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Differential Geometry·Captain: wurtle

A Smooth Metric with No Local Isometric Immersion into Three-SpaceResearch Paper

Motivation: can every surface be realized locally in R3\mathbb R^3R3?

A Riemannian surface is abstract: it is given by a rule ggg for measuring lengths and angles in local coordinates, not as a surface sitting in space. The local isometric realization problem asks whether every such surface can, near each point, be realized as an honest smooth surface in Euclidean three-space with the same lengths. The question goes back to the classical theory of surfaces. It is settled for real-analytic metrics and for smooth metrics with nonvanishing curvature, while the unrestricted smooth case is listed as open by Yau (Yau 2000, p. 236) and in Ghomi's problem survey (Ghomi 2019, §1.5, Problem 1.9).

Timeline

  • 1926–1927 — Janet and Cartan: every real-analytic surface metric is locally realizable analytically in R3\mathbb R^3R3 (Janet 1926; Cartan 1927).
  • 1954–1955 — Nash and Kuiper: C1C^1C1 isometric realizations exist with great flexibility (Nash 1954; Kuiper 1955). At C1C^1C1 regularity there is no curvature constraint.
  • 1971 — Pogorelov constructs a C2,1C^{2,1}C2,1 metric with no local C2C^2C2 realization (Pogorelov 1971).
  • 1985–1986 — C.-S. Lin: local realization for nonnegative curvature and for curvature changing sign cleanly, with finite differentiability (Lin 1985; Lin 1986).
  • 1989 — Nakamura and Maeda: smooth local existence when the curvature changes sign cleanly (Trans. AMS 1989).
  • 2002 — A Nadirashvili–Yuan preprint states a smooth counterexample with K≤0K\le0K≤0 (arXiv:math/0208127); their published 2008 paper instead proves a C2,1C^{2,1}C2,1 counterexample with K≥0K\ge0K≥0 and leaves the smooth question open (Calc. Var. PDE 2008).
  • 2007–2009 — Khuri: counterexamples to local solvability for general Monge–Ampère equations (CPDE 2007), and work on Darboux's equation that leaves the needed curvature profile open (Khuri 2009).
  • 2010–2016 — Positive results under finite-order conditions on the curvature zero set (Han–Khuri 2010; T.-Y. Lin 2016).
  • 2026 — An OpenAI preprint, A Smooth Metric with No Local Isometric Immersion into Three-Space (OpenAI Math Release, September 24, 2026), claims a smooth metric on (−1,1)2(-1,1)^2(−1,1)2 that has no smooth isometric immersion on any neighborhood of the origin. It has not been peer reviewed, and the claim has not been formally verified.

Setting

Work in coordinates p=(p1,p2)p=(p_1,p_2)p=(p1​,p2​) on the open square Q=(−1,1)2⊂R2Q=(-1,1)^2\subset\mathbb R^2Q=(−1,1)2⊂R2. A Riemannian metric on QQQ is a map p↦g(p)p\mapsto g(p)p↦g(p) to symmetric 2×22\times22×2 real matrices that are positive definite; it is C∞C^\inftyC∞ if every entry gijg_{ij}gij​ is smooth. An isometric immersion of (U,g)(U,g)(U,g), for an open set U⊆QU\subseteq QU⊆Q, is a map F:U→R3F:U\to\mathbb R^3F:U→R3 whose differential reproduces ggg:

⟨dFp(v), dFp(w)⟩R3=vTg(p) w(p∈U, v,w∈R2),\langle dF_p(v),\,dF_p(w)\rangle_{\mathbb R^3}=v^{\mathsf T} g(p)\,w\qquad(p\in U,\ v,w\in\mathbb R^2),⟨dFp​(v),dFp​(w)⟩R3​=vTg(p)w(p∈U, v,w∈R2),

equivalently ⟨∂iF,∂jF⟩=gij\langle\partial_iF,\partial_jF\rangle=g_{ij}⟨∂i​F,∂j​F⟩=gij​. Positive definiteness forces dFdFdF to have rank 222. In Lean, Coord = Fin 2 → ℝ, Ambient = EuclideanSpace ℝ (Fin 3), square is QQQ, and LocalSmoothPositive packages smoothness of every entry and Matrix.PosDef at every point.

Formalization targets

Goal: a nonrealizable smooth metric (Theorem A)

∃ g smooth, positive definite on Q  such that for every open U⊆Q with 0∈U, there is no C∞ F:U→R3 with F∗⟨⋅,⋅⟩=g.\exists\, g\ \text{smooth, positive definite on } Q\ \text{ such that for every open } U\subseteq Q \text{ with } 0\in U,\ \text{there is no } C^\infty\ F:U\to\mathbb R^3 \text{ with } F^*\langle\cdot,\cdot\rangle=g .∃g smooth, positive definite on Q  such that for every open U⊆Q with 0∈U, there is no C∞ F:U→R3 with F∗⟨⋅,⋅⟩=g.

This is Theorem A of the source (p. 1). Because a smooth isometric immersion restricts to an embedding near any point, it also rules out local smooth isometric embeddings. The stronger statement that ggg can be chosen with the full Euclidean Taylor jet at the origin (Corollary 5.3) is not part of the goal. The goal is published on the platform with status Open: no machine-checked proof exists yet.

Significance

The result itself. The theorem shows that smooth local isometric realization in R3\mathbb R^3R3 can fail, which answers negatively the unrestricted smooth problem recorded by Yau and Ghomi. It separates the smooth case from the analytic case (Janet–Cartan) and from finite regularity (Pogorelov, Nadirashvili–Yuan 2008). It also shows, by Corollary 5.3, that the infinite-order jet of the metric at a point does not decide realizability. It leaves open the same question under a sign condition K≥0K\ge0K≥0 or K≤0K\le0K≤0, since the construction uses both signs of curvature.

Formalizing it. The statement is short, but the claimed proof combines PDE estimates for Darboux's equation, hyperbolic propagation, a Baire-category argument and a boundary-saddle geometric step. The literature has disagreed about the status of the smooth question (NY2002 versus NY2008), so a machine-checked proof would remove the ambiguity. Mathlib has the manifold calculus needed to state the result (ContMDiff, mfderiv) but none of the PDE layer.

Difficulty

Where the Gaussian curvature KKK is nonzero, the realization equations are elliptic or hyperbolic and can be solved locally, so any counterexample must exploit degeneracy where KKK vanishes and changes type. Finite-regularity counterexamples (Pogorelov) do not carry over: existence at every finite order, on neighborhoods that shrink with the order, does not give one smooth map on a fixed neighborhood. Nonsolvable Monge–Ampère equations are also not enough by themselves, because the coefficients of the Darboux equation come from the same metric, so the obstruction has to be built into ggg itself. Finally, the conclusion must hold for every neighborhood of the origin and every smooth immersion, with no a priori bounds on FFF.

Formalization scope

  • The metric is a function on the subtype of the open set coordinateSquareOpen with values in Matrix (Fin 2) (Fin 2) ℝ. Each entry is ContMDiff … ∞ and each value is Matrix.PosDef, which includes symmetry (Hermitian over ℝ).
  • The quantifier ranges over all U : Opens Coord with U⊆QU\subseteq QU⊆Q and 0∈U0\in U0∈U, and over all maps F : U → Ambient that are ContMDiff … ∞ on the open submanifold UUU. The isometry condition is stated with mfderiv and the Euclidean inner product: ⟨dFpv,dFpw⟩=v⋅(g(p)w)\langle dF_p v, dF_p w\rangle = v\cdot(g(p)w)⟨dFp​v,dFp​w⟩=v⋅(g(p)w).
  • The conclusion is a negation of existence, so it is not trivialized by a junk value: ggg must be genuinely smooth and positive definite, and an immersion on any neighborhood, however small, is excluded.
  • Infrastructure needed: Gauss equation and second fundamental form in coordinates, Darboux's equation, energy and weighted elliptic estimates, hyperbolic propagation, and the Baire category theorem (available in Mathlib). The surface-theory layer is reusable for other isometric-embedding projects.

Selected references

  • M. Janet, Sur la possibilité de plonger un espace riemannien donné dans un espace euclidien, Ann. Soc. Polon. Math. 5 (1926), 38–43. https://rcin.org.pl/dlibra/publication/31746/edition/15034
  • É. Cartan, Sur la possibilité de plonger un espace riemannien donné dans un espace euclidien, Ann. Soc. Polon. Math. 6 (1927), 1–7. https://rcin.org.pl/dlibra/publication/32955/edition/18106
  • J. Nash, C1C^1C1 isometric imbeddings, Ann. of Math. 60 (1954), 383–396. https://doi.org/10.2307/1969840
  • N. H. Kuiper, On C1C^1C1-isometric imbeddings. I, Nederl. Akad. Wetensch. Proc. Ser. A 58 (1955), 545–556.
  • A. V. Pogorelov, An example of a two-dimensional Riemannian metric admitting no local realization in E3E^3E3, Dokl. Akad. Nauk SSSR 198 (1971), 42–43. https://www.mathnet.ru/eng/dan36135
  • C.-S. Lin, The local isometric embedding in R3\mathbb R^3R3 of 2-dimensional Riemannian manifolds with nonnegative curvature, J. Differential Geom. 21 (1985), 213–230. https://doi.org/10.4310/jdg/1214439563
  • C.-S. Lin, The local isometric embedding in R3\mathbb R^3R3 of two-dimensional Riemannian manifolds with Gaussian curvature changing sign cleanly, Comm. Pure Appl. Math. 39 (1986), 867–887. https://doi.org/10.1002/cpa.3160390607
  • G. Nakamura and Y. Maeda, Local smooth isometric embeddings of low-dimensional Riemannian manifolds into Euclidean spaces, Trans. Amer. Math. Soc. 313 (1989), 1–51. https://doi.org/10.1090/S0002-9947-1989-0992597-8
  • N. Nadirashvili and Y. Yuan, Counterexamples for local isometric embedding, preprint (2002). https://arxiv.org/abs/math/0208127v1
  • N. Nadirashvili and Y. Yuan, Improving Pogorelov's isometric embedding counterexample, Calc. Var. PDE 32 (2008), 319–323. https://doi.org/10.1007/s00526-007-0140-7
  • M. A. Khuri, Counterexamples to the local solvability of Monge–Ampère equations in the plane, Comm. PDE 32 (2007), 665–674. https://doi.org/10.1080/03605300600635061
  • M. A. Khuri, On the local solvability of Darboux's equation, Discrete Contin. Dyn. Syst. (2009, Supplement), 451–456. https://doi.org/10.3934/proc.2009.2009.451
  • Q. Han and M. Khuri, Comm. Anal. Geom. 18 (2010), 649–704. https://doi.org/10.4310/CAG.2010.v18.n4.a2
  • T.-Y. Lin, Comm. PDE 41 (2016), 1553–1592. https://doi.org/10.1080/03605302.2016.1227336
  • S.-T. Yau, Review of geometry and analysis, Asian J. Math. 4 (2000), 235–278. https://doi.org/10.4310/AJM.2000.v4.n1.a16
  • M. Ghomi, Open problems in geometry of curves and surfaces, survey (2019), §1.5. https://ghomi.math.gatech.edu/Papers/op.pdf
  • OpenAI, A Smooth Metric with No Local Isometric Immersion into Three-Space, OpenAI Math Release preprint, September 24, 2026 (Theorem A, p. 1). https://github.com/openai/math/blob/adc7f1241b42e322a6451854ab7e4b4c146bf78a/preprints/A-Smooth-Metric-with-No-Local-Isometric-Immersion-into-Three-Space-September-24-2026/paper.pdf
2 thms1 active userReviewed
Differential Geometry·Captain: wurtle

Smooth isometric immersions of closed surfaces into Euclidean four-spaceResearch Paper

Motivation

An isometric immersion realizes an abstract Riemannian manifold as a surface in Euclidean space whose induced lengths are exactly the prescribed ones. How many dimensions are needed is a classical question. Nash showed that every compact Riemannian nnn-manifold embeds smoothly and isometrically in some Euclidean space; for surfaces his bound is R17\mathbb R^{17}R17 (Nash 1956). Gromov lowered the immersion dimension for closed surfaces to R5\mathbb R^5R5 (Partial Differential Relations, 1986, §3.2.4). Three dimensions do not suffice even locally in the smooth category, and Gromov recorded the question whether every smooth Riemannian surface admits a smooth isometric immersion into R4\mathbb R^4R4 (Gromov 2000, §I, Remark (d)), later attributing it to Chern around 1950 (Gromov 2015, p. 4).

This mission asks for a machine-checked proof of Theorem 1.1 of an OpenAI preprint dated September 23, 2026 (source), which answers the compact, boundaryless form of that question: every closed smooth Riemannian surface admits a smooth isometric immersion into R4\mathbb R^4R4. The preprint has not been peer reviewed and its claim has not been independently verified; on the platform the Lean goal is open.

Background

  • 1926–1927 — Janet and Cartan: analytic Riemannian surfaces embed locally isometrically in R3\mathbb R^3R3 (Janet 1926; Cartan 1927).
  • 1954–1955 — Nash and Kuiper: strictly short immersions in positive codimension can be uniformly approximated by C1C^1C1 isometric immersions (Nash 1954; Kuiper 1955).
  • 1956 — Nash's smooth embedding theorem, dimension n(3n+11)/2n(3n+11)/2n(3n+11)/2, i.e. 171717 for surfaces.
  • 1973 — Poznyak: C3,αC^{3,\alpha}C3,α metrics on compact parts of simply connected planar domains admit C2,αC^{2,\alpha}C2,α isometric immersions into R4\mathbb R^4R4 (Russ. Math. Surveys 1973).
  • 1986 — Gromov: smooth isometric immersions of closed surfaces into R5\mathbb R^5R5.
  • 2026 — Lewicka proves C1,αC^{1,\alpha}C1,α flexibility in R4\mathbb R^4R4 for low-regularity metrics on disk-type planar domains (arXiv:2511.16305); a companion OpenAI preprint gives a smooth metric on a square with no local smooth isometric immersion into R3\mathbb R^3R3; the present preprint claims the closed-surface case in R4\mathbb R^4R4 (Theorem 1.1, p. 2).

Setting

A closed surface MMM is a compact smooth two-dimensional manifold without boundary; it need not be orientable or connected. A Riemannian metric ggg assigns to each p∈Mp\in Mp∈M a positive definite inner product gpg_pgp​ on TpMT_pMTp​M, depending smoothly on ppp. A smooth map F:M→R4F:M\to\mathbb R^4F:M→R4 is an isometric immersion if

⟨dFp(v),dFp(w)⟩=gp(v,w)(p∈M, v,w∈TpM).\langle dF_p(v),dF_p(w)\rangle=g_p(v,w)\qquad(p\in M,\ v,w\in T_pM).⟨dFp​(v),dFp​(w)⟩=gp​(v,w)(p∈M, v,w∈Tp​M).

Positive definiteness of ggg forces dFpdF_pdFp​ to be injective, so FFF is an immersion; self-intersections are allowed.

Formalization targets

Goal: Theorem 1.1 (p. 2)

For every closed smooth Riemannian surface (M,g)(M,g)(M,g) there is a C∞C^\inftyC∞ map F:M→R4F:M\to\mathbb R^4F:M→R4 with F∗δ4=gF^*\delta_4=gF∗δ4​=g, where δ4=∑i=14dxi2\delta_4=\sum_{i=1}^4dx_i^2δ4​=∑i=14​dxi2​. In Lean this is OAI.ClosedSurfaceR4.FiniteOrderSmoothing.smooth_isometric_immersion.

Significance

The result itself. The theorem lowers Gromov's immersion dimension for closed surfaces from five to four, with no restriction on curvature or topology, and settles the closed case of the question Gromov attributes to Chern. Dimension four is the first codimension in which the smooth problem can have a global answer for all surfaces, since smooth metrics with no local isometric immersion into R3\mathbb R^3R3 exist. The open (noncompact) case of the question is not addressed.

Formalizing it. Mathlib now has smooth manifolds, tangent bundles and smooth Riemannian metrics, so the statement is expressible without custom geometry. A complete proof would add Whitney's immersion theorem, Sard's theorem in equal dimensions, metric decompositions into rank-one terms, Nash–Moser-type smoothing estimates, and oscillatory correction schemes; none of these are formalized at this level, and all are reusable in geometric analysis.

Difficulty

The isometric immersion equation dFTdF=gdF^{\mathsf T}dF=gdFTdF=g is a nonlinear system of three equations in four unknown functions, and its linearization loses derivatives, so a direct implicit function argument fails. Convex integration in the Nash–Kuiper style produces only C1C^1C1 solutions. Poznyak's smooth theory works on planar domains with boundary, but on a closed surface the successive local corrections must remain compatible globally. The preprint keeps a nondegenerate normal geometry (a nonzero vector-valued second fundamental form) through every step, adds the metric deficit one positive rank-one term a2dx2a^2dx^2a2dx2 at a time via a velocity loop in a plane normal to FyF_yFy​ and FyyF_{yy}Fyy​ (Proposition 3.1, p. 8; Proposition 7.1, p. 25), and then corrects the approximate metric exactly by a smoothing scheme that solves the linearized equation only on oscillatory modes (Proposition 5.1, p. 15). Nonorientable surfaces are handled by starting from an immersion into a small round 333-sphere, whose radial direction is a global normal (Lemma 9.1, p. 35).

