀x∈D)≥p,(24)

with FFF convex and Fréchet differentiable and p∈(0,1]p\in(0,1]p∈(0,1].

The analysis uses the spherical-radial decomposition. Let μζ\mu_\zetaμζ​ be the uniform distribution on the unit sphere Sm−1\mathbb S^{m-1}Sm−1, μη\mu_\etaμη​ the chi distribution with mmm degrees of freedom and density χ(t)=Ktm−1e−t2/2\chi(t)=Kt^{m-1}e^{-t^2/2}χ(t)=Ktm−1e−t2/2, Σ1/2\Sigma^{1/2}Σ1/2 the square root of Σ\SigmaΣ. The radial probability function is e(u,v)=μη{r≥0∣g(u,rΣ1/2v)≤0}e(u,v)=\mu_\eta\{r\ge0\mid g(u,r\Sigma^{1/2}v)\le0\}e(u,v)=μη​{r≥0∣g(u,rΣ1/2v)≤0} and the radius function ρ(u,v)∈[0,∞]\rho(u,v)\in[0,\infty]ρ(u,v)∈[0,∞] is the supremum of that set. For x∈Dˉx\in\bar Dx∈Dˉ, ux∈L2(D)u_x\in L^2(D)ux​∈L2(D) is defined by (ux,h)L2(D)=(A−1h)(x)(u_x,h)_{L^2(D)}=(A^{-1}h)(x)(ux​,h)L2(D)​=(A−1h)(x), and

M∗(uˉ,v)={x∈Dˉ∣[P(0,Σ1/2v)](x)>0, yˉ(x)+ρ(uˉ,v)[P(0,Σ1/2v)](x)=α},yˉ=S(uˉ,0).M^*(\bar u,v)=\{x\in\bar D\mid[P(0,\Sigma^{1/2}v)](x)>0,\ \bar y(x)+\rho(\bar u,v)[P(0,\Sigma^{1/2}v)](x)=\alpha\},\qquad \bar y=S(\bar u,0).M∗(uˉ,v)={x∈Dˉ∣[P(0,Σ1/2v)](x)>0, yˉ​(x)+ρ(uˉ,v)[P(0,Σ1/2v)](x)=α},yˉ​=S(uˉ,0).

∂C\partial^C∂C is the Clarke subdifferential, with L2(D)∗L^2(D)^*L2(D)∗ identified with L2(D)L^2(D)L2(D), and integrals of set-valued maps are Aumann integrals.

Formalization targets

Goal: Theorem 2.16

Assume a control u^\hat uu^ with φ(u^)>p\varphi(\hat u)>pφ(u^)>p (41), and let u∗u^*u∗ be feasible with expected state y~=S(u∗,0)\tilde y=S(u^*,0)y~​=S(u∗,0) satisfying y~(x)<α\tilde y(x)<\alphay~​(x)<α on Dˉ\bar DDˉ (42). If u∗u^*u∗ solves (24), there is λ≥0\lambda\ge0λ≥0 with

DF(u∗)∈−λ∫{v∣ρ(u∗,v)<∞}χ(ρ(u∗,v))⋅clco⁡{ux[P(0,Σ1/2v)](x) ∣ x∈M∗(u∗,v)} dμζ(v),DF(u^*)\in-\lambda\int_{\{v\mid\rho(u^*,v)<\infty\}}\chi(\rho(u^*,v))\cdot\operatorname{clco}\Big\{\frac{u_x}{[P(0,\Sigma^{1/2}v)](x)}\ \Big|\ x\in M^*(u^*,v)\Big\}\,d\mu_\zeta(v),DF(u∗)∈−λ∫{v∣ρ(u∗,v)<∞}​χ(ρ(u∗,v))⋅clco{[P(0,Σ1/2v)](x)ux​​ ​ x∈M∗(u∗,v)}dμζ​(v), λ(P(y∗(x,ω)≤α ∀x∈D)−p)=0,\lambda\big(\mathbb P(y^*(x,\omega)\le\alpha\ \forall x\in D)-p\big)=0,λ(P(y∗(x,ω)≤α ∀x∈D)−p)=0,

and these conditions are sufficient when M∗(u∗,v)M^*(u^*,v)M∗(u∗,v) is a singleton for μζ\mu_\zetaμζ​-a.e. vvv with ρ(u∗,v)<∞\rho(u^*,v)<\inftyρ(u∗,v)<∞, or the set {z∣g(u∗,z)≤0}\{z\mid g(u^*,z)\le0\}{z∣g(u∗,z)≤0} is bounded. The goal has no hard-coded constants; it asserts the form of the optimality system.

Milestones

In attack order: well-posedness of the state equation with the bound ∥y^∥C(Dˉ)≤C(∥z∥2+∥u+f0∥L2(D))\|\hat y\|_{C(\bar D)}\le C(\|z\|_2+\|u+f_0\|_{L^2(D)})∥y^​∥C(Dˉ)​≤C(∥z∥2​+∥u+f0​∥L2(D)​) (Lemma 1.2); measurability of the random state (Lemma 1.4); convexity and global Lipschitz continuity of ggg (Lemma 2.9); moderate growth (Lemma 2.10); the Lipschitz and subdifferential conclusions of the general theory under (26) (Corollary 2.11); the optimality conditions (21), (22) for (24) (Corollary 2.12); ∂uCe(uˉ,v)={0}\partial^C_ue(\bar u,v)=\{0\}∂uC​e(uˉ,v)={0} when ρ(uˉ,v)=∞\rho(\bar u,v)=\inftyρ(uˉ,v)=∞ (Lemma 2.13); the explicit formula ∂uCe(uˉ,v)=−χ(ρ(uˉ,v))⋅clco⁡{ux/[P(0,Σ1/2v)](x)∣x∈M∗(uˉ,v)}\partial^C_ue(\bar u,v)=-\chi(\rho(\bar u,v))\cdot\operatorname{clco}\{u_x/[P(0,\Sigma^{1/2}v)](x)\mid x\in M^*(\bar u,v)\}∂uC​e(uˉ,v)=−χ(ρ(uˉ,v))⋅clco{ux​/[P(0,Σ1/2v)](x)∣x∈M∗(uˉ,v)} when ρ(uˉ,v)<∞\rho(\bar u,v)<\inftyρ(uˉ,v)<∞ (Lemma 2.14); and the upper estimate (40) of ∂Cφ(uˉ)\partial^C\varphi(\bar u)∂Cφ(uˉ) with its equality cases (Theorem 2.15).

Significance

The result turns an abstract statement — DF(u∗)DF(u^*)DF(u∗) lies in a multiple of the Clarke subdifferential of a probability function that has no closed form — into a condition written in the problem data: Green-type functions uxu_xux​, the expected state, and the radius function along each direction of the sphere. This is what makes the conditions usable for checking candidate controls and for designing algorithms, and Example 2.18 of the paper computes a solution this way. The sufficiency half identifies when the nonconvex chance-constrained problem behaves like a convex one.

The paper's proofs are on paper only; to our knowledge none of these results, nor the spherical-radial decomposition, Clarke calculus in Hilbert spaces, or Aumann integrals in L2L^2L2, has a machine-checked proof. Formalizing Theorem 2.16 requires connecting elliptic regularity, Gaussian measure theory and nonsmooth analysis, and the milestones are reusable on their own: Lemma 1.2 is a regularity statement for the Poisson equation, and Lemmas 2.13 and 2.14 are max-function subdifferential formulas in an infinite-dimensional space.

Difficulty

The obvious route — differentiate φ\varphiφ and use a Lagrange multiplier — fails because φ\varphiφ is generally not differentiable even for smooth data (Example 2.17 of the paper), and because ggg is only Lipschitz, being a maximum over Dˉ\bar DDˉ. The general subdifferential estimate (Theorem 2.2, from Hantoute–Henrion–Pérez-Aros) needs a growth condition and only gives an inclusion, since the radial probability function is not Clarke regular; the radius function ρ(⋅,v)\rho(\cdot,v)ρ(⋅,v) is an infimum over the open set where P(0,Σ1/2v)>0P(0,\Sigma^{1/2}v)>0P(0,Σ1/2v)>0, which is neither compact nor independent of uuu, so standard max-function formulas do not apply directly. Directions with ρ=∞\rho=\inftyρ=∞ require a separate limiting argument through the Mordukhovich subdifferential (Lemma 2.13). The regularity input, continuity of solutions on Dˉ\bar DDˉ for class-S domains (Kinderlehrer–Stampacchia 1980), is not in Mathlib.

Formalization scope

All declarations are in the namespace ChanceStateCtrl.PDE. Rd\mathbb R^dRd and Rm\mathbb R^mRm are EuclideanSpace ℝ (Fin d) and EuclideanSpace ℝ (Fin m), indices are Fin m, L2(D)L^2(D)L2(D) is Lp ℝ 2 (volume.restrict D). Weak derivatives are the published HunterPDE.Shared.HasWeakDeriv; a weak solution is a function continuous on Dˉ\bar DDˉ, zero on ∂D\partial D∂D, in L2(D)L^2(D)L2(D) with weak first derivatives in L2(D)L^2(D)L2(D), satisfying the weak form against Cc∞(D)C_c^\infty(D)Cc∞​(D).

