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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 It has not been peer reviewed and its theorems are not formally verified.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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Convex OptimizationNumerical Analysis·Captain: mikedeng1

Mean Field Games: Numerical Methods for the Planning Problem II: Solutions of the Penalized Scheme Converge to a Solution of the Discrete Planning Scheme as ε → 0Research Paper

Motivation

Mean field games (MFG), introduced by Lasry and Lions and by Huang, Caines and Malhamé, describe Nash equilibria of very large populations of identical rational agents. The equilibrium is a coupled system: a backward Hamilton–Jacobi–Bellman equation for the value function uuu of a representative agent and a forward Fokker–Planck equation for the density mmm of the population. In the planning problem, proposed by P.-L. Lions, both the initial density m0m_0m0​ and the final density mTm_TmT​ are prescribed, and one asks for a cost structure under which the population moves from one to the other. This is a mean field analogue of optimal transport.

Achdou, Camilli and Capuzzo-Dolcetta (hal-00465404, SIAM J. Control Optim. 2012) propose finite-difference schemes for the planning problem. Mission I of this series treats the existence of a solution of the discrete planning scheme. Since the two boundary conditions on mmm make the discrete system hard to solve directly, the paper also introduces a penalized scheme, in which the initial condition M0=m0M^0 = m_0M0=m0​ is replaced by a penalty U0=(M0−m0)/εU^0 = (M^0 - m_0)/\varepsilonU0=(M0−m0​)/ε; for each ε>0\varepsilon > 0ε>0 this is a standard discrete MFG system with a unique solution. This mission formalizes the paper's §3.2: the penalized solutions converge, as ε→0\varepsilon \to 0ε→0, to a solution of the planning scheme.

Setting

Fix integers Nh≥1N_h \ge 1Nh​≥1, NT≥1N_T \ge 1NT​≥1, a horizon T>0T > 0T>0 and a viscosity ν≥0\nu \ge 0ν≥0; put h=1/Nhh = 1/N_hh=1/Nh​ and Δt=T/NT\Delta t = T/N_TΔt=T/NT​. The grid Th2\mathbb T^2_hTh2​ consists of the points xi,jx_{i,j}xi,j​, (i,j)∈(Z/NhZ)2(i,j) \in (\mathbb Z/N_h\mathbb Z)^2(i,j)∈(Z/Nh​Z)2 (periodic indices). A grid function is a real function on Th2\mathbb T^2_hTh2​; time levels are n=0,…,NTn = 0, \dots, N_Tn=0,…,NT​.

  • (D1+U)i,j=(Ui+1,j−Ui,j)/h(D_1^+U)_{i,j} = (U_{i+1,j} - U_{i,j})/h(D1+​U)i,j​=(Ui+1,j​−Ui,j​)/h, (D2+U)i,j=(Ui,j+1−Ui,j)/h(D_2^+U)_{i,j} = (U_{i,j+1} - U_{i,j})/h(D2+​U)i,j​=(Ui,j+1​−Ui,j​)/h, and the discrete gradient is [DhU]i,j=((D1+U)i,j,(D1+U)i−1,j,(D2+U)i,j,(D2+U)i,j−1)∈R4[D_hU]_{i,j} = ((D_1^+U)_{i,j}, (D_1^+U)_{i-1,j}, (D_2^+U)_{i,j}, (D_2^+U)_{i,j-1}) \in \mathbb R^4[Dh​U]i,j​=((D1+​U)i,j​,(D1+​U)i−1,j​,(D2+​U)i,j​,(D2+​U)i,j−1​)∈R4.
  • Δh\Delta_hΔh​ is the five-point Laplacian.
  • A numerical Hamiltonian g(xi,j,q)g(x_{i,j}, q)g(xi,j​,q), q∈R4q \in \mathbb R^4q∈R4, is monotone (G1), C1C^1C1 (G3), convex (G4) and coercive (G5) in qqq.
  • Bi,j(U,M)\mathcal B_{i,j}(U, M)Bi,j​(U,M) is the discrete transport term divh(M ∇qg(⋅,[DhU]))\mathrm{div}_h\big(M\,\nabla_q g(\cdot, [D_hU])\big)divh​(M∇q​g(⋅,[Dh​U])).
  • W:R→RW : \mathbb R \to \mathbb RW:R→R is strictly convex, superlinear and C2C^2C2, with V=W′V = W'V=W′ (hypothesis (24)).
  • K={M≥0:h2∑i,jMi,j=1}\mathcal K = \{M \ge 0 : h^2\sum_{i,j} M_{i,j} = 1\}K={M≥0:h2∑i,j​Mi,j​=1} is the set of discrete probability densities, and m0,mT∈Km_0, m_T \in \mathcal Km0​,mT​∈K with m0>0m_0 > 0m0​>0.

The planning scheme (18) asks for families (Un,Mn)(U^n, M^n)(Un,Mn) with, for n<NTn < N_Tn<NT​,

Un+1−UnΔt−νΔhUn+1+g(x,[DhUn+1])=V(Mn),Mn+1−MnΔt+νΔhMn+B(Un+1,Mn)=0,\frac{U^{n+1} - U^n}{\Delta t} - \nu\Delta_hU^{n+1} + g(x, [D_hU^{n+1}]) = V(M^n), \qquad \frac{M^{n+1} - M^n}{\Delta t} + \nu\Delta_hM^n + \mathcal B(U^{n+1}, M^n) = 0,ΔtUn+1−Un​−νΔh​Un+1+g(x,[Dh​Un+1])=V(Mn),ΔtMn+1−Mn​+νΔh​Mn+B(Un+1,Mn)=0,

Mn∈KM^n \in \mathcal KMn∈K, M0=m0M^0 = m_0M0=m0​ and MNT=mTM^{N_T} = m_TMNT​=mT​. The penalized scheme (20)–(23) has the same two equations, Mn∈KM^n \in \mathcal KMn∈K for n<NTn < N_Tn<NT​, MNT=mTM^{N_T} = m_TMNT​=mT​, and U0=(M0−m0)/εU^0 = (M^0 - m_0)/\varepsilonU0=(M0−m0​)/ε in place of M0=m0M^0 = m_0M0=m0​.

Formalization targets

Goal: Proposition 4

Under the hypotheses of Theorem 1, for every sequence εk↓0\varepsilon_k \downarrow 0εk​↓0, every choice of penalized solutions (Uεk,Mεk)(U^{\varepsilon_k}, M^{\varepsilon_k})(Uεk​,Mεk​), and every limit Mεk→MM^{\varepsilon_k} \to MMεk​→M in KNT+1\mathcal K^{N_T+1}KNT​+1,

∃ U, a subsequence with Uεk→U,(U,M) solves (43)–(46).\exists\, U,\ \text{a subsequence with } U^{\varepsilon_k} \to U, \quad (U, M) \text{ solves (43)–(46)}.∃U, a subsequence with Uεk​→U,(U,M) solves (43)–(46).

If ggg is strictly convex, the whole sequence (Uεk,Mεk)(U^{\varepsilon_k}, M^{\varepsilon_k})(Uεk​,Mεk​) converges to the unique solution of (43)–(46) with ∑i,jUi,j0=0\sum_{i,j} U^0_{i,j} = 0∑i,j​Ui,j0​=0.

Milestones

  1. (13): (G5) implies max⁡i,jg(xi,j,[DhU]i,j)/∥[DhU]∥∞→+∞\max_{i,j} g(x_{i,j}, [D_hU]_{i,j}) / \|[D_hU]\|_\infty \to +\inftymaxi,j​g(xi,j​,[Dh​U]i,j​)/∥[Dh​U]∥∞​→+∞.
  2. Theorem 2: the penalized control problem (50), min⁡Θ∗(M,Z)+12εΔt∑(M0−m0)2\min \Theta^*(M,Z) + \frac{1}{2\varepsilon\Delta t}\sum(M^0 - m_0)^2minΘ∗(M,Z)+2εΔt1​∑(M0−m0​)2 under the discrete Fokker–Planck constraint, has a minimizer whose optimality system is (20)–(23).
  3. Proposition 2: max⁡i,j∣Mi,jε,0−(m0)i,j∣≤Cε1/2\max_{i,j}|M^{\varepsilon,0}_{i,j} - (m_0)_{i,j}| \le C\varepsilon^{1/2}maxi,j​∣Mi,jε,0​−(m0​)i,j​∣≤Cε1/2.
  4. Proposition 3: max⁡n,i,j∣Ui,jε,n∣≤C\max_{n,i,j}|U^{\varepsilon,n}_{i,j}| \le Cmaxn,i,j​∣Ui,jε,n​∣≤C.
  5. Corollary 1: max⁡i,j∣Mi,jε,0−(m0)i,j∣≤Cε\max_{i,j}|M^{\varepsilon,0}_{i,j} - (m_0)_{i,j}| \le C\varepsilonmaxi,j​∣Mi,jε,0​−(m0​)i,j​∣≤Cε.
  6. Proposition 1: uniqueness of MMM for (18), and of UUU normalized by ∑U0=0\sum U^0 = 0∑U0=0 when ggg is strictly convex.

In 3–5 the constant CCC depends on hhh, Δt\Delta tΔt and the data, never on ε\varepsilonε.

Significance

Proposition 4 justifies the penalized scheme as a way to compute solutions of the discrete planning problem. The penalized system has a standard initial–terminal structure that Newton's method (the paper's §4) handles well. The planning system does not, because it prescribes two conditions on MMM and none on UUU. The estimates of Propositions 2–3 and Corollary 1 also give a rate: the initial mismatch of the penalized density is O(ε)O(\varepsilon)O(ε).

The results are proved in the paper. None of them has been machine-checked: the platform holds no formalization of mean field games, of their finite-difference schemes, or of the Lasry–Lions monotonicity argument. A complete development would yield a reusable library of the monotone finite-difference operators on the discrete torus, a formal Lasry–Lions uniqueness argument for discrete MFG systems, and a template for compactness-plus-uniqueness convergence proofs in finite dimension.

Difficulty

Compactness of the densities is free, since KNT+1\mathcal K^{N_T+1}KNT​+1 is compact. Passing to the limit in the scheme needs only continuity of ggg, ∇qg\nabla_q g∇q​g and VVV. The substance lies in the two uniform estimates.

  • Bounding UεU^\varepsilonUε uniformly in ε\varepsilonε (Proposition 3) is the central difficulty. The initial condition Uε,0=(Mε,0−m0)/εU^{\varepsilon,0} = (M^{\varepsilon,0} - m_0)/\varepsilonUε,0=(Mε,0−m0​)/ε involves division by ε\varepsilonε, so the obvious bound ∣Uε,0∣≤2/(h2ε)|U^{\varepsilon,0}| \le 2/(h^2\varepsilon)∣Uε,0∣≤2/(h2ε) blows up. The comparison principle for the discrete HJB equation, which is the natural first idea, cannot repair this: it propagates whatever bound U0U^0U0 has. The HJB equation alone does not bound UεU^\varepsilonUε; the coupling with the Fokker–Planck equation, the coercivity (13), and a lower bound on Mε,0M^{\varepsilon,0}Mε,0 that is uniform in ε\varepsilonε (which is where Proposition 2 enters) all have to be used.
  • Proposition 2 compares the penalized problem with the planning problem through the convex duality of Theorem 2. It therefore needs a solution of the planning scheme, which is mission I's goal.
  • Proposition 1 needs the discrete Lasry–Lions identity, a summation by parts across the coupled system.

Formalization scope

All objects live in the namespace MFGPlanning.Penalized.

  • Grid points are ZMod Nh × ZMod Nh (periodicity is built in), time levels are Fin (NT + 1), and the four momentum components q1,…,q4q_1, \dots, q_4q1​,…,q4​ are Fin 4 indices 0, …, 3.
  • The data structure carries Nh,NT≥1N_h, N_T \ge 1Nh​,NT​≥1, T>0T > 0T>0 and ν≥0\nu \ge 0ν≥0.
  • ggg is given only at the grid points. (G2), which only defines the continuous Hamiltonian, is not encoded.
  • "Coercive" in (24) is read as superlinear.
  • Vh[M]=V(Mi,j)V_h[M] = V(M_{i,j})Vh​[M]=V(Mi,j​), as (24) prescribes.
  • Θ∗\Theta^*Θ∗ and (W+χ)∗(W+\chi)^*(W+χ)∗ take values in EReal, so unbounded suprema are +∞+\infty+∞.
  • Convergence is in the product topology, which on these finite-dimensional spaces is max⁡n∥⋅∥∞\max_n \|\cdot\|_\inftymaxn​∥⋅∥∞​ convergence.
  • "The unique solution" of (43)–(46) means unique under the normalization ∑i,jUi,j0=0\sum_{i,j} U^0_{i,j} = 0∑i,j​Ui,j0​=0, because UUU is otherwise determined only up to a constant.

Three trivializing formalizations are ruled out. The constants in Propositions 2–3 and Corollary 1 are quantified before ε\varepsilonε and before the solution. The goal quantifies over every sequence εk→0\varepsilon_k \to 0εk​→0 and assumes no convergence of UUU and no limit solution. Its part 2 does not assume convergence of MMM.