Formalization scope

  • MMM is a type with ChartedSpace (EuclideanSpace ℝ (Fin 2)) M and IsManifold 𝓘(ℝ, ℝ²) ∞ M, assumed compact, Hausdorff and second countable. Being modeled on R2\mathbb R^2R2 (not a half-space) encodes "without boundary"; no orientability or connectedness is assumed.
  • The metric is Mathlib's Bundle.ContMDiffRiemannianMetric of class C∞C^\inftyC∞ on the tangent bundle.
  • The conclusion asks for ContMDiff … ∞ F and equality of the Euclidean inner product of mfderiv images with g.inner p v w for all tangent vectors; immersivity follows and is not stated separately.
  • The statement is not trivialized: the conclusion is an exact pointwise identity for a smooth map, and the hypotheses are satisfied by every closed surface with any metric.

Selected references

  • OpenAI, Smooth isometric immersions of closed surfaces into Euclidean four-space, OpenAI Math Release preprint, September 23, 2026. https://github.com/openai/math/blob/adc7f1241b42e322a6451854ab7e4b4c146bf78a/preprints/Smooth-isometric-immersions-of-closed-surfaces-into-Euclidean-four-space-September-23-2026/paper.pdf
  • J. Nash, The imbedding problem for Riemannian manifolds, Ann. of Math. 63 (1956). https://doi.org/10.2307/1969989
  • J. Nash, C¹-isometric imbeddings, Ann. of Math. 60 (1954). https://doi.org/10.2307/1969840
  • M. Gromov, Partial Differential Relations, Springer (1986). https://doi.org/10.1007/978-3-662-02267-2
  • M. Gromov, Spaces and questions, Geom. Funct. Anal. (2000). https://www.ihes.fr/~gromov/wp-content/uploads/2018/08/SpacesandQuestions.pdf
  • M. Gromov, Geometric, algebraic and analytic descendants of Nash isometric embedding theorems (2015). https://www.ihes.fr/~gromov/wp-content/uploads/2018/08/nash-copy-Oct9.pdf
  • E. G. Poznyak, Isometric immersions of two-dimensional Riemannian metrics in Euclidean space, Russian Math. Surveys (1973). https://doi.org/10.1070/RM1973v028n04ABEH001591
  • M. Lewicka, Full flexibility of isometric immersions of metrics with low Hölder regularity in Poznyak theorem's dimension, arXiv:2511.16305v3 (2026). https://arxiv.org/abs/2511.16305v3
  • H. Whitney, The singularities of a smooth n-manifold in (2n−1)-space, Ann. of Math. 45 (1944). https://doi.org/10.2307/1969266
  • R. S. Hamilton, The inverse function theorem of Nash and Moser, Bull. AMS 7 (1982). https://doi.org/10.1090/S0273-0979-1982-15004-2
2 thms1 active userReviewed
AnalysisMathematical Physics·Captain: wurtle

Sharp one-dimensional Lieb–Thirring constantsResearch Paper

Motivation

Lieb–Thirring inequalities bound the negative eigenvalues of a Schrödinger operator −Δ−W-\Delta-W−Δ−W by an integral of the potential. Lieb and Thirring introduced them in 1975 to give a short proof of the stability of matter, and they remain basic tools in mathematical physics, spectral theory and the analysis of many-fermion systems. The sharp constants are known only in a few cases. In one dimension, the Lieb–Thirring conjecture predicts the sharp constant for every exponent γ\gammaγ: for 1/2<γ<3/21/2<\gamma<3/21/2<γ<3/2 it should be the constant of the best potential with a single bound state, given by an explicit sech⁡2\operatorname{sech}^2sech2 profile.

Timeline

  • 1961. Keller solves the one-bound-state variational problem (doi:10.1063/1.1703708).
  • 1971, 1974. Inverse-scattering trace identities for the KdV equation give the sharp value L3/2,1=3/16L_{3/2,1}=3/16L3/2,1​=3/16 (Zakharov–Faddeev, doi:10.1007/BF01086739; Gardner–Greene–Kruskal–Miura, doi:10.1002/cpa.3160270108).
  • 1975–1976. Lieb and Thirring prove their inequalities and state the one-dimensional conjecture (doi:10.1103/PhysRevLett.35.687).
  • 1978. Aizenman and Lieb extend semiclassical equality to all γ≥3/2\gamma\ge3/2γ≥3/2 (doi:10.1016/0375-9601(78)90385-7).
  • 1996, 1998. Weidl proves finiteness of L1/2,1L_{1/2,1}L1/2,1​ (doi:10.1007/BF02104912); Hundertmark, Lieb and Thomas obtain its sharp value 1/21/21/2 (doi:10.4310/ATMP.1998.v2.n4.a2).
  • 2000. Laptev and Weidl prove sharp semiclassical constants in all dimensions for γ≥3/2\gamma\ge3/2γ≥3/2 (doi:10.1007/BF02392782); Hundertmark, Laptev and Weidl prove Lγ,1≤2Lγ,1clL_{\gamma,1}\le2L^{\rm cl}_{\gamma,1}Lγ,1​≤2Lγ,1cl​ for 1/2≤γ<3/21/2\le\gamma<3/21/2≤γ<3/2 (doi:10.1007/s002220000077).
  • 2008–2025. Improved constants at γ=1\gamma=1γ=1 by Dolbeault–Laptev–Loss (doi:10.4171/JEMS/142), Frank–Hundertmark–Jex–Nam (doi:10.4171/JEMS/1062) and Corso–Ried (doi:10.1007/s00220-024-05216-y); Levitt's numerics support the conjectured value (doi:10.4171/JST/65).
  • 2026. Read and Schulz prove the sharp case γ=1\gamma=1γ=1 (arXiv:2609.10478).

The source of this mission, an OpenAI preprint dated September 23, 2026, proves the conjectured sharp constant for every 1/2<γ<3/21/2<\gamma<3/21/2<γ<3/2.

Setting

For 0≤W∈Lγ+1/2(R)0\le W\in L^{\gamma+1/2}(\mathbb R)0≤W∈Lγ+1/2(R), let H−WH_{-W}H−W​ be the self-adjoint operator of the quadratic form

h−W[v]=∫R∣v′∣2 dx−∫RW∣v∣2 dx,v∈H1(R).h_{-W}[v]=\int_{\mathbb R}|v'|^2\,dx-\int_{\mathbb R}W|v|^2\,dx,\qquad v\in H^1(\mathbb R).h−W​[v]=∫R​∣v′∣2dx−∫R​W∣v∣2dx,v∈H1(R).

For γ>1/2\gamma>1/2γ>1/2 its negative spectrum is discrete; write Tr⁡(H−W)−γ=∑λj<0∣λj∣γ\operatorname{Tr}(H_{-W})_-^\gamma=\sum_{\lambda_j<0}|\lambda_j|^\gammaTr(H−W​)−γ​=∑λj​<0​∣λj​∣γ with multiplicity, possibly +∞+\infty+∞ a priori. The optimal constant is

Lγ,1=sup⁡0≤W∈Lγ+1/2, W≢0Tr⁡(H−W)−γ∫Wγ+1/2,L_{\gamma,1}=\sup_{0\le W\in L^{\gamma+1/2},\ W\not\equiv0}\frac{\operatorname{Tr}(H_{-W})_-^\gamma}{\int W^{\gamma+1/2}},Lγ,1​=0≤W∈Lγ+1/2, W≡0sup​∫Wγ+1/2Tr(H−W​)−γ​​,

Lγ,1(1)L^{(1)}_{\gamma,1}Lγ,1(1)​ is the same supremum with only the lowest eigenvalue retained, and the semiclassical constant is

Lγ,1cl=Γ(γ+1)2π Γ(γ+3/2).L^{\rm cl}_{\gamma,1}=\frac{\Gamma(\gamma+1)}{2\sqrt\pi\,\Gamma(\gamma+3/2)}.Lγ,1cl​=2π​Γ(γ+3/2)Γ(γ+1)​.

Formalization targets

Goal: Theorem 1.1

For 1/2<γ<3/21/2<\gamma<3/21/2<γ<3/2 and every 0≤W∈Lγ+1/2(R)0\le W\in L^{\gamma+1/2}(\mathbb R)0≤W∈Lγ+1/2(R),

Tr⁡(H−W)−γ ≤ 2(γ−1/2γ+1/2)γ−1/2Lγ,1cl∫RWγ+1/2;\operatorname{Tr}(H_{-W})_-^\gamma\ \le\ 2\Bigl(\frac{\gamma-1/2}{\gamma+1/2}\Bigr)^{\gamma-1/2}L^{\rm cl}_{\gamma,1}\int_{\mathbb R}W^{\gamma+1/2};Tr(H−W​)−γ​ ≤ 2(γ+1/2γ−1/2​)γ−1/2Lγ,1cl​∫R​Wγ+1/2;

the constant equals Lγ,1=Lγ,1(1)L_{\gamma,1}=L^{(1)}_{\gamma,1}Lγ,1​=Lγ,1(1)​, and with r=(γ−1/2)−1r=(\gamma-1/2)^{-1}r=(γ−1/2)−1 equality holds for W(x)=(r+1)sech⁡2(rx)W(x)=(r+1)\operatorname{sech}^2(rx)W(x)=(r+1)sech2(rx). The Lean statement OAI.SharpLiebThirring.sharp_lieb_thirring is open on the platform.

Significance

The theorem settles the one-dimensional Lieb–Thirring conjecture on the whole interval 1/2<γ<3/21/2<\gamma<3/21/2<γ<3/2, extending the case γ=1\gamma=1γ=1 of Read and Schulz: allowing many bound states never beats a single optimally shaped well. Combined with the known endpoint results (γ=1/2\gamma=1/2γ=1/2 and γ≥3/2\gamma\ge3/2γ≥3/2), it completes the sharp one-dimensional constants. It also gives the corresponding bound for signed potentials (Corollary 7.3), and through the Laptev–Weidl lifting method one-dimensional sharp constants feed into higher-dimensional estimates.

The result is proved in an OpenAI preprint; it has not been peer reviewed, and no machine-checked proof exists. A formal proof would certify a proof whose key step is a finite-interval action inequality established by a continuation and degree argument for matrix fields.

Difficulty

Single-state bounds and numerical evidence say nothing about potentials with many bound states, and the conjecture requires a bound uniform over all orthonormal families of eigenfunctions. Methods that work at γ=1\gamma=1γ=1 (where the inequality is dual to a kinetic-energy bound for orthonormal families) do not directly apply at other exponents, since the moment ∑∣λj∣γ\sum|\lambda_j|^\gamma∑∣λj​∣γ is not linear in the density matrix. The proof must keep track of the individual eigenvalue scales.

Formalization scope

  • H1 packages u∈L2(R;C)u\in L^2(\mathbb R;\mathbb C)u∈L2(R;C) with a weak derivative in L2L^2L2, tested against smooth compactly supported functions.
  • A negative eigenvalue −k2-k^2−k2 (k>0k>0k>0) is a weak eigenvalue of the form: h−W(v,u)=−k2⟨v,u⟩h_{-W}(v,u)=-k^2\langle v,u\rangleh−W​(v,u)=−k2⟨v,u⟩ for all v∈H1v\in H^1v∈H1.
  • negativeMoment γ W is the supremum, in [0,∞][0,\infty][0,∞], over all finite orthonormal families of such eigenfunctions of ∑iki2γ\sum_ik_i^{2\gamma}∑i​ki2γ​; this counts multiplicity and does not presuppose finiteness. oneStateMoment retains one eigenfunction.
  • Admissible γ W is W≥0W\ge0W≥0 a.e. and W∈Lγ+1/2W\in L^{\gamma+1/2}W∈Lγ+1/2; potentialMass is the lower Lebesgue integral of Wγ+1/2W^{\gamma+1/2}Wγ+1/2; the optimal constants are suprema over admissible WWW with positive mass.
  • For admissible WWW the integral ∫Wuˉv\int W\bar uv∫Wuˉv converges for u,v∈H1u,v\in H^1u,v∈H1, so the form is correctly defined.

A complete development needs Sobolev space H1(R)H^1(\mathbb R)H1(R) and form methods, the variational characterization of negative eigenvalues, Gamma-function identities for Lγ,1clL^{\rm cl}_{\gamma,1}Lγ,1cl​, the explicit sech⁡2\operatorname{sech}^2sech2 eigenvalue computation, and the paper's action inequality. Contributions formalizing Theorem 2.1 (action inequality) and the equality computation for the sech⁡2\operatorname{sech}^2sech2 potential are welcome.

Selected references

  • OpenAI, Sharp one-dimensional Lieb–Thirring constants, preprint, September 23, 2026. https://github.com/openai/math/blob/adc7f1241b42e322a6451854ab7e4b4c146bf78a/preprints/Sharp-One-Dimensional-Lieb-Thirring-Constants-September-23-2026/paper.pdf
  • E. H. Lieb, W. E. Thirring, Bound for the kinetic energy of fermions which proves the stability of matter, Phys. Rev. Lett., 1975. https://doi.org/10.1103/PhysRevLett.35.687
  • J. B. Keller, Lower bounds and isoperimetric inequalities for eigenvalues of the Schrödinger equation, J. Math. Phys., 1961. https://doi.org/10.1063/1.1703708
  • D. Hundertmark, E. H. Lieb, L. E. Thomas, A sharp bound for an eigenvalue moment of the one-dimensional Schrödinger operator, Adv. Theor. Math. Phys., 1998. https://doi.org/10.4310/ATMP.1998.v2.n4.a2
  • A. Laptev, T. Weidl, Sharp Lieb–Thirring inequalities in high dimensions, Acta Math., 2000. https://doi.org/10.1007/BF02392782
  • D. Hundertmark, A. Laptev, T. Weidl, New bounds on the Lieb–Thirring constants, Invent. Math., 2000. https://doi.org/10.1007/s002220000077
  • R. L. Frank, D. Hundertmark, M. Jex, P. T. Nam, The Lieb–Thirring inequality revisited, J. Eur. Math. Soc., 2021. https://doi.org/10.4171/JEMS/1062
  • A. Levitt, Best constants in Lieb–Thirring inequalities: a numerical investigation, J. Spectr. Theory, 2014. https://doi.org/10.4171/JST/65
  • L. Read, M. R. Schulz, The sharp one-dimensional Lieb–Thirring inequality for the sum of eigenvalues, preprint, 2026. https://arxiv.org/abs/2609.10478
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Probability·Captain: mikedeng1

An Optimal Variance Estimate in Stochastic Homogenization of Discrete Elliptic Equations: Scale-L Averages of the Approximate-Corrector Energy Density Have Variance ≲ L^−d, Times (ln T)^q if d = 2Research Paper

Motivation

A random conductance model puts a random conductivity on every edge of the lattice Zd\mathbb Z^dZd. It is the simplest discrete model of diffusion in a heterogeneous medium, and its generator is the generator of a random walk in a random environment. Classical stochastic homogenization shows that on large scales the random operator behaves like a constant-coefficient elliptic operator whose homogenized coefficient AhomA_{\mathrm{hom}}Ahom​ is deterministic. The characterization of AhomA_{\mathrm{hom}}Ahom​, however, involves an equation on the whole lattice for every realization of the coefficients. In practice one computes a spatial average over a box of size LLL of the energy density of an approximate corrector, as in Gloria and Otto (arXiv:1104.1291, §1). The random part of the error of this procedure is a variance. Its size as a function of LLL determines how large a computational box must be.

Timeline:

  • 1979–1981: Kozlov (MR542557) and Papanicolaou–Varadhan (MR712714) prove qualitative homogenization for continuum elliptic equations with random coefficients.
  • 1983: Künnemann (MR714611) proves the discrete version, the diffusion limit of reversible jump processes on Zd\mathbb Z^dZd with ergodic bond conductivities. It provides the corrector and the approximate corrector used here.
  • 1986: Yurinskii (MR867870) gives the first quantitative rates, far from optimal.
  • 1998: Naddaf and Spencer (preprint, Estimates on the variance of some homogenization problems) introduce the spectral-gap approach and obtain optimal variance bounds under a small-contrast assumption on the conductivities.
  • 2011: Gloria and Otto (DOI 10.1214/10-AOP571) prove the optimal variance estimate without any small-contrast assumption, with a logarithmic loss in d=2d = 2d=2. This mission formalizes that estimate.

Setting

Fix d≥2d \ge 2d≥2 and 0<α≤β0 < \alpha \le \beta0<α≤β. Sites are x∈Zdx \in \mathbb Z^dx∈Zd and e1,…,ede_1,\dots,e_de1​,…,ed​ is the canonical basis. An edge [z,z+ei][z, z+e_i][z,z+ei​] carries a conductivity a(z,i)∈[α,β]a(z,i) \in [\alpha,\beta]a(z,i)∈[α,β]; such a field aaa belongs to the class Aαβ\mathcal A_{\alpha\beta}Aαβ​. The discrete gradients are ∇iu(x)=u(x+ei)−u(x)\nabla_i u(x) = u(x+e_i) - u(x)∇i​u(x)=u(x+ei​)−u(x) and ∇i∗u(x)=u(x)−u(x−ei)\nabla^*_i u(x) = u(x) - u(x-e_i)∇i∗​u(x)=u(x)−u(x−ei​), and A(x)=diag[a(x,1),…,a(x,d)]A(x) = \mathrm{diag}[a(x,1),\dots,a(x,d)]A(x)=diag[a(x,1),…,a(x,d)].