Standing hypotheses on every theorem: DDD open, bounded and nonempty, d∈{1,2,3}d\in\{1,2,3\}d∈{1,2,3}, class S, and CompactSpace (closure D) (a consequence of boundedness). Nonemptiness of DDD is the one added hypothesis: Lean's supremum over an empty domain is 000, not −∞-\infty−∞, and Lemma 2.9's identification of events fails for D=∅D=\emptysetD=∅. A−1A^{-1}A−1 is a continuous linear map to C(Dˉ)C(\bar D)C(Dˉ) together with the hypothesis that it returns the weak solution; it is never an arbitrary operator. m≥1m\ge1m≥1, as the uniform distribution on Sm−1\mathbb S^{m-1}Sm−1 requires. Σ1/2\Sigma^{1/2}Σ1/2 is the positive semidefinite root; ∥Σ1/2∥\|\Sigma^{1/2}\|∥Σ1/2∥ is its operator norm. The Clarke directional derivative is lim sup⁡u′→u,t↓0(f(u′+th)−f(u′))/t\limsup_{u'\to u,t\downarrow0}(f(u'+th)-f(u'))/tlimsupu′→u,t↓0​(f(u′+th)−f(u′))/t (the page's denominator hhh is a misprint). ρ\rhoρ takes values in [0,∞][0,\infty][0,∞]. clco is the norm closure of the convex hull. The integral in (40)/(43) is over the restriction of μζ\mu_\zetaμζ​ to {ρ<∞}\{\rho<\infty\}{ρ<∞}, not a renormalization. A solution is a global minimizer over {u∣φ(u)≥p}\{u\mid\varphi(u)\ge p\}{u∣φ(u)≥p}; the page's "solution to (9)" refers to this instance of the abstract problem (9).

Trivializing formalizations are ruled out: every Clarke subdifferential is taken at a point where the function is locally Lipschitz (proved in Corollary 2.11 and Theorem 2.15), the state operator is tied to the PDE, the multiplier carries its sign and complementarity, Aumann selections must be scalarly integrable, and optimality is global.

Needed infrastructure: elliptic regularity in C(Dˉ)C(\bar D)C(Dˉ) for class-S domains; the spherical-radial decomposition of N(0,Σ)\mathcal N(0,\Sigma)N(0,Σ); Clarke calculus (chain rule, max functions) on Hilbert spaces; Clarke's theorem on subdifferentials of integral functionals. Contributions of any of these as stand-alone theorems are welcome.

Selected references

  • C. Geiersbach, R. Henrion, Optimality conditions in control problems with random state constraints in probabilistic or almost-sure form, arXiv:2306.03965v2, 2024; Math. Oper. Res., 2025. https://arxiv.org/abs/2306.03965
  • A. Hantoute, R. Henrion, P. Pérez-Aros, Subdifferential characterization of probability functions under Gaussian distribution, Math. Program. 174 (2019), 167–194. https://doi.org/10.1007/s10107-018-1237-9
  • F. H. Clarke, Optimization and Nonsmooth Analysis, Wiley, 1983; SIAM reprint 1990. https://doi.org/10.1137/1.9781611971309
  • D. Kinderlehrer, G. Stampacchia, An Introduction to Variational Inequalities and Their Applications, Academic Press, 1980; SIAM reprint 2000. https://doi.org/10.1137/1.9780898719451
  • A. Prékopa, Stochastic Programming, Kluwer, 1995. https://doi.org/10.1007/978-94-017-3087-7
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Mathematical PhysicsProbabilityStochastic Systems·Captain: mikedeng1

Global-in-Time Mean-Field Convergence for Singular Riesz-Type Diffusive Flows 2: A Uniform-in-Time Modulated-Energy Bound for Globally Superharmonic Riesz-Type PotentialsResearch Paper

Motivation

Systems of many particles that interact through a singular pair potential and are subject to independent noise appear in plasma physics (Coulomb interactions), in vortex models of fluids, in models of collective behaviour and in the analysis of training dynamics of wide neural networks. When the number of particles NNN is large, the empirical measure of the system is expected to follow a deterministic nonlinear partial differential equation, the mean-field limit. For singular interactions the classical coupling arguments, which need Lipschitz forces, do not apply. The modulated-energy method of Serfaty (Duke Math. J. 2020) and its extensions by Duerinckx, Nguyen, Rosenzweig and Serfaty (NRS21, arXiv:2107.02592) give quantitative convergence for Riesz-type potentials ∣x∣−s|x|^{-s}∣x∣−s, but with rates that degrade exponentially in time.

M. Rosenzweig and S. Serfaty (arXiv:2108.09878v1, 2021) show that additive noise improves this: the expected modulated energy grows at most polynomially in time for sub-Coulombic potentials (their Theorem 1.1, the subject of the first mission of this series), and stays bounded uniformly in time when the potential is globally superharmonic (their Theorem 1.2, the subject of this mission). Uniform-in-time propagation of chaos had been known for smooth or convex interactions; this result covers singular, non-gradient interactions on the whole space.

Setting

Fix d≥3d\ge3d≥3, an exponent 0≤s<d−20\le s<d-20≤s<d−2, a diffusion strength σ>0\sigma>0σ>0 and a d×dd\times dd×d matrix M\mathbb MM with Mξ⋅ξ≤0\mathbb M\xi\cdot\xi\le0Mξ⋅ξ≤0 for all ξ\xiξ. The particle system is

dxit=1N∑j≠iM∇g(xit−xjt) dt+2σ dWit,i=1,…,N,dx^t_i=\frac1N\sum_{j\ne i}\mathbb M\nabla\mathsf g(x^t_i-x^t_j)\,dt+\sqrt{2\sigma}\,dW^t_i,\qquad i=1,\dots,N,dxit​=N1​j=i∑​M∇g(xit​−xjt​)dt+2σ​dWit​,i=1,…,N,

started from pairwise distinct points xN0=(x10,…,xN0)x^0_N=(x^0_1,\dots,x^0_N)xN0​=(x10​,…,xN0​) and driven by independent standard Brownian motions W1,…,WNW_1,\dots,W_NW1​,…,WN​ in Rd\mathbb R^dRd. The potential g\mathsf gg is admissible: it satisfies ten assumptions (i)–(x) on symmetry, blow-up at 000, superharmonicity near 000, derivative bounds of order ∣x∣−s−k|x|^{-s-k}∣x∣−s−k, a doubling property, a Fourier transform comparable to ∣ξ∣−(d−s)|\xi|^{-(d-s)}∣ξ∣−(d−s), an extension to Rd+m\mathbb R^{d+m}Rd+m when d−4<sd-4<sd−4<s, a Calderón–Zygmund property in the cases s=d−2ks=d-2ks=d−2k, and M:∇⊗2g≥0\mathbb M:\nabla^{\otimes2}\mathsf g\ge0M:∇⊗2g≥0. The model case is g(x)=∣x∣−s\mathsf g(x)=|x|^{-s}g(x)=∣x∣−s.

The mean-field equation is

∂tμ=−div⁡(μ M∇g∗μ)+σΔμ,μ∣t=0=μ0,\partial_t\mu=-\operatorname{div}(\mu\,\mathbb M\nabla\mathsf g*\mu)+\sigma\Delta\mu,\qquad\mu|_{t=0}=\mu^0,∂t​μ=−div(μM∇g∗μ)+σΔμ,μ∣t=0​=μ0,

for a probability density μ0∈L∞\mu^0\in L^\inftyμ0∈L∞, solved in the mild (Duhamel) sense in C([0,∞);L1∩L∞)C([0,\infty);L^1\cap L^\infty)C([0,∞);L1∩L∞). Closeness of the empirical measure μNt=1N∑iδxit\mu_N^t=\frac1N\sum_i\delta_{x^t_i}μNt​=N1​∑i​δxit​​ to μt\mu^tμt is measured by the modulated energy

FN(xN,μ)=∫(Rd)2∖△g(x−y) d(1N∑i=1Nδxi−μ)⊗2(x,y),F_N(x_N,\mu)=\int_{(\mathbb R^d)^2\setminus\triangle}\mathsf g(x-y)\,d\Big(\frac1N\sum_{i=1}^N\delta_{x_i}-\mu\Big)^{\otimes2}(x,y),FN​(xN​,μ)=∫(Rd)2∖△​g(x−y)d(N1​i=1∑N​δxi​​−μ)⊗2(x,y),

where the diagonal △\triangle△ is removed. The potential is globally superharmonic if Δg≤0\Delta\mathsf g\le0Δg≤0 on all of Rd∖{0}\mathbb R^d\setminus\{0\}Rd∖{0} ("r0=∞r_0=\inftyr0​=∞" in assumption (iii)).

Formalization targets

Goal: Theorem 1.2 for 0<s<d−20<s<d-20<s<d−2

For globally superharmonic admissible g\mathsf gg and every d/(s+2)<p≤∞d/(s+2)<p\le\inftyd/(s+2)<p≤∞ there are βp>0\beta_p>0βp​>0 (depending on s,d,ps,d,ps,d,p), C>0C>0C>0 (depending on s,d,σ,M,g,∥μ0∥L∞s,d,\sigma,\mathbb M,\mathsf g,\|\mu^0\|_{L^\infty}s,d,σ,M,g,∥μ0∥L∞​), Cp>0C_p>0Cp​>0 and N0N_0N0​ such that for all t≥0t\ge0t≥0 and N≥N0N\ge N_0N≥N0​,

E(∣FN(xNt,μt)∣)≤C(∣FN(xN0,μ0)∣+CpN−βp).\mathbb E\big(|F_N(x^t_N,\mu^t)|\big)\le C\big(|F_N(x^0_N,\mu^0)|+C_pN^{-\beta_p}\big).E(∣FN​(xNt​,μt)∣)≤C(∣FN​(xN0​,μ0)∣+Cp​N−βp​).

The right side does not depend on ttt. The case s=0s=0s=0 of the paper's display (1.19) is not part of the goal (see Formalization scope).