The existence of a solution of the planning scheme (Theorem 1) is posed in mission I and not restated here. A solver of Proposition 2 will need it once mission I's goal is proved. The existence and uniqueness of solutions of (20)–(23) are quoted by the paper from Achdou–Capuzzo-Dolcetta (2010) and are not items. Welcome contributions include discrete summation-by-parts lemmas on the torus, the discrete comparison principle for monotone schemes, and the Poincaré-type inequality ∥W∥∞≤c∥[DhW]∥∞\|W\|_\infty \le c\|[D_hW]\|_\infty∥W∥∞​≤c∥[Dh​W]∥∞​ on zero-mean grid functions.

Selected references

  • Y. Achdou, F. Camilli, I. Capuzzo-Dolcetta, Mean field games: numerical methods for the planning problem, HAL preprint hal-00465404v1, 2010; SIAM J. Control Optim. 50 (2012). https://hal.science/hal-00465404v1, https://doi.org/10.1137/100790069
  • Y. Achdou, I. Capuzzo-Dolcetta, Mean field games: numerical methods, SIAM J. Numer. Anal. 48 (2010) 1136–1162. https://doi.org/10.1137/090758477
  • J.-M. Lasry, P.-L. Lions, Mean field games, Japanese Journal of Mathematics 2 (2007) 229–260. https://doi.org/10.1007/s11537-007-0657-8
  • M. Huang, R. P. Malhamé, P. E. Caines, Large population stochastic dynamic games: closed-loop McKean–Vlasov systems and the Nash certainty equivalence principle, Communications in Information and Systems 6 (2006) 221–252. https://doi.org/10.4310/CIS.2006.v6.n3.a5
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Convex OptimizationNumerical Analysis·Captain: mikedeng1

Mean Field Games: Numerical Methods for the Planning Problem I: The Discrete Planning Scheme Has a Solution, Given by a Fenchel–Rockafellar Saddle PointResearch Paper

Motivation

Mean field games (Lasry and Lions, 2006–2007; Huang, Malhamé and Caines, 2006) model the limit of a large population of identical rational agents. Each agent solves an optimal control problem whose cost depends on the distribution mmm of all agents, and the distribution is in turn transported by the agents' optimal feedback. In the continuous setting this gives a coupled system: a backward Hamilton–Jacobi equation for the value function uuu and a forward Fokker–Planck equation for the density mmm.

In the usual formulation, mmm is prescribed at the initial time and uuu at the final time. The planning problem, introduced by P.-L. Lions in his Collège de France lectures, prescribes instead both the initial density m0m_0m0​ and the final density mTm_TmT​, and asks for a cost (through uuu) that steers the population from one to the other. According to the paper (§1, pp. 2–3), Lions proved existence for the continuous planning problem in mainly two cases: ν=0\nu = 0ν=0 with a smooth, strictly convex, superlinear Hamiltonian; and ν>0\nu > 0ν>0 with H(p)=c∣p∣2H(p) = c|p|^2H(p)=c∣p∣2 or close to it. In both cases the coupling is local and the densities are smooth and bounded away from 000. Existence for ν>0\nu > 0ν>0 and more general Hamiltonians was then open, and for sublinear HHH, m0≠mTm_0\ne m_Tm0​=mT​ and short horizons there is no solution.

Achdou, Camilli and Capuzzo-Dolcetta (hal-00465404, 2010; SIAM J. Control Optim. 2012) introduced a finite-difference scheme for the planning problem and proved that the discrete system has a solution. The proof writes the scheme as the optimality system of a discrete optimal control problem, a Fokker–Planck equation driven by a control, and obtains a solution from a saddle point given by the Fenchel–Rockafellar duality theorem. This mission formalizes that existence result: Theorem 1 of §3.1 together with the lemmas on which its proof rests.

Setting

Fix integers Nh,NT≥1N_h, N_T \ge 1Nh​,NT​≥1, a horizon T>0T > 0T>0 and a viscosity ν≥0\nu \ge 0ν≥0; let h=1/Nhh = 1/N_hh=1/Nh​ and Δt=T/NT\Delta t = T/N_TΔt=T/NT​. The grid Th2\mathbb T^2_hTh2​ is the periodic Nh×NhN_h\times N_hNh​×Nh​ grid on the two-dimensional torus, with points xi,jx_{i,j}xi,j​, (i,j)∈(Z/Nh)2(i,j)\in(\mathbb Z/N_h)^2(i,j)∈(Z/Nh​)2. On grid functions UUU the scheme uses the forward differences D1+D_1^+D1+​, D2+D_2^+D2+​, the four-component discrete gradient [DhU]i,j=((D1+U)i,j,(D1+U)i−1,j,(D2+U)i,j,(D2+U)i,j−1)[D_hU]_{i,j} = ((D_1^+U)_{i,j}, (D_1^+U)_{i-1,j}, (D_2^+U)_{i,j}, (D_2^+U)_{i,j-1})[Dh​U]i,j​=((D1+​U)i,j​,(D1+​U)i−1,j​,(D2+​U)i,j​,(D2+​U)i,j−1​), the five-point Laplacian Δh\Delta_hΔh​, a discrete divergence divh\mathrm{div}_hdivh​ of four-component fields, and the transport operator B(U,M)=divh(M ∇qg(⋅,[DhU]))\mathcal B(U, M) = \mathrm{div}_h(M\,\nabla_q g(\cdot, [D_hU]))B(U,M)=divh​(M∇q​g(⋅,[Dh​U])).

A numerical Hamiltonian g(xi,j,q1,q2,q3,q4)g(x_{i,j}, q_1,q_2,q_3,q_4)g(xi,j​,q1​,q2​,q3​,q4​) is monotone (nonincreasing in q1,q3q_1, q_3q1​,q3​, nondecreasing in q2,q4q_2, q_4q2​,q4​), C1C^1C1, convex, and superlinearly coercive in the directions where monotonicity does not bound it. The coupling is local: V=W′V = W'V=W′, with WWW strictly convex, superlinear and C2C^2C2. The set K\mathcal KK consists of the discrete probability densities, h2∑i,jMi,j=1h^2\sum_{i,j}M_{i,j} = 1h2∑i,j​Mi,j​=1, M≥0M\ge 0M≥0. The discrete planning scheme (18) asks for (Un,Mn)0≤n≤NT(U^n, M^n)_{0\le n\le N_T}(Un,Mn)0≤n≤NT​​ with

Un+1−UnΔt−νΔhUn+1+g(x,[DhUn+1])=V(Mn),Mn+1−MnΔt+νΔhMn+B(Un+1,Mn)=0,\frac{U^{n+1}-U^n}{\Delta t} - \nu\Delta_hU^{n+1} + g(x,[D_hU^{n+1}]) = V(M^n),\qquad \frac{M^{n+1}-M^n}{\Delta t} + \nu\Delta_hM^n + \mathcal B(U^{n+1},M^n) = 0,ΔtUn+1−Un​−νΔh​Un+1+g(x,[Dh​Un+1])=V(Mn),ΔtMn+1−Mn​+νΔh​Mn+B(Un+1,Mn)=0,

for 0≤n<NT0\le n<N_T0≤n<NT​, with Mn∈KM^n\in\mathcal KMn∈K, M0=m0M^0 = m_0M0=m0​ and MNT=mTM^{N_T} = m_TMNT​=mT​.

The duality is set up as follows. With χ\chiχ the indicator of {m≥0}\{m\ge0\}{m≥0}, let Θ(α,β)=∑n,i,j(W+χ)∗(αi,jn+g(xi,j,[βn]i,j))\Theta(\alpha,\beta) = \sum_{n,i,j}(W+\chi)^*(\alpha^n_{i,j} + g(x_{i,j},[\beta^n]_{i,j}))Θ(α,β)=∑n,i,j​(W+χ)∗(αi,jn​+g(xi,j​,[βn]i,j​)) on dual variables (αn,βn)1≤n≤NT(\alpha^n,\beta^n)_{1\le n\le N_T}(αn,βn)1≤n≤NT​​. Let Λ(Ψ)\Lambda(\Psi)Λ(Ψ) be the linear map sending Ψ=(Ψn)0≤n≤NT\Psi = (\Psi^n)_{0\le n\le N_T}Ψ=(Ψn)0≤n≤NT​​ to the discrete Hamilton–Jacobi operator and the discrete gradient of Ψn+1\Psi^{n+1}Ψn+1. Let Σ(α,β)=F(Ψ)\Sigma(\alpha,\beta) = \mathcal F(\Psi)Σ(α,β)=F(Ψ) if (α,β)=Λ(Ψ)(\alpha,\beta) = \Lambda(\Psi)(α,β)=Λ(Ψ) with ∑Ψ0=0\sum\Psi^0 = 0∑Ψ0=0, and +∞+\infty+∞ otherwise, where F(Ψ)=1Δt(∑m0Ψ0−∑mTΨNT)\mathcal F(\Psi) = \frac1{\Delta t}(\sum m_0\Psi^0 - \sum m_T\Psi^{N_T})F(Ψ)=Δt1​(∑m0​Ψ0−∑mT​ΨNT​). The Legendre–Fenchel transforms Θ∗\Theta^*Θ∗, Σ∗\Sigma^*Σ∗ act on primal variables (Mn,Zn)0≤n<NT(M^n, Z^n)_{0\le n<N_T}(Mn,Zn)0≤n<NT​​, where MnM^nMn is paired with αn+1\alpha^{n+1}αn+1 (Remark 2).

Formalization targets

Goal: Theorem 1

Under (G1), (G3)–(G5), (24), m0,mT∈Km_0, m_T\in\mathcal Km0​,mT​∈K, m0>0m_0 > 0m0​>0, and either ν>0\nu > 0ν>0 or (ν=0\nu = 0ν=0 and mT>0m_T > 0mT​>0):

min⁡M,Z Θ∗(M,Z)+Σ∗(−M,−Z)=−min⁡α,β(Θ(α,β)+Σ(α,β))\min_{M,Z}\ \Theta^*(M,Z) + \Sigma^*(-M,-Z) = -\min_{\alpha,\beta}\big(\Theta(\alpha,\beta) + \Sigma(\alpha,\beta)\big)M,Zmin​ Θ∗(M,Z)+Σ∗(−M,−Z)=−α,βmin​(Θ(α,β)+Σ(α,β))

has a solution (M,Z)(M,Z)(M,Z), (α,β)(\alpha,\beta)(α,β) with a finite common value. Moreover (α,β)=Λ(U)(\alpha,\beta) = \Lambda(U)(α,β)=Λ(U) for some UUU, and (U,M)(U, M)(U,M), with MNT=mTM^{N_T} = m_TMNT​=mT​ appended, solves the scheme (18), with Zk,n=Mn ∂qkg(x,[DhUn+1])Z^{k,n} = M^n\,\partial_{q_k}g(x,[D_hU^{n+1}])Zk,n=Mn∂qk​​g(x,[Dh​Un+1]).

Milestones, in attack order

  1. §3.1, p. 7. VVV maps (0,∞)(0,\infty)(0,∞) onto (λ,∞)(\lambda,\infty)(λ,∞); (W+χ)∗(W+\chi)^*(W+χ)∗ is finite, convex, continuous and nondecreasing, with explicit values on and off JV\mathcal J_VJV​.
  2. Lemma 1. Θ\ThetaΘ is convex and continuous, Σ\SigmaΣ is convex and l.s.c., and Σ\SigmaΣ and Θ\ThetaΘ are both finite at some point.
  3. Lemma 2. Θ∗\Theta^*Θ∗ and Σ∗\Sigma^*Σ∗ are convex and l.s.c., with explicit formulas.
  4. (30). Σ∗(−M,−Z)\Sigma^*(-M,-Z)Σ∗(−M,−Z) is 000 on the constraint set of the control problem (26) and +∞+\infty+∞ off it.
  5. Lemma 3. If m0>0m_0 > 0m0​>0, some (M,Z)(M,Z)(M,Z) has Θ∗\Theta^*Θ∗, Σ∗(−M,−Z)\Sigma^*(-M,-Z)Σ∗(−M,−Z) finite and Θ∗\Theta^*Θ∗ finite and continuous near it.
  6. Positivity. A discrete strong maximum principle from the proof of Theorem 1: densities in K\mathcal KK that solve the discrete Fokker–Planck equation (42) are strictly positive before the final time.

Significance

Theorem 1 is the existence result for the finite-difference planning problem. It is used in the paper's second part (§3.2), where solutions of a penalized scheme, in which the final condition is relaxed into a penalty, are shown to converge to a solution of (18) as the penalty parameter vanishes. The penalized scheme is what is solved numerically. The discrete existence result covers general convex, monotone, coercive numerical Hamiltonians and every ν≥0\nu\ge0ν≥0, which includes discretizations of the continuous cases that were still open when the paper was written.

The result has a published proof. What this mission adds is a machine-checked version of it: a complete discrete model of the planning problem (grid, operators, scheme, duality functionals) and the convex-analytic chain that connects it to the Fenchel–Rockafellar theorem. As far as a search of the platform shows, no part of this has been formalized; the series' second mission formalizes the convergence of the penalized scheme on the same model.