The conductivities are i.i.d.: they are distributed according to the product ν⊗E\nu^{\otimes E}ν⊗E over all edges of one probability law ν\nuν on [α,β][\alpha,\beta][α,β]. No density is assumed, so atomic laws are allowed. ⟨⋅⟩\langle\cdot\rangle⟨⋅⟩ is the expectation and var⁡\operatorname{var}var the variance.

For a direction ξ∈Rd\xi \in \mathbb R^dξ∈Rd with ∣ξ∣=1|\xi| = 1∣ξ∣=1 and a cut-off T>0T > 0T>0, the approximate corrector ϕT\phi_TϕT​ solves

T−1ϕT(x)−∇∗⋅A(x)(∇ϕT(x)+ξ)=0(x∈Zd).T^{-1}\phi_T(x) - \nabla^*\cdot A(x)\big(\nabla\phi_T(x) + \xi\big) = 0 \qquad (x \in \mathbb Z^d).T−1ϕT​(x)−∇∗⋅A(x)(∇ϕT​(x)+ξ)=0(x∈Zd).

The zero-order term introduces the length scale T\sqrt TT​. The Green's function GT(x,y;a)G_T(x,y;a)GT​(x,y;a) is the ℓ2\ell^2ℓ2 solution of (T−1−∇∗⋅A∇)GT(⋅,y)=δy(T^{-1} - \nabla^*\cdot A\nabla)G_T(\cdot,y) = \delta_y(T−1−∇∗⋅A∇)GT​(⋅,y)=δy​ in weak form.

A mask ηL:Zd→[0,1]\eta_L : \mathbb Z^d \to [0,1]ηL​:Zd→[0,1] is supported in the box (−L,L)d(-L,L)^d(−L,L)d, sums to 111 and satisfies ∣∇ηL∣≤CηL−d−1|\nabla\eta_L| \le C_\eta L^{-d-1}∣∇ηL​∣≤Cη​L−d−1. The averaged energy density is

ξ⋅AL,Tξ=∑x∈Zd(T−1ϕT(x)2+(∇ϕT(x)+ξ)⋅A(x)(∇ϕT(x)+ξ))ηL(x).\xi\cdot A_{L,T}\xi = \sum_{x\in\mathbb Z^d}\Big(T^{-1}\phi_T(x)^2 + \big(\nabla\phi_T(x)+\xi\big)\cdot A(x)\big(\nabla\phi_T(x)+\xi\big)\Big)\eta_L(x).ξ⋅AL,T​ξ=x∈Zd∑​(T−1ϕT​(x)2+(∇ϕT​(x)+ξ)⋅A(x)(∇ϕT​(x)+ξ))ηL​(x).

Formalization targets

Goal: Theorem 2.1, estimate (2.5)

There are an exponent q>0q > 0q>0 and a threshold T0T_0T0​, depending only on d,α,βd, \alpha, \betad,α,β, and for each mask constant CηC_\etaCη​ a constant CCC, such that for every law ν\nuν on [α,β][\alpha,\beta][α,β], every unit ξ\xiξ, every T≥T0T \ge T_0T≥T0​, every L>0L > 0L>0 and every mask ηL\eta_LηL​:

var⁡[ξ⋅AL,Tξ]≤{C L−2(ln⁡T)q,d=2,C L−d,d>2.\operatorname{var}[\xi\cdot A_{L,T}\xi] \le \begin{cases} C\,L^{-2}(\ln T)^q, & d = 2,\\ C\,L^{-d}, & d > 2.\end{cases}var[ξ⋅AL,T​ξ]≤{CL−2(lnT)q,CL−d,​d=2,d>2.​

The statement fixes the shape of the bound, not the value of qqq or CCC, which is why it is the goal.

Milestones

The milestones follow the paper's proof:

  • well-posedness: the Green's function (Definition 2.7) and the approximate corrector (Lemma 2.2, pathwise form);
  • the variance estimate Lemma 2.3 for functions of countably many i.i.d. variables;
  • deterministic Green's-function bounds: Lemma 2.8 (BMO and decay on dyadic annuli), Lemma 2.9 (Meyers-type higher integrability), Corollaries 2.2 and 2.3;
  • susceptibility formulas: Lemmas 2.4 and 2.5, which give ∂ϕT/∂a(e)\partial\phi_T/\partial a(e)∂ϕT​/∂a(e) and ∂GT/∂a(e)\partial G_T/\partial a(e)∂GT​/∂a(e);
  • measurability: Lemma 2.6;
  • a Caccioppoli inequality in probability: Lemma 2.7;
  • a convolution estimate: Lemma 2.10;
  • moment bounds: Proposition 2.1, which gives ⟨∣ϕT(0)∣q⟩≲1\langle|\phi_T(0)|^q\rangle \lesssim 1⟨∣ϕT​(0)∣q⟩≲1 for d>2d > 2d>2 and ≲(ln⁡T)γ(q)\lesssim(\ln T)^{\gamma(q)}≲(lnT)γ(q) for d=2d = 2d=2;
  • the two steps of §3.2: the derivative formula (3.17) and its uniform bound (3.22).

Significance

The result. The estimate says that smooth averages of the energy density fluctuate as if the density were independent from site to site, at the rate L−d/2L^{-d/2}L−d/2. That rate is the best possible, since the coefficients themselves are independent. In the error analysis of approximations of AhomA_{\mathrm{hom}}Ahom​, this controls the random error and separates it from the systematic error caused by the cut-off TTT. Proposition 2.1, a byproduct, shows that the approximate corrector has all moments bounded uniformly in TTT when d>2d > 2d>2, which yields a stationary corrector (Corollary 2.1 of the paper).

Formalizing it. The theorem has been proved since 2011, and no machine-checked version is known. A formal proof would combine three components that are reusable well beyond this paper:

  • a variance inequality for functions of countably many independent variables, in the infinite product measure;
  • quantitative regularity of discrete elliptic Green's functions, uniform in the coefficients;
  • the sensitivity calculus of solutions with respect to a single coefficient.

Difficulty

The obvious argument fails because the energy density is not independent from site to site: the corrector couples all conductivities through the inverse of a random elliptic operator. Bounding the variance needs the sensitivity of ξ⋅AL,Tξ\xi\cdot A_{L,T}\xiξ⋅AL,T​ξ to each single conductivity, and that sensitivity is expressed through gradients of the Green's function. Pointwise bounds on ∇GT\nabla G_T∇GT​ that are uniform in the coefficients do not exist: the continuum counterpart fails, by examples from quasi-conformal mappings. Only averaged decay on dyadic annuli and a small gain of integrability are available, which is why the proof needs the moment bounds of Proposition 2.1. In d=2d = 2d=2 the Green's function does not decay, so only BMO-type control is available, and a logarithm of TTT is lost.

Formalization scope

Statements follow the arXiv v1 reprint (arXiv:1104.1291v1) of the Annals of Probability article; theorem and page numbers refer to it.

  • The lattice is Fin d → ℤ. An edge [z,z+ei][z,z+e_i][z,z+ei​] is the pair (z, i), and a coefficient field is a real function on edges; the theorems assume it takes values in [α,β][\alpha,\beta][α,β].
  • The i.i.d. law is Measure.infinitePi of one probability measure ν\nuν on R\mathbb RR with ν([α,β]c)=0\nu([\alpha,\beta]^c) = 0ν([α,β]c)=0.
  • ϕT\phi_TϕT​ is the unique bounded solution of (2.3) and GT(⋅,y)G_T(\cdot,y)GT​(⋅,y) the unique ℓ2\ell^2ℓ2 solution of (2.11). The definitions file explains why the bounded solution is the paper's stationary ϕT\phi_TϕT​.
  • Norms are Euclidean. The mask's gradient bound is componentwise with an explicit constant CηC_\etaCη​.
  • Every ≲\lesssim≲ becomes an explicit constant chosen before the law, the coefficients and the spatial variables, and every ≫1\gg 1≫1 becomes an explicit threshold.
  • Variances, lower integrals and infinite sums that could otherwise default to 000 are either taken in [0,∞][0,\infty][0,∞] or come with square-integrability in the conclusion.

Ruling out a trivial formalization. If the constant CCC were allowed to depend on the law ν\nuν or on the mask, the goal would follow from the boundedness of the energy average alone. If the variance were taken of a function that is not square-integrable, it would be 000 by convention. The goal fixes CCC before ν\nuν and ηL\eta_LηL​ and requires square-integrability as part of the conclusion.

Not formalized:

  • the last sentence of Theorem 2.1, the variance estimate for the corrector ϕ\phiϕ itself when d>2d > 2d>2. It needs the stationary corrector of Lemma 2.1, whose existence is quoted from Künnemann;
  • Lemma 2.8 (ii);
  • the stochastic part of Lemma 2.2 (stationarity and zero mean of ϕT\phi_TϕT​), which follows from the pathwise statement as explained in the definitions file.

Welcome contributions are proofs of any milestone and reusable infrastructure: infinite-product variance inequalities, discrete integration by parts, and discrete maximum principles.

Selected references

  • A. Gloria, F. Otto, An optimal variance estimate in stochastic homogenization of discrete elliptic equations, Ann. Probab. 39(3) (2011) 779–856. arXiv:1104.1291, DOI 10.1214/10-AOP571
  • R. Künnemann, The diffusion limit for reversible jump processes on Zd\mathbb Z^dZd with ergodic random bond conductivities, Comm. Math. Phys. 90 (1983) 27–68. MR714611
  • S. M. Kozlov, The averaging of random operators, Mat. Sb. 109(151) (1979) 188–202. MR542557
  • G. C. Papanicolaou, S. R. S. Varadhan, Boundary value problems with rapidly oscillating random coefficients, Colloq. Math. Soc. János Bolyai 27 (1981) 835–873. MR712714
  • V. V. Yurinskii, Averaging of symmetric diffusion in a random medium, Sibirsk. Mat. Zh. 27 (1986) 167–180. MR867870
  • N. G. Meyers, An LpL^pLp estimate for the gradient of solutions of second order elliptic divergence equations, Ann. Scuola Norm. Sup. Pisa 17 (1963) 189–206. MR0159110
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Dynamical Systems·Captain: shivm

Catalytic Reaction–Diffusion: Global Attraction of the Positive Equilibrium (AIM 416)Open Problem

Motivation

Nguyen and Tang study the irreversible catalytic network A+B→B+C\mathcal A+\mathcal B\to\mathcal B+\mathcal CA+B→B+C, B+C→A+B\mathcal B+\mathcal C\to\mathcal A+\mathcal BB+C→A+B, a simple reaction–diffusion system with both a positive and a boundary equilibrium (catalyst used up). They settle every mass regime but one and leave it as a conjecture (AIM problem 416).

Timeline. 2021: Fellner–Morgan–Tang give global classical solutions with uniform bounds. 2026: Nguyen–Tang prove convergence for M1<M2M_1<M_2M1​<M2​ and M1≥2M2M_1\ge2M_2M1​≥2M2​ and local results in between, conjecturing global attraction there.

Setting

On a bounded connected smooth domain Ω⊂Rn\Omega\subset\mathbb R^nΩ⊂Rn with ∣Ω∣=1|\Omega|=1∣Ω∣=1 and d1,d2,d3>0d_1,d_2,d_3>0d1​,d2​,d3​>0:

at−d1Δa=b(c−a),bt−d2Δb=b(c−a),ct−d3Δc=−b(c−a),a_t-d_1\Delta a=b(c-a),\quad b_t-d_2\Delta b=b(c-a),\quad c_t-d_3\Delta c=-b(c-a),at​−d1​Δa=b(c−a),bt​−d2​Δb=b(c−a),ct​−d3​Δc=−b(c−a),

with homogeneous Neumann conditions and strictly positive C2C^2C2 compatible initial data. The masses M1=∫Ω(a0+c0)M_1=\int_\Omega(a_0+c_0)M1​=∫Ω​(a0​+c0​), M2=∫Ω(b0+c0)M_2=\int_\Omega(b_0+c_0)M2​=∫Ω​(b0​+c0​) are conserved. The equilibria are the positive one (M12, M2−M12, M12)(\frac{M_1}2,\,M_2-\frac{M_1}2,\,\frac{M_1}2)(2M1​​,M2​−2M1​​,2M1​​) and the boundary one (M1−M2, 0, M2)(M_1-M_2,\,0,\,M_2)(M1​−M2​,0,M2​).

Formalization target

If M2≤M1<2M2M_2\le M_1<2M_2M2​≤M1​<2M2​, every classical solution converges uniformly on Ω\OmegaΩ to the positive equilibrium (no rate required).

Significance

This is the last open regime of Nguyen–Tang's stability analysis. Strict positivity is essential: with b0≡0b_0\equiv0b0​≡0 the solution stays away from the positive equilibrium.

Difficulty

For M1≥M2M_1\ge M_2M1​≥M2​ there is no positive lower bound on ∫Ωb\int_\Omega b∫Ω​b, so entropy dissipation can degenerate near the boundary equilibrium (b=0b=0b=0), and the local results do not exclude trajectories approaching it.

Formalization scope

Rn\mathbb R^nRn is EuclideanSpace ℝ (Fin n) and Δ\DeltaΔ is Mathlib's Laplacian. The domain is Ω={φ<0}\Omega=\{\varphi<0\}Ω={φ<0} for a C∞C^\inftyC∞ function φ\varphiφ with ∇φ≠0\nabla\varphi\ne0∇φ=0 on {φ=0}\{\varphi=0\}{φ=0}; the Neumann condition is the derivative within Ω‾\overline\OmegaΩ in the direction ∇φ\nabla\varphi∇φ. Solutions are continuous on [0,∞)×Ω‾[0,\infty)\times\overline\Omega[0,∞)×Ω and C1,2C^{1,2}C1,2 for t>0t>0t>0, and L∞L^\inftyL∞ convergence is TendstoUniformlyOn. The goal quantifies over classical solutions; their existence is proved in the literature (Fellner–Morgan–Tang; Nguyen–Tang, Theorem 2.1) but is not part of this statement.

Selected references

  • T. L. Nguyen, B. Q. Tang, Stability analysis of irreversible chemical reaction-diffusion systems with boundary equilibria, Z. Angew. Math. Phys. 77, 2026, 199. DOI
  • K. Fellner, J. Morgan, B. Q. Tang, Uniform-in-time bounds for quadratic reaction-diffusion systems with mass dissipation in higher dimensions, DCDS-S 14, 2021, 635–651. DOI
  • AIM open problems list, problem 416. github.com/MColbrook/AIM
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Control TheoryMathematical PhysicsOptimization+2·Captain: mikedeng1

Optimization of Mean-field Spin Glasses III: The Lagrangian Value of the Stochastic Control Problem Equals the Parisi FunctionalResearch Paper

Motivation

The ground-state energy of a mixed ppp-spin spin glass, OPTN=max⁡σ∈{±1}NHN(σ)/N\mathsf{OPT}_N=\max_{\sigma\in\{\pm1\}^N}H_N(\sigma)/NOPTN​=maxσ∈{±1}N​HN​(σ)/N, converges almost surely to the infimum of the Parisi functional over non-decreasing order parameters (Auffinger–Chen 2017). El Alaoui, Montanari and Sellke (arXiv:2001.00904v1) study algorithms that find near-optimal configurations. They introduce incremental approximate message passing (IAMP) and show that, among a broad class of such algorithms, the best achievable energy is the infimum of the Parisi functional over a larger space of order parameters (their Theorem 4).

The upper bound in Theorem 4 is reduced, in Section 4 of the paper, to a stochastic optimal control problem. The energy reached by a message-passing algorithm becomes the objective of a control problem driven by a Brownian motion, with a terminal constraint and a variance constraint. The variance constraint is removed by a Lagrange multiplier 12ξ′′γ\tfrac12\xi''\gamma21​ξ′′γ. Proposition 4.1 states that the resulting Lagrangian value is exactly the Parisi functional P(γ)\mathsf P(\gamma)P(γ). This mission formalizes that duality and the verification argument behind it (Section 7).

Setting

Mixture. Real coefficients (ck)k≥2(c_k)_{k\ge2}(ck​)k≥2​ define the mixture ξ(t)=∑k≥2ck2tk\xi(t)=\sum_{k\ge2}c_k^2t^kξ(t)=∑k≥2​ck2​tk, with the standing assumption 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 nonnegative and nondecreasing on [0,1][0,1][0,1].

Order parameters. SF+\mathsf{SF}_+SF+​ is the set of nonnegative step functions

γ=∑i=1mγi I[ti−1,ti),0=t0<t1<⋯<tm=1, γi≥0.\gamma=\sum_{i=1}^m\gamma_i\,\mathbb I_{[t_{i-1},t_i)},\qquad 0=t_0<t_1<\dots<t_m=1,\ \gamma_i\ge0 .γ=i=1∑m​γi​I[ti−1​,ti​)​,0=t0​<t1​<⋯<tm​=1, γi​≥0.

Put ν(t)=∫t1ξ′′(s)γ(s) ds\nu(t)=\int_t^1\xi''(s)\gamma(s)\,dsν(t)=∫t1​ξ′′(s)γ(s)ds.