Milestones

The proof combines an inequality for the time derivative of the expected modulated energy (Proposition 6.3), lower bounds for the energy and for the diffusion term (Remarks 5.10, 5.11, Proposition 5.12, Remark 5.13, Corollary 5.14), a commutator estimate for the transport term (Proposition 5.15), and decay of ∥μt∥Lp\|\mu^t\|_{L^p}∥μt∥Lp​ (Remark 3.4, Proposition 3.8), with the potential estimates of Lemma 2.3 and Remark 2.5.

Significance

A uniform-in-time bound means that the mean-field description is valid on time scales that do not shrink as the accuracy requirement grows. Combined with the control of negative Sobolev norms by the modulated energy, it yields uniform-in-time convergence in law of the empirical measure and, for chaotic initial data, uniform-in-time propagation of chaos at an explicit rate, for singular interactions such as sub-Coulombic Riesz gases with dissipative or conservative dynamics.

The result is proved in the paper. No part of it, nor of the modulated-energy method, is formalized in any proof assistant. A formalization would produce a reusable library: Riesz potentials and their L1L^1L1–LpL^pLp interpolation, heat-type decay of nonlinear Fokker–Planck equations, smeared potentials and electric-energy lower bounds, renormalized commutator estimates, and a pathwise treatment of interacting diffusions with additive noise. The milestones are independent statements and can be proved separately.

Difficulty

The obvious Gronwall argument on the modulated energy fails twice. First, FNF_NFN​ is not nonnegative; it is bounded below only up to errors involving ∥μ∥L∞\|\mu\|_{L^\infty}∥μ∥L∞​, and the lower bounds near the singularity need the smearing of point charges on spheres. Second, the error terms produced when the commutator and diffusion terms are bounded must be integrable on [0,∞)[0,\infty)[0,∞); with the estimates of the general (local superharmonicity) case they grow linearly in time. Global superharmonicity removes an η2\eta^2η2 error term and lets every error carry a power of ∥μt∥L∞\|\mu^t\|_{L^\infty}∥μt∥L∞​, which decays like (σt)−d/2(\sigma t)^{-d/2}(σt)−d/2 by the Carlen–Loss method; for s=0s=0s=0 long-range effects still produce growth, which is why that case is excluded. Itô's formula cannot be applied directly to the singular energy and requires a truncation, whose stochastic integrals are removed in expectation only in the limit.

Formalization scope

All objects live in the Lean namespace RieszMF.Global and in one definitions module. Space is EuclideanSpace ℝ (Fin d); derivatives are iteratedFDeriv (operator norm), gradient and the Laplacian of Mathlib. The committed conventions:

  1. Fourier conditions (vi) and (1.17) are read away from the origin: a function g^\hat{\mathsf g}g^​ with ∫g Fφ=∫g^φ\int\mathsf g\,\mathcal F\varphi=\int\hat{\mathsf g}\varphi∫gFφ=∫g^​φ for Schwartz φ\varphiφ vanishing near 000.
  2. Assumption (iv) has a constant CkC_kCk​ for each kkk; quantities singular at 000 are required for x≠0x\neq0x=0 only; (ix) is stated componentwise with an L2L^2L2-bounded operator represented by the kernel off the support.
  3. Global superharmonicity is Δg≤0\Delta\mathsf g\le0Δg≤0 on Rd∖{0}\mathbb R^d\setminus\{0\}Rd∖{0}, together with (1.15)–(1.16) on all of Rd+m∖{0}\mathbb R^{d+m}\setminus\{0\}Rd+m∖{0} when d−4<sd-4<sd−4<s; (v) and (vii) keep a finite radius.
  4. Doubling condition (vii) for s>0s>0s>0 is read as g(y)<csg(x)\mathsf g(y)<c_s\mathsf g(x)g(y)<cs​g(x) whenever ∣y∣≥2∣x∣|y|\ge2|x|∣y∣≥2∣x∣, x≠0x\ne0x=0, with cs<1c_s<1cs​<1. The page prints g(x)<csg(y)\mathsf g(x)<c_s\mathsf g(y)g(x)<cs​g(y), which contradicts the blow-up (ii) and would leave no admissible potential, so the goal would hold vacuously. The model potential ∣x∣−s|x|^{-s}∣x∣−s satisfies the reading used here.
  5. The particle system is the pathwise integral equation (no Itô integral is needed for additive noise), with continuous paths and no collisions almost surely; the Brownian family is N⋅dN\cdot dN⋅d jointly independent standard real Brownian motions.
  6. The mild formulation of (1.5) requires every integral to converge absolutely and continuity in L1∩L∞L^1\cap L^\inftyL1∩L∞.
  7. Expectations of ∣FN∣|F_N|∣FN​∣ are lower Lebesgue integrals, and Proposition 6.3 moves positive and negative parts across the inequality, so no integrability is presupposed and no ∞−∞\infty-\infty∞−∞ arises.
  8. Constants are quantified after exactly the objects they may depend on: βp\beta_pβp​ after s,d,ps,d,ps,d,p; CCC after σ,M,g\sigma,\mathbb M,\mathsf gσ,M,g and ∥μ0∥L∞\|\mu^0\|_{L^\infty}∥μ0∥L∞​; CpC_pCp​ and N0N_0N0​ after ppp; all before μ0\mu^0μ0, NNN, the configuration, the probability space and ttt.

Restriction. The goal is Theorem 1.2 for 0<s<d−20<s<d-20<s<d−2 only, where the paper's time factor 1+(t1/σlog⁡(1+t))1s=01+(t^{1/\sigma}\log(1+t))\mathbf 1_{s=0}1+(t1/σlog(1+t))1s=0​ equals 111. For s=0s=0s=0 the proof yields a factor of order tC/σt^{C/\sigma}tC/σ rather than the printed t1/σlog⁡(1+t)t^{1/\sigma}\log(1+t)t1/σlog(1+t); the logarithmic case is covered by the first mission of this series.

Excluded trivializations. A statement in which CCC is chosen after μ0\mu^0μ0, NNN or the configuration, in which a divergent integral is read as 000, in which the solution classes are empty, or which uses N=0N=0N=0 or a division by zero is not a formalization of the theorem; the statements here avoid each of these.

Contributions are welcome on any milestone, on the existence of solutions in the classes used (which shows the hypotheses are satisfiable), and on general infrastructure (Riesz potentials, sphere averages, heat-kernel estimates) that other missions can reuse.

Selected references

  • M. Rosenzweig, S. Serfaty, Global-in-time mean-field convergence for singular Riesz-type diffusive flows, arXiv:2108.09878v1, 2021; Ann. Appl. Probab. 33(2), 2023. https://arxiv.org/abs/2108.09878
  • Q.-H. Nguyen, M. Rosenzweig, S. Serfaty, Mean-field limits of Riesz-type singular flows, Ars Inveniendi Analytica, 2022. https://arxiv.org/abs/2107.02592
  • S. Serfaty, Mean field limit for Coulomb-type flows, Duke Math. J. 169(15), 2020. https://doi.org/10.1215/00127094-2020-0019
  • M. Duerinckx, Mean-field limits for some Riesz interaction gradient flows, SIAM J. Math. Anal. 48(3), 2016. https://doi.org/10.1137/15M1042620
  • E. A. Carlen, M. Loss, Optimal smoothing and decay estimates for viscously damped conservation laws, with applications to the 2-D Navier–Stokes equation, Duke Math. J. 81(1), 1995. https://doi.org/10.1215/S0012-7094-95-08110-1
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Mathematical PhysicsProbabilityStochastic Systems·Captain: mikedeng1

Global-in-Time Mean-Field Convergence for Singular Riesz-Type Diffusive Flows 1: The Expected Modulated Energy Grows at Most Polynomially in TimeResearch Paper

Motivation

Systems of NNN particles that interact through a singular pair potential and are driven by independent noise are used to model vortices in viscous fluids, collective motion of micro-organisms, aggregation phenomena and, more recently, the training dynamics of wide neural networks and stochastic gradient methods. When NNN is large, one expects the empirical measure of the particles to be close to the solution of a deterministic nonlinear PDE, the mean-field limit. Proving this with an explicit rate is difficult when the interaction is singular, because the classical coupling arguments need a Lipschitz force.

The modulated-energy method (Duerinckx 2016, Serfaty 2020, Nguyen–Rosenzweig–Serfaty 2021) measures the distance between the particles and the limit through a renormalized Coulomb/Riesz energy and closes a Gronwall argument on it. Rosenzweig and Serfaty (arXiv:2108.09878) extended it to systems with additive noise in the sub-Coulombic range. This mission formalizes their first main result, Theorem 1.1: the expected modulated energy grows at most linearly in time (polynomially for logarithmic interactions). A companion mission covers their uniform-in-time Theorem 1.2.

Setting

Fix d≥3d\ge3d≥3 and 0≤s<d−20\le s<d-20≤s<d−2. Positions live in Rd\mathbb R^dRd with Lebesgue measure. A d×dd\times dd×d real matrix M\mathbb MM satisfies Mξ⋅ξ≤0\mathbb M\xi\cdot\xi\le0Mξ⋅ξ≤0 for all ξ\xiξ (gradient flows M=−I\mathbb M=-\mathbb IM=−I, Hamiltonian flows M\mathbb MM antisymmetric, and mixtures). The interaction potential g:Rd→R\mathsf g:\mathbb R^d\to\mathbb Rg:Rd→R is admissible: it satisfies ten assumptions (i)–(x), with model cases g(x)=−log⁡∣x∣\mathsf g(x)=-\log|x|g(x)=−log∣x∣ (s=0s=0s=0) and g(x)=∣x∣−s\mathsf g(x)=|x|^{-s}g(x)=∣x∣−s (0<s<d−20<s<d-20<s<d−2). In short: g\mathsf gg is even, blows up at 000, is superharmonic on a punctured ball B(0,r0)∖{0}B(0,r_0)\setminus\{0\}B(0,r0​)∖{0}, is smooth off the origin with ∣∇⊗kg(x)∣≤Ck∣x∣−(s+k)|\nabla^{\otimes k}\mathsf g(x)|\le C_k|x|^{-(s+k)}∣∇⊗kg(x)∣≤Ck​∣x∣−(s+k) (plus a logarithm when s=k=0s=k=0s=k=0), has a Fourier transform comparable to ∣ξ∣s−d|\xi|^{s-d}∣ξ∣s−d, has a doubling property near 000, admits a superharmonic extension to Rd+m\mathbb R^{d+m}Rd+m when d−4<sd-4<sd−4<s, has a Calderón–Zygmund kernel condition when s=d−2ks=d-2ks=d−2k, and satisfies M:∇⊗2g≥0\mathbb M:\nabla^{\otimes2}\mathsf g\ge0M:∇⊗2g≥0.