Difficulty

Existence for a coupled forward–backward nonlinear system with conditions at both ends of the time interval is not reachable by a fixed-point or time-marching argument: the Hamilton–Jacobi equation runs backward and the Fokker–Planck equation forward, and the final density is imposed rather than computed. The approach goes through duality, and three points are delicate.

  1. All the functionals in the duality take the value +∞+\infty+∞, and Fenchel–Rockafellar needs a qualification condition on each side. Lemma 1 gives it for the dual problem; Lemma 3 gives it for the primal one, and needs m0>0m_0 > 0m0​>0 and the coercivity (G5).
  2. The optimality conditions only give a complementarity system: the Hamilton–Jacobi equation holds where Mn>0M^n > 0Mn>0 and becomes an inequality where Mn=0M^n = 0Mn=0. Recovering the scheme (18) needs the strict positivity of MnM^nMn, a discrete strong maximum principle. That principle uses the monotonicity (G1) and either diffusion or a positive final density.
  3. The bookkeeping of the time lag between primal and dual variables and of the discrete integration by parts in Σ∗\Sigma^*Σ∗ must be exact.

Formalization scope

The Lean development lives in the namespace MFGPlanning.Existence. A structure Data carries Nh,NT≥1N_h, N_T \ge 1Nh​,NT​≥1, T>0T > 0T>0, ν≥0\nu\ge0ν≥0, ggg at the grid points, WWW, m0m_0m0​ and mTm_TmT​. Committed conventions:

  • grid indices are ZMod Nh × ZMod Nh (periodic), and d=2d = 2d=2 as in the paper;
  • the components q1,…,q4q_1,\dots,q_4q1​,…,q4​ and Z1,…,Z4Z^1,\dots,Z^4Z1,…,Z4 are the Fin 4 indices 0..3;
  • time levels are Fin (NT+1) for UUU and the scheme, and Fin NT for the duality variables. M k is MkM^kMk and α k is αk+1\alpha^{k+1}αk+1 (Remark 2), and Fin.snoc M mT appends MNT=mTM^{N_T} = m_TMNT​=mT​;
  • (W+χ)∗(W+\chi)^*(W+χ)∗, Θ\ThetaΘ, Θ∗\Theta^*Θ∗, Σ\SigmaΣ, Σ∗\Sigma^*Σ∗ are EReal-valued lattice suprema and infima, so unbounded suprema are +∞+\infty+∞ and not a junk value. Convexity of an extended-valued functional is convexity of its epigraph.

Disclosed encodings:

  • (G2) is not encoded, since it only defines the continuous Hamiltonian;
  • "coercive" in (24) is read as superlinear growth W(m)/∣m∣→∞W(m)/|m|\to\inftyW(m)/∣m∣→∞, which the paper's own consequence V((0,∞))=(λ,∞)V((0,\infty)) = (\lambda,\infty)V((0,∞))=(λ,∞) requires;
  • ggg is given only at grid points;
  • the optimality conditions (32)–(33) are stated through what Theorem 1 says they are equivalent to: the scheme (18) and the relation (39).

Theorem 1 is not reducible to "the scheme (18) has a solution". The goal also asserts that the primal and dual problems attain their minima, that there is no duality gap with a finite value, and that (α,β)=Λ(U)(\alpha,\beta) = \Lambda(U)(α,β)=Λ(U). The duality functionals are never real-valued suprema, which would make (30) and (31) hold or fail for junk reasons. A complete development needs finite-dimensional convex analysis on extended-valued functions: conjugates, the Fenchel–Rockafellar theorem with attainment, and subdifferential optimality conditions. These parts are reusable well beyond this mission, and proofs of them as separate theorems are welcome.

Selected references

  • Y. Achdou, F. Camilli, I. Capuzzo-Dolcetta, Mean field games: numerical methods for the planning problem, preprint hal-00465404v1, 2010. https://hal.science/hal-00465404 ; published in SIAM J. Control Optim. 50(1), 2012. https://doi.org/10.1137/100790069
  • Y. Achdou, I. Capuzzo-Dolcetta, Mean field games: numerical methods, SIAM J. Numer. Anal. 48(3), 2010. https://doi.org/10.1137/090758477
  • J.-M. Lasry, P.-L. Lions, Mean field games, Japanese Journal of Mathematics 2(1), 2007. https://doi.org/10.1007/s11537-007-0657-8
  • I. Ekeland, R. Temam, Convex Analysis and Variational Problems, North-Holland, 1976 (SIAM Classics reprint 1999). https://doi.org/10.1137/1.9781611971088
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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
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Operations ResearchProbabilityStochastic Systems·Captain: mikedeng1

Revenue Management of a Make-to-Stock Queue: Exponential Stationary Density under Normal Reflection (Proposition 2)Research Paper

Motivation

A make-to-stock manufacturer who also sells on a spot market must decide, at every moment, whether to keep producing and whether to accept or reject incoming orders at the prevailing price. Caldentey and Wein (Revenue Management of a Make-to-Stock Queue, Operations Research 54(5), 2006) study this problem in heavy traffic. The limit is a two-dimensional singular control problem for a diffusion: the inventory level and the logarithm of the price move jointly as a correlated Brownian motion, and the controls push the inventory only when it reaches one of two free boundaries. The optimal boundaries are characterized by an elliptic free-boundary problem that the authors could not solve in closed form.

The paper's way forward is an approximation: change the direction of reflection on the boundary so that the stationary distribution of the controlled process becomes an explicit exponential. Proposition 2 states that exponential form, and it turns the free-boundary problem into a calculus-of-variations problem for the two boundary curves. Explicit stationary densities of reflected diffusions in two dimensions are rare; the classical condition for an exponential stationary density of a reflected Brownian motion, and the characterization of the stationary law by a basic adjoint relation, are due to Harrison and Williams, Multidimensional reflected Brownian motions having exponential stationary distributions, Annals of Probability 15, 1987, the reference the paper cites. This mission formalizes the analytic core of Proposition 2: the exponential density satisfies that relation for the reflection field the proposition singles out.

Setting

Points of the plane are (x,y)(x,y)(x,y), with xxx the inventory level and yyy the logarithm of the price. The limiting process (X,Y)(\mathcal X,\mathcal Y)(X,Y) has drift (θ,0)(\theta,0)(θ,0) and covariance matrix

Σ=(σ2σδϱσδϱδ2),σ>0, δ>0, −1<ϱ<1,\Sigma=\begin{pmatrix}\sigma^2&\sigma\delta\varrho\\ \sigma\delta\varrho&\delta^2\end{pmatrix},\qquad \sigma>0,\ \delta>0,\ -1<\varrho<1,Σ=(σ2σδϱ​σδϱδ2​),σ>0, δ>0, −1<ϱ<1,

so its generator is

Γ=θ∂∂x+σ22∂2∂x2+σδϱ∂2∂x ∂y+δ22∂2∂y2.\Gamma=\theta\frac{\partial}{\partial x}+\frac{\sigma^2}{2}\frac{\partial^2}{\partial x^2}+\sigma\delta\varrho\frac{\partial^2}{\partial x\,\partial y}+\frac{\delta^2}{2}\frac{\partial^2}{\partial y^2}.Γ=θ∂x∂​+2σ2​∂x2∂2​+σδϱ∂x∂y∂2​+2δ2​∂y2∂2​.

Two curves bound the region where the process lives: the rejection boundary x=η(y)x=\eta(y)x=η(y) (below it, orders are rejected) and the idleness boundary x=ξ(y)x=\xi(y)x=ξ(y) (above it, production stops). For ymin⁡<ymax⁡y_{\min}<y_{\max}ymin​<ymax​ the region is

Ω={(x,y): ymin⁡<y<ymax⁡, η(y)<x<ξ(y)},\Omega=\{(x,y):\ y_{\min}<y<y_{\max},\ \eta(y)<x<\xi(y)\},Ω={(x,y): ymin​<y<ymax​, η(y)<x<ξ(y)},

and its boundary splits into four pieces: x=η(y)x=\eta(y)x=η(y), x=ξ(y)x=\xi(y)x=ξ(y), y=ymin⁡y=y_{\min}y=ymin​, y=ymax⁡y=y_{\max}y=ymax​. Write n⃗\vec nn for the inward unit normal on ∂Ω\partial\Omega∂Ω and dldldl for arc length. A reflection field v⃗\vec vv on ∂Ω\partial\Omega∂Ω gives the direction in which the process is pushed back into Ω\OmegaΩ. The basic adjoint relation (BAR) of the paper, equation (43), is

∫ΩΓf πΩ ds+12∫∂Ωv⃗⋅∇f πΩ dl=0for all test functions f,\int_\Omega \Gamma f\,\pi_\Omega\,ds+\frac12\int_{\partial\Omega}\vec v\cdot\nabla f\,\pi_\Omega\,dl=0\quad\text{for all test functions } f,∫Ω​ΓfπΩ​ds+21​∫∂Ω​v⋅∇fπΩ​dl=0for all test functions f,

and the paper cites Harrison and Williams for the fact that the stationary distribution πΩ\pi_\OmegaπΩ​ of the reflected process satisfies it. Proposition 2 introduces the eigen-decomposition Σ=V′EV\Sigma=V'EVΣ=V′EV (VVV a rotation whose rows are eigenvectors, EEE diagonal), the whitening map T=E−1/2VT=E^{-1/2}VT=E−1/2V and Ω∗=T(Ω)\Omega^*=T(\Omega)Ω∗=T(Ω), and assumes that Tv⃗T\vec vTv is normal to ∂Ω∗\partial\Omega^*∂Ω∗. The exponents are

mx=2θσ2(1−ϱ2),my=−2ϱθσδ(1−ϱ2).(47)m_x=\frac{2\theta}{\sigma^2(1-\varrho^2)},\qquad m_y=\frac{-2\varrho\theta}{\sigma\delta(1-\varrho^2)}.\tag{47}mx​=σ2(1−ϱ2)2θ​,my​=σδ(1−ϱ2)−2ϱθ​.(47)

Formalization targets

Goal: the exponential density satisfies the BAR under conormal reflection

For η,ξ\eta,\xiη,ξ continuously differentiable with η<ξ\eta<\xiη<ξ on [ymin⁡,ymax⁡][y_{\min},y_{\max}][ymin​,ymax​], π(x,y)=emxx+myy\pi(x,y)=e^{m_xx+m_yy}π(x,y)=emx​x+my​y, and every C2C^2C2 function fff on R2\mathbb R^2R2,

∫ΩΓf  π ds+12∫∂Ω(Σn⃗)⋅∇f  π dl=0.\int_\Omega \Gamma f\;\pi\,ds+\frac12\int_{\partial\Omega}(\Sigma\vec n)\cdot\nabla f\;\pi\,dl=0 .∫Ω​Γfπds+21​∫∂Ω​(Σn)⋅∇fπdl=0.

The boundary integral is written out on the four pieces, with n⃗ dl\vec n\,dlndl equal to (1,−η′(y)) dy(1,-\eta'(y))\,dy(1,−η′(y))dy, (−1,ξ′(y)) dy(-1,\xi'(y))\,dy(−1,ξ′(y))dy, (0,1) dx(0,1)\,dx(0,1)dx and (0,−1) dx(0,-1)\,dx(0,−1)dx respectively. The normalizing constant is left out because the relation is linear in π\piπ.

Milestones

  1. The interior equation: Γ∗π=−θπx+σ22πxx+σδϱ πxy+δ22πyy=0\Gamma^*\pi=-\theta\pi_x+\frac{\sigma^2}{2}\pi_{xx}+\sigma\delta\varrho\,\pi_{xy}+\frac{\delta^2}{2}\pi_{yy}=0Γ∗π=−θπx​+2σ2​πxx​+σδϱπxy​+2δ2​πyy​=0 everywhere.
  2. The zero-flux identity: 12Σ∇π=(θ,0) π\frac12\Sigma\nabla\pi=(\theta,0)\,\pi21​Σ∇π=(θ,0)π everywhere.
  3. The meaning of the hypothesis: with T=E−1/2VT=E^{-1/2}VT=E−1/2V, (Tv)⋅(Tw)=v⋅Σ−1w(Tv)\cdot(Tw)=v\cdot\Sigma^{-1}w(Tv)⋅(Tw)=v⋅Σ−1w, and for n≠0n\neq0n=0, TvTvTv is orthogonal to TTT of every vector orthogonal to nnn exactly when vvv is a multiple of Σn\Sigma nΣn.
  4. The normalizing constant: π\piπ is integrable on Ω\OmegaΩ and a unique KΩ>0K_\Omega>0KΩ​>0 makes KΩπK_\Omega\piKΩ​π integrate to one.

Significance

For the operations model, Proposition 2 is what makes the problem computable. Once the stationary density is explicit, the long-run average cost of any pair of boundary curves is an explicit integral, and optimizing over (η,ξ)(\eta,\xi)(η,ξ) becomes a variational problem with Euler–Lagrange equations; the paper's proposed policy and its numerical comparisons all rest on it.

For formalization, the mission produces a machine-checked version of a statement whose proof the paper does not contain (it is in an online companion) and whose hypothesis is stated only in words. The formal statements fix exactly which reflection field makes the claim true, which the prose leaves ambiguous. None of the statements has, to our knowledge, a machine-checked proof anywhere; the result itself is classical in spirit (an integration by parts on a planar region), but no divergence theorem on a region between two graphs with an anisotropic operator is currently available as a ready-made statement.