Parisi PDE and functional. Φγ:[0,1]×R→R\Phi_\gamma:[0,1]\times\mathbb R\to\mathbb RΦγ​:[0,1]×R→R solves

∂tΦγ+12ξ′′(t)(∂x2Φγ+γ(t)(∂xΦγ)2)=0,Φγ(1,x)=∣x∣.\partial_t\Phi_\gamma+\tfrac12\xi''(t)\big(\partial_x^2\Phi_\gamma+\gamma(t)(\partial_x\Phi_\gamma)^2\big)=0,\qquad\Phi_\gamma(1,x)=|x| .∂t​Φγ​+21​ξ′′(t)(∂x2​Φγ​+γ(t)(∂x​Φγ​)2)=0,Φγ​(1,x)=∣x∣.

For γ∈SF+\gamma\in\mathsf{SF}_+γ∈SF+​ it is given explicitly by the Cole–Hopf recursion: with r(t)=ξ′(1)−ξ′(t)r(t)=\xi'(1)-\xi'(t)r(t)=ξ′(1)−ξ′(t) and G∼N(0,1)G\sim\mathsf N(0,1)G∼N(0,1), for t∈[ti−1,ti)t\in[t_{i-1},t_i)t∈[ti−1​,ti​),

Φγ(t,x)=1γilog⁡Eexp⁡{γiΦγ(ti,x+r(t)−r(ti) G)}.\Phi_\gamma(t,x)=\frac1{\gamma_i}\log\mathbb E\exp\big\{\gamma_i\Phi_\gamma(t_i,x+\sqrt{r(t)-r(t_i)}\,G)\big\}.Φγ​(t,x)=γi​1​logEexp{γi​Φγ​(ti​,x+r(t)−r(ti​)​G)}.

The Parisi functional is P(γ)=Φγ(0,0)−12∫01t ξ′′(t)γ(t) dt\mathsf P(\gamma)=\Phi_\gamma(0,0)-\tfrac12\int_0^1t\,\xi''(t)\gamma(t)\,dtP(γ)=Φγ​(0,0)−21​∫01​tξ′′(t)γ(t)dt.

Control problem. Let BBB be a standard Brownian motion. A control u∈D[t,1]u\in D[t,1]u∈D[t,1] is a process on [t,1][t,1][t,1], progressively measurable for the filtration of (Br)r∈[t,1](B_r)_{r\in[t,1]}(Br​)r∈[t,1]​, with E∫t1ξ′′(s)us2 ds<∞\mathbb E\int_t^1\xi''(s)u_s^2\,ds<\inftyE∫t1​ξ′′(s)us2​ds<∞. The value is

Jγ(t,z)=sup⁡u∈D[t,1]E[∫t1ξ′′(s)us ds+12∫t1ν(s)(ξ′′(s)us2−1)ds]s.t.z+∫t1ξ′′(s) us dBs∈(−1,1) a.s.\mathcal J_\gamma(t,z)=\sup_{u\in D[t,1]}\mathbb E\Big[\int_t^1\xi''(s)u_s\,ds+\frac12\int_t^1\nu(s)\big(\xi''(s)u_s^2-1\big)ds\Big]\quad\text{s.t.}\quad z+\int_t^1\sqrt{\xi''(s)}\,u_s\,dB_s\in(-1,1)\ \text{a.s.}Jγ​(t,z)=u∈D[t,1]sup​E[∫t1​ξ′′(s)us​ds+21​∫t1​ν(s)(ξ′′(s)us2​−1)ds]s.t.z+∫t1​ξ′′(s)​us​dBs​∈(−1,1) a.s.

Candidate value function. With Φγ∗(t,z)=inf⁡x{Φγ(t,x)−xz}\Phi^*_\gamma(t,z)=\inf_x\{\Phi_\gamma(t,x)-xz\}Φγ∗​(t,z)=infx​{Φγ​(t,x)−xz},

V(t,z)=Φγ∗(t,z)−12ν(t)z2−12∫t1ν(s) ds.V(t,z)=\Phi^*_\gamma(t,z)-\tfrac12\nu(t)z^2-\tfrac12\int_t^1\nu(s)\,ds .V(t,z)=Φγ∗​(t,z)−21​ν(t)z2−21​∫t1​ν(s)ds.

Formalization targets

Goal: Proposition 4.1

Jγ(0,0)=P(γ)for every γ∈SF+.\mathcal J_\gamma(0,0)=\mathsf P(\gamma)\qquad\text{for every }\gamma\in\mathsf{SF}_+ .Jγ​(0,0)=P(γ)for every γ∈SF+​.

Milestones

  1. Lemma 7.2 (a)–(e): Φγ(t,⋅)\Phi_\gamma(t,\cdot)Φγ​(t,⋅) is smooth for t<1t<1t<1, with derivatives jointly continuous on [0,1)×R[0,1)\times\mathbb R[0,1)×R and C1C^1C1 in time where γ\gammaγ is constant. The range of ∂xΦγ(t,⋅)\partial_x\Phi_\gamma(t,\cdot)∂x​Φγ​(t,⋅) is (−1,1)(-1,1)(−1,1), it is strictly increasing, and 0<∂x2Φγ(t′,x)≤C(t,γ)0<\partial_x^2\Phi_\gamma(t',x)\le C(t,\gamma)0<∂x2​Φγ​(t′,x)≤C(t,γ) for t′≤tt'\le tt′≤t.
  2. Envelope identities (proof of Lemma 7.3): ∂zΦγ∗(t,z)=−xt∗(z)\partial_z\Phi^*_\gamma(t,z)=-x^*_t(z)∂z​Φγ∗​(t,z)=−xt∗​(z) and ∂z2Φγ∗(t,z)=−1/∂x2Φγ(t,xt∗(z))\partial_z^2\Phi^*_\gamma(t,z)=-1/\partial_x^2\Phi_\gamma(t,x^*_t(z))∂z2​Φγ∗​(t,z)=−1/∂x2​Φγ​(t,xt∗​(z)), where xt∗(z)x^*_t(z)xt∗​(z) is the unique root of ∂xΦγ(t,x)=z\partial_x\Phi_\gamma(t,x)=z∂x​Φγ​(t,x)=z.
  3. Lemma 7.3: VVV solves the HJB equation
∂tV+ξ′′(t)sup⁡λ∈R{λ+λ22(ν(t)+∂z2V)}−12ν(t)=0,V(1,z)=0.\partial_tV+\xi''(t)\sup_{\lambda\in\mathbb R}\Big\{\lambda+\frac{\lambda^2}{2}\big(\nu(t)+\partial_z^2V\big)\Big\}-\frac12\nu(t)=0,\qquad V(1,z)=0 .∂t​V+ξ′′(t)λ∈Rsup​{λ+2λ2​(ν(t)+∂z2​V)}−21​ν(t)=0,V(1,z)=0.
  1. Evaluation at the origin: V(0,0)=P(γ)V(0,0)=\mathsf P(\gamma)V(0,0)=P(γ).
  2. Proposition 7.1: Jγ(t,z)=V(t,z)\mathcal J_\gamma(t,z)=V(t,z)Jγ​(t,z)=V(t,z) for all (t,z)∈[0,1]×(−1,1)(t,z)\in[0,1]\times(-1,1)(t,z)∈[0,1]×(−1,1).

Proposition 7.1 at (0,0)(0,0)(0,0) together with milestone 4 gives the goal.

Significance

The result. By integration by parts (Eq. (4.4) of the paper), Jγ(0,0)\mathcal J_\gamma(0,0)Jγ​(0,0) bounds the value of the constrained control problem (4.2). That problem in turn bounds the asymptotic energy of every message-passing algorithm in the class of Theorem 4. Proposition 4.1 turns the bound into inf⁡γ∈SF+P(γ)\inf_{\gamma\in\mathsf{SF}_+}\mathsf P(\gamma)infγ∈SF+​​P(γ), which is the analytic core of the optimality statement for IAMP. It is also an instance of a broader principle: the Parisi functional has a stochastic-control representation (Jagannath–Tobasco 2016).

Formalizing it. The result is proved in the paper; no machine-checked version exists. A complete formalization needs a verification theorem for a control problem with a state constraint (M1∈(−1,1)M_1\in(-1,1)M1​∈(−1,1)), Itô's formula for a C1,2C^{1,2}C1,2 function that is only piecewise C1C^1C1 in time, and quantitative regularity of the Cole–Hopf solution. Each of these is reusable well beyond spin glasses.

Difficulty

The value function Jγ\mathcal J_\gammaJγ​ is not known to be smooth, and the dynamic-programming equation (4.6) is only heuristic. The proof therefore guesses a solution and verifies it. Two steps carry the difficulty.

First, the guess VVV is a Legendre transform. Its regularity, and the sign ν+∂z2V<0\nu+\partial_z^2V<0ν+∂z2​V<0 that makes the HJB supremum finite, rest on strict convexity and bounded curvature of Φγ(t,⋅)\Phi_\gamma(t,\cdot)Φγ​(t,⋅) (Lemma 7.2). These must be proved by induction through the Cole–Hopf recursion, including the steps with γi=0\gamma_i=0γi​=0.

Second, the verification argument applies Itô's formula to V(s,Msu)V(s,M^u_s)V(s,Msu​), where MuM^uMu is a martingale confined to (−1,1)(-1,1)(−1,1) and VVV is only C1C^1C1 in time between the jumps of γ\gammaγ. The boundary θ→1\theta\to1θ→1 needs a dominated-convergence argument, and attaining the supremum needs an explicit optimal feedback control built from an SDE.

Formalization scope

  • Mixture. ξ\xiξ is a coefficient sequence c:N→Rc:\mathbb N\to\mathbb Rc:N→R with c0=c1=0c_0=c_1=0c0​=c1​=0 imposed. ξ′\xi'ξ′ and ξ′′\xi''ξ′′ are explicit termwise series.
  • Step functions. SF+\mathsf{SF}_+SF+​ is represented by its data (breakpoints and values). γ\gammaγ is extended by 000 outside [0,1)[0,1)[0,1); its value at t=1t=1t=1 never matters.
  • Cole–Hopf. Φγ\Phi_\gammaΦγ​ is defined by the recursion. When γi=0\gamma_i=0γi​=0, the recursion uses its limit, the heat semigroup, instead of dividing by zero. Expectations over GGG are integrals against gaussianReal 0 1.
  • Derivatives. Space derivatives are deriv/iteratedDeriv. Time derivatives are right derivatives, because γ\gammaγ jumps.
  • Legendre transform. Φγ∗\Phi^*_\gammaΦγ∗​ is a real infimum, used only for ∣z∣<1|z|<1∣z∣<1, where it is bounded below.
  • Brownian motion and filtration. BBB is a Mathlib IsBrownianReal process on R≥0\mathbb R_{\ge0}R≥0​, with each BrB_rBr​ measurable. The filtration is Fst=σ(Br:t≤r≤s)\mathcal F^t_s=\sigma(B_r:t\le r\le s)Fst​=σ(Br​:t≤r≤s).
  • Stochastic integral. It is the L2L^2L2 Itô integral of the published definition Peng1990.SMP.IsItoIntegral (horizon 111), whose integrability class is exactly E∫ξ′′u2<∞\mathbb E\int\xi''u^2<\inftyE∫ξ′′u2<∞.
  • Supremum. Jγ(t,z)=v\mathcal J_\gamma(t,z)=vJγ​(t,z)=v is stated as "vvv is the least upper bound of the objective values of admissible controls" (IsLUB), never as a real sSup. A default value of an empty or unbounded supremum therefore cannot make a statement trivially true.
  • Disclosed hypothesis. Lemma 7.2, the envelope identities and Lemma 7.3 assume that ξ\xiξ is not identically zero (some ck≠0c_k\neq0ck​=0). For ξ≡0\xi\equiv0ξ≡0 one has Φγ(t,x)=∣x∣\Phi_\gamma(t,x)=|x|Φγ​(t,x)=∣x∣ for all ttt, and these statements fail. Proposition 7.1, the evaluation at the origin and the goal need no such hypothesis.
  • Lemma 7.3. The statement includes the inequality ν+∂z2V<0\nu+\partial_z^2V<0ν+∂z2​V<0, which the page proves. This rules out reading the HJB supremum as a default value.

The paper's algorithmic results (Theorems 2–4, Corollary 2.2) are out of scope. They need the AMP and state-evolution machinery of Section 5 and Appendix A, and an informal model of computation. The optional bound (4.4) is not stated.

Welcome contributions include the regularity of Cole–Hopf solutions (Gaussian convolution, log-moment-generating functions), a general verification theorem for one-dimensional controlled martingales with a terminal state constraint, and Itô's formula for C1,2C^{1,2}C1,2 functions.

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, Ann. Probab. 45(6b), 2017. https://arxiv.org/abs/1606.05335
  • A. Jagannath, I. Tobasco, A dynamic programming approach to the Parisi functional, Proc. AMS 144, 2016. https://arxiv.org/abs/1502.04398
  • N. Touzi, Optimal Stochastic Control, Stochastic Target Problems, and Backward SDE, Fields Institute Monographs 29, Springer, 2012 (cited as [Tou12] in the paper; the verification argument of Section 7 follows its Theorem 4.1).
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Mathematical PhysicsOptimizationProbability·Captain: mikedeng1

Optimization of Mean-field Spin Glasses II: Under No Overlap Gap, the Monotone Parisi Minimizer Also Minimizes the Extended FunctionalResearch Paper

Motivation

The mixed ppp-spin model is a random polynomial on the hypercube {−1,+1}N\{-1,+1\}^N{−1,+1}N: a centered Gaussian process HN(σ)H_N(\boldsymbol\sigma)HN​(σ) with covariance E{HN(σ)HN(σ′)}=Nξ(⟨σ,σ′⟩/N)\mathbb E\{H_N(\boldsymbol\sigma)H_N(\boldsymbol\sigma')\} = N\xi(\langle\boldsymbol\sigma,\boldsymbol\sigma'\rangle/N)E{HN​(σ)HN​(σ′)}=Nξ(⟨σ,σ′⟩/N). Its maximum OPTN=max⁡σHN(σ)/N\mathrm{OPT}_N = \max_{\boldsymbol\sigma} H_N(\boldsymbol\sigma)/NOPTN​=maxσ​HN​(σ)/N is a canonical random optimization problem; for ξ(t)=c22t2\xi(t) = c_2^2t^2ξ(t)=c22​t2 it is the ground state of the Sherrington–Kirkpatrick model. Auffinger and Chen (AC17) proved that OPTN\mathrm{OPT}_NOPTN​ converges almost surely to the infimum of the zero-temperature Parisi functional P\mathsf PP over a space U\mathscr UU of non-decreasing order parameters.

El Alaoui, Montanari and Sellke (arXiv:2001.00904v1) characterize what a class of message-passing algorithms achieves on this problem. The answer is the infimum of the same functional over a larger space L\mathscr LL of order parameters that need not be monotone. Whether these algorithms reach the true optimum is therefore the question whether inf⁡UP=inf⁡LP\inf_{\mathscr U}\mathsf P = \inf_{\mathscr L}\mathsf PinfU​P=infL​P. The paper proves this equality under the no-overlap gap assumption, that the Parisi minimizer over U\mathscr UU can be taken strictly increasing (Assumption 2, p. 8). This is believed to hold for the Sherrington–Kirkpatrick model and to fail for pure ppp-spin models with p≥3p \ge 3p≥3. This mission formalizes that equality, stated as a property of the minimizer.

Timeline. Parisi's formula (1979) was proved by Talagrand (2006) and Panchenko (2013). Auffinger and Chen (2017) gave its zero-temperature form (1.7). Jagannath and Tobasco (JT16) gave a PDE and variational treatment of the Parisi functional at positive temperature, including its convexity. Montanari (Mon19) gave a message-passing algorithm for the Sherrington–Kirkpatrick model under no overlap gap. El Alaoui, Montanari and Sellke (2020) extended it to mixed ppp-spin models and introduced the extended principle over 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, with derivatives ξ′\xi'ξ′ and ξ′′\xi''ξ′′ given by the termwise series. Order parameters are functions γ:[0,1)→R≥0\gamma : [0,1) \to \mathbb R_{\ge0}γ:[0,1)→R≥0​, in one of two spaces:

U={γ non-decreasing, ∫01γ(t) dt<∞},L={∥ξ′′γ∥TV[0,t]<∞ ∀t<1, ∫01ξ′′(t)γ(t) dt<∞}.\mathscr U = \Big\{\gamma \text{ non-decreasing},\ \int_0^1\gamma(t)\,dt < \infty\Big\},\qquad \mathscr L = \Big\{\|\xi''\gamma\|_{TV[0,t]} < \infty\ \forall t<1,\ \int_0^1\xi''(t)\gamma(t)\,dt < \infty\Big\}.U={γ non-decreasing, ∫01​γ(t)dt<∞},L={∥ξ′′γ∥TV[0,t]​<∞ ∀t<1, ∫01​ξ′′(t)γ(t)dt<∞}.

Here ∥⋅∥TV[0,t]\|\cdot\|_{TV[0,t]}∥⋅∥TV[0,t]​ is total variation on [0,t][0,t][0,t], and U⊆L\mathscr U \subseteq \mathscr LU⊆L.

For a step function γ=∑iγiI[ti−1,ti)\gamma = \sum_i \gamma_i \mathbb I_{[t_{i-1},t_i)}γ=∑i​γi​I[ti−1​,ti​)​ with γi≥0\gamma_i \ge 0γi​≥0 (the space SF+\mathrm{SF}_+SF+​), the Parisi PDE

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

is solved explicitly by the Cole–Hopf recursion (7.3). It is a Gaussian log-moment-generating step on each piece, and a heat-semigroup step where γi=0\gamma_i = 0γi​=0. For general 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 norm ∫01ξ′′∣γn−γ∣\int_0^1\xi''|\gamma_n - \gamma|∫01​ξ′′∣γn​−γ∣. 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.