The particle system (1.1) is

dxit=1N∑j≠iM∇g(xit−xjt) dt+2σ dWit,xit∣t=0=xi0,dx^t_i=\frac1N\sum_{j\ne i}\mathbb M\nabla\mathsf g(x^t_i-x^t_j)\,dt+\sqrt{2\sigma}\,dW^t_i,\qquad x^t_i|_{t=0}=x^0_i,dxit​=N1​j=i∑​M∇g(xit​−xjt​)dt+2σ​dWit​,xit​∣t=0​=xi0​,

with distinct initial points, σ>0\sigma>0σ>0, and W1,…,WNW_1,\dots,W_NW1​,…,WN​ independent standard Brownian motions in Rd\mathbb R^dRd. The mean-field equation (1.5) is

∂tμ=−div⁡(μ M∇g∗μ)+σΔμ,μ∣t=0=μ0,\partial_t\mu=-\operatorname{div}(\mu\,\mathbb M\nabla\mathsf g*\mu)+\sigma\Delta\mu,\qquad\mu|_{t=0}=\mu^0,∂t​μ=−div(μM∇g∗μ)+σΔμ,μ∣t=0​=μ0,

for a bounded probability density μ0\mu^0μ0, solved in the class C([0,∞);P(Rd)∩L∞(Rd))C([0,\infty);\mathcal P(\mathbb R^d)\cap L^\infty(\mathbb R^d))C([0,∞);P(Rd)∩L∞(Rd)). The modulated energy (1.6) is

FN(xN,μ)=∫(Rd)2∖△g(x−y) d(1N∑i=1Nδxi−μ)⊗2(x,y),F_N(x_N,\mu)=\int_{(\mathbb R^d)^2\setminus\triangle}\mathsf g(x-y)\,d\Big(\frac1N\sum_{i=1}^N\delta_{x_i}-\mu\Big)^{\otimes2}(x,y),FN​(xN​,μ)=∫(Rd)2∖△​g(x−y)d(N1​i=1∑N​δxi​​−μ)⊗2(x,y),

the diagonal △\triangle△ being removed to discard the infinite self-interaction of each particle.

Formalization targets

Goal: Theorem 1.1

There are β>0\beta>0β>0 depending on s,ds,ds,d only and, for every σ\sigmaσ, M\mathbb MM, admissible g\mathsf gg and value of ∥μ0∥L∞\|\mu^0\|_{L^\infty}∥μ0∥L∞​, a constant C>0C>0C>0 and a threshold N0N_0N0​ such that for all N≥N0N\ge N_0N≥N0​ and t≥0t\ge0t≥0

E(∣FN(xNt,μt)∣)≤C(1+t+tσ+Cσ1s=0)(∣FN(xN0,μ0)∣+N−β).\mathbb E\big(|F_N(x^t_N,\mu^t)|\big)\le C\Big(1+t+t^{\frac{\sigma+C}\sigma}\mathbf 1_{s=0}\Big)\Big(|F_N(x^0_N,\mu^0)|+N^{-\beta}\Big).E(∣FN​(xNt​,μt)∣)≤C(1+t+tσσ+C​1s=0​)(∣FN​(xN0​,μ0)∣+N−β).

The exponent β\betaβ and the constant are left unspecified, as in the paper.

Milestones

In the order the proof uses them:

  1. Lemma 2.3 and Remark 2.5: L∞L^\inftyL∞ bounds for Riesz potentials and for ∇⊗kg∗f\nabla^{\otimes k}\mathsf g*f∇⊗kg∗f.
  2. Remark 3.4, Proposition 3.9 and Proposition 3.8: LpL^pLp monotonicity, the sharp log-Sobolev inequality, and heat-equation decay ∥μt∥Lq≲(σt)−d2(1p−1q)∥μ0∥Lp\|\mu^t\|_{L^q}\lesssim(\sigma t)^{-\frac d2(\frac1p-\frac1q)}\|\mu^0\|_{L^p}∥μt∥Lq​≲(σt)−2d​(p1​−q1​)∥μ0∥Lp​.
  3. Proposition 4.5: the particle system has a unique strong solution whose particles never collide, obtained as the limit of smoothly truncated systems.
  4. Remarks 5.2, 5.3 and Proposition 5.4: lower bounds on FNF_NFN​ through smeared point charges.
  5. Corollary 5.6: the diffusion term ∬(−Δg) d(μN−μ)⊗2\iint(-\Delta\mathsf g)\,d(\mu_N-\mu)^{\otimes2}∬(−Δg)d(μN​−μ)⊗2 is bounded below by −C(1+∥μ∥L∞)N−min⁡{2,d−s−2}/min⁡{s+4,d}-C(1+\|\mu\|_{L^\infty})N^{-\min\{2,d-s-2\}/\min\{s+4,d\}}−C(1+∥μ∥L∞​)N−min{2,d−s−2}/min{s+4,d}.
  6. Proposition 5.7: the renormalized commutator estimate.
  7. Proposition 6.3: the expected Itô inequality for FNF_NFN​.

Significance

The theorem is a quantitative mean-field limit for singular interactions with additive noise on the whole space, covering conservative and dissipative dynamics at once. Since FNF_NFN​ controls a negative-order Sobolev distance between μNt\mu_N^tμNt​ and μt\mu^tμt, it gives convergence of the empirical measure, at a rate in NNN that deteriorates at most linearly in ttt for s>0s>0s>0. Its proof isolates estimates (the LpL^pLp decay of the nonlinear equation, the sign of the diffusion term, the commutator bound) that are reused for the uniform-in-time result of the companion mission.

The paper's results are proved; none of them has a machine-checked proof. Formalizing the theorem requires the modulated-energy machinery (smeared charges, Fourier positivity, commutator estimates), a Carlen–Loss decay argument, and an Itô-free treatment of the stochastic system. The milestones of §§2–3 are classical harmonic analysis (Riesz potentials, the Gross–Carlen log-Sobolev inequality) and are of independent use.

Difficulty

A direct Gronwall argument on E∣FN∣\mathbb E|F_N|E∣FN​∣ fails twice. The diffusion term σ∬Δg d(μN−μ)⊗2\sigma\iint\Delta\mathsf g\,d(\mu_N-\mu)^{\otimes2}σ∬Δgd(μN​−μ)⊗2 has no sign for a general configuration, because the singularity of Δg\Delta\mathsf gΔg at the origin is integrated against a signed measure with atoms; its control needs a second modulated-energy estimate for −Δg-\Delta\mathsf g−Δg, which is a potential of order s+2s+2s+2 and may be super-Coulombic, hence the extension of assumption (viii). The commutator term requires ∥∇ut∥L∞\|\nabla u^t\|_{L^\infty}∥∇ut∥L∞​, and bounding it by ∥μ0∥L∞\|\mu^0\|_{L^\infty}∥μ0∥L∞​ alone produces exponential growth in time; the polynomial bound needs the time decay of ∥μt∥L∞\|\mu^t\|_{L^\infty}∥μt∥L∞​, which for a nonlinear, non-divergence-free drift is not given by comparison with the heat equation. Finally, the Itô computation for FNF_NFN​ along the singular dynamics needs truncation and stopping times, since g\mathsf gg is not C2C^2C2 at collisions.

Formalization scope

All objects are defined in one module RieszMF.Linear.Setting. Space is EuclideanSpace ℝ (Fin d) with Lebesgue measure; derivatives are iteratedFDeriv with operator norms, Δ\DeltaΔ is Mathlib's Laplacian, and the Fourier transform is Mathlib's ∫e−2πix⋅ξφ(x) dx\int e^{-2\pi ix\cdot\xi}\varphi(x)\,dx∫e−2πix⋅ξφ(x)dx. Assumption (iv) is read with a constant CkC_kCk​ for each kkk; (vi) and (1.17) as Fourier transforms paired with Schwartz functions vanishing near the origin; (iii) pointwise on the punctured ball; one radius r0r_0r0​ for (iii), (v), (vii), (viii); m≥1m\ge1m≥1 in (viii). Assumption (vii) for s>0s>0s>0 is printed as g(x)<csg(y)\mathsf g(x)<c_s\mathsf g(y)g(x)<cs​g(y) for ∣y∣≥2∣x∣|y|\ge2|x|∣y∣≥2∣x∣, which together with (ii) is unsatisfiable; it is stated as g(y)<csg(x)\mathsf g(y)<c_s\mathsf g(x)g(y)<cs​g(x).