Difficulty

The interior equation and the zero-flux identity are finite computations with the exponential. The difficulty is the goal: it is an integration-by-parts identity on a curved planar region with an anisotropic second-order operator. The obvious first step, "apply Green's identity", presupposes a divergence theorem on a region bounded by two graphs x=η(y)x=\eta(y)x=η(y), x=ξ(y)x=\xi(y)x=ξ(y) and two horizontal segments, with the boundary integral written in the parametrization of each piece and the orientation of every normal tracked. Mathlib has the divergence theorem on rectangular boxes, not on such regions, and the moving limits η(y)\eta(y)η(y), ξ(y)\xi(y)ξ(y) are exactly where the terms in η′\eta'η′ and ξ′\xi'ξ′ of the boundary integral come from.

The second trap is the reflection field. The page describes the modification as substituting the inward unit normal n⃗\vec nn for v⃗\vec vv; with v⃗=n⃗\vec v=\vec nv=n the identity is false as soon as Σ\SigmaΣ is not a multiple of the identity (on a random instance the residual is of order one). Only the conormal field Σn⃗\Sigma\vec nΣn, which is what the hypothesis of Proposition 2 selects, gives a true statement.

Formalization scope

Everything lives in the namespace MakeToStockRM.ExpDensity. The plane is ℝ × ℝ with the inventory first; partial derivatives are Fréchet derivatives applied to (1, 0) and (0, 1), and the mixed partial is ∂x(∂yf)\partial_x(\partial_y f)∂x​(∂y​f). Parameters satisfy σ>0\sigma>0σ>0, δ>0\delta>0δ>0, ∣ϱ∣<1|\varrho|<1∣ϱ∣<1; θ\thetaθ is any real number, and θ=0\theta=0θ=0 (then π≡1\pi\equiv1π≡1) is allowed.

This is the analytic, pinned-down content of Proposition 2. The identification "the BAR characterizes the stationary law of the reflected diffusion" (Harrison–Williams 1987) is out of scope: Mathlib has no reflected Brownian motion. Relative to the page, the formalization commits to the following:

  • The reflection field is v⃗=Σn⃗\vec v=\Sigma\vec nv=Σn with n⃗\vec nn the inward unit normal and dldldl arc length. The hypothesis "Tv⃗T\vec vTv is normal to ∂Ω∗\partial\Omega^*∂Ω∗" fixes only the direction of v⃗\vec vv (milestone 3); the length Σn⃗\Sigma\vec nΣn is the one for which the BAR holds. The page's phrase "substituting the inward unit normal n⃗\vec nn for v⃗\vec vv" is inconsistent with the proposition's own hypothesis and is not followed.
  • The boundary curves are C1C^1C1 on R\mathbb RR with η<ξ\eta<\xiη<ξ on [ymin⁡,ymax⁡][y_{\min},y_{\max}][ymin​,ymax​], and ymin⁡<ymax⁡y_{\min}<y_{\max}ymin​<ymax​, so Ω\OmegaΩ is a nonempty bounded region; the paper assumes this implicitly.
  • Test functions are all C2C^2C2 functions on R2\mathbb R^2R2, which are bounded with bounded derivatives on the closure of Ω\OmegaΩ (the paper's "twice continuous and bounded").
  • The constant KΩK_\OmegaKΩ​ is dropped from the goal and treated in milestone 4.

The goal quantifies over every C2C^2C2 test function; restricting to functions supported inside Ω\OmegaΩ would delete the boundary term and reduce the goal to milestone 1, and that trivialization is ruled out. The second half of Proposition 2 ("(45)–(46) is equivalent to (48)–(49)"), Proposition 1, the heavy-traffic limit, the HJB equation and the proposed policy are not formalized: their normalizations or proofs are only in the online companion.

A complete development needs a divergence theorem on regions between two C1C^1C1 graphs, which is reusable for any planar PDE statement on such regions. Contributions of that lemma, and of the four milestones, are welcome.

Selected references

  • R. Caldentey, L. M. Wein, Revenue Management of a Make-to-Stock Queue, Operations Research 54(5):859–875, 2006. https://doi.org/10.1287/opre.1060.0289
  • J. M. Harrison, R. J. Williams, Multidimensional reflected Brownian motions having exponential stationary distributions, Annals of Probability 15(1):115–137, 1987. https://doi.org/10.1214/aop/1176992259
  • F. John, Partial Differential Equations, 4th ed., Springer, 1982. https://doi.org/10.1007/978-1-4684-9333-7
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Mathematical Physics·Captain: Lucas

Schrödinger Equation I: Energy Quantization in the One-Dimensional Infinite Potential WellTextbook

Motivation

The Schrödinger equation is the equation of motion of non-relativistic quantum mechanics: it determines how the state of an isolated quantum system evolves in time. Its time-independent form is an eigenvalue equation whose eigenvalues are the energies the system can have. The single most elementary illustration that this eigenvalue problem forces energies to be discrete is the particle in a one-dimensional box, also called the infinite potential well: a particle of mass mmm confined to an interval [0,L][0, L][0,L] by walls of infinite potential energy. It is the first worked example in essentially every introduction to quantum mechanics, and it is the model in which "quantization" can be derived in a few lines from a boundary-value problem for an ordinary differential equation.

This mission is the first in a series formalizing the mathematical content of the Schrödinger equation. It targets exactly the particle-in-a-box computation: that the admissible energies are En=n2π2ℏ2/(2mL2)E_n = n^2 \pi^2 \hbar^2 / (2 m L^2)En​=n2π2ℏ2/(2mL2) for positive integers nnn, and nothing else.

Setting

Fix three positive real constants: the reduced Planck constant ℏ\hbarℏ, the mass mmm, and the width LLL of the box. A stationary state of energy E∈RE \in \mathbb{R}E∈R is a function ψ:R→C\psi : \mathbb{R} \to \mathbb{C}ψ:R→C such that

−ℏ22m ψ′′(x)  =  E ψ(x)for all x∈(0,L),-\frac{\hbar^2}{2m}\,\psi''(x) \;=\; E\,\psi(x) \qquad \text{for all } x \in (0, L),−2mℏ2​ψ′′(x)=Eψ(x)for all x∈(0,L),

together with the regularity needed to state it — ψ\psiψ is continuous on [0,L][0, L][0,L] and twice differentiable at every interior point — and the Dirichlet boundary conditions imposed by the infinite walls,

ψ(0)=0,ψ(L)=0.\psi(0) = 0, \qquad \psi(L) = 0 .ψ(0)=0,ψ(L)=0.

Inside the box the potential vanishes, which is why only the kinetic term appears; outside the box the potential is infinite and the wave function is identically zero, which is what forces the two boundary values. A stationary state is non-trivial if ψ(x)≠0\psi(x) \neq 0ψ(x)=0 for at least one x∈(0,L)x \in (0, L)x∈(0,L); the trivial solution ψ≡0\psi \equiv 0ψ≡0 is excluded because a physical state must be normalizable to unit probability.

Write En:=n2π2ℏ2/(2mL2)E_n := n^2 \pi^2 \hbar^2 / (2 m L^2)En​:=n2π2ℏ2/(2mL2) for n∈Nn \in \mathbb{N}n∈N, and ψn(x):=sin⁡(nπx/L)\psi_n(x) := \sin(n \pi x / L)ψn​(x):=sin(nπx/L) for the corresponding unnormalized eigenfunction.

Formalization targets

Goal — energy quantization

If ψ is a non-trivial stationary state of energy E, then ∃ n≥1 with E=n2π2ℏ22mL2.\text{If } \psi \text{ is a non-trivial stationary state of energy } E, \text{ then } \exists\, n \ge 1 \text{ with } E = \frac{n^2 \pi^2 \hbar^2}{2 m L^2}.If ψ is a non-trivial stationary state of energy E, then ∃n≥1 with E=2mL2n2π2ℏ2​.

This is the weakest statement that carries the physical content: it fixes no eigenfunction, no normalization and no phase, only the set of admissible energies.

Supporting targets

E≤0  ⟹  ψ≡0 on [0,L],E \le 0 \;\Longrightarrow\; \psi \equiv 0 \text{ on } [0, L],E≤0⟹ψ≡0 on [0,L], E>0  ⟹  ∃ C∈C,  ψ(x)=Csin⁡ ⁣(kx) on [0,L],k=2mEℏ,E > 0 \;\Longrightarrow\; \exists\, C \in \mathbb{C},\; \psi(x) = C \sin\!\big(k x\big) \text{ on } [0, L], \quad k = \frac{\sqrt{2 m E}}{\hbar},E>0⟹∃C∈C,ψ(x)=Csin(kx) on [0,L],k=ℏ2mE​​, k>0,  L>0,  sin⁡(kL)=0  ⟹  ∃ n≥1,  kL=nπ,k > 0,\; L > 0,\; \sin(kL) = 0 \;\Longrightarrow\; \exists\, n \ge 1,\; kL = n\pi,k>0,L>0,sin(kL)=0⟹∃n≥1,kL=nπ, ψn is a non-trivial stationary state of energy En(n≥1),\psi_n \text{ is a non-trivial stationary state of energy } E_n \quad (n \ge 1),ψn​ is a non-trivial stationary state of energy En​(n≥1), ∫0L∣ψn(x)∣2 dx=L2(n≥1).\int_0^L |\psi_n(x)|^2 \, dx = \frac{L}{2} \quad (n \ge 1).∫0L​∣ψn​(x)∣2dx=2L​(n≥1).

The last two give the converse direction — every EnE_nEn​ really occurs — and the normalization constant 2/L\sqrt{2/L}2/L​ that turns ψn\psi_nψn​ into a unit vector of L2([0,L])L^2([0,L])L2([0,L]).

Significance

The result itself is the standard textbook derivation: confinement plus the time-independent Schrödinger equation yields a discrete spectrum, with a strictly positive ground-state energy E1=π2ℏ2/(2mL2)E_1 = \pi^2\hbar^2/(2mL^2)E1​=π2ℏ2/(2mL2) (no state of zero energy exists) and level spacing growing like nnn. As a piece of mathematics it is the computation of the Dirichlet spectrum of the one-dimensional Laplacian on an interval, which is the model case for spectral theory on domains.

What the mission adds is a machine-checked version of both halves of that derivation, in a form that later missions in this series can import: a reusable predicate for "stationary state with Dirichlet boundary conditions", the classification of the solutions of ψ′′=−k2ψ\psi'' = -k^2\psiψ′′=−k2ψ with one boundary zero, and the quantization step. Mathlib contains the ordinary-differential-equation uniqueness results and the trigonometric API needed, but does not contain this boundary-value classification.

Difficulty

The physics derivation writes down the general solution ψ(x)=Aeikx+Be−ikx\psi(x) = A e^{ikx} + B e^{-ikx}ψ(x)=Aeikx+Be−ikx and is done. Formally, that step is the whole problem: one must prove that every twice-differentiable solution of ψ′′=−k2ψ\psi'' = -k^2 \psiψ′′=−k2ψ on an interval has this form, rather than assume it. The usual route is a uniqueness theorem for the associated first-order system applied to the difference of ψ\psiψ and an explicit sine solution, which requires converting the second-order scalar equation into a system and supplying a Lipschitz estimate. Two further traps: the sign case E≤0E \le 0E≤0 must be excluded separately (hyperbolic solutions with two zeros are identically zero), and the equation is assumed only on the open interval, so the values at the walls are reached by continuity rather than by evaluating the equation there.

Formalization scope

Wave functions are complex-valued functions of a real variable, ψ:R→C\psi : \mathbb{R} \to \mathbb{C}ψ:R→C; energies, ℏ\hbarℏ, mmm, LLL are real. Derivatives are the ordinary derivative of a complex-valued function of a real variable, the second derivative being the derivative of the derivative. The equation is imposed pointwise on the open interval (0,L)(0, L)(0,L) only, with continuity on the closed interval [0,L][0, L][0,L] and differentiability at interior points; nothing is assumed about ψ\psiψ outside [0,L][0, L][0,L], so the junk values of the derivative outside the box never enter a statement. The constants ℏ,m,L\hbar, m, Lℏ,m,L are hypothesized strictly positive, so no division by zero occurs in EnE_nEn​.

The goal is not vacuous: the supporting target exhibiting ψn\psi_nψn​ shows that its hypotheses are satisfiable for every n≥1n \ge 1n≥1, so the mission cannot be closed by proving that no non-trivial stationary state exists. Conversely the non-triviality hypothesis cannot be dropped: ψ≡0\psi \equiv 0ψ≡0 solves the boundary value problem for every real EEE.

Contributions welcome: the ODE classification lemma (solutions of ψ′′=−k2ψ\psi'' = -k^2\psiψ′′=−k2ψ on an interval), orthogonality of the ψn\psi_nψn​ in L2([0,L])L^2([0,L])L2([0,L]), and the finite-well and harmonic-oscillator analogues, which are planned as later missions in this series.