The process XXX is the strong solution of 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 (Eq. (6.3)), driven by a standard Brownian motion BBB.

Formalization targets

Goal: the monotone minimizer is a minimizer over L\mathscr LL (Section 6.3, p. 34)

If γ∗∈U\gamma_* \in \mathscr Uγ∗​∈U is strictly increasing on [0,1)[0,1)[0,1) and P(γ∗)≤P(γ)\mathsf P(\gamma_*) \le \mathsf P(\gamma)P(γ∗​)≤P(γ) for every γ∈U\gamma \in \mathscr Uγ∈U, then

P(γ∗)≤P(γ)for every γ∈L.\mathsf P(\gamma_*) \le \mathsf P(\gamma)\qquad\text{for every }\gamma \in \mathscr L .P(γ∗​)≤P(γ)for every γ∈L.

Since U⊆L\mathscr U \subseteq \mathscr LU⊆L, this is the paper's main result 2 (p. 4), inf⁡UP=inf⁡LP\inf_{\mathscr U}\mathsf P = \inf_{\mathscr L}\mathsf PinfU​P=infL​P under no overlap gap.

Milestones

  1. Lemma 6.7 (p. 27): for γ∈L\gamma\in\mathscr Lγ∈L, 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).
  2. Proposition 6.8 (p. 27): the right derivative of s↦P(γ+sδ)s\mapsto\mathsf P(\gamma+s\delta)s↦P(γ+sδ) at 000 is 12∫01ξ′′(t)δ(t)(E{∂xΦ(t,Xt)2}−t) dt\frac12\int_0^1\xi''(t)\delta(t)\big(\mathbb E\{\partial_x\Phi(t,X_t)^2\}-t\big)\,dt21​∫01​ξ′′(t)δ(t)(E{∂x​Φ(t,Xt​)2}−t)dt, for admissible directions δ\deltaδ that vanish near t=1t = 1t=1.
  3. Lemma 6.15 (p. 33): under no overlap gap, E{∂xΦγ∗(t,Xt)2}=t\mathbb E\{\partial_x\Phi^{\gamma_*}(t,X_t)^2\} = tE{∂x​Φγ∗​(t,Xt​)2}=t for every t∈[0,1)t\in[0,1)t∈[0,1).
  4. Convexity (Section 6.3, p. 34): P\mathsf PP is convex on L\mathscr LL.

Significance

The result. The goal identifies the value reached by the paper's message-passing algorithm with the ground-state energy whenever the Parisi minimizer is strictly increasing. Combined with the paper's algorithmic theorem, it yields a (1−ε)(1-\varepsilon)(1−ε)-approximation of OPTN\mathrm{OPT}_NOPTN​ in time linear in the input size, for the Sherrington–Kirkpatrick model and any other mixture with no overlap gap (Corollary 2.2). It also gives a structural fact about the variational problem: when the minimizer is strictly increasing, the monotonicity constraint in U\mathscr UU is not binding.

Formalizing it. The result is proved in the paper, but the proof leans on an external citation ([JT16, Theorem 20]) for convexity of P\mathsf PP on L\mathscr LL. It also applies the first-variation formula in a direction that does not meet that formula's stated hypotheses. A machine-checked development closes both gaps. No part of this theory (the Parisi PDE, its Cole–Hopf solution, or the extended functional) has been formalized before, to our knowledge.

Difficulty

The obvious argument is: convexity plus stationarity gives a global minimum. Both inputs are hard. Stationarity (Lemma 6.15) needs the first variation of P\mathsf PP in directions that keep γ∗+sδ\gamma_*+s\deltaγ∗​+sδ monotone. That variation is a derivative of the solution of a nonlinear PDE with respect to its coefficient, expressed through an SDE driven by that solution's own gradient. Convexity of P\mathsf PP on L\mathscr LL is not visible from the formula: Φγ(0,0)\Phi^\gamma(0,0)Φγ(0,0) is defined through a limit of nested Cole–Hopf recursions, and the paper does not prove it, citing a positive-temperature argument instead. Finally, the goal needs the first variation in the direction γ−γ∗\gamma - \gamma_*γ−γ∗​, which is generally non-zero near t=1t = 1t=1, where ξ′′γ\xi''\gammaξ′′γ may blow up. Proposition 6.8 as stated excludes such directions.

Formalization scope

  • Mixture. A coefficient sequence c : ℕ → ℝ with c0=c1=0c_0 = c_1 = 0c0​=c1​=0 and ∑kck2(1+ε)k<∞\sum_k c_k^2(1+\varepsilon)^k < \infty∑k​ck2​(1+ε)k<∞ for some ε>0\varepsilon>0ε>0. ξ′\xi'ξ′ and ξ′′\xi''ξ′′ are explicit power series.
  • Order parameters. Functions R→R\mathbb R\to\mathbb RR→R; membership in U\mathscr UU and L\mathscr LL reads only [0,1)[0,1)[0,1). Total variation is eVariationOn; finiteness of integrals is IntegrableOn (which includes measurability).
  • Cole–Hopf. Step-function data (m,t,a)(m,t,a)(m,t,a) with m≥1m\ge1m≥1. The γi=0\gamma_i = 0γi​=0 pieces use the heat semigroup, the limit of (7.3). The terminal condition is ∣x∣|x|∣x∣. Gaussian expectations are integrals against gaussianReal 0 1.
  • Φγ\Phi^\gammaΦγ on L\mathscr LL. limUnder of the Cole–Hopf values along step-function data converging to γ\gammaγ in the weighted L1L^1L1 distance. ∂x\partial_x∂x​ is deriv in xxx.
  • SDE. The published definition EthierKurtz.SolvesBrownianSDE in dimension one, with coefficients extended by 000 after time 111. Brownian motion is Mathlib's IsBrownianReal, and expectations are Bochner integrals.
  • Minimality. Always attainment, P(γ∗)≤P(γ)\mathsf P(\gamma_*)\le\mathsf P(\gamma)P(γ∗​)≤P(γ) for all γ\gammaγ in the space, never a real infimum (which Lean sets to 000 on unbounded sets).
  • Disclosed hypothesis. Lemma 6.15 assumes that some ck≠0c_k \ne 0ck​=0. For ξ≡0\xi\equiv0ξ≡0 it is false: P≡0\mathsf P\equiv0P≡0, X≡0X\equiv0X≡0, and the left side is constant in ttt. The goal does not need it.
  • Ruled out. A formalization that defines Φγ\Phi^\gammaΦγ as an arbitrary weak solution of the PDE, or via a choice from an unproved existence statement, would make P\mathsf PP unconstrained. It is not acceptable. Encoding the hypothesis on γ∗\gamma_*γ∗​ as minimality over L\mathscr LL would make the goal trivial.
  • Proof gaps in the source. Convexity of P\mathsf PP on L\mathscr LL is cited, not proved. The step from stationarity to the goal applies Proposition 6.8 outside its stated hypotheses. The statements are the paper's and are believed true.
  • Out of scope. The paper's algorithmic results (Theorems 2–4, Corollary 2.2) assert algorithms with complexity bounds in an informal computation model, and rest on a long state-evolution analysis. They are not part of this mission.

Contributions welcome: Cole–Hopf regularity (smoothness and the bound ∣∂xΦ∣≤1|\partial_x\Phi|\le1∣∂x​Φ∣≤1), the Lipschitz estimate in γ\gammaγ that makes Φγ\Phi^\gammaΦγ well defined, well-posedness of the SDE, and Itô calculus for the first variation. The Cole–Hopf layer and the SDE well-posedness are reusable for the companion missions on the full-support theorem and the stochastic-control duality of the same paper.

Selected references

  • A. El Alaoui, A. Montanari, M. Sellke, Optimization of Mean-field Spin Glasses, arXiv:2001.00904v1, 2020. https://arxiv.org/abs/2001.00904v1
  • A. Auffinger, W.-K. Chen, Parisi formula for the ground state energy in the mixed p-spin model, Ann. Probab. 45(6b), 2017. https://arxiv.org/abs/1606.05335
  • A. Jagannath, I. Tobasco, A dynamic programming approach to the Parisi functional, Proc. AMS 144(7), 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, Ann. Math. 163(1), 2006. https://doi.org/10.4007/annals.2006.163.221
  • D. Panchenko, The Parisi ultrametricity conjecture, Ann. Math. 177(1), 2013. https://arxiv.org/abs/1112.1003
11 thms1 active userReviewed
AnalysisControl Theory·Captain: mikedeng1

Stability and Instability Results of the Wave Equation with a Delay Term in the Boundary or Internal Feedbacks II: Exponential Decay under Delayed Internal DampingResearch Paper

Motivation

Feedback laws that damp vibrations in elastic structures are implemented by sensors and actuators, and a physical loop always reacts with some time delay τ>0\tau>0τ>0: the damping force at time ttt is computed from the velocity measured at time t−τt-\taut−τ. Datko, Lagnese and Polis showed in 1986 that an arbitrarily small delay in a boundary feedback can destroy the stability of a one-dimensional wave equation (Datko–Lagnese–Polis, SIAM J. Control Optim. 24 (1986)), and Datko showed that such fragility is common to a broad class of feedback-stabilized hyperbolic systems (Datko, SIAM J. Control Optim. 26 (1988)). Delay-robustness is therefore a genuine question for every stabilizing feedback, not a technicality.

Nicaise and Pignotti (SIAM J. Control Optim. 45 (2006) 1561–1585) identified a simple sufficient condition in several space dimensions: if the feedback contains an undelayed velocity term with gain μ1\mu_1μ1​ and a delayed one with gain μ2\mu_2μ2​, and μ2<μ1\mu_2<\mu_1μ2​<μ1​, the energy still decays exponentially; if μ2≥μ1\mu_2\ge\mu_1μ2​≥μ1​, instabilities appear for some delays. This mission formalizes the stability half for internal (distributed) damping, localized near the Neumann part of the boundary.

Timeline.

  • 1986: Datko, Lagnese, Polis — small delays destabilize a boundary-damped 1D wave equation.
  • 1988: Datko — many feedback-stabilized hyperbolic systems are not robust with respect to small delays.
  • 1990: Zuazua — exponential decay for the semilinear wave equation with locally distributed damping, without delay (Comm. PDE 15 (1990)); Liu (1997) treats locally distributed damping for general conservative systems (SIAM J. Control Optim. 35 (1997)).
  • 2006: Nicaise, Pignotti — exponential decay with a delayed boundary or internal feedback under μ2<μ1\mu_2<\mu_1μ2​<μ1​ (Theorems 1.1 and 1.3), and instability examples when μ2≥μ1\mu_2\ge\mu_1μ2​≥μ1​ (Theorems 1.2 and 1.4).

Setting

Let Ω⊂Rn\Omega\subset\mathbb{R}^nΩ⊂Rn, n≥1n\ge1n≥1, 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, dΓd\GammadΓ for the surface measure, ut,uttu_t,u_{tt}ut​,utt​ for time derivatives and Δ\DeltaΔ for the Laplacian in xxx.

Geometric hypothesis (1.6)–(1.7): there are a C2C^2C2 function vvv and α>0\alpha>0α>0 with ⟨D2v(x)ξ,ξ⟩≥2α∣ξ∣2\langle D^2v(x)\xi,\xi\rangle\ge2\alpha|\xi|^2⟨D2v(x)ξ,ξ⟩≥2α∣ξ∣2 for all x∈Ω‾x\in\overline\Omegax∈Ω, ξ∈Rn\xi\in\mathbb{R}^nξ∈Rn, and ∇v(x)⋅ν(x)≤0\nabla v(x)\cdot\nu(x)\le0∇v(x)⋅ν(x)≤0 on ΓD\Gamma_DΓD​.

Damping coefficient. ω⊂Ω\omega\subset\Omegaω⊂Ω is an open neighbourhood of ΓN\Gamma_NΓN​ (in Ω\OmegaΩ), and a∈L∞(Ω)a\in L^\infty(\Omega)a∈L∞(Ω) satisfies

a(x)≥0 a.e. in Ω(1.17),a(x)>a0>0 a.e. in ω(1.18).a(x)\ge0\ \text{a.e. in }\Omega\quad(1.17),\qquad a(x)>a_0>0\ \text{a.e. in }\omega\quad(1.18).a(x)≥0 a.e. in Ω(1.17),a(x)>a0​>0 a.e. in ω(1.18).

The system (1.12)–(1.16): for gains μ1,μ2>0\mu_1,\mu_2>0μ1​,μ2​>0 and delay τ>0\tau>0τ>0,

utt(x,t)−Δu(x,t)+a(x)[μ1ut(x,t)+μ2ut(x,t−τ)]=0in Ω×(0,∞),u_{tt}(x,t)-\Delta u(x,t)+a(x)\big[\mu_1u_t(x,t)+\mu_2u_t(x,t-\tau)\big]=0\quad\text{in }\Omega\times(0,\infty),utt​(x,t)−Δu(x,t)+a(x)[μ1​ut​(x,t)+μ2​ut​(x,t−τ)]=0in Ω×(0,∞),

with u=0u=0u=0 on ΓD\Gamma_DΓD​, ∂u/∂ν=0\partial u/\partial\nu=0∂u/∂ν=0 on ΓN\Gamma_NΓN​, initial data u(⋅,0)=u0u(\cdot,0)=u_0u(⋅,0)=u0​, ut(⋅,0)=u1u_t(\cdot,0)=u_1ut​(⋅,0)=u1​, and history ut(x,t−τ)=g0(x,t−τ)u_t(x,t-\tau)=g_0(x,t-\tau)ut​(x,t−τ)=g0​(x,t−τ) for t∈(0,τ)t\in(0,\tau)t∈(0,τ).

The energy. Assume μ2<μ1\mu_2<\mu_1μ2​<μ1​ (1.8) and fix ξ\xiξ with τμ2<ξ<τ(2μ1−μ2)\tau\mu_2<\xi<\tau(2\mu_1-\mu_2)τμ2​<ξ<τ(2μ1​−μ2​) (1.10). Then

F(t)=12∫Ω{ut2(x,t)+∣∇u(x,t)∣2}dx+ξ2∫Ωa(x)∫01ut2(x,t−τρ) dρ dx(1.19).\mathcal F(t)=\frac12\int_\Omega\big\{u_t^2(x,t)+|\nabla u(x,t)|^2\big\}dx+\frac\xi2\int_\Omega a(x)\int_0^1u_t^2(x,t-\tau\rho)\,d\rho\,dx\qquad(1.19).F(t)=21​∫Ω​{ut2​(x,t)+∣∇u(x,t)∣2}dx+2ξ​∫Ω​a(x)∫01​ut2​(x,t−τρ)dρdx(1.19).

The first summand is the standard energy E(t)\mathcal E(t)E(t); the second accounts for the velocity history on the delay window.

Formalization targets

Goal: Theorem 1.3

There exist C1,C2>0C_1,C_2>0C1​,C2​>0, depending on the data but not on the solution, such that every solution satisfies

F(t)≤C1 F(0) e−C2t∀t≥0.\mathcal F(t)\le C_1\,\mathcal F(0)\,e^{-C_2t}\qquad\forall t\ge0.F(t)≤C1​F(0)e−C2​t∀t≥0.

The constants are left existential, as in the paper, so no later sharpening of rates invalidates the goal.

Milestones (in the order of the proof)

  1. (4.4) The energy identity
F′(t)=−μ1 ⁣∫Ωaut2(t)−μ2 ⁣∫Ωaut(t)ut(t−τ)+ξτ−12 ⁣∫Ωaut2(t)−ξτ−12 ⁣∫Ωaut2(t−τ).\mathcal F'(t)=-\mu_1\!\int_\Omega a u_t^2(t)-\mu_2\!\int_\Omega a u_t(t)u_t(t-\tau)+\frac{\xi\tau^{-1}}2\!\int_\Omega a u_t^2(t)-\frac{\xi\tau^{-1}}2\!\int_\Omega a u_t^2(t-\tau).F′(t)=−μ1​∫Ω​aut2​(t)−μ2​∫Ω​aut​(t)ut​(t−τ)+2ξτ−1​∫Ω​aut2​(t)−2ξτ−1​∫Ω​aut2​(t−τ).
  1. Proposition 4.1 F\mathcal FF is nonincreasing and F′(t)≤−C∫Ωa{ut2(t)+ut2(t−τ)}dx\mathcal F'(t)\le-C\int_\Omega a\{u_t^2(t)+u_t^2(t-\tau)\}dxF′(t)≤−C∫Ω​a{ut2​(t)+ut2​(t−τ)}dx with C>0C>0C>0.
  2. Proposition 4.2 Observability for the undamped mixed problem: for TTT larger than some T0T_0T0​, Ew(0)≤C1∫0T∫ωwt2 dx dt\mathcal E_w(0)\le C_1\int_0^T\int_\omega w_t^2\,dx\,dtEw​(0)≤C1​∫0T​∫ω​wt2​dxdt.
  3. Proposition 4.3 Observability for the delayed system: for TTT larger than some T‾\overline TT, F(0)≤C0∫0T∫Ωa{ut2(t)+ut2(t−τ)}dx dt\mathcal F(0)\le C_0\int_0^T\int_\Omega a\{u_t^2(t)+u_t^2(t-\tau)\}dx\,dtF(0)≤C0​∫0T​∫Ω​a{ut2​(t)+ut2​(t−τ)}dxdt.
  4. Contraction step (p. 1579): some T>0T>0T>0 and C~∈[0,1)\widetilde C\in[0,1)C∈[0,1) with F(T)≤C~ F(0)\mathcal F(T)\le\widetilde C\,\mathcal F(0)F(T)≤CF(0) for every solution.