The solution of (1.5) is a mild solution (3.1) in C([0,∞);L1∩L∞)C([0,\infty);L^1\cap L^\infty)C([0,∞);L1∩L∞) with continuity in the L1+L∞L^1+L^\inftyL1+L∞ norm, with each μt\mu^tμt a probability density; every integral of (3.1) is required to converge. Because the noise is additive, a solution of (1.1) is a measurable process whose paths almost surely are continuous, never collide, and satisfy the integral equation with the Brownian path; no stochastic integral appears. Brownian motions are Mathlib's IsBrownianReal coordinates, jointly independent over all N⋅dN\cdot dN⋅d coordinates. Expectations are lower Lebesgue integrals of nonnegative quantities, and Proposition 6.3 is stated in [0,∞][0,\infty][0,∞] with positive and negative parts on opposite sides, so no ∞−∞\infty-\infty∞−∞ and no default value of a divergent integral enters.

The constants follow the paper's dependency lists: β\betaβ depends on s,ds,ds,d only and is chosen before σ,M,g\sigma,\mathbb M,\mathsf gσ,M,g; CCC and N0N_0N0​ are chosen after σ,M,g,r0\sigma,\mathbb M,\mathsf g,r_0σ,M,g,r0​ and ∥μ0∥L∞\|\mu^0\|_{L^\infty}∥μ0∥L∞​, before the data, NNN, the configuration, the probability space and ttt. A formalization with constants chosen after μ0\mu^0μ0, NNN or the configuration, with N=0N=0N=0, with a junk-zero integral in FNF_NFN​ or in (3.1), or with an empty solution class does not count. Corollary 5.6 is posed exactly under its printed assumptions, although its proof for 0≤s≤d−40\le s\le d-40≤s≤d−4 uses the superharmonicity of −Δg-\Delta\mathsf g−Δg, which those assumptions do not list.

Contributions welcome: proofs of the milestones, a Lean development of Riesz potentials and of the sharp log-Sobolev inequality on Rd\mathbb R^dRd, and the well-posedness of the mean-field equation that the goal takes as a hypothesis (Proposition 3.1 and its global continuation, not posed here).

Selected references

  • M. Rosenzweig, S. Serfaty, Global-in-time mean-field convergence for singular Riesz-type diffusive flows, arXiv:2108.09878v1, 2021; Ann. Appl. Probab. 33(2), 2023. https://arxiv.org/abs/2108.09878
  • Q. H. Nguyen, M. Rosenzweig, S. Serfaty, Mean-field limits of Riesz-type singular flows with possible multiplicative transport noise, arXiv:2107.02592, 2021. https://arxiv.org/abs/2107.02592
  • S. Serfaty, Mean field limit for Coulomb-type flows, Duke Math. J. 169(15), 2887–2935, 2020 (appendix with M. Duerinckx). https://arxiv.org/abs/1803.08345
  • E. Carlen, M. Loss, Optimal smoothing and decay estimates for viscously damped conservation laws, with applications to the 2-D Navier–Stokes equation, Duke Math. J. 81(1), 1995. https://doi.org/10.1215/S0012-7094-95-08110-1
  • L. Gross, Logarithmic Sobolev inequalities, Amer. J. Math. 97(4), 1975. https://doi.org/10.2307/2373688
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Operations ResearchProbabilityStochastic Systems·Captain: mikedeng1

Diffusion Approximation for Fully Coupled Stochastic Differential Equations 2: The Slow Component Converges Weakly to the Averaged SDE at an Explicit Rate (Regime 1)Research Paper

Motivation

Many stochastic models evolve on two time scales: a fast component that equilibrates quickly and a slow component driven by it. Planetary motion, climate models, geophysical flows and intracellular reaction networks are standard examples, and multiscale numerical methods for them approximate the slow component by a reduced equation. Such approximations are only useful with an error bound, and for the fully coupled case, where the fast and slow equations each depend on both components and the slow equation contains a large fluctuating drift, rates of convergence were missing.

Röckner and Xie (Ann. Probab. 49 (2021) 1205–1236) treat this case with only Hölder continuous coefficients and obtain explicit rates in four regimes. This mission poses the first regime, the classical averaging principle.

Timeline. Papanicolaou, Stroock and Varadhan (1977) proved the diffusion approximation for αε=βε=γε\alpha_\varepsilon=\beta_\varepsilon=\gamma_\varepsilonαε​=βε​=γε​ with a compact fast state space and time-independent coefficients. Pardoux and Veretennikov (2001, 2003, 2005) treated a noncompact homogeneous case with c≡0c\equiv0c≡0 and αε=γε\alpha_\varepsilon=\gamma_\varepsilonαε​=γε​ by martingale problems and the Poisson equation. Rates for the averaging principle when c=H≡0c=H\equiv0c=H≡0 were obtained by several authors, e.g. Givon (2007) and Liu (2010). Röckner and Xie (2021) give rates for the fully coupled system with Hölder coefficients in all four regimes.

Setting

Let x∈Rd1x\in\mathbb R^{d_1}x∈Rd1​ (fast) and y∈Rd2y\in\mathbb R^{d_2}y∈Rd2​ (slow), d1,d2≥1d_1,d_2\ge1d1​,d2​≥1. For small parameters αε,βε,γε>0\alpha_\varepsilon,\beta_\varepsilon,\gamma_\varepsilon>0αε​,βε​,γε​>0 tending to 000, with αε2/βε→0\alpha_\varepsilon^2/\beta_\varepsilon\to0αε2​/βε​→0, the two-scale system (1.4) is

dXtε=αε−2b(Xtε,Ytε)dt+βε−1c(Xtε,Ytε)dt+αε−1σ(Xtε,Ytε)dWt1,dX^\varepsilon_t=\alpha_\varepsilon^{-2}b(X^\varepsilon_t,Y^\varepsilon_t)dt+\beta_\varepsilon^{-1}c(X^\varepsilon_t,Y^\varepsilon_t)dt+\alpha_\varepsilon^{-1}\sigma(X^\varepsilon_t,Y^\varepsilon_t)dW^1_t,dXtε​=αε−2​b(Xtε​,Ytε​)dt+βε−1​c(Xtε​,Ytε​)dt+αε−1​σ(Xtε​,Ytε​)dWt1​, dYtε=F(t,Xtε,Ytε)dt+γε−1H(t,Xtε,Ytε)dt+G(t,Xtε,Ytε)dWt2,dY^\varepsilon_t=F(t,X^\varepsilon_t,Y^\varepsilon_t)dt+\gamma_\varepsilon^{-1}H(t,X^\varepsilon_t,Y^\varepsilon_t)dt+G(t,X^\varepsilon_t,Y^\varepsilon_t)dW^2_t,dYtε​=F(t,Xtε​,Ytε​)dt+γε−1​H(t,Xtε​,Ytε​)dt+G(t,Xtε​,Ytε​)dWt2​,

with X0ε=xX^\varepsilon_0=xX0ε​=x, Y0ε=yY^\varepsilon_0=yY0ε​=y and independent Brownian motions W1,W2W^1,W^2W1,W2.

Freezing yyy gives the frozen equation dXty=b(Xty,y)dt+σ(Xty,y)dWt1dX^y_t=b(X^y_t,y)dt+\sigma(X^y_t,y)dW^1_tdXty​=b(Xty​,y)dt+σ(Xty​,y)dWt1​ (1.7), with generator L0(x,y)=∑ijaij∂xixj2+∑ibi∂xi\mathscr L_0(x,y)=\sum_{ij}a^{ij}\partial^2_{x_ix_j}+\sum_ib^i\partial_{x_i}L0​(x,y)=∑ij​aij∂xi​xj​2​+∑i​bi∂xi​​, a=σσ∗/2a=\sigma\sigma^*/2a=σσ∗/2, and invariant probability measure μy\mu^yμy. A function is centered if its μy\mu^yμy-average vanishes for every yyy. The standing assumptions are: (Aσ), uniform nondegeneracy of σσ∗\sigma\sigma^*σσ∗; (Ab), lim⁡∣x∣→∞sup⁡y⟨x,b(x,y)⟩=−∞\lim_{|x|\to\infty}\sup_y\langle x,b(x,y)\rangle=-\inftylim∣x∣→∞​supy​⟨x,b(x,y)⟩=−∞; (AG), uniform nondegeneracy of GG∗GG^*GG∗; (AH), HHH is centered; and (2.7), the analogue of (Ab) for b+κcb+\kappa cb+κc, κ>0\kappa>0κ>0 small.

The averaged coefficients of Regime 1 are F^1(t,y)=∫F(t,x,y)μy(dx)\hat F_1(t,y)=\int F(t,x,y)\mu^y(dx)F^1​(t,y)=∫F(t,x,y)μy(dx) and G^1=(∫GG∗(t,x,y)μy(dx))1/2\hat G_1=(\int GG^*(t,x,y)\mu^y(dx))^{1/2}G^1​=(∫GG∗(t,x,y)μy(dx))1/2, and the averaged equation (2.9) is dY^t1=F^1(t,Y^t1)dt+G^1(t,Y^t1)dWt2d\hat Y^1_t=\hat F_1(t,\hat Y^1_t)dt+\hat G_1(t,\hat Y^1_t)dW^2_tdY^t1​=F^1​(t,Y^t1​)dt+G^1​(t,Y^t1​)dWt2​, Y^01=y\hat Y^1_0=yY^01​=y.

Regularity is measured in weighted Hölder classes: Cpδ,ϑC^{\delta,\vartheta}_pCpδ,ϑ​ (index δ\deltaδ in xxx, ϑ\varthetaϑ in yyy, polynomial growth in xxx), its bounded version Cbδ,ϑC^{\delta,\vartheta}_bCbδ,ϑ​, the time-dependent Cpϑ/2,δ,ϑC^{\vartheta/2,\delta,\vartheta}_pCpϑ/2,δ,ϑ​, the class Lp∞L^\infty_pLp∞​ of measurable functions of polynomial growth, and Cb2+ϑ(Rd2)C^{2+\vartheta}_b(\mathbb R^{d_2})Cb2+ϑ​(Rd2​) for test functions.