Selected references

  • Schrödinger equation, Wikipedia. https://en.wikipedia.org/wiki/Schr%C3%B6dinger_equation
  • Particle in a box, Wikipedia. https://en.wikipedia.org/wiki/Particle_in_a_box
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Mathematical Physics·Captain: Lucas

Quantum Electrodynamics I: Classical Field Equations of the QED ActionTextbook

Motivation

Quantum electrodynamics (QED) is the relativistic quantum field theory of electrodynamics: it describes how light and charged matter interact, and it is the most precisely tested theory in physics, reproducing quantities such as the anomalous magnetic moment of the electron and the Lamb shift of hydrogen to many digits. Its modern covariant formulation was developed by Tomonaga, Schwinger and Feynman, with Dyson showing the equivalence of the operator and diagrammatic approaches.

Every one of those computations starts from a single classical object: the QED action, a functional of a Dirac spinor field and an electromagnetic four-potential on Minkowski space. Perturbation theory, Feynman rules, renormalization and the S-matrix are all built on top of the classical Lagrangian and the structural facts about it — the Clifford algebra of the Dirac matrices, the U(1)U(1)U(1) gauge symmetry, the conserved Noether current, and the Euler–Lagrange field equations. This mission formalizes exactly that classical layer, in the notation of the "Mathematical formulation" section of the Wikipedia article on quantum electrodynamics.

Nothing quantized is attempted here: no Fock space, no Dyson series, no renormalization. Those require a separate infrastructure and, in the interacting case, are not covered by any complete rigorous construction in four spacetime dimensions. What is formalizable today, and what this mission asks for, is the classical field theory that the quantum theory quantizes.

Setting

Spacetime is R4\mathbb{R}^4R4 with coordinates x=(x0,x1,x2,x3)x = (x^0, x^1, x^2, x^3)x=(x0,x1,x2,x3) and the Minkowski metric η\etaη of signature (+,−,−,−)(+,-,-,-)(+,−,−,−): η00=1\eta_{00} = 1η00​=1, η11=η22=η33=−1\eta_{11} = \eta_{22} = \eta_{33} = -1η11​=η22​=η33​=−1, and ημν=0\eta_{\mu\nu} = 0ημν​=0 for μ≠ν\mu \ne \nuμ=ν. Since η\etaη is its own inverse, the same array serves as the contravariant metric ημν\eta^{\mu\nu}ημν used to raise indices. The symbol ∂μ\partial_\mu∂μ​ denotes the partial derivative in the μ\muμ-th coordinate direction, and □=ημν∂μ∂ν\Box = \eta^{\mu\nu}\partial_\mu\partial_\nu□=ημν∂μ​∂ν​ is the wave operator.

The Dirac matrices are four complex 4×44\times44×4 matrices γ0,…,γ3\gamma^0,\dots,\gamma^3γ0,…,γ3 subject to the Clifford relation

γμγν+γνγμ=2ημνI4\gamma^\mu\gamma^\nu + \gamma^\nu\gamma^\mu = 2\eta^{\mu\nu} I_4γμγν+γνγμ=2ημνI4​

together with the hermiticity relation (γμ)†=γ0γμγ0(\gamma^\mu)^\dagger = \gamma^0\gamma^\mu\gamma^0(γμ)†=γ0γμγ0, which makes γ0\gamma^0γ0 hermitian and γ1,γ2,γ3\gamma^1,\gamma^2,\gamma^3γ1,γ2,γ3 anti-hermitian. The standard Dirac basis is one concrete solution of these relations.

A spinor field is a map ψ:R4→C4\psi : \mathbb{R}^4 \to \mathbb{C}^4ψ:R4→C4; its Dirac adjoint is ψˉ=ψ†γ0\bar\psi = \psi^\dagger\gamma^0ψˉ​=ψ†γ0, and for a 4×44\times44×4 matrix MMM the pairing ψˉMχ\bar\psi M \chiψˉ​Mχ is the complex number ∑i,jψi‾ (γ0M)ij χj\sum_{i,j}\overline{\psi_i}\,(\gamma^0 M)_{ij}\,\chi_j∑i,j​ψi​​(γ0M)ij​χj​. A gauge field is a map A:R4→R4A : \mathbb{R}^4 \to \mathbb{R}^4A:R4→R4 whose value Aμ(x)A_\mu(x)Aμ​(x) is the covariant component of the electromagnetic four-potential. From it one forms the field tensor (the curvature of the gauge connection)

Fμν=∂μAν−∂νAμ,Fμν=ημαηνβFαβ,F_{\mu\nu} = \partial_\mu A_\nu - \partial_\nu A_\mu, \qquad F^{\mu\nu} = \eta^{\mu\alpha}\eta^{\nu\beta}F_{\alpha\beta},Fμν​=∂μ​Aν​−∂ν​Aμ​,Fμν=ημαηνβFαβ​,

and, for a coupling constant eee, the gauge covariant derivative Dμψ=∂μψ+ieAμψD_\mu\psi = \partial_\mu\psi + ieA_\mu\psiDμ​ψ=∂μ​ψ+ieAμ​ψ. The Dirac current is Jμ=ψˉγμψJ^\mu = \bar\psi\gamma^\mu\psiJμ=ψˉ​γμψ.

With mmm the mass of the spinor field, the QED Lagrangian density is

L=ψˉ (iγμDμ−m) ψ−14FμνFμν.\mathcal{L} = \bar\psi\,(i\gamma^\mu D_\mu - m)\,\psi - \tfrac{1}{4}F_{\mu\nu}F^{\mu\nu}.L=ψˉ​(iγμDμ​−m)ψ−41​Fμν​Fμν.

Its Euler–Lagrange equations are the Dirac equation (iγμDμ−m)ψ=0(i\gamma^\mu D_\mu - m)\psi = 0(iγμDμ​−m)ψ=0 and the Maxwell equation ∂μFμν=eJν\partial_\mu F^{\mu\nu} = e J^\nu∂μ​Fμν=eJν. The Lorenz gauge condition is ημν∂μAν=0\eta^{\mu\nu}\partial_\mu A_\nu = 0ημν∂μ​Aν​=0.

Formalization targets

Goal

For a coupled solution (ψ,A)(\psi, A)(ψ,A) of the QED field equations in the Lorenz gauge, the four-potential obeys an inhomogeneous wave equation whose source is a conserved current:

□Aν=e Jνand∂νJν=0.\Box A^\nu = e\,J^\nu \qquad\text{and}\qquad \partial_\nu J^\nu = 0 .□Aν=eJνand∂ν​Jν=0.

This is the "QED version of the classical Maxwell equations in the Lorenz gauge" of the source, together with the conservation law that makes the source of that wave equation consistent. It fixes no gauge beyond Lorenz, no representation of the Dirac matrices, and no sign or normalization beyond those of the stated Lagrangian.

Supporting targets

γμγν+γνγμ=2ημνI4,(γμ)†=γ0γμγ0for the Dirac basis;\gamma^\mu\gamma^\nu+\gamma^\nu\gamma^\mu = 2\eta^{\mu\nu}I_4,\qquad (\gamma^\mu)^\dagger = \gamma^0\gamma^\mu\gamma^0 \quad\text{for the Dirac basis;}γμγν+γνγμ=2ημνI4​,(γμ)†=γ0γμγ0for the Dirac basis; ∂λFμν+∂μFνλ+∂νFλμ=0;\partial_\lambda F_{\mu\nu} + \partial_\mu F_{\nu\lambda} + \partial_\nu F_{\lambda\mu} = 0;∂λ​Fμν​+∂μ​Fνλ​+∂ν​Fλμ​=0; Fμν[A+dχ]=Fμν[A],Dμ(e−ieχψ)[A+dχ]=e−ieχDμψ[A],L[e−ieχψ,A+dχ]=L[ψ,A];F_{\mu\nu}[A + d\chi] = F_{\mu\nu}[A],\qquad D_\mu\big(e^{-ie\chi}\psi\big)\big[A + d\chi\big] = e^{-ie\chi} D_\mu\psi[A],\qquad \mathcal{L}\big[e^{-ie\chi}\psi, A + d\chi\big] = \mathcal{L}[\psi, A];Fμν​[A+dχ]=Fμν​[A],Dμ​(e−ieχψ)[A+dχ]=e−ieχDμ​ψ[A],L[e−ieχψ,A+dχ]=L[ψ,A]; ψˉγμψ∈R,∂μ(ψˉγμψ)=0  for solutions of the Dirac equation,□Aν=eJν  in Lorenz gauge.\bar\psi\gamma^\mu\psi \in \mathbb{R},\qquad \partial_\mu(\bar\psi\gamma^\mu\psi) = 0 \ \text{ for solutions of the Dirac equation},\qquad \Box A^\nu = eJ^\nu \ \text{ in Lorenz gauge.}ψˉ​γμψ∈R,∂μ​(ψˉ​γμψ)=0  for solutions of the Dirac equation,□Aν=eJν  in Lorenz gauge.

Significance

The classical layer is what every later construction quantizes. The Clifford relation is what makes the Dirac operator a square root of the wave operator; the U(1)U(1)U(1) invariance of L\mathcal{L}L is what forces the coupling to be through DμD_\muDμ​ and what makes the current conserved by Noether's theorem; conservation of JμJ^\muJμ is the consistency condition without which ∂μFμν=eJν\partial_\mu F^{\mu\nu} = eJ^\nu∂μ​Fμν=eJν has no solutions at all, since the left side is annihilated by ∂ν\partial_\nu∂ν​ identically. The Lorenz-gauge wave equation is the form in which the photon propagator is read off.

Formalizing it adds a reusable, machine-checked Minkowski-space field-theory layer: a metric with index raising, coordinate partial derivatives on R4\mathbb{R}^4R4 with a wave operator, an abstract Dirac representation together with a concrete basis satisfying it, the field tensor, the covariant derivative, the Dirac current and the QED Lagrangian. Mathlib has Clifford algebras and Fréchet calculus, but not this concrete apparatus. None of the statements in this mission is currently known to have a machine-checked proof; all are standard textbook results with well-understood proofs, so the work is formalization rather than discovery.

Difficulty

The arguments are elementary on paper and awkward in Lean for three separate reasons.

First, all index manipulation is explicit: raising an index is a sum over Fin 4\mathrm{Fin}\ 4Fin 4, and every "obvious" rearrangement of ∑μαβημαηνβ∂μ∂αAβ\sum_{\mu\alpha\beta}\eta^{\mu\alpha}\eta^{\nu\beta}\partial_\mu\partial_\alpha A_\beta∑μαβ​ημαηνβ∂μ​∂α​Aβ​ has to be done by hand with Finset.sum lemmas.

Second, differentiation is Fréchet differentiation in disguise: ∂μf\partial_\mu f∂μ​f is the derivative of fff evaluated at a basis vector, so the product rule, the sum rule and the symmetry of second derivatives each require the corresponding differentiability side conditions. The naive move of treating ∂μ\partial_\mu∂μ​ as a formal symbol that commutes with everything fails: without a C2C^2C2 hypothesis, ∂μ∂ν≠∂ν∂μ\partial_\mu\partial_\nu \ne \partial_\nu\partial_\mu∂μ​∂ν​=∂ν​∂μ​, and without differentiability the derivative takes the junk value 000, so an identity that "obviously" holds termwise may hold only under the stated smoothness assumption.

Third, the current conservation law is not a pure computation: it needs the Dirac equation, the hermiticity relation (γμ)†=γ0γμγ0(\gamma^\mu)^\dagger = \gamma^0\gamma^\mu\gamma^0(γμ)†=γ0γμγ0, and the reality of mmm, eee and AμA_\muAμ​, in the precise combination that cancels the terms containing AμA_\muAμ​ between ∂μψˉ\partial_\mu\bar\psi∂μ​ψˉ​ and ∂μψ\partial_\mu\psi∂μ​ψ. Any attempt to prove it from smoothness alone, without the equation of motion, cannot work — the current of an arbitrary smooth spinor field is not conserved.

Formalization scope

Spacetime is Fin 4 → ℝ, a gauge field is Spacetime → Fin 4 → ℝ with lower index, a spinor field is Spacetime → Fin 4 → ℂ, and the Dirac matrices are Fin 4 → Matrix (Fin 4) (Fin 4) ℂ. Sums over indices are Finset.sum over Fin 4. Partial derivatives are fderiv ℝ f x (Pi.single μ 1), which is 000 when fff is not differentiable at xxx; smoothness hypotheses are stated as ContDiff ℝ 1 or ContDiff ℝ 2 exactly where they are used. Complex conjugation is starRingEnd ℂ, matrix adjoint is Matrix.conjTranspose, and the coupling constant eee, the mass mmm and the gauge parameter χ\chiχ are real, with no positivity or nonvanishing assumption on eee or mmm.

Conventions fixed once and shared by every statement: signature (+,−,−,−)(+,-,-,-)(+,−,−,−); Dμ=∂μ+ieAμD_\mu = \partial_\mu + ieA_\muDμ​=∂μ​+ieAμ​; Fμν=∂μAν−∂νAμF_{\mu\nu} = \partial_\mu A_\nu - \partial_\nu A_\muFμν​=∂μ​Aν​−∂ν​Aμ​; Jμ=ψˉγμψJ^\mu = \bar\psi\gamma^\mu\psiJμ=ψˉ​γμψ taken as a real number via its real part, with the reality of the underlying complex pairing stated as a separate target; the Maxwell equation carries the coupling on the right-hand side as ∂μFμν=eJν\partial_\mu F^{\mu\nu} = eJ^\nu∂μ​Fμν=eJν; and the Dirac equation is ∑μiγμDμψ=mψ\sum_\mu i\gamma^\mu D_\mu\psi = m\psi∑μ​iγμDμ​ψ=mψ.