Significance

The result. Theorem 1.3 shows that a localized viscous damping acting only near the Neumann boundary keeps its exponential stabilizing effect when part of the feedback is delayed, provided the delayed gain is dominated by the undelayed one. Together with Theorem 1.4 of the same paper (instability for μ2≥μ1\mu_2\ge\mu_1μ2​≥μ1​ and suitable delays) it gives a sharp threshold in terms of the gains. The energy F\mathcal FF with its history term became the standard Lyapunov functional for delayed wave and plate equations in the literature that followed.

Formalizing it. The theorem is proved in the paper; no machine-checked proof of it, or of any exponential decay result for a multidimensional wave equation, is known to exist. A complete development would produce reusable Lean infrastructure: energy identities for the wave equation on C2C^2C2 domains via the divergence theorem, the delay-energy calculus, and an observability inequality for the wave equation with mixed boundary conditions. Each milestone has value on its own; Proposition 4.2 in particular is a classical control-theoretic result.

Difficulty

The energy estimates (milestones 1 and 2) are calculus once the divergence theorem is available. The central difficulty is observability. Energy dissipation alone gives only F\mathcal FF nonincreasing; exponential decay needs the energy at time 000 to be controlled by the energy dissipated on [0,T][0,T][0,T] (Proposition 4.3), and that needs the conservative wave equation to be observable from ω\omegaω (Proposition 4.2). The observability inequality does not follow from energy identities: the paper relies on Carleman estimates of Lasiecka–Triggiani–Yao (1999) and a compactness–uniqueness argument, neither of which is available in Mathlib. The obvious attempt, a multiplier identity with ∇v⋅∇u\nabla v\cdot\nabla u∇v⋅∇u alone, leaves boundary terms on ΓN\Gamma_NΓN​ that cannot be absorbed without a localization near ΓN\Gamma_NΓN​ and a lower-order compactness step.

Formalization scope

  • Points are EuclideanSpace ℝ (Fin n) with 1 ≤ n; solutions are real valued.
  • The C2C^2C2 boundary is given by a global C2C^2C2 defining function ψ\psiψ with Ω={ψ<0}\Omega=\{\psi<0\}Ω={ψ<0}, ∂Ω={ψ=0}\partial\Omega=\{\psi=0\}∂Ω={ψ=0}, ∇ψ≠0\nabla\psi\ne0∇ψ=0 on ∂Ω\partial\Omega∂Ω; ν=∇ψ/∣∇ψ∣\nu=\nabla\psi/|\nabla\psi|ν=∇ψ/∣∇ψ∣.
  • The surface measure dΓd\GammadΓ is a finite measure carried by ∂Ω\partial\Omega∂Ω for which the Gauss–Green formula holds for every C1C^1C1 vector field; this determines it uniquely. It is not Mathlib's unnormalized Hausdorff measure.
  • Solutions are classical: uuu is C2C^2C2 on Rn×R\mathbb{R}^n\times\mathbb{R}Rn×R, the equation holds for every t>0t>0t>0 and almost every x∈Ωx\in\Omegax∈Ω (because aaa is only L∞L^\inftyL∞), and the initial data and history are the values of uuu and utu_tut​ at t≤0t\le0t≤0. This is a subclass of the paper's solutions, so the formal theorems are consequences of the paper's.
  • aaa is measurable and essentially bounded on Ω\OmegaΩ; (1.17) and (1.18) are almost-everywhere conditions. "Open neighbourhood of ΓN\Gamma_NΓN​" means ω⊇O∩Ω\omega\supseteq O\cap\Omegaω⊇O∩Ω for some open O⊇ΓNO\supseteq\Gamma_NO⊇ΓN​ (a subset of Ω\OmegaΩ cannot contain ΓN\Gamma_NΓN​ itself).
  • Added hypothesis (Propositions 4.2, 4.3, the contraction step and Theorem 1.3): the closure of every connected component of Ω\OmegaΩ meets ΓD\Gamma_DΓD​; this holds whenever Ω\OmegaΩ is connected. The proof of Proposition 4.2 uses Poincaré's inequality for functions vanishing on ΓD\Gamma_DΓD​, and its compactness–uniqueness step concludes that a harmonic function vanishing on ΓD\Gamma_DΓD​ with zero normal derivative on ΓN\Gamma_NΓN​ is zero; both need this condition.
  • "Decreasing" in Proposition 4.1 is read as nonincreasing; its constant C>0C>0C>0 is existential, chosen before the solution.
  • Printed slips on p. 1575: the last line of (4.3) integrates with dΓd\GammadΓ where dxdxdx is meant, and its first line repeats uρ(x,t−τ)u_\rho(x,t-\tau)uρ​(x,t−τ) for uρ(x,t−τρ)u_\rho(x,t-\tau\rho)uρ​(x,t−τρ). Neither affects any formal statement; (4.4) itself is correct.
  • A formalization in which the aaa-weighted integrals are Lean's junk value 000 (non-measurable aaa), in which ω\omegaω is required to contain ΓN\Gamma_NΓN​ (unsatisfiable), or in which the surface measure is arbitrary, would trivialize or falsify the targets; all three are excluded by the definitions.

Needed infrastructure: the divergence theorem on C2C^2C2 domains (assumed here as a structure field), differentiation under the integral sign for the energies, Carleman estimates or another route to observability for the mixed wave problem, and a compactness argument (Rellich). Contributions of any of these as standalone lemmas 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
  • E. Zuazua, Exponential decay for the semilinear wave equation with locally distributed damping, Comm. Partial Differential Equations 15:205–235, 1990. https://doi.org/10.1080/03605309908820684
  • K. Liu, Locally distributed control and damping for the conservative systems, SIAM J. Control Optim. 35:1574–1590, 1997. https://doi.org/10.1137/S0363012995284928
  • I. Lasiecka, R. Triggiani, P. F. Yao, Inverse/observability estimates for second-order hyperbolic equations with variable coefficients, J. Math. Anal. Appl. 235:13–57, 1999 (reference [14] of the paper; the Carleman estimates used in Proposition 4.2). https://doi.org/10.1006/jmaa.1999.6348
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AnalysisFunctional AnalysisMathematical Physics·Captain: mikedeng1

Mathematical Methods in Quantum Mechanics XIV: Wave Operators and Cook's CriterionTextbook

Motivation

In a scattering experiment a particle arrives from far away, interacts with a target, and leaves again. Far from the target the forces are negligible, so long before and long after the collision the particle should move like a free particle. Scattering theory makes this precise by comparing two quantum dynamics: the free evolution e−itH0\mathrm e^{-\mathrm itH_0}e−itH0​ generated by the kinetic energy H0=−ΔH_0 = -\DeltaH0​=−Δ, and the full evolution e−itH\mathrm e^{-\mathrm itH}e−itH generated by H=H0+VH = H_0 + VH=H0​+V. The objects that compare them are the wave operators (Møller operators) Ω±\Omega_\pmΩ±​, introduced by Møller (1945) and put on a rigorous footing by Jauch (1958) and Kato. Cook (1957) gave the first practical criterion for their existence. Kuroda, Birman, Agmon, Enß and others later developed the theory up to asymptotic completeness for short-range potentials.

This mission formalizes the abstract part of Chapter 12 of Teschl's Mathematical Methods in Quantum Mechanics (AMS GSM 99, 2009): the definition and basic structure of the wave operators, Cook's criterion, and the existence of the wave operators for a square-integrable potential in three dimensions.

Setting

Let H\mathfrak HH be a complex Hilbert space. An operator AAA is a linear map on a subspace D(A)\mathfrak D(A)D(A), its domain; AAA is self-adjoint if D(A)\mathfrak D(A)D(A) is dense and A=A∗A = A^*A=A∗. A projection-valued measure PPP assigns to each Borel set Ω⊆R\Omega \subseteq \mathbb RΩ⊆R an orthogonal projection P(Ω)P(\Omega)P(Ω), with P(R)=IP(\mathbb R) = \mathbb IP(R)=I and P(⋃nΩn)ψ=∑nP(Ωn)ψP(\bigcup_n\Omega_n)\psi = \sum_n P(\Omega_n)\psiP(⋃n​Ωn​)ψ=∑n​P(Ωn​)ψ for disjoint Ωn\Omega_nΩn​. The spectral measure of ψ\psiψ is μψ(Ω)=⟨ψ,P(Ω)ψ⟩\mu_\psi(\Omega) = \langle\psi, P(\Omega)\psi\rangleμψ​(Ω)=⟨ψ,P(Ω)ψ⟩. By the spectral theorem every self-adjoint AAA equals ∫λ dP(λ)\int\lambda\,dP(\lambda)∫λdP(λ) for a unique PPP: D(A)={ψ∣∫λ2 dμψ<∞}\mathfrak D(A) = \{\psi \mid \int\lambda^2\,d\mu_\psi < \infty\}D(A)={ψ∣∫λ2dμψ​<∞} and ⟨ψ,Aψ⟩=∫λ dμψ\langle\psi, A\psi\rangle = \int\lambda\,d\mu_\psi⟨ψ,Aψ⟩=∫λdμψ​. The time evolution e−itA\mathrm e^{-\mathrm itA}e−itA is the bounded operator with ⟨ψ,e−itAψ⟩=∫e−itλ dμψ(λ)\langle\psi, \mathrm e^{-\mathrm itA}\psi\rangle = \int\mathrm e^{-\mathrm it\lambda}\,d\mu_\psi(\lambda)⟨ψ,e−itAψ⟩=∫e−itλdμψ​(λ).

For two self-adjoint operators H0H_0H0​, HHH the wave operators are

D(Ω±)={ψ∈H∣∃lim⁡t→±∞eitHe−itH0ψ},Ω±ψ=lim⁡t→±∞eitHe−itH0ψ.\mathfrak D(\Omega_\pm) = \{\psi \in \mathfrak H \mid \exists\lim_{t\to\pm\infty}\mathrm e^{\mathrm itH}\mathrm e^{-\mathrm itH_0}\psi\}, \qquad \Omega_\pm\psi = \lim_{t\to\pm\infty}\mathrm e^{\mathrm itH}\mathrm e^{-\mathrm itH_0}\psi .D(Ω±​)={ψ∈H∣∃t→±∞lim​eitHe−itH0​ψ},Ω±​ψ=t→±∞lim​eitHe−itH0​ψ.

D(Ω±)\mathfrak D(\Omega_\pm)D(Ω±​) is the set of asymptotic states and Ran⁡(Ω±)=Ω±D(Ω±)\operatorname{Ran}(\Omega_\pm) = \Omega_\pm\mathfrak D(\Omega_\pm)Ran(Ω±​)=Ω±​D(Ω±​) the set of states that have one. A closed subspace H1\mathfrak H_1H1​ with projection P1P_1P1​ reduces AAA if P1D(A)⊆D(A)P_1\mathfrak D(A) \subseteq \mathfrak D(A)P1​D(A)⊆D(A) and P1Aψ=AP1ψP_1A\psi = AP_1\psiP1​Aψ=AP1​ψ for ψ∈D(A)\psi \in \mathfrak D(A)ψ∈D(A).

On L2(Rn)L^2(\mathbb R^n)L2(Rn) the free Schrödinger operator is H0=−ΔH_0 = -\DeltaH0​=−Δ with domain the Sobolev space H2(Rn)H^2(\mathbb R^n)H2(Rn): under the Fourier transform it is multiplication by p2p^2p2 on {φ∣p2φ∈L2}\{\varphi \mid p^2\varphi \in L^2\}{φ∣p2φ∈L2}. For a real potential VVV, H=H0+VH = H_0 + VH=H0​+V has D(H)=H2(Rn)\mathfrak D(H) = H^2(\mathbb R^n)D(H)=H2(Rn) and (Hψ)(x)=(H0ψ)(x)+V(x)ψ(x)(H\psi)(x) = (H_0\psi)(x) + V(x)\psi(x)(Hψ)(x)=(H0​ψ)(x)+V(x)ψ(x).

Formalization targets

Goal: existence of the wave operators for V∈L2(R3)V \in L^2(\mathbb R^3)V∈L2(R3) (Theorem 12.4)

Let H0H_0H0​ be the free Schrödinger operator on L2(R3)L^2(\mathbb R^3)L2(R3) and H=H0+VH = H_0 + VH=H0​+V with a real V∈L2(R3)V \in L^2(\mathbb R^3)V∈L2(R3). Then

D(Ω+)=D(Ω−)=L2(R3),\mathfrak D(\Omega_+) = \mathfrak D(\Omega_-) = L^2(\mathbb R^3),D(Ω+​)=D(Ω−​)=L2(R3),

that is, lim⁡t→±∞eitHe−itH0ψ\lim_{t\to\pm\infty}\mathrm e^{\mathrm itH}\mathrm e^{-\mathrm itH_0}\psilimt→±∞​eitHe−itH0​ψ exists for every ψ\psiψ and both signs. Since the spectrum of H0H_0H0​ is purely absolutely continuous, this is exactly what Teschl calls "the wave operators exist" (12.14).

Milestones

  • Lemma 12.1. D(Ω±)\mathfrak D(\Omega_\pm)D(Ω±​) and Ran⁡(Ω±)\operatorname{Ran}(\Omega_\pm)Ran(Ω±​) are closed and Ω±:D(Ω±)→Ran⁡(Ω±)\Omega_\pm : \mathfrak D(\Omega_\pm) \to \operatorname{Ran}(\Omega_\pm)Ω±​:D(Ω±​)→Ran(Ω±​) is unitary.
  • Theorem 12.2. D(Ω±)\mathfrak D(\Omega_\pm)D(Ω±​) reduces H0H_0H0​, Ran⁡(Ω±)\operatorname{Ran}(\Omega_\pm)Ran(Ω±​) reduces HHH, and the restricted operators are unitarily equivalent: Ω±H0ψ=HΩ±ψ\Omega_\pm H_0\psi = H\Omega_\pm\psiΩ±​H0​ψ=HΩ±​ψ for ψ∈D(Ω±)∩D(H0)\psi \in \mathfrak D(\Omega_\pm) \cap \mathfrak D(H_0)ψ∈D(Ω±​)∩D(H0​).
  • Lemma 12.3 (Cook). If D(H)⊆D(H0)\mathfrak D(H) \subseteq \mathfrak D(H_0)D(H)⊆D(H0​), ψ∈D(H0)\psi \in \mathfrak D(H_0)ψ∈D(H0​) and ∫0∞∥(H−H0)exp⁡(∓itH0)ψ∥ dt<∞\int_0^\infty\|(H - H_0)\exp(\mp\mathrm itH_0)\psi\|\,dt < \infty∫0∞​∥(H−H0​)exp(∓itH0​)ψ∥dt<∞, then ψ∈D(Ω±)\psi \in \mathfrak D(\Omega_\pm)ψ∈D(Ω±​) and ∥(Ω±−I)ψ∥≤∫0∞∥(H−H0)exp⁡(∓itH0)ψ∥ dt\|(\Omega_\pm - \mathbb I)\psi\| \le \int_0^\infty\|(H - H_0)\exp(\mp\mathrm itH_0)\psi\|\,dt∥(Ω±​−I)ψ∥≤∫0∞​∥(H−H0​)exp(∓itH0​)ψ∥dt.

Significance

Existence of the wave operators is the first step of every scattering theory for Schrödinger operators: without it the scattering operator S=Ω+−1Ω−S = \Omega_+^{-1}\Omega_-S=Ω+−1​Ω−​ is not defined on a useful set of states, and the questions of completeness and asymptotic completeness (Enß's theorem, Theorem 12.12 of the same chapter) cannot be posed. Lemma 12.1 and Theorem 12.2 are the structural facts that make Ω±\Omega_\pmΩ±​ partial isometries intertwining the two Hamiltonians; they imply that HHH restricted to Ran⁡(Ω±)\operatorname{Ran}(\Omega_\pm)Ran(Ω±​) has absolutely continuous spectrum whenever H0H_0H0​ does, and that kinetic energy is conserved in scattering. Cook's criterion is the tool used in practice to prove existence for concrete potentials, including Coulomb-type and time-dependent problems.

The results are classical and proved in the literature. They are not formalized. Mathlib has neither the spectral theorem nor a functional calculus for unbounded self-adjoint operators, and no scattering theory. The platform has no statement about wave operators; its BookProof development contains Stone's theorem for its own structure of unbounded operators, which this mission does not use.

Difficulty

The limit defining Ω±\Omega_\pmΩ±​ involves two unitary groups whose generators do not commute, and neither group is explicit for the perturbed operator HHH. For Cook's criterion the product eitHe−itH0ψ\mathrm e^{\mathrm itH}\mathrm e^{-\mathrm itH_0}\psieitHe−itH0​ψ has to be differentiated in ttt, which needs control of domains: e−itH0ψ\mathrm e^{-\mathrm itH_0}\psie−itH0​ψ must stay in the domain of H−H0H - H_0H−H0​, and the derivative of a strongly continuous unitary group exists only on the domain of its generator. For the goal, the time evolution of a general ψ∈L2(R3)\psi \in L^2(\mathbb R^3)ψ∈L2(R3) has no decay rate at all, and the potential V∈L2V \in L^2V∈L2 is unbounded and has no decay assumption beyond square integrability, so the integrability condition of Cook's criterion cannot be checked for every ψ\psiψ directly. The intertwining relation (12.8) concerns unbounded operators and needs the reduction of the domains, not only an identity between bounded operators.