Formalization targets

Goal: Theorem 2.3(i)

In Regime 1, αε/γε→0\alpha_\varepsilon/\gamma_\varepsilon\to0αε​/γε​→0 and αε2/(βεγε)→0\alpha_\varepsilon^2/(\beta_\varepsilon\gamma_\varepsilon)\to0αε2​/(βε​γε​)→0, assume b,σ∈Cbδ,ϑb,\sigma\in C^{\delta,\vartheta}_bb,σ∈Cbδ,ϑ​, F,H,G∈Cpϑ/2,δ,ϑF,H,G\in C^{\vartheta/2,\delta,\vartheta}_pF,H,G∈Cpϑ/2,δ,ϑ​ with ϑ∈(0,2]\vartheta\in(0,2]ϑ∈(0,2], c∈Lp∞c\in L^\infty_pc∈Lp∞​ and αεϑ/γε→0\alpha_\varepsilon^\vartheta/\gamma_\varepsilon\to0αεϑ​/γε​→0. Then for every T>0T>0T>0 and φ∈Cb2+ϑ\varphi\in C^{2+\vartheta}_bφ∈Cb2+ϑ​,

sup⁡t∈[0,T]∣Eφ(Ytε)−Eφ(Y^t1)∣≤CT(αεϑγε+αε2γε2+αε2βεγε).\sup_{t\in[0,T]}\big|\mathbb E\varphi(Y^\varepsilon_t)-\mathbb E\varphi(\hat Y^1_t)\big|\le C_T\Big(\frac{\alpha_\varepsilon^\vartheta}{\gamma_\varepsilon}+\frac{\alpha_\varepsilon^2}{\gamma_\varepsilon^2}+\frac{\alpha_\varepsilon^2}{\beta_\varepsilon\gamma_\varepsilon}\Big).t∈[0,T]sup​​Eφ(Ytε​)−Eφ(Y^t1​)​≤CT​(γε​αεϑ​​+γε2​αε2​​+βε​γε​αε2​​).

Milestones

  1. Lemma 4.1: mollification in (t,y)(t,y)(t,y) at scales n−2n^{-2}n−2 and n−1n^{-1}n−1 costs n−ϑn^{-\vartheta}n−ϑ and gains n2−ϑn^{2-\vartheta}n2−ϑ on ∂t\partial_t∂t​ and ∇y2\nabla_y^2∇y2​.
  2. Lemma 4.2: for centered fff, E∫0tf(s,Xsε,Ysε)ds≤Ct(αεϑ+αεϑ∧1αε/γε+αε2/βε)\mathbb E\int_0^tf(s,X^\varepsilon_s,Y^\varepsilon_s)ds\le C_t(\alpha_\varepsilon^\vartheta+\alpha_\varepsilon^{\vartheta\wedge1}\alpha_\varepsilon/\gamma_\varepsilon+\alpha_\varepsilon^2/\beta_\varepsilon)E∫0t​f(s,Xsε​,Ysε​)ds≤Ct​(αεϑ​+αεϑ∧1​αε​/γε​+αε2​/βε​).
  3. Lemma 4.4(i): in Regime 1, E γε−1∫0tf ds≤Ct(αεϑ/γε+αε2/γε2+αε2/(βεγε))\mathbb E\,\gamma_\varepsilon^{-1}\int_0^tf\,ds\le C_t(\alpha_\varepsilon^\vartheta/\gamma_\varepsilon+\alpha_\varepsilon^2/\gamma_\varepsilon^2+\alpha_\varepsilon^2/(\beta_\varepsilon\gamma_\varepsilon))Eγε−1​∫0t​fds≤Ct​(αεϑ​/γε​+αε2​/γε2​+αε2​/(βε​γε​)).
  4. Lemma 5.1 (k=1k=1k=1): G^1=G^1G^1∗/2\hat{\mathcal G}_1=\hat G_1\hat G_1^*/2G^​1​=G^1​G^1∗​/2 is uniformly nondegenerate and F^1,G^1∈Cbϑ/2,ϑ\hat F_1,\hat{\mathcal G}_1\in C^{\vartheta/2,\vartheta}_bF^1​,G^​1​∈Cbϑ/2,ϑ​.

Significance

The result. The theorem gives a rate for the weak error of the averaging principle under Hölder regularity only, and the rate depends only on the regularity in the slow variable yyy, not on δ\deltaδ. It covers the fully coupled case, in which the slow equation contains the singular drift γε−1H\gamma_\varepsilon^{-1}Hγε−1​H, and it identifies the extra condition αεϑ/γε→0\alpha_\varepsilon^\vartheta/\gamma_\varepsilon\to0αεϑ​/γε​→0 under which this drift averages out. For c=H≡0c=H\equiv0c=H≡0 it reduces to the rate αεϑ\alpha_\varepsilon^\varthetaαεϑ​ (Remark 2.5), optimal for ϑ=2\vartheta=2ϑ=2. Error bounds of this kind are what heterogeneous multiscale methods need to be quantitative.

Formalizing it. The result is proved in the paper; nothing in it is machine-checked. A formalization needs an Itô calculus for weak solutions, the elliptic Poisson equation in xxx with parameter yyy (the companion mission's Theorem 2.1), and the parabolic Kolmogorov equation of the averaged SDE. The two fluctuation lemmas are stated for general centered functions and are reusable for other limit theorems.

Difficulty

The obvious argument writes Eφ(YTε)−Eφ(Y^T1)\mathbb E\varphi(Y^\varepsilon_T)-\mathbb E\varphi(\hat Y^1_T)Eφ(YTε​)−Eφ(Y^T1​) through the Kolmogorov equation of the averaged SDE and Itô's formula, which leaves E∫0T(L1−L^1)u~ ds\mathbb E\int_0^T(\mathscr L_1-\hat{\mathscr L}_1)\tilde u\,dsE∫0T​(L1​−L^1​)u~ds and γε−1E∫0TH⋅∇yu~ ds\gamma_\varepsilon^{-1}\mathbb E\int_0^TH\cdot\nabla_y\tilde u\,dsγε−1​E∫0T​H⋅∇y​u~ds. Both integrands are centered but only Hölder continuous in (t,y)(t,y)(t,y), so the standard corrector argument, which applies Itô's formula to the solution of the Poisson equation along (Xε,Yε)(X^\varepsilon,Y^\varepsilon)(Xε,Yε), needs derivatives in ttt and yyy that do not exist. The term with γε−1\gamma_\varepsilon^{-1}γε−1​ is a central-limit-scale fluctuation, which is why its control needs the regime conditions. Existence and regularity of the averaged coefficients also have to come from the Poisson equation, since μy\mu^yμy is not explicit.

Formalization scope

Spaces are EuclideanSpace ℝ (Fin d). Coefficients are b,c:Rd1×Rd2→Rd1b,c:\mathbb R^{d_1}\times\mathbb R^{d_2}\to\mathbb R^{d_1}b,c:Rd1​×Rd2​→Rd1​, σ\sigmaσ a d1×d1d_1\times d_1d1​×d1​ matrix, F,H:R+×Rd1×Rd2→Rd2F,H:\mathbb R_+\times\mathbb R^{d_1}\times\mathbb R^{d_2}\to\mathbb R^{d_2}F,H:R+​×Rd1​×Rd2​→Rd2​, GGG a d2×d2d_2\times d_2d2​×d2​ matrix. The Itô layer (Brownian motion, Itô integral, Itô processes, SDE solutions) is the published Peng1990.SMP.Stochastic. A solution of (1.4) is a weak solution: any filtered probability space, any Brownian motion for that filtration, any progressive process satisfying the integral equation. The theorem compares every weak solution of (1.4) with every weak solution of (2.9). The paper does not prove existence for (1.4), so the statement is conditional on solutions, as it is used in the paper. A sanity file shows the parameter hypotheses are consistent (αε=ε\alpha_\varepsilon=\varepsilonαε​=ε, βε=γε=ε1/2\beta_\varepsilon=\gamma_\varepsilon=\varepsilon^{1/2}βε​=γε​=ε1/2) and that (2.7) holds for a bounded dissipative drift.

Committed conventions and readings of the page:

  • μy\mu^yμy is any family of probability measures that are infinitesimally invariant for L0\mathscr L_0L0​ with a=σσ∗/2a=\sigma\sigma^*/2a=σσ∗/2, the generator of (1.7). Under the standing assumptions this is the unique invariant measure.
  • (2.7) is read with κ=αε2/βε\kappa=\alpha_\varepsilon^2/\beta_\varepsilonκ=αε2​/βε​, the factor that actually multiplies ccc in the fast drift, for all small κ>0\kappa>0κ>0.
  • G^1\hat G_1G^1​ is any measurable matrix field with G^1G^1∗=∫GG∗ dμy\hat G_1\hat G_1^*=\int GG^*\,d\mu^yG^1​G^1∗​=∫GG∗dμy, which covers the printed square root.
  • The Hölder classes include polynomial growth, constrain all lower yyy-derivatives, and take their constants uniformly in time, including in the time-Hölder clause.
  • The constants CTC_TCT​, CtC_tCt​, C0C_0C0​ exist after all data are fixed (coefficients, μ\muμ, TTT, φ\varphiφ, xxx, yyy, the parameter functions) and before ε\varepsilonε or nnn.
  • Lemma 4.1 takes fff on all of R\mathbb RR in time, since (4.1) evaluates fff at negative times, and assumes the kernels have the finite moments ∫∣r∣ϑ/2ρ1<∞\int|r|^{\vartheta/2}\rho_1<\infty∫∣r∣ϑ/2ρ1​<∞, ∫∣z∣ϑρ2<∞\int|z|^\vartheta\rho_2<\infty∫∣z∣ϑρ2​<∞ that its proof uses; without them (4.2) fails for a Cauchy-type kernel.
  • Solutions are Itô processes in the sense of the referenced layer: progressive, with sup⁡t≤TE∣Zt∣2<∞\sup_{t\le T}\mathbb E|Z_t|^2<\inftysupt≤T​E∣Zt​∣2<∞ and square-integrable diffusion integrands.
  • Lemma 4.4(i) carries the Regime 1 limits of its label.
  • Lemmas 4.2 and 4.4(i) are one-sided, as printed, and include integrability of the path integral in their conclusion.