The statements are not vacuous: ψ=0\psi = 0ψ=0, A=0A = 0A=0 satisfies all field equations, plane-wave solutions of the free Dirac equation satisfy the Dirac hypothesis with A=0A = 0A=0, and the concrete Dirac basis witnesses the abstract representation hypothesis, so no hypothesis in the mission is unsatisfiable. The goal is not trivially true: it asserts a pointwise identity between second derivatives of AAA and a quadratic expression in ψ\psiψ, not an implication between definitionally equal objects.

A complete development needs Mathlib's fderiv calculus (product rule, symmetry of the second derivative via IsSymmSndFDerivAt), Finset.sum manipulation, Matrix arithmetic over ℂ, and Complex.exp. The Minkowski-space layer — metric, partial derivatives, wave operator, field tensor, Dirac representation — is reusable for any later mission on classical field theory or on the quantized theory. Contributions of further structural results in this notation (energy–momentum tensor, plane-wave solutions, the free-field propagator) are welcome as follow-up problems.

Selected references

  • Wikipedia, Quantum electrodynamics, section "Mathematical formulation". https://en.wikipedia.org/wiki/Quantum_electrodynamics
  • C. Itzykson and J.-B. Zuber, Quantum Field Theory, McGraw-Hill, 1980.
  • M. E. Peskin and D. V. Schroeder, An Introduction to Quantum Field Theory, Addison-Wesley, 1995.
  • R. P. Feynman, QED: The Strange Theory of Light and Matter, Princeton University Press, 1985.
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AnalysisMathematical Physics·Captain: Lucas

Kinetic Theory I: The Boltzmann-BGK Equation, Conservation Laws and the H-TheoremTextbook

Motivation

A gas of NNN interacting particles is described exactly by 6N6N6N coordinates, and by no useful equation. Kinetic theory replaces that description by a single scalar field, the one-particle distribution function f(x,v,t)f(x,v,t)f(x,v,t), whose evolution is governed by the Boltzmann equation. The price is the collision operator: the true Boltzmann collision integral is quadratic and five-dimensional, and almost every statement about it is hard. The BGK operator (Bhatnagar, Gross and Krook, 1954) replaces it by simple relaxation of fff towards the local Maxwellian at a fixed rate 1/τ1/\tau1/τ. It is the standard first model for rarefied gas dynamics, the basis of lattice-Boltzmann numerics, and the model in which the structural features of kinetic theory — conserved moments, an HHH-theorem, hydrodynamic closure — can be exhibited in closed form.

This mission formalizes the BGK material as it is posed in Question 1 of the Oxford MMathPhys Kinetic Theory examination paper of Hilary Term 2019: the conservation of the hydrodynamic moments by the collision operator, the sign of the entropy production together with the characterisation of equality, the slab-geometry reduction to a closed two-field system, and the vanishing of the resulting stress and heat-flux corrections at equilibrium.

Setting

Velocities and positions range over R3\mathbb R^3R3. A distribution function is a map f:R3→Rf : \mathbb R^3 \to \mathbb Rf:R3→R on velocity space (at a fixed position and time), assumed everywhere positive, integrable, and with finite second velocity moment. Particles have unit mass and the Boltzmann constant is set to 111. Its moments are

ρ[f]=∫f dv,u[f]=1ρ[f]∫v f dv,θ[f]=13ρ[f]∫∣v−u[f]∣2f dv,\rho[f] = \int f\,\mathrm dv, \qquad u[f] = \frac 1{\rho[f]}\int v\,f\,\mathrm dv, \qquad \theta[f] = \frac 1{3\rho[f]}\int |v-u[f]|^2 f\,\mathrm dv,ρ[f]=∫fdv,u[f]=ρ[f]1​∫vfdv,θ[f]=3ρ[f]1​∫∣v−u[f]∣2fdv,

the mass density, the bulk velocity and the temperature. The Maxwellian with parameters (ρ,u,θ)(\rho,u,\theta)(ρ,u,θ) is

Mρ,u,θ(v)=ρ(2πθ)3/2exp⁡(−∣v−u∣22θ),M_{\rho,u,\theta}(v) = \frac{\rho}{(2\pi\theta)^{3/2}} \exp\Big(-\frac{|v-u|^2}{2\theta}\Big),Mρ,u,θ​(v)=(2πθ)3/2ρ​exp(−2θ∣v−u∣2​),

and the local Maxwellian of fff is f(0)=Mρ[f], u[f], θ[f]f^{(0)} = M_{\rho[f],\,u[f],\,\theta[f]}f(0)=Mρ[f],u[f],θ[f]​: the Maxwellian carrying the same three moments as fff. The BGK collision operator with relaxation time τ>0\tau>0τ>0 is

C[f]=−1τ(f−f(0)),C[f] = -\frac 1\tau\big(f - f^{(0)}\big),C[f]=−τ1​(f−f(0)),

and the Boltzmann equation with this operator is

∂f∂t+v⋅∇xf=C[f].\frac{\partial f}{\partial t} + v\cdot\nabla_x f = C[f].∂t∂f​+v⋅∇x​f=C[f].

In the slab geometry of parts (c)-(d) of the source, x=(x,y,z)x=(x,y,z)x=(x,y,z), u=(u,0,0)u=(u,0,0)u=(u,0,0), v=(v,v⊥)v=(v,v_\perp)v=(v,v⊥​) with v⊥=(vy,vz)v_\perp=(v_y,v_z)v⊥​=(vy​,vz​), and fff is independent of yyy and zzz; the reduced fields are g=∫f dv⊥g=\int f\,\mathrm dv_\perpg=∫fdv⊥​ and h=∫∣v⊥∣2f dv⊥h=\int |v_\perp|^2 f\,\mathrm dv_\perph=∫∣v⊥​∣2fdv⊥​.

Formalization targets

Goal — the BGK HHH-theorem with its equality case

∫dv (log⁡f) C[f]≤0,with equality iff f=f(0) almost everywhere.\int \mathrm dv\,(\log f)\,C[f] \le 0, \qquad\text{with equality iff } f = f^{(0)} \text{ almost everywhere.}∫dv(logf)C[f]≤0,with equality iff f=f(0) almost everywhere.

This is part (b) of the source question, including the answer to "under what conditions does equality hold". It is stated for every admissible fff and every τ>0\tau>0τ>0; it fixes no rate and no constant, so it is not invalidated by sharper quantitative versions.

Milestones

  1. The Gaussian moments of Mρ,u,θM_{\rho,u,\theta}Mρ,u,θ​: mass ρ\rhoρ, momentum ρu\rho uρu, and central second moment 3ρθ3\rho\theta3ρθ; consequently Mρ,u,θM_{\rho,u,\theta}Mρ,u,θ​ is its own local Maxwellian.
  2. Part (a): ∫C[f] dv=0\int C[f]\,\mathrm dv = 0∫C[f]dv=0, ∫v C[f] dv=0\int v\,C[f]\,\mathrm dv = 0∫vC[f]dv=0, ∫∣v∣2C[f] dv=0\int |v|^2 C[f]\,\mathrm dv = 0∫∣v∣2C[f]dv=0 — the conservation of ρ\rhoρ, uuu and θ\thetaθ by the collision operator.
  3. The inequality of part (b) on its own.
  4. Maxwellians, viewed as xxx- and ttt-independent distributions, solve the BGK equation.
  5. Part (c): ∫M dv⊥=g(0)\int M\,\mathrm dv_\perp = g^{(0)}∫Mdv⊥​=g(0) and ∫∣v⊥∣2M dv⊥=2θ g(0)\int |v_\perp|^2 M\,\mathrm dv_\perp = 2\theta\,g^{(0)}∫∣v⊥​∣2Mdv⊥​=2θg(0), where g(0)(v)=ρ(2πθ)−1/2exp⁡(−(v−u)2/2θ)g^{(0)}(v)=\rho(2\pi\theta)^{-1/2}\exp(-(v-u)^2/2\theta)g(0)(v)=ρ(2πθ)−1/2exp(−(v−u)2/2θ), together with the expressions for ρ\rhoρ, uuu, θ\thetaθ in the reduced system.
  6. Part (d): the quantities T=−2ρθ+∫h dvT = -2\rho\theta + \int h\,\mathrm dvT=−2ρθ+∫hdv and q=12∫w3g dv+12∫w h dvq = \tfrac12\int w^3 g\,\mathrm dv + \tfrac12\int w\,h\,\mathrm dvq=21​∫w3gdv+21​∫whdv (with w=v−uw=v-uw=v−u) vanish when g=g(0)g=g^{(0)}g=g(0) and h=h(0)h=h^{(0)}h=h(0).

Significance

The three conservation identities say that the BGK operator, however crude as a model of binary collisions, respects the exact conservation laws of the gas: they are what makes the moment hierarchy of the BGK equation reduce to the Euler equations at leading order. The entropy inequality is the model's HHH-theorem: it forces the entropy −∫flog⁡f dv-\int f\log f\,\mathrm dv−∫flogfdv to be non-decreasing under collisions and singles out the Maxwellians as the only collisional equilibria, which is the statement that fixes the direction of time in the model. The slab reduction of part (c) is the standard device by which a three-dimensional kinetic problem is reduced to a pair of one-dimensional kinetic equations, used throughout computational rarefied gas dynamics; part (d) identifies exactly which moments of the reduced fields carry the non-equilibrium stress and heat flux.

Formalizing this material requires building the moment calculus of Gaussians on R3\mathbb R^3R3 against Lebesgue measure — normalisation, first and central second moments, and the partial integration over two of the three velocity components — none of which exists in Mathlib in a form adapted to kinetic theory. The mathematics is classical and the proofs are known; the work is in the analysis bookkeeping: integrability of moments, dominated convergence, and the a.e. equality case of a strict pointwise inequality.

Difficulty

The obvious computation for the HHH-theorem — expand ∫(log⁡f)(f−f(0))\int (\log f)(f-f^{(0)})∫(logf)(f−f(0)) and integrate term by term — does not by itself give a sign: log⁡f\log flogf has no sign, and neither does f−f(0)f - f^{(0)}f−f(0). The argument needs the conservation identities as an input, because they are what allows log⁡f(0)\log f^{(0)}logf(0), which is a quadratic polynomial in vvv, to be subtracted for free. Only then is the integrand pointwise of one sign. Formally, the obstacle is that none of the pieces of the integrand is separately integrable in general: the statements are formulated with the integrability of the entropy-production integrand as an explicit hypothesis, and any splitting of it must be justified.

The equality case adds a second difficulty. Vanishing of the integral of a non-negative integrable function gives vanishing only almost everywhere, so the conclusion is an a.e. identity f=f(0)f = f^{(0)}f=f(0), and the strictness of (log⁡a−log⁡b)(a−b)>0(\log a - \log b)(a-b) > 0(loga−logb)(a−b)>0 for a≠ba \ne ba=b must be used pointwise.

Formalization scope

Velocity space is EuclideanSpace ℝ (Fin 3) with its Lebesgue (volume) measure, and integrals are Bochner integrals; vector-valued moments are integrals of EuclideanSpace-valued functions. Distribution functions are total functions R3→R\mathbb R^3 \to \mathbb RR3→R with no measurability packaged into the type, so every statement carries its own integrability hypotheses; admissibility (positivity everywhere, integrability, finite second moment) is bundled in a predicate. The Maxwellian prefactor is written with a real power (2πθ)3/2(2\pi\theta)^{3/2}(2πθ)3/2, so θ>0\theta>0θ>0 is required wherever it appears. The relaxation time satisfies τ>0\tau>0τ>0.

Two traps are worth naming. First, in Lean the integral of a non-integrable function is 000 by convention, so an entropy inequality stated without an integrability hypothesis would be satisfiable for trivial reasons; the goal therefore assumes the entropy-production integrand is integrable, and states the equality case as an iff, which is not satisfiable by a degenerate reading. Second, the local Maxwellian is defined from the moments of fff itself, not from externally supplied parameters, so none of the conservation statements can be discharged by choosing convenient parameters.

The slab-geometry part of the mission is developed in its own definition file, with the perpendicular velocity in EuclideanSpace ℝ (Fin 2) and the reduced fields as functions R→R\mathbb R\to\mathbb RR→R. The Gaussian moment lemmas produced here are reusable for any Maxwellian-based kinetic model; contributions that add Mathlib-level lemmas on Gaussian moments in Rn\mathbb R^nRn, rather than ad-hoc computations, are especially welcome.