Formalization scope

The formalization uses Lean 4 with Mathlib. Operators are LinearPMaps H →ₗ.[ℂ] H on a complex Hilbert space; self-adjointness is Mathlib's IsSelfAdjoint. Separability is not assumed.

The spectral theorem is not part of this mission. Every statement takes projection-valued measures P0P_0P0​ and PPP as data, with the hypotheses H0=∫λ dP0(λ)H_0 = \int\lambda\,dP_0(\lambda)H0​=∫λdP0​(λ) and H=∫λ dP(λ)H = \int\lambda\,dP(\lambda)H=∫λdP(λ) (domain and quadratic form as above), which is the form the spectral theorem guarantees and which determines P0P_0P0​ and PPP. The time evolutions are e−itH0=∫e−itλ dP0\mathrm e^{-\mathrm itH_0} = \int\mathrm e^{-\mathrm it\lambda}\,dP_0e−itH0​=∫e−itλdP0​ and e−itH=∫e−itλ dP\mathrm e^{-\mathrm itH} = \int\mathrm e^{-\mathrm it\lambda}\,dPe−itH=∫e−itλdP. In the goal, the self-adjointness of H=H0+VH = H_0 + VH=H0​+V (Theorem 10.2 of the book) enters only through the existence of PPP. Nothing is assumed about Ω±\Omega_\pmΩ±​.

The sign of Ω±\Omega_\pmΩ±​ is a unit s : ℤˣ, and t→±∞t \to \pm\inftyt→±∞ is written as t→+∞t \to +\inftyt→+∞ in the variable ststst. Ω±\Omega_\pmΩ±​ is Mathlib's limUnder and is used only on D(Ω±)\mathfrak D(\Omega_\pm)D(Ω±​). A formalization that set Ω±ψ=0\Omega_\pm\psi = 0Ω±​ψ=0 where the limit fails and then proved only that Ω±\Omega_\pmΩ±​ is isometric would lose the content of the goal; here the goal asserts that the limit exists for every ψ∈L2(R3)\psi \in L^2(\mathbb R^3)ψ∈L2(R3). In Cook's lemma the finiteness of the integral is integrability on (0,∞)(0,\infty)(0,∞), the bound uses the Bochner integral, and the hypothesis that exp⁡(∓itH0)ψ\exp(\mp\mathrm itH_0)\psiexp(∓itH0​)ψ lies in D(H)\mathfrak D(H)D(H) for t≥0t \ge 0t≥0, which the integrand presupposes, is explicit.

L2(R3)L^2(\mathbb R^3)L2(R3) is Mathlib's Lp ℂ 2 on EuclideanSpace ℝ (Fin 3). The free Schrödinger operator is characterized through Mathlib's unitary L2L^2L2 Fourier transform FMf(ξ)=∫e−2πi⟨x,ξ⟩f(x) dx\mathcal F_M f(\xi) = \int\mathrm e^{-2\pi\mathrm i\langle x,\xi\rangle}f(x)\,dxFM​f(ξ)=∫e−2πi⟨x,ξ⟩f(x)dx, not the book's (2π)−n/2∫e−ipxf(x) dx(2\pi)^{-n/2}\int\mathrm e^{-\mathrm ipx}f(x)\,dx(2π)−n/2∫e−ipxf(x)dx. The constants are translated: D(H0)={ψ∣∣ξ∣2FMψ∈L2}\mathfrak D(H_0) = \{\psi \mid |\xi|^2\mathcal F_M\psi \in L^2\}D(H0​)={ψ∣∣ξ∣2FM​ψ∈L2} and FM(H0ψ)=4π2∣ξ∣2FMψ\mathcal F_M(H_0\psi) = 4\pi^2|\xi|^2\mathcal F_M\psiFM​(H0​ψ)=4π2∣ξ∣2FM​ψ. H=H0+VH = H_0 + VH=H0​+V has D(H)=D(H0)\mathfrak D(H) = \mathfrak D(H_0)D(H)=D(H0​) and Hψ=H0ψ+VψH\psi = H_0\psi + V\psiHψ=H0​ψ+Vψ almost everywhere.

A complete development needs a functional calculus for projection-valued measures (strong continuity and differentiability of e−itA\mathrm e^{-\mathrm itA}e−itA on D(A)\mathfrak D(A)D(A), Theorem 5.1), the explicit L1→L∞L^1 \to L^\inftyL1→L∞ decay of the free Schrödinger group in R3\mathbb R^3R3 ((7.31) of the book), and density of L1∩H2L^1 \cap H^2L1∩H2 in L2L^2L2. These pieces are reusable for the rest of Chapter 12 (incoming and outgoing states, short-range potentials, asymptotic completeness). Proofs of any milestone and of such supporting lemmas are welcome.

Selected references

  • G. Teschl, Mathematical Methods in Quantum Mechanics, With Applications to Schrödinger Operators, Graduate Studies in Mathematics 99, American Mathematical Society, 2009. doi:10.1090/gsm/099. Chapter 12, pp. 247–257.
  • J. M. Cook, Convergence to the Møller wave-matrix, J. Math. and Phys. 36 (1957), 82–87. doi:10.1002/sapm195736182.
  • J. M. Jauch, Theory of the scattering operator, Helv. Phys. Acta 31 (1958), 127–158.
  • M. Reed, B. Simon, Methods of Modern Mathematical Physics III: Scattering Theory, Academic Press, 1979.
  • V. Enß, Asymptotic completeness for quantum mechanical potential scattering. I. Short range potentials, Comm. Math. Phys. 61 (1978), 285–291. doi:10.1007/BF01940771.
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AnalysisFunctional AnalysisMathematical Physics·Captain: mikedeng1

Mathematical Methods in Quantum Mechanics XIII: Atomic Schrödinger Operators and the HVZ TheoremTextbook

Motivation

An atom with NNN electrons is described, with the nucleus fixed at the origin, by a Schrödinger operator on L2(R3N)L^2(\mathbb R^{3N})L2(R3N) whose potential does not decay in all directions: moving one electron to infinity while the others stay near the nucleus leaves the remaining Coulomb attraction untouched. For this reason the standard route to the essential spectrum of a one-particle operator, showing that the potential is a relatively compact perturbation of −Δ-\Delta−Δ, fails for N≥2N \ge 2N≥2. The HVZ theorem, due to Zhislin (1960), van Winter (1964) and Hunziker (1966), gives the answer anyway: the essential spectrum of the NNN-electron atom begins exactly at the ground state energy of the ion with one electron removed. It is the basic structural result of NNN-body quantum mechanics, and the starting point for every discussion of bound states, ionization energies and the stability of atoms and molecules.

This mission follows Chapter 11 of Teschl, Mathematical Methods in Quantum Mechanics (AMS GSM 99, 2009), which proves self-adjointness by Kato's theorem and the HVZ theorem by the localization method of Ismagilov, Morgan, Simon and Sigal.

Setting

Write Rn\mathbb R^nRn for Euclidean space with Lebesgue measure. The Sobolev space H2(Rn)H^2(\mathbb R^n)H2(Rn) is the set of ψ∈L2(Rn)\psi \in L^2(\mathbb R^n)ψ∈L2(Rn) with ∣p∣2ψ^(p)∈L2(Rn)|p|^2 \hat\psi(p) \in L^2(\mathbb R^n)∣p∣2ψ^​(p)∈L2(Rn), and the free Schrödinger operator is H0ψ=−Δψ=(∣p∣2ψ^)∨H_0\psi = -\Delta\psi = (|p|^2\hat\psi)^\veeH0​ψ=−Δψ=(∣p∣2ψ^​)∨ with domain H2(Rn)H^2(\mathbb R^n)H2(Rn) (units ℏ=1\hbar = 1ℏ=1, mass 1/21/21/2). A measurable function VVV acts as the multiplication operator (Vψ)(x)=V(x)ψ(x)(V\psi)(x) = V(x)\psi(x)(Vψ)(x)=V(x)ψ(x) on its maximal domain {ψ∈L2∣Vψ∈L2}\{\psi \in L^2 \mid V\psi \in L^2\}{ψ∈L2∣Vψ∈L2}.

For an operator AAA with domain D(A)\mathfrak D(A)D(A) in a Hilbert space, the resolvent set ρ(A)\rho(A)ρ(A) is the set of z∈Cz \in \mathbb Cz∈C for which A−zA - zA−z maps D(A)\mathfrak D(A)D(A) bijectively onto the space with bounded inverse RA(z)R_A(z)RA​(z), and σ(A)=C∖ρ(A)\sigma(A) = \mathbb C \setminus \rho(A)σ(A)=C∖ρ(A) is the spectrum. The discrete spectrum σd(A)\sigma_d(A)σd​(A) consists of the eigenvalues that are isolated points of σ(A)\sigma(A)σ(A) and have finite-dimensional eigenspaces; 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). 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 γ∈R\gamma \in \mathbb Rγ∈R. BBB is AAA bounded if D(A)⊆D(B)\mathfrak D(A) \subseteq \mathfrak D(B)D(A)⊆D(B) and ∥Bψ∥≤a∥Aψ∥+b∥ψ∥\|B\psi\| \le a\|A\psi\| + b\|\psi\|∥Bψ∥≤a∥Aψ∥+b∥ψ∥; the infimum of admissible aaa is the AAA-bound. KKK is relatively compact with respect to AAA if KRA(z)K R_A(z)KRA​(z) is compact for one z∈ρ(A)z \in \rho(A)z∈ρ(A).

For an atom with NNN electrons at x=(x1,…,xN)∈R3Nx = (x_1, \dots, x_N) \in \mathbb R^{3N}x=(x1​,…,xN​)∈R3N, xj∈R3x_j \in \mathbb R^3xj​∈R3, and constants γne,γee>0\gamma_{ne}, \gamma_{ee} > 0γne​,γee​>0, the atomic Hamiltonian is

H(N)=−∑j=1NΔj−∑j=1Nγne∣xj∣+∑1≤j<k≤Nγee∣xj−xk∣,D(H(N))=H2(R3N).H^{(N)} = -\sum_{j=1}^N \Delta_j - \sum_{j=1}^N \frac{\gamma_{ne}}{|x_j|} + \sum_{1 \le j < k \le N} \frac{\gamma_{ee}}{|x_j - x_k|}, \qquad \mathfrak D(H^{(N)}) = H^2(\mathbb R^{3N}).H(N)=−j=1∑N​Δj​−j=1∑N​∣xj​∣γne​​+1≤j<k≤N∑​∣xj​−xk​∣γee​​,D(H(N))=H2(R3N).

H(N−1)H^{(N-1)}H(N−1) denotes the same operator for N−1N - 1N−1 electrons with the same constants.

Formalization targets

Goal: the HVZ theorem (Theorem 11.2)

For N≥1N \ge 1N≥1, H(N)H^{(N)}H(N) is bounded from below, and

σess(H(N))=[λN−1,∞),λN−1=min⁡σ(H(N−1)),\sigma_{ess}(H^{(N)}) = [\lambda^{N-1}, \infty), \qquad \lambda^{N-1} = \min \sigma(H^{(N-1)}),σess​(H(N))=[λN−1,∞),λN−1=minσ(H(N−1)),

with λN−1<0\lambda^{N-1} < 0λN−1<0 for N≥2N \ge 2N≥2. The minimum is attained and, for N≥2N \ge 2N≥2, negative; both are part of the claim.

Milestones

  • Kato's theorem (Theorem 11.1). For real-valued Vk∈L∞∞(Rd)+L2(Rd)V_k \in L^\infty_\infty(\mathbb R^d) + L^2(\mathbb R^d)Vk​∈L∞∞​(Rd)+L2(Rd), d≤3d \le 3d≤3, composed with the first ddd coordinates of orthogonal transformations of RNd\mathbb R^{Nd}RNd, each Vk(y(k))V_k(y^{(k)})Vk​(y(k)) has H0H_0H0​-bound 000, and H=H0+∑kVk(y(k))H = H_0 + \sum_k V_k(y^{(k)})H=H0​+∑k​Vk​(y(k)) with D(H)=H2(RNd)\mathfrak D(H) = H^2(\mathbb R^{Nd})D(H)=H2(RNd) is self-adjoint with core C0∞(RNd)C_0^\infty(\mathbb R^{Nd})C0∞​(RNd).
  • IMS localization formula (Lemma 11.3). If φj∈C∞(Rn)\varphi_j \in C^\infty(\mathbb R^n)φj​∈C∞(Rn) satisfy ∑jφj2=1\sum_j \varphi_j^2 = 1∑j​φj2​=1, then for ψ∈H2(Rn)\psi \in H^2(\mathbb R^n)ψ∈H2(Rn)
Δψ=∑j(φjΔ(φjψ)+∣∂φj∣2ψ).\Delta\psi = \sum_{j} \big(\varphi_j\Delta(\varphi_j\psi) + |\partial\varphi_j|^2\psi\big).Δψ=j∑​(φj​Δ(φj​ψ)+∣∂φj​∣2ψ).
  • Localizing partition (Lemma 11.4). For C∈(0,1/N)C \in (0, 1/\sqrt N)C∈(0,1/N​) there are smooth φj:R3N→[0,1]\varphi_j : \mathbb R^{3N} \to [0,1]φj​:R3N→[0,1] with ∑jφj2=1\sum_j \varphi_j^2 = 1∑j​φj2​=1, supp⁡φj∩{∣x∣≥1}⊆{∣xj∣≥C∣x∣}\operatorname{supp}\varphi_j \cap \{|x| \ge 1\} \subseteq \{|x_j| \ge C|x|\}suppφj​∩{∣x∣≥1}⊆{∣xj​∣≥C∣x∣} and ∣∂φj(x)∣→0|\partial\varphi_j(x)| \to 0∣∂φj​(x)∣→0 as ∣x∣→∞|x| \to \infty∣x∣→∞.
  • A compactness criterion (Lemma 11.5). A multiplication operator VVV with H0H_0H0​-bound 000 and ∥χ{∣x∣≥R}VRH0(z)∥→0\|\chi_{\{|x| \ge R\}} V R_{H_0}(z)\| \to 0∥χ{∣x∣≥R}​VRH0​​(z)∥→0 as R→∞R \to \inftyR→∞ is relatively compact with respect to H0H_0H0​.

Significance

The result. The HVZ theorem separates the spectrum of an atom into a continuum [λN−1,∞)[\lambda^{N-1}, \infty)[λN−1,∞), fixed by the (N−1)(N-1)(N−1)-electron ion, and a discrete part below it consisting of bound states. The ionization energy of the atom is λN−λN−1\lambda^N - \lambda^{N-1}λN−λN−1. Questions such as whether a given atom or negative ion has a bound state at all, whether it has infinitely many (Zhislin's theorem for neutral atoms and positive ions), and how many electrons a nucleus can bind are all formulated relative to the threshold the HVZ theorem identifies. The same argument, with additional notation, covers molecules with fixed nuclei and general NNN-body systems.

Formalizing it. The results are classical and proved in the standard texts (Reed–Simon IV, Cycon–Froese–Kirsch–Simon, Teschl). None is formalized. Mathlib now has the unitary Fourier transform on L2L^2L2, tempered distributions and Sobolev spaces defined through the Fourier transform, but no self-adjoint Schrödinger operators, no essential spectrum and no many-body Hamiltonians. This mission asks for formal proofs of Teschl's four supporting results and of the HVZ theorem, and in doing so fixes a concrete representation of H0H_0H0​, of Coulomb-type multiplication operators and of the NNN-electron atom on which later work (bound states of atoms, scattering) can build.

Difficulty

The obvious argument for the essential spectrum of −Δ+V-\Delta + V−Δ+V, relative compactness of VVV followed by Weyl's theorem, is not available: γne/∣xj∣\gamma_{ne}/|x_j|γne​/∣xj​∣ does not vanish as ∣x∣→∞|x| \to \infty∣x∣→∞ in directions where xjx_jxj​ stays bounded, and it is not relatively compact with respect to H0H_0H0​ on L2(R3N)L^2(\mathbb R^{3N})L2(R3N). The inclusion σess(H(N))⊆[λN−1,∞)\sigma_{ess}(H^{(N)}) \subseteq [\lambda^{N-1}, \infty)σess​(H(N))⊆[λN−1,∞) therefore requires decomposing configuration space into regions in which one specific electron is far from the nucleus, controlling the error terms of that decomposition, and comparing the localized pieces with decoupled operators whose spectrum is known; this uses self-adjointness and relative bounds for operators built from the same potentials with one electron removed. The reverse inclusion requires approximate eigenfunctions built from those of H(N−1)H^{(N-1)}H(N−1) and of the free one-electron operator, and a statement that λN−1\lambda^{N-1}λN−1 is attained. Negativity of λN−1\lambda^{N-1}λN−1 needs the hydrogen-like ground state and a comparison argument across NNN.