A formalization in which the expectations are junk Bochner integrals, the constant depends on ε\varepsilonε, or a single strong solution is fixed would be a different and weaker statement; the posed statements rule these out.

Not posed: Regimes 2–4 of Theorem 2.3 and Lemma 4.4(ii)–(iv). The printed G^3=G^4\hat G_3=\hat G_4G^3​=G^4​ differs by a factor 222 in the HΦ∗H\Phi^*HΦ∗ term from the generator used in the proof, so a faithful statement needs a correction that is left to moderation. Regime 2 needs the Poisson solution Φ\PhiΦ in the averaged drift. Lemma 5.2 is also not posed: as printed, uk(t,y)=Eφ(Y^tk(y))u_k(t,y)=\mathbb E\varphi(\hat Y^k_t(y))uk​(t,y)=Eφ(Y^tk​(y)) solves (5.1) only for time-independent coefficients, and its class Cb(2+ϑ)/2,2+ϑC^{(2+\vartheta)/2,2+\vartheta}_bCb(2+ϑ)/2,2+ϑ​ has time index above 111, which the paper's notations do not define. Contributions toward Itô's formula for these processes, the Poisson equation (companion mission 1) and parabolic Schauder theory are welcome.

Selected references

  • M. Röckner, L. Xie, Diffusion approximation for fully coupled stochastic differential equations, Ann. Probab. 49(3) (2021) 1205–1236. https://doi.org/10.1214/20-AOP1475
  • G. Papanicolaou, D. Stroock, S. R. S. Varadhan, Martingale approach to some limit theorems, Duke Turbulence Conference, Duke Univ. Math. Ser. III (1977).
  • E. Pardoux, A. Yu. Veretennikov, On the Poisson equation and diffusion approximation. I, Ann. Probab. 29 (2001) 1061–1085. https://doi.org/10.1214/aop/1015345596
  • E. Pardoux, A. Yu. Veretennikov, On Poisson equation and diffusion approximation. II, Ann. Probab. 31 (2003) 1166–1192. https://doi.org/10.1214/aop/1055425774
  • E. Pardoux, A. Yu. Veretennikov, On the Poisson equation and diffusion approximation. III, Ann. Probab. 33 (2005) 1111–1133. https://doi.org/10.1214/009117905000000062
  • D. Givon, Strong convergence rate for two-time-scale jump-diffusion stochastic differential systems, Multiscale Model. Simul. 6 (2007) 577–594. https://doi.org/10.1137/060673345
  • D. Liu, Strong convergence of principle of averaging for multiscale stochastic dynamical systems, Commun. Math. Sci. 8 (2010) 999–1020.
  • S. Peng, A general stochastic maximum principle for optimal control problems, SIAM J. Control Optim. 28 (1990) 966–979 (source of the Itô layer). https://doi.org/10.1137/0328054
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AnalysisProbabilityStochastic Systems·Captain: mikedeng1

Diffusion Approximation for Fully Coupled Stochastic Differential Equations 1: The Parametric Poisson Equation Has a Unique Centered Solution with Optimal Regularity in x and yResearch Paper

Motivation

Poisson equations for the generator of an ergodic diffusion are a standard tool in stochastic averaging, homogenization and diffusion approximation: to show that a fast ergodic component averages out in a slow equation, one writes the fluctuation f(Xt,Yt)f(X_t,Y_t)f(Xt​,Yt​) as L0u\mathscr L_0 uL0​u and applies Itô's formula to uuu. This requires a solution uuu whose regularity is controlled in two variables at once: the fast variable xxx, in which the operator is elliptic, and the slow variable yyy, which enters as a parameter.

  • Pardoux and Veretennikov (Ann. Probab. 2001, 2003, 2005) studied this equation in the whole space Rd1\mathbb R^{d_1}Rd1​ and used it for diffusion approximation of slow–fast SDEs. In parts I and III the operator does not depend on the parameter, and the solution's regularity in xxx is of Sobolev type; regularity in yyy was obtained by differentiating the associated semigroup in the parameter (Röckner–Xie, Remark 2.2(iii) and p. 1213).
  • Röckner and Xie (2021) prove optimal Hölder regularity in xxx and show that regularity in yyy follows from it, for fully coupled coefficients that depend on both variables and are only Hölder continuous. This mission formalizes that result (their Theorem 2.1) and the steps of its proof.

Setting

Fix d1,d2≥1d_1,d_2\ge1d1​,d2​≥1, a matrix field a(x,y)=(aij(x,y))a(x,y)=(a^{ij}(x,y))a(x,y)=(aij(x,y)) and a vector field b(x,y)∈Rd1b(x,y)\in\mathbb R^{d_1}b(x,y)∈Rd1​ on Rd1×Rd2\mathbb R^{d_1}\times\mathbb R^{d_2}Rd1​×Rd2​. The frozen operator acts on functions of xxx with yyy held fixed:

L0(x,y)=∑i,j=1d1aij(x,y)∂2∂xi∂xj+∑i=1d1bi(x,y)∂∂xi.\mathscr L_0(x,y)=\sum_{i,j=1}^{d_1}a^{ij}(x,y)\frac{\partial^2}{\partial x_i\partial x_j}+\sum_{i=1}^{d_1}b^i(x,y)\frac{\partial}{\partial x_i}.L0​(x,y)=i,j=1∑d1​​aij(x,y)∂xi​∂xj​∂2​+i=1∑d1​​bi(x,y)∂xi​∂​.

The Poisson equation (1.1) is L0(x,y)u(x,y)=f(x,y)\mathscr L_0(x,y)u(x,y)=f(x,y)L0​(x,y)u(x,y)=f(x,y) for all x∈Rd1x\in\mathbb R^{d_1}x∈Rd1​, for each parameter y∈Rd2y\in\mathbb R^{d_2}y∈Rd2​.

The standing assumptions are:

  • (Aσ): a=σσ∗a=\sigma\sigma^*a=σσ∗ is uniformly nondegenerate, i.e. λ−1∣ξ∣2≤∣a(x,y)ξ∣2≤λ∣ξ∣2\lambda^{-1}|\xi|^2\le|a(x,y)\xi|^2\le\lambda|\xi|^2λ−1∣ξ∣2≤∣a(x,y)ξ∣2≤λ∣ξ∣2 for some λ>1\lambda>1λ>1;
  • (Ab): lim⁡∣x∣→∞sup⁡y⟨x,b(x,y)⟩=−∞\lim_{|x|\to\infty}\sup_y\langle x,b(x,y)\rangle=-\inftylim∣x∣→∞​supy​⟨x,b(x,y)⟩=−∞, a weak recurrence condition.

Under these, for each yyy the frozen diffusion dXt=b(Xt,y) dt+σ(Xt,y) dWtdX_t=b(X_t,y)\,dt+\sigma(X_t,y)\,dW_tdXt​=b(Xt​,y)dt+σ(Xt​,y)dWt​ has a unique invariant measure μy\mu^yμy. Since constants solve L0u=0\mathscr L_0u=0L0​u=0, the equation is only solvable for centered right-hand sides, ∫f(x,y) μy(dx)=0\int f(x,y)\,\mu^y(dx)=0∫f(x,y)μy(dx)=0 for every yyy (1.3), and the solution is fixed by requiring it to be centered as well.

Regularity is measured in weighted Hölder classes. f∈Cpδ,0f\in C^{\delta,0}_pf∈Cpδ,0​ (0<δ≤10<\delta\le10<δ≤1) means ∣f(x,y)∣≤C(1+∣x∣m)|f(x,y)|\le C(1+|x|^m)∣f(x,y)∣≤C(1+∣x∣m) and ∣f(x1,y)−f(x2,y)∣≤C(∣x1−x2∣δ∧1)(1+∣x1∣m+∣x2∣m)|f(x_1,y)-f(x_2,y)|\le C(|x_1-x_2|^\delta\wedge1)(1+|x_1|^m+|x_2|^m)∣f(x1​,y)−f(x2​,y)∣≤C(∣x1​−x2​∣δ∧1)(1+∣x1​∣m+∣x2​∣m), uniformly in yyy. Cpδ,ηC^{\delta,\eta}_pCpδ,η​ adds η\etaη derivatives in yyy, with a (η−[η])(\eta-[\eta])(η−[η])-Hölder top derivative. The subscript bbb denotes the bounded version, and Cp2+δ,ηC^{2+\delta,\eta}_pCp2+δ,η​ asks the same of ∇x2u\nabla^2_xu∇x2​u together with growth bounds on uuu and ∇xu\nabla_xu∇x​u.