Selected references

  • P. L. Bhatnagar, E. P. Gross, M. Krook, A model for collision processes in gases. I. Small amplitude processes in charged and neutral one-component systems, Physical Review 94 (1954) 511-525. https://doi.org/10.1103/PhysRev.94.511
  • C. Cercignani, The Boltzmann Equation and Its Applications, Applied Mathematical Sciences 67, Springer, 1988. https://doi.org/10.1007/978-1-4612-1039-9
  • Oxford MMathPhys Kinetic Theory examination paper A15089W1, Hilary Term 2019, Question 1. https://web.archive.org/web/20250913150648/https://mmathphys.physics.ox.ac.uk/sites/default/files/mmathphys/documents/media/kt_2019.pdf
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Mathematical Physics·Captain: Lucas

Laplace's Tidal Equations: normal modes and the energy budgetResearch Paper

Why the tides need their own equations

The rise and fall of the ocean surface under the gravitational pull of the moon and the sun is the oldest quantitative problem in physical oceanography, and it is still a working one: satellite altimetry can only see ocean circulation after the tidal signal has been removed, and the removal is done with a numerical solution of Laplace's tidal equations (LTE) constrained by tide-gauge and altimeter data (Le Provost et al., J. Geophys. Res. 99 (1994) 24777). The same equations carry the global tidal energy budget: an estimate of where the roughly 3.5 TW of tidal energy is dissipated — shallow-sea bottom drag versus conversion into internal tides over deep-ocean topography — is obtained by integrating the energy identity of these equations against observed elevation data (Egbert and Ray, Nature 405 (2000) 775).

The material formalized here is M. Hendershott, Lecture 3: Solutions to Laplace's Tidal Equations (Woods Hole Oceanographic Institution, Geophysical Fluid Dynamics Program lecture notes, pp. 34–44), notes taken by V. Birman and E. Williams Frajka. The lecture states the separable normal-mode solutions of the stratified problem, the solid Earth tide and the Love number decomposition, models of dissipation, coastal boundary conditions, and finally the energy equation of the tides, both ignoring and including the yielding of the solid Earth.

Setting

Write u(x,y,t)u(x,y,t)u(x,y,t) and v(x,y,t)v(x,y,t)v(x,y,t) for the two components of the depth-independent horizontal velocity, ζ(x,y,t)\zeta(x,y,t)ζ(x,y,t) for the free-surface elevation, δ(x,y,t)\delta(x,y,t)δ(x,y,t) for the solid Earth tide (the elastic displacement of the crust under the tidal load), and ζ0=ζ−δ\zeta_0 = \zeta - \deltaζ0​=ζ−δ for the observed, geocentric tide. The ocean has resting depth D(x,y)>0D(x,y) > 0D(x,y)>0, constant density ρ>0\rho > 0ρ>0, gravity ggg, and constant Coriolis parameter fff. The astronomical forcing enters through the tide generating potential Γ(x,y,t)\Gamma(x,y,t)Γ(x,y,t) and the dissipation through a force per unit area (Fx,Fy)(F^x, F^y)(Fx,Fy).

Laplace's tidal equations are the two momentum equations

ut−fv=−g(ζ−Γg)x+FxρD,vt+fu=−g(ζ−Γg)y+FyρD,u_t - f v = -g\left(\zeta - \tfrac{\Gamma}{g}\right)_x + \frac{F^x}{\rho D}, \qquad v_t + f u = -g\left(\zeta - \tfrac{\Gamma}{g}\right)_y + \frac{F^y}{\rho D},ut​−fv=−g(ζ−gΓ​)x​+ρDFx​,vt​+fu=−g(ζ−gΓ​)y​+ρDFy​,

together with the continuity equation, which in the presence of the solid Earth tide reads

(ζ−δ)t+(uD)x+(vD)y=0.(\zeta - \delta)_t + (uD)_x + (vD)_y = 0 .(ζ−δ)t​+(uD)x​+(vD)y​=0.

For a stratified ocean the same system arises mode by mode after separation of variables, with DDD replaced by the equivalent depth DnD_nDn​ of the nnn-th mode and the vertical structure Fw(z)F_w(z)Fw​(z) solving Fwzz+(N2/(gDn))Fw=0F_{wzz} + (N^2/(gD_n))F_w = 0Fwzz​+(N2/(gDn​))Fw​=0, where N(z)N(z)N(z) is the buoyancy frequency.

Formalization targets

Goal — the energy equation including the solid Earth tide (eqs. (35)–(39))

KEt+PEt+∇⋅P⃗  =  Wt+u⃗⋅F⃗,\mathrm{KE}_t + \mathrm{PE}_t + \nabla\cdot \vec{P} \;=\; W_t + \vec{u}\cdot \vec{F},KEt​+PEt​+∇⋅P=Wt​+u⋅F,

with

KE=12ρD(u2+v2),PE=12ρg (ζ02+2ζ0δ+2δD),P⃗=ρgDu⃗(ζ0+δ),\mathrm{KE} = \tfrac12\rho D (u^2+v^2), \quad \mathrm{PE} = \tfrac12\rho g\,(\zeta_0^2 + 2\zeta_0\delta + 2\delta D), \quad \vec{P} = \rho g D \vec{u}(\zeta_0+\delta),KE=21​ρD(u2+v2),PE=21​ρg(ζ02​+2ζ0​δ+2δD),P=ρgDu(ζ0​+δ), Wt=ρ ζ0tΓ+ρ ∇⋅(u⃗DΓ)+ρg(ζ0+D)δt.W_t = \rho\,\zeta_{0t}\Gamma + \rho\,\nabla\cdot(\vec{u}D\Gamma) + \rho g(\zeta_0 + D)\delta_t .Wt​=ρζ0t​Γ+ρ∇⋅(uDΓ)+ρg(ζ0​+D)δt​.

This is a pointwise identity, valid at every (x,y,t)(x,y,t)(x,y,t) for every solution of the equations above, with variable depth D(x,y)D(x,y)D(x,y) and no assumption on the form of the dissipation.

Supporting targets

The milestone list covers the corresponding identity with the solid Earth tide ignored (eqs. (29)–(30)), the two normal-mode facts of §2 — the vertical structure equation with the equivalent depth DnD_nDn​ (eq. (4)) and the nonrotating barotropic plane wave with its dispersion relation σ=±kgD∗\sigma = \pm k\sqrt{gD_*}σ=±kgD∗​​ (§2.1) — and the two averaging statements of §6: that the period mean of the time derivative of a periodic energy density vanishes (eq. (31)) and the resulting period-averaged balance ∇⋅⟨P⟩=⟨Wt⟩+⟨u⃗⋅F⃗⟩\nabla\cdot\langle P\rangle = \langle W_t\rangle + \langle \vec{u}\cdot\vec{F}\rangle∇⋅⟨P⟩=⟨Wt​⟩+⟨u⋅F⟩ (eq. (32)).

Significance

The energy identity is what converts elevation observations into a dissipation estimate: averaged over a tidal period and integrated over a basin with no flux through its boundary, the flux divergence drops out and the work done by the tide generating potential equals the dissipation, so ∫⟨u⃗⋅F⃗⟩\int \langle \vec{u}\cdot\vec{F}\rangle∫⟨u⋅F⟩ is computable from ζ0\zeta_0ζ0​ alone. Every term in that chain — which terms are exact, which vanish only on average, which require the Love numbers to be real — is a hypothesis that a formal statement has to carry explicitly, and the lecture is explicit that the identity holds "provided that the Love numbers are real", i.e. provided the solid Earth tide is dissipation-free.

Formalizing this material produces a reusable model of a rotating shallow-water system with forcing, dissipation and an elastic bottom boundary, together with the calculus lemmas needed to differentiate products of fields of several variables. Nothing here is an open problem: the results are classical, and the contribution is a machine-checked derivation from a precisely stated model, including the bookkeeping that textbook derivations compress.

Difficulty

The obstacle is not depth of argument but faithfulness of the model. The derivation multiplies the two momentum equations by ρuD\rho u DρuD and ρvD\rho v DρvD, the continuity equation by ρgζ\rho g \zetaρgζ, and adds; every step needs a product rule for a field of three variables, and the Coriolis terms must cancel exactly rather than approximately. Two places in the source require care before they can be formalized: equation (29) prints the surface term with coefficient 1gρg\tfrac1g \rho gg1​ρg, and the printed PEtPE_tPEt​ in §6.1 has signs that do not follow from the printed PEPEPE; the identities are true with 12ρg(ζ2)t\tfrac12\rho g(\zeta^2)_t21​ρg(ζ2)t​ and PEt=ρg(ζζt−δδt+Dδt)PE_t = \rho g(\zeta\zeta_t - \delta\delta_t + D\delta_t)PEt​=ρg(ζζt​−δδt​+Dδt​) respectively. The potential energy (37) also differs from ∫−D+δζρgz dz\int_{-D+\delta}^{\zeta}\rho g z\,dz∫−D+δζ​ρgzdz by a term independent of time, which is invisible in PEtPE_tPEt​ and therefore harmless. A naive formalization that copies the printed formulas without checking these will state something false.

Formalization scope

Fields are real-valued functions of xxx, yyy and ttt; partial derivatives are Lean's one-dimensional deriv applied slot-wise, and differentiability is imposed as an explicit hypothesis in each variable separately, rather than through Fréchet derivatives. Depth is a function D(x,y)D(x,y)D(x,y) that does not depend on time, and positivity of ρ\rhoρ and DDD is assumed where the momentum equations are divided by ρD\rho DρD. The equations themselves are packaged as a structure with three fields, one per equation, so that a solution is an explicit witness rather than an assumption schema; this rules out a vacuous reading, since constant fields with zero forcing satisfy the structure. The barotropic plane wave of §2.1 is stated with complex-valued ZZZ and UUU and the physical normalization a≠0a \neq 0a=0, σ≠0\sigma \neq 0σ=0, and is an equivalence: the wave solves the system exactly when σ=±kgD∗\sigma = \pm k\sqrt{gD_*}σ=±kgD∗​​. The vertical mode statement uses the rigid-lid conditions Fw(−D∗)=Fw(0)=0F_w(-D_*) = F_w(0) = 0Fw​(−D∗​)=Fw​(0)=0; the lecture's free-surface condition Fw−DnFwz=0F_w - D_n F_{wz} = 0Fw​−Dn​Fwz​=0 at z=0z = 0z=0 is satisfied by the sine modes only in the limit of small equivalent depth, and is not claimed. Period averaging is formalized as 1T∫0T\frac1T\int_0^TT1​∫0T​ of an interval integral at a fixed horizontal position, with periodicity and continuity of the relevant time derivative as hypotheses.

Contributions extending this mission are welcome in three directions: the derivation of the equations from the linearized Euler equations of Lecture 2, the solid Earth tide of §3 with the Love number decomposition (17)–(20), and the basin-integrated form of the energy budget (33), which needs a divergence theorem for the flux term.

Selected references

  • M. Hendershott, Lecture 3: Solutions to Laplace's Tidal Equations, WHOI GFD Program lecture notes, pp. 34–44. PDF
  • C. Le Provost, M. L. Genco, F. Lyard, P. Vincent, P. Canceil, "Spectroscopy of the world ocean tides from a finite element hydrodynamic model", J. Geophys. Res. 99 (1994) 24777. DOI
  • G. D. Egbert, R. D. Ray, "Significant dissipation of tidal energy in the deep ocean inferred from satellite altimeter data", Nature 405 (2000) 775. DOI
  • W. E. Farrell, "Deformation of the Earth by surface loads", Rev. Geophys. 10 (1972) 761. DOI
7 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
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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).
31 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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Actuarial ScienceOperations ResearchStochastic Systems·Captain: mikedeng1

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.
22 thms1 active userReviewed
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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🏆Completed
Harmonic Analysis·Captain: Mazecto

Calderón–Zygmund Theory and the L^p Estimate for the Cauchy–Riemann OperatorTextbook

Motivation

The Cauchy–Riemann operator ∂ˉ=∂s+i ∂t\bar\partial=\partial_s+i\,\partial_t∂ˉ=∂s​+i∂t​ on C\mathbb{C}C is the model elliptic operator of symplectic topology: pseudoholomorphic curves solve nonlinear perturbations of ∂ˉu=0\bar\partial u=0∂ˉu=0, and their regularity, compactness and Fredholm theory all start from an LpL^pLp a priori estimate for ∂ˉ\bar\partial∂ˉ. In Hofer–Wysocki–Zehnder's asymptotic analysis of pseudoholomorphic curves in symplectisations, this estimate appears as formula (49): on a disc BBB of radius RRR, every smooth map φ\varphiφ supported in the interior of BBB satisfies

∥φ∥Wk,p(B)≤M(k,p,R) ∥∂ˉφ∥Wk−1,p(B),k≥1, p>1.\|\varphi\|_{W^{k,p}(B)}\le M(k,p,R)\,\|\bar\partial\varphi\|_{W^{k-1,p}(B)},\qquad k\ge1,\ p>1 .∥φ∥Wk,p(B)​≤M(k,p,R)∥∂ˉφ∥Wk−1,p(B)​,k≥1, p>1.

Hofer–Wysocki–Zehnder cite it from E. M. Stein's Singular Integrals and Differentiability Properties of Functions and from Abbas–Hofer's Holomorphic Curves and Global Questions in Contact Geometry.