Behind all of this sits the analytic layer: Kato's theorem requires that 1/∣x∣1/|x|1/∣x∣ in three dimensions is infinitesimally bounded with respect to −Δ-\Delta−Δ and that this survives the passage to R3N\mathbb R^{3N}R3N through an orthogonal change of variables; the IMS formula requires relating the Fourier definition of H0H_0H0​ to derivatives of products.

Formalization scope

The Hilbert space is Lp ℂ 2 volume over EuclideanSpace ℝ ι; for the atom, ι=Fin N × Fin 3\iota = \texttt{Fin N × Fin 3}ι=Fin N × Fin 3, so ∣x∣|x|∣x∣ is the Euclidean norm on R3N\mathbb R^{3N}R3N and xjx_jxj​ is electron x j. Operators are Mathlib LinearPMaps, self-adjointness is Mathlib's IsSelfAdjoint, and sums of unbounded operators are LinearPMap sums with the intersection of the domains. H0H_0H0​ (freeHamiltonian) is defined as F−1 (4π2∥ξ∥2) F\mathcal F^{-1}\,(4\pi^2\|\xi\|^2)\,\mathcal FF−1(4π2∥ξ∥2)F with Mathlib's unitary L2L^2L2 Fourier transform (kernel e−2πi⟨x,ξ⟩e^{-2\pi i\langle x,\xi\rangle}e−2πi⟨x,ξ⟩, no prefactor); this is the same operator −Δ-\Delta−Δ on the same domain H2H^2H2 as Teschl's F−1∣p∣2FF^{-1}|p|^2FF−1∣p∣2F. Multiplication operators (mulOp) have their maximal domains. H(N)H^{(N)}H(N) (atomicHamiltonian) is freeHamiltonian + mulOp V^{(N)}; the equality of its domain with H2(R3N)H^2(\mathbb R^{3N})H2(R3N) is a claim of Theorem 11.1, not an assumption. Resolvent set, spectrum, discrete and essential spectrum are defined from the bounded two-sided inverse of A−zA - zA−z, not from Mathlib's Banach-algebra spectrum. The AAA-bound takes values in [0,∞][0, \infty][0,∞]. The IMS formula is stated in the sense of distributions, tested against C0∞C_0^\inftyC0∞​ functions, since for merely smooth φj\varphi_jφj​ its right-hand side need not lie in L2L^2L2. No projection-valued measure or functional calculus is taken as data.

A trivializing formalization is ruled out: λN−1\lambda^{N-1}λN−1 is defined as the minimum of the spectrum of the independently constructed (N−1)(N-1)(N−1)-electron operator, never as the infimum of σess(H(N))\sigma_{ess}(H^{(N)})σess​(H(N)), which would make (11.9) circular; its attainment and negativity are conclusions. The goal covers N≥1N \ge 1N≥1; for N=1N = 1N=1 the ion has no electrons, λ0=0\lambda^0 = 0λ0=0 is not negative, so the negativity of λN−1\lambda^{N-1}λN−1 is claimed for N≥2N \ge 2N≥2 only.

A complete development needs the L2L^2L2 theory of the Fourier transform and H2H^2H2, Hardy- or Sobolev-type bounds for 1/∣x∣1/|x|1/∣x∣ in R3\mathbb R^3R3, the Kato–Rellich theorem, Weyl's theorem on relatively compact perturbations, a smooth partition of unity on the sphere, and the Weyl criterion for essential spectrum. The definitions of H0H_0H0​, multiplication operators, resolvent and essential spectrum are shared with other chapters of this series and are intended for reuse; contributions of general lemmas about them are welcome.

Selected references

  • G. Teschl, Mathematical Methods in Quantum Mechanics, With Applications to Schrödinger Operators, Graduate Studies in Mathematics 99, AMS, 2009, Chapter 11. https://doi.org/10.1090/gsm/099
  • G. M. Zhislin, Discussion of the spectrum of Schrödinger operators for systems of many particles, Trudy Moskovskogo Matematicheskogo Obshchestva 9 (1960), 81–120.
  • C. van Winter, Theory of finite systems of particles I. The Green function, Matematisk-Fysiske Skrifter Danske Videnskabernes Selskab 2 (1964), no. 8.
  • W. Hunziker, On the spectra of Schrödinger multiparticle Hamiltonians, Helvetica Physica Acta 39 (1966), 451–462.
  • 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
  • H. L. Cycon, R. G. Froese, W. Kirsch, B. Simon, Schrödinger Operators with Application to Quantum Mechanics and Global Geometry, Springer, 1987.
  • M. Reed and B. Simon, Methods of Modern Mathematical Physics IV: Analysis of Operators, Academic Press, 1978, Section XIII.5.
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AnalysisDifferential GeometryPure Mathematics·Captain: mikedeng1

Tasty Bits of Several Complex Variables VII: The Dolbeault Lemma on Polydiscs and the Cousin I ProblemTextbook

Motivation

In one complex variable, every smooth function ggg on a disc is ∂ψ/∂zˉ\partial\psi/\partial\bar z∂ψ/∂zˉ of some smooth ψ\psiψ, and this is what makes the Mittag-Leffler theorem work: local principal parts can be glued into a global meromorphic function. In several variables the corresponding equation is the ∂ˉ\bar\partial∂ˉ-problem: given a differential form η\etaη with ∂ˉη=0\bar\partial\eta = 0∂ˉη=0, find ω\omegaω with ∂ˉω=η\bar\partial\omega = \eta∂ˉω=η. Whether it is solvable on a domain U⊂CnU \subset \mathbb{C}^nU⊂Cn is measured by the Dolbeault cohomology groups H(p,q)(U)H^{(p,q)}(U)H(p,q)(U). Their vanishing characterizes domains of holomorphy, and it drives the solution of the additive Cousin I problem, the several-variable Mittag-Leffler problem.

This mission follows §4.4–4.6 of Jiří Lebl's open textbook Tasty Bits of Several Complex Variables (version 4.4, 2026). There the ∂ˉ\bar\partial∂ˉ-problem is solved on polydiscs, from the one-variable Cauchy transform through the Dolbeault–Grothendieck lemma. The result is then applied to the Cousin I problem and to domains of holomorphy. The Dolbeault lemma goes back to P. Dolbeault (1953) and A. Grothendieck. The global theory on pseudoconvex domains is due to Hörmander (An Introduction to Complex Analysis in Several Variables, 1966) and to Cartan's Theorem B.

Setting

Write zk=xk+iykz_k = x_k + i y_kzk​=xk​+iyk​ for the coordinates of Cn\mathbb{C}^nCn. The Wirtinger derivative of a function fff is ∂f/∂zˉk=12(∂f/∂xk+i ∂f/∂yk)\partial f/\partial\bar z_k = \tfrac12(\partial f/\partial x_k + i\,\partial f/\partial y_k)∂f/∂zˉk​=21​(∂f/∂xk​+i∂f/∂yk​).

For strictly increasing tuples α=(α1<⋯<αp)\alpha = (\alpha_1<\dots<\alpha_p)α=(α1​<⋯<αp​) and β=(β1<⋯<βq)\beta = (\beta_1<\dots<\beta_q)β=(β1​<⋯<βq​) in {1,…,n}\{1,\dots,n\}{1,…,n}, write dzα=dzα1∧⋯∧dzαpdz_\alpha = dz_{\alpha_1}\wedge\cdots\wedge dz_{\alpha_p}dzα​=dzα1​​∧⋯∧dzαp​​ and dzˉβ=dzˉβ1∧⋯∧dzˉβqd\bar z_\beta = d\bar z_{\beta_1}\wedge\cdots\wedge d\bar z_{\beta_q}dzˉβ​=dzˉβ1​​∧⋯∧dzˉβq​​. A smooth (p,q)(p,q)(p,q)-form on an open U⊂CnU\subset\mathbb{C}^nU⊂Cn is

η=∑α,βηαβ dzα∧dzˉβ,\eta = \sum_{\alpha,\beta}\eta_{\alpha\beta}\,dz_\alpha\wedge d\bar z_\beta,η=α,β∑​ηαβ​dzα​∧dzˉβ​,

where α\alphaα and β\betaβ run over the increasing ppp- and qqq-tuples and each ηαβ\eta_{\alpha\beta}ηαβ​ is C∞C^\inftyC∞ on UUU. The operator

∂ˉη=∑α,β∑k=1n∂ηαβ∂zˉk dzˉk∧dzα∧dzˉβ\bar\partial\eta = \sum_{\alpha,\beta}\sum_{k=1}^n \frac{\partial\eta_{\alpha\beta}}{\partial\bar z_k}\,d\bar z_k\wedge dz_\alpha\wedge d\bar z_\beta∂ˉη=α,β∑​k=1∑n​∂zˉk​∂ηαβ​​dzˉk​∧dzα​∧dzˉβ​

maps (p,q)(p,q)(p,q)-forms to (p,q+1)(p,q+1)(p,q+1)-forms. A form is ∂ˉ\bar\partial∂ˉ-closed if ∂ˉη=0\bar\partial\eta = 0∂ˉη=0 and ∂ˉ\bar\partial∂ˉ-exact if η=∂ˉω\eta = \bar\partial\omegaη=∂ˉω; by convention the only exact (p,0)(p,0)(p,0)-form is 000. The statement H(p,q)(U)=0H^{(p,q)}(U) = 0H(p,q)(U)=0 means that every smooth ∂ˉ\bar\partial∂ˉ-closed (p,q)(p,q)(p,q)-form on UUU is ∂ˉ\bar\partial∂ˉ-exact.

A possibly unbounded polydisc is a product Δ=D1×⋯×Dn\Delta = D_1\times\cdots\times D_nΔ=D1​×⋯×Dn​ in which each DkD_kDk​ is either a disc {∣zk−ak∣<ρk}\{|z_k - a_k|<\rho_k\}{∣zk​−ak​∣<ρk​} or all of C\mathbb{C}C; for example Cn\mathbb{C}^nCn itself. The finite polydisc is Δr(w)={z:∣zℓ−wℓ∣<rℓ ∀ℓ}\Delta_r(w) = \{z : |z_\ell - w_\ell| < r_\ell\ \forall\ell\}Δr​(w)={z:∣zℓ​−wℓ​∣<rℓ​ ∀ℓ}.

Cousin I data on an open UUU consist of an open covering {Uι}ι∈I\{U_\iota\}_{\iota\in I}{Uι​}ι∈I​ of UUU and holomorphic hικh_{\iota\kappa}hικ​ on Uι∩UκU_\iota\cap U_\kappaUι​∩Uκ​ with hικ+hκι=0h_{\iota\kappa}+h_{\kappa\iota}=0hικ​+hκι​=0 and hικ+hκλ+hλι=0h_{\iota\kappa}+h_{\kappa\lambda}+h_{\lambda\iota}=0hικ​+hκλ​+hλι​=0 on the respective intersections. A solution is a family of holomorphic fιf_\iotafι​ on UιU_\iotaUι​ with hικ=fι−fκh_{\iota\kappa} = f_\iota - f_\kappahικ​=fι​−fκ​. The problem is solvable on UUU if all Cousin I data on UUU have solutions.

In Lean these are wirtingerBar, FormCoeffs, dbar, IsSmoothForm, DolbeaultVanishes, polydisc, IsPossiblyUnboundedPolydisc, IsCousinISolvable and IsDomainOfHolomorphy in the namespace LeblSCV.Dolbeault.

Formalization targets

Goal: Theorem 4.4.5

Let Δ⊂Cn\Delta\subset\mathbb{C}^nΔ⊂Cn be a possibly unbounded polydisc, p≥0p\ge0p≥0, q≥1q\ge1q≥1, and η\etaη a smooth (p,q)(p,q)(p,q)-form on Δ\DeltaΔ with ∂ˉη=0\bar\partial\eta = 0∂ˉη=0. Then there is a smooth (p,q−1)(p,q-1)(p,q−1)-form ω\omegaω on Δ\DeltaΔ with

∂ˉω=ηon Δ,that is,H(p,q)(Δ)=0  (q≥1).\bar\partial\omega = \eta\quad\text{on }\Delta,\qquad\text{that is,}\qquad H^{(p,q)}(\Delta) = 0 \ \ (q\ge1).∂ˉω=ηon Δ,that is,H(p,q)(Δ)=0  (q≥1).

Milestones

  1. Lemma 4.4.6 (for a disc UUU). If ggg is smooth near U‾\overline UU, then ψ(z)=12πi∫Ug(ζ)ζ−z dζ∧dζˉ\psi(z) = \frac{1}{2\pi i}\int_U \frac{g(\zeta)}{\zeta-z}\,d\zeta\wedge d\bar\zetaψ(z)=2πi1​∫U​ζ−zg(ζ)​dζ∧dζˉ​ is smooth on UUU and ∂ψ/∂zˉ=g\partial\psi/\partial\bar z = g∂ψ/∂zˉ=g.
  2. Lemma 4.4.7 (Dolbeault–Grothendieck). If 0<sℓ<rℓ0<s_\ell<r_\ell0<sℓ​<rℓ​, every smooth ∂ˉ\bar\partial∂ˉ-closed (p,q)(p,q)(p,q)-form on Δr(w)\Delta_r(w)Δr​(w), q≥1q\ge1q≥1, is ∂ˉ\bar\partial∂ˉ of a smooth (p,q−1)(p,q-1)(p,q−1)-form on Δs(w)\Delta_s(w)Δs​(w).
  3. Lemma 4.6.4. Smooth Cousin I data on any open set have smooth solutions.
  4. Theorem 4.6.5. On a domain with H(0,1)(U)=0H^{(0,1)}(U)=0H(0,1)(U)=0 the Cousin I problem is solvable.
  5. Corollary 4.6.6. The Cousin I problem is solvable on every possibly unbounded polydisc.
  6. Theorem 4.5.6. A domain U⊂CnU\subset\mathbb{C}^nU⊂Cn with H(0,q)(U)=0H^{(0,q)}(U)=0H(0,q)(U)=0 for 1≤q≤n−11\le q\le n-11≤q≤n−1 is a domain of holomorphy.

Significance

Theorem 4.4.5 is the model case of the vanishing theorem H(p,q)(U)=0H^{(p,q)}(U)=0H(p,q)(U)=0, q≥1q\ge1q≥1, on domains of holomorphy. In particular it solves the ∂ˉ\bar\partial∂ˉ-problem on all of Cn\mathbb{C}^nCn. Through Theorem 4.6.5 it gives the Cousin I problem on polydiscs, and therefore the existence of meromorphic functions with prescribed local principal parts there. Theorem 4.5.6 is one half of the cohomological characterization of domains of holomorphy (Remark 4.5.8, item (viii)). The other half is Cartan's Theorem B, which the book states without proof as Theorem 4.4.2.

All targets are classical and fully proved in the book. As far as a search of the Prove2Me corpus and of Mathlib shows, none of them is formalized. Mathlib has real Fréchet derivatives, smooth bump functions and partitions of unity, and Lebesgue measure on C\mathbb{C}C. It has no bidegree forms, no ∂ˉ\bar\partial∂ˉ operator on forms, no Cauchy transform and no Dolbeault cohomology. This mission builds the (p,q)(p,q)(p,q)-form layer and the first global solvability theorem for ∂ˉ\bar\partial∂ˉ.

Difficulty

The one-variable step needs the Cauchy–Pompeiu formula and differentiation under an integral with a weakly singular kernel. Both the smoothness of ψ\psiψ and the identity ∂ψ/∂zˉ=g\partial\psi/\partial\bar z = g∂ψ/∂zˉ=g require care near ζ=z\zeta = zζ=z.

In several variables, the natural idea is to solve ∂ˉω=η\bar\partial\omega=\eta∂ˉω=η on each of an exhausting sequence of polydiscs and take a limit. It fails as stated: solutions on successive polydiscs differ by ∂ˉ\bar\partial∂ˉ-closed forms and need not converge. For q≥2q\ge2q≥2 the discrepancy has to be corrected exactly, by applying the lemma again with a cutoff. For q=1q=1q=1 the discrepancies are holomorphic functions, and they have to be made small by polynomial approximation, so that the corrected solutions converge. The Dolbeault–Grothendieck lemma loses a little of the polydisc at each step, so the argument has to shrink the polydiscs at each stage.

On the formal side, ∂ˉ\bar\partial∂ˉ on forms carries signs from reordering wedge products. A wrong sign changes which forms are closed. So the sign convention is fixed in the definition and checked against ∂ˉ∘∂ˉ=0\bar\partial\circ\bar\partial = 0∂ˉ∘∂ˉ=0.

Formalization scope

  • Cn\mathbb{C}^nCn is Fin n → ℂ with 0-based indices. Polydiscs use the modulus in each coordinate, as in the book, so the sup norm of Fin n → ℂ agrees with them. No Euclidean ball occurs.
  • A form is a coefficient family FormCoeffs n = Finset (Fin n) → Finset (Fin n) → (Fin n → ℂ) → ℂ: an increasing tuple is the set of its entries, and η A B z is the coefficient of dzA∧dzˉBdz_A\wedge d\bar z_BdzA​∧dzˉB​. IsSmoothForm U p q η requires every coefficient to be ContDiffOn ℝ ∞ on UUU and the coefficients of the wrong bidegree to vanish on UUU. Only values on UUU matter.
  • dbar is Definition 4.4.1 written in the increasing basis. The coefficient of dzA∧dzˉCdz_A\wedge d\bar z_CdzA​∧dzˉC​ is ∑k∈C(−1)∣A∣+#{j∈C:j<k} ∂ηA