Formalization targets

Goal: Theorem 2.1

If (Aσ), (Ab) hold and a,b∈Cbδ,ηa,b\in C^{\delta,\eta}_ba,b∈Cbδ,η​ with 0<δ≤10<\delta\le10<δ≤1, η≥0\eta\ge0η≥0, then for every centered f∈Cpδ,ηf\in C^{\delta,\eta}_pf∈Cpδ,η​ there is a unique centered u∈Cp2+δ,ηu\in C^{2+\delta,\eta}_pu∈Cp2+δ,η​ with L0u=f\mathscr L_0u=fL0​u=f. For some C0,m>0C_0,m>0C0​,m>0,

∣u∣+∣∇xu∣+∣∇x2u∣≤C0(1+∣x∣m),∣∇x2u(x1,y)−∇x2u(x2,y)∣≤C0(∣x1−x2∣δ∧1)(1+∣x1∣m+∣x2∣m),|u|+|\nabla_xu|+|\nabla^2_xu|\le C_0(1+|x|^m),\qquad|\nabla^2_xu(x_1,y)-\nabla^2_xu(x_2,y)|\le C_0(|x_1-x_2|^\delta\wedge1)(1+|x_1|^m+|x_2|^m),∣u∣+∣∇x​u∣+∣∇x2​u∣≤C0​(1+∣x∣m),∣∇x2​u(x1​,y)−∇x2​u(x2​,y)∣≤C0​(∣x1​−x2​∣δ∧1)(1+∣x1​∣m+∣x2​∣m),

and, for η>0\eta>0η>0, ∥u(x,⋅)∥Cbη≤C0(1+∣x∣m)\|u(x,\cdot)\|_{C^\eta_b}\le C_0(1+|x|^m)∥u(x,⋅)∥Cbη​​≤C0​(1+∣x∣m).

Milestones, in the order of the proof

  1. The transfer formula for η=1\eta=1η=1 (Remark 3.3(ii), Lemma 3.2(i)): if u∈Cp2+δ,0u\in C^{2+\delta,0}_pu∈Cp2+δ,0​ solves L0u=h−hˉ\mathscr L_0u=h-\bar hL0​u=h−hˉ, then
∂y∫h(x,y) μy(dx)=∫[∂yh−∂L0∂yu](x,y) μy(dx).\partial_y\int h(x,y)\,\mu^y(dx)=\int\Big[\partial_yh-\frac{\partial\mathscr L_0}{\partial y}u\Big](x,y)\,\mu^y(dx).∂y​∫h(x,y)μy(dx)=∫[∂y​h−∂y∂L0​​u](x,y)μy(dx).
  1. The increment formula (3.10) for η∈(0,1)\eta\in(0,1)η∈(0,1) (Lemma 3.2(ii)), with hˉ∈Cbη\bar h\in C^\eta_bhˉ∈Cbη​.
  2. Theorem 2.1 for η=0\eta=0η=0: existence, uniqueness and the xxx-estimates (2.1)–(2.2).
  3. Step 3: the right-hand side ∂yf−∂yL0 u\partial_yf-\partial_y\mathscr L_0\,u∂y​f−∂y​L0​u of the differentiated equation is centered.
  4. Step 3: for η=1\eta=1η=1 the solution satisfies ∂yu∈Cp2+δ,0\partial_yu\in C^{2+\delta,0}_p∂y​u∈Cp2+δ,0​ and ∣∂yu∣≤C(1+∣x∣m)|\partial_yu|\le C(1+|x|^m)∣∂y​u∣≤C(1+∣x∣m).
  5. Step 4: for η∈(0,1)\eta\in(0,1)η∈(0,1), ∣u(x,y1)−u(x,y2)∣≤C(∣y1−y2∣η∧1)(1+∣x∣m)|u(x,y_1)-u(x,y_2)|\le C(|y_1-y_2|^\eta\wedge1)(1+|x|^m)∣u(x,y1​)−u(x,y2​)∣≤C(∣y1​−y2​∣η∧1)(1+∣x∣m).

Significance

The theorem supplies the corrector used in Theorem 2.3 of the same paper, the weak convergence rate of the slow component of a fully coupled multiscale SDE to its averaged limit. Its form, regularity in yyy matching that of the data and no derivative of μy\mu^yμy in yyy, is what lets the rates depend only on the regularity of the coefficients in the slow variable. The transfer formulas (3.9)–(3.10) also show that averaged coefficients hˉ(y)=∫h dμy\bar h(y)=\int h\,d\mu^yhˉ(y)=∫hdμy inherit the yyy-regularity of hhh, a question that comes up in every averaging or homogenization limit.

The result is proved in the paper. None of it is formalized: Lean and Mathlib have no fundamental solutions of non-divergence elliptic operators, no Schauder theory and no invariant measures of diffusions. The mission poses the statements, so that the proof can be built in layers and the parts that do not depend on the Gaussian kernel bounds (the transfer formulas given a solution, the induction in Steps 3–4) can be proved separately.

Difficulty

Existence and the estimates (2.1)–(2.2) rest on the probabilistic representation u=∫0∞Ttf dtu=\int_0^\infty T_tf\,dtu=∫0∞​Tt​fdt and on Gaussian bounds and ergodic decay for the fundamental solution pt(x,x′;y)p_t(x,x';y)pt​(x,x′;y) of L0(⋅,y)\mathscr L_0(\cdot,y)L0​(⋅,y) (Lemma 3.1, cited from Ladyzhenskaya–Solonnikov–Ural'tseva and Pardoux–Veretennikov II, Proposition 3). The coefficients are only Hölder in xxx, so the Hessian bound needs the cancellation ∫∇x2pt dx′\int\nabla^2_xp_t\,dx'∫∇x2​pt​dx′ (3.3), not just a size estimate on ∇x2pt\nabla^2_xp_t∇x2​pt​. The obvious approach to yyy-regularity, differentiating TtfT_tfTt​f or μy\mu^yμy in yyy, needs derivatives of the invariant density in the parameter, which are hard to control. The paper's route, differentiating the equation and using the transfer formula to recenter, only works if the differentiated right-hand side is again centered. That centering is the content of Lemma 3.2.

Formalization scope

  • Rd\mathbb R^dRd is EuclideanSpace ℝ (Fin d); ∇x\nabla_x∇x​, ∇x2\nabla^2_x∇x2​ are fderiv and iteratedFDeriv ℝ 2 in xxx, ∂yj\partial^j_y∂yj​ is iteratedFDeriv ℝ j in yyy, with operator norms. yyy-derivatives in the milestones are directional.
  • (Aσ) includes symmetric positive semidefiniteness of aaa (the content of a=σσ∗a=\sigma\sigma^*a=σσ∗). (Ab) is the ∀M ∃R\forall M\,\exists R∀M∃R form.
  • μy\mu^yμy is a hypothesis: a family of probability measures, each infinitesimally invariant for L0(⋅,y)\mathscr L_0(\cdot,y)L0​(⋅,y) (∫L0g dμy=0\int\mathscr L_0g\,d\mu^y=0∫L0​gdμy=0 for smooth compactly supported ggg). Under the assumptions this is the unique invariant measure of the frozen SDE (1.7); the SDE itself is not formalized. No moment bounds on μy\mu^yμy are assumed, since they are consequences.
  • Centering includes μy\mu^yμy-integrability, and every integral formula in a conclusion asserts integrability of its integrand, so no statement can hold through a junk zero integral.
  • The classes include the polynomial growth bound and all lower yyy-derivatives; matrix coefficients are in Cbδ,ηC^{\delta,\eta}_bCbδ,η​ entrywise; η≥0\eta\ge0η≥0 is real, split as [η]+[\eta]+[η]+ fractional part; a yyy-derivative is read as continuous (CkC^kCk in yyy). The CbηC^\eta_bCbη​ norm is in max form.
  • Not posed: the clause that C0,mC_0,mC0​,m depend "only on d1,d2d_1,d_2d1​,d2​, ∥a∥Cbδ,0\|a\|_{C^{\delta,0}_b}∥a∥Cbδ,0​​, ∥b∥Cbδ,0\|b\|_{C^{\delta,0}_b}∥b∥Cbδ,0​​, [f]Cpδ,0[f]_{C^{\delta,0}_p}[f]Cpδ,0​​", which is false as printed ([f]Cpδ,0[f]_{C^{\delta,0}_p}[f]Cpδ,0​​ is a supremum over the unit ball, and λ\lambdaλ and the rate in (Ab) are missing), and the recursive constant Kη\mathcal K_\etaKη​ of (2.4)–(2.5). The constants exist for each fixed (a,b,f)(a,b,f)(a,b,f). (2.1)–(2.2), printed under "Case η = 0", are asserted for every η\etaη.
  • Uniqueness is stated for the whole class Cp2+δ,ηC^{2+\delta,\eta}_pCp2+δ,η​, not only among solutions that satisfy the estimates. Without the invariance of μy\mu^yμy for the same a,ba,ba,b, or without centering, the statement would be false; both are part of the hypotheses.
  • Useful contributions beyond this mission: Hölder spaces with polynomial weights, fundamental solutions of non-divergence-form operators, invariant measures of elliptic diffusions, and the identification of infinitesimally invariant measures with invariant measures of the diffusion.

Selected references

  • M. Röckner, L. Xie, Diffusion approximation for fully coupled stochastic differential equations, Ann. Probab. 49(3), 1205–1236, 2021. https://doi.org/10.1214/20-AOP1475
  • E. Pardoux, A. Yu. Veretennikov, On the Poisson equation and diffusion approximation. I, Ann. Probab. 29(3), 1061–1085, 2001. https://doi.org/10.1214/aop/1015345596
  • E. Pardoux, A. Yu. Veretennikov, On Poisson equation and diffusion approximation. II, Ann. Probab. 31(3), 1166–1192, 2003. https://doi.org/10.1214/aop/1055425774
  • E. Pardoux, A. Yu. Veretennikov, On the Poisson equation and diffusion approximation 3, Ann. Probab. 33(3), 1111–1133, 2005. https://doi.org/10.1214/009117905000000062
  • O. A. Ladyzhenskaya, V. A. Solonnikov, N. N. Ural'tseva, Linear and Quasi-linear Equations of Parabolic Type, AMS Translations of Mathematical Monographs 23, 1968. https://mathscinet.ams.org/mathscinet-getitem?mr=0241822
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