This mission formalizes estimate (49), together with the core of the real-variable theory of singular integrals on Rd\mathbb{R}^dRd from Stein, Chapters I–III, and the L2L^2L2 and LpL^pLp estimates for ar\partial of Abbas–Hofer, § 4.2. None of these results is in Mathlib, which has no Hardy–Littlewood maximal function, no Calderón–Zygmund decomposition, no Marcinkiewicz interpolation theorem and no LpL^pLp theory of singular integral operators.

Setting

  • Rd\mathbb{R}^dRd carries Lebesgue measure mmm, and ∥⋅∥p\|\cdot\|_p∥⋅∥p​ is the Lp(Rd)L^p(\mathbb{R}^d)Lp(Rd) norm for complex-valued functions.
  • Maximal function. Mf(x)=sup⁡r>0m(B(x,r))−1∫B(x,r)∣f∣∈[0,∞]Mf(x)=\sup_{r>0}m(B(x,r))^{-1}\int_{B(x,r)}|f|\in[0,\infty]Mf(x)=supr>0​m(B(x,r))−1∫B(x,r)​∣f∣∈[0,∞].
  • Weak type. An operator TTT is of weak type (q,q)(q,q)(q,q), q<∞q<\inftyq<∞, if m{∣Tf∣>α}≤(A∥f∥q/α)qm\{|Tf|>\alpha\}\le(A\|f\|_q/\alpha)^qm{∣Tf∣>α}≤(A∥f∥q​/α)q for all α>0\alpha>0α>0, and of strong type (p,p)(p,p)(p,p) if ∥Tf∥p≤A∥f∥p\|Tf\|_p\le A\|f\|_p∥Tf∥p​≤A∥f∥p​.
  • Truncated singular integrals. For a kernel KKK on Rd∖{0}\mathbb{R}^d\setminus\{0\}Rd∖{0} and ε>0\varepsilon>0ε>0, Tεf(x)=∫∣y∣≥εf(x−y)K(y) dyT_\varepsilon f(x)=\int_{|y|\ge\varepsilon}f(x-y)K(y)\,dyTε​f(x)=∫∣y∣≥ε​f(x−y)K(y)dy.
  • Cauchy–Riemann operator. For φ:C→Cn\varphi:\mathbb{C}\to\mathbb{C}^nφ:C→Cn and z=s+itz=s+itz=s+it, ∂ˉφ=φs+iφt\bar\partial\varphi=\varphi_s+i\varphi_t∂ˉφ=φs​+iφt​ (without the factor 12\tfrac1221​).
  • Sobolev norms of smooth maps on a set U⊂CU\subset\mathbb{C}U⊂C: ∥φ∥Wk,p(U)=∑j≤k∥Djφ∥Lp(U)\|\varphi\|_{W^{k,p}(U)}=\sum_{j\le k}\|D^j\varphi\|_{L^p(U)}∥φ∥Wk,p(U)​=∑j≤k​∥Djφ∥Lp(U)​, where DjφD^j\varphiDjφ is the jjj-th derivative.

Formalization targets

Goal: the Wk,pW^{k,p}Wk,p estimate for ∂ˉ\bar\partial∂ˉ on a disc

For an integer k≥1k\ge1k≥1, p>1p>1p>1 and R>0R>0R>0 there is M=M(k,p,R)M=M(k,p,R)M=M(k,p,R) such that for every disc B⊂CB\subset\mathbb{C}B⊂C of radius RRR and every smooth φ:C→Cn\varphi:\mathbb{C}\to\mathbb{C}^nφ:C→Cn supported in the interior of BBB, ∥φ∥Wk,p(B)≤M∥∂ˉφ∥Wk−1,p(B)\|\varphi\|_{W^{k,p}(B)}\le M\|\bar\partial\varphi\|_{W^{k-1,p}(B)}∥φ∥Wk,p(B)​≤M∥∂ˉφ∥Wk−1,p(B)​ (Hofer–Wysocki–Zehnder I, estimate (49), p. 366).

Milestones

  1. Maximal theorem. MfMfMf is finite a.e. for f∈Lpf\in L^pf∈Lp, 1≤p≤∞1\le p\le\infty1≤p≤∞; MMM is of weak type (1,1)(1,1)(1,1) and of strong type (p,p)(p,p)(p,p) for 1<p≤∞1<p\le\infty1<p≤∞ (Stein I, § 1.3, Theorem 1).
  2. Calderón–Zygmund decomposition. A non-negative integrable fff and a height α>0\alpha>0α>0 give Rd=F∪Ω\mathbb{R}^d=F\cup\OmegaRd=F∪Ω with f≤αf\le\alphaf≤α a.e. on FFF and Ω\OmegaΩ a union of cubes with disjoint interiors on which the average of fff lies in (α,2dα](\alpha,2^d\alpha](α,2dα] (Stein I, § 3.2, Theorem 4).
  3. Marcinkiewicz interpolation theorem. A sub-additive operator of weak types (1,1)(1,1)(1,1) and (r,r)(r,r)(r,r), 1<r≤∞1<r\le\infty1<r≤∞, is of strong type (p,p)(p,p)(p,p) for 1<p<r1<p<r1<p<r (Stein I, § 4.2, Theorem 5).
  4. Convolution kernels with bounded Fourier transform. If K∈L2K\in L^2K∈L2, ∣K^∣≤B|\hat K|\le B∣K^∣≤B and ∣∇K(x)∣≤B∣x∣−d−1|\nabla K(x)|\le B|x|^{-d-1}∣∇K(x)∣≤B∣x∣−d−1, then f↦K∗ff\mapsto K*ff↦K∗f is bounded on LpL^pLp, 1<p<∞1<p<\infty1<p<∞, with a constant depending only on ppp, BBB, ddd (Stein II, § 2.2, Theorem 1).
  5. Truncated singular integrals. If ∣K(x)∣≤B∣x∣−d|K(x)|\le B|x|^{-d}∣K(x)∣≤B∣x∣−d, ∫∣x∣≥2∣y∣∣K(x−y)−K(x)∣ dx≤B\int_{|x|\ge2|y|}|K(x-y)-K(x)|\,dx\le B∫∣x∣≥2∣y∣​∣K(x−y)−K(x)∣dx≤B and KKK has integral zero over every annulus, then the truncations TεT_\varepsilonTε​ are bounded on LpL^pLp uniformly in ε\varepsilonε and converge in LpL^pLp as ε→0\varepsilon\to0ε→0 (Stein II, § 3.2, Theorem 2).
  6. Homogeneous kernels. The same conclusion for K(y)=Ω(y)/∣y∣dK(y)=\Omega(y)/|y|^dK(y)=Ω(y)/∣y∣d with Ω\OmegaΩ homogeneous of degree 000, of mean zero on the unit sphere and Dini-continuous there (Stein II, § 4.2, Theorem 3 (a), (b)).
  7. The Cauchy–Riemann estimate on the plane. ∥∂1f∥p+∥∂2f∥p≤Ap∥∂1f+i∂2f∥p\|\partial_1f\|_p+\|\partial_2f\|_p\le A_p\|\partial_1f+i\partial_2f\|_p∥∂1​f∥p​+∥∂2​f∥p​≤Ap​∥∂1​f+i∂2​f∥p​ for compactly supported C1C^1C1 functions f:R2→Cf:\mathbb{R}^2\to\mathbb{C}f:R2→C, 1<p<∞1<p<\infty1<p<∞ (Stein III, § 1.3, Proposition 4).
  8. L2L^2L2 identity. ∥∂ˉφ∥L22=∥φs∥L22+∥φt∥L22\|\bar\partial\varphi\|_{L^2}^2=\|\varphi_s\|_{L^2}^2+\|\varphi_t\|_{L^2}^2∥∂ˉφ∥L22​=∥φs​∥L22​+∥φt​∥L22​ for smooth compactly supported φ:C→Cn\varphi:\mathbb{C}\to\mathbb{C}^nφ:C→Cn (Abbas–Hofer, § 4.2, (4.4)).
  9. L2L^2L2 estimate on a disc. ∥φs∥L22+∥φt∥L22+∥φ∥L22≤(4R2+1)∥∂ˉφ∥L22\|\varphi_s\|_{L^2}^2+\|\varphi_t\|_{L^2}^2+\|\varphi\|_{L^2}^2\le(4R^2+1)\|\bar\partial\varphi\|_{L^2}^2∥φs​∥L22​+∥φt​∥L22​+∥φ∥L22​≤(4R2+1)∥∂ˉφ∥L22​ for φ\varphiφ with compact support in BR(0)B_R(0)BR​(0) (Abbas–Hofer, Theorem 4.2.1).
  10. LpL^pLp estimate on a disc. ∥φ∥W1,p≤c(p,R)∥∂ˉφ∥Lp\|\varphi\|_{W^{1,p}}\le c(p,R)\|\bar\partial\varphi\|_{L^p}∥φ∥W1,p​≤c(p,R)∥∂ˉφ∥Lp​ for φ\varphiφ with compact support in BR(0)B_R(0)BR​(0), 1<p<∞1<p<\infty1<p<∞ (Abbas–Hofer, Theorem 4.2.2).

Significance

The result. The Wk,pW^{k,p}Wk,p estimate for ∂ˉ\bar\partial∂ˉ is the analytic input behind elliptic bootstrapping for pseudoholomorphic curves: interior regularity, C∞C^\inftyC∞ bounds from gradient bounds, removal of singularities, and the Fredholm theory of linearized Cauchy–Riemann operators on Sobolev spaces. In Hofer–Wysocki–Zehnder's work it controls the derivatives of pseudoholomorphic half-cylinders near a nondegenerate periodic orbit.

Formalizing it. The milestones from Stein are the standard real-variable toolkit of harmonic analysis on Rd\mathbb{R}^dRd: the maximal theorem, the Calderón–Zygmund decomposition, Marcinkiewicz interpolation and the LpL^pLp theory of singular integrals with smooth or homogeneous kernels. None of them is in Mathlib, and each is reusable well beyond this mission, for instance for elliptic estimates of other operators, Sobolev embeddings in LpL^pLp, and other LpL^pLp estimates.

Difficulty

The statements are quantitative and the order of quantifiers matters: the constants are chosen before the functions, and in milestones 3 and 4 also before the operator or the kernel, with the dependence stated by the source. Several objects take infinite values or are defined only almost everywhere: the maximal function is valued in [0,∞][0,\infty][0,∞], the case r=∞r=\inftyr=∞ of the interpolation theorem uses a strong-type bound in place of a weak-type one, and the singular integrals are limits in LpL^pLp of absolutely convergent truncated integrals. The Dini condition on Ω\OmegaΩ is a condition on a supremum over pairs of points of the unit sphere. The Cauchy–Riemann statements involve vector-valued maps C→Cn\mathbb{C}\to\mathbb{C}^nC→Cn, real derivatives of all orders and Sobolev norms on discs.

Formalization scope

  • Namespace DbarRegularity. The definition module DbarRegularity_Setting defines maximalFunction, closedCube, dbar and sobolevNorm. The mission is standalone and imports no definitions from other missions.
  • Spaces. Rd\mathbb{R}^dRd is EuclideanSpace ℝ (Fin d) with volume, functions on it are complex-valued, R2\mathbb{R}^2R2 in milestone 7 is EuclideanSpace ℝ (Fin 2), and Cn\mathbb{C}^nCn is EuclideanSpace ℂ (Fin n). Stein's dimension is written ddd throughout, and nnn is the dimension of the target Cn\mathbb{C}^nCn.
  • Norms and exponents. LpL^pLp norms are eLpNorm in ℝ≥0∞. Exponents 1<p<∞1<p<\infty1<p<∞ are real and enter as ENNReal.ofReal p; exponents allowed to be infinite are in ℝ≥0∞. Constants are in ℝ≥0 or ℝ, never in ℝ≥0∞.
  • Derivatives. φs\varphi_sφs​, φt\varphi_tφt​ are fderiv ℝ φ z 1, fderiv ℝ φ z Complex.I; smoothness is ContDiff ℝ ∞ (C∞C^\inftyC∞, not analytic); higher derivatives are iteratedFDeriv ℝ j. Supports are tsupport.
  • Limits. Limits as ε→0\varepsilon\to0ε→0 are along 𝓝[>] 0, in the LpL^pLp seminorm.

Contributions welcome: reusable general lemmas of real-variable harmonic analysis on Rd\mathbb{R}^dRd, and calculus lemmas for smooth compactly supported maps on C\mathbb{C}C.

Selected references

  • E. M. Stein, Singular Integrals and Differentiability Properties of Functions, Princeton Mathematical Series 30, Princeton University Press (1970), Chapters I–III. ISBN 0-691-08079-8.
  • C. Abbas, H. Hofer, Holomorphic Curves and Global Questions in Contact Geometry, Birkhäuser Advanced Texts Basler Lehrbücher, Birkhäuser (2019), § 4.2. https://doi.org/10.1007/978-3-030-11803-7
  • H. Hofer, K. Wysocki, E. Zehnder, Properties of pseudoholomorphic curves in symplectisations I: asymptotics, Ann. Inst. H. Poincaré Anal. Non Linéaire 13(3) (1996), 337–379. http://www.numdam.org/item/AIHPC_1996__13_3_337_0/
  • A. P. Calderón, A. Zygmund, On the existence of certain singular integrals, Acta Math. 88 (1952), 85–139. https://doi.org/10.1007/BF02392130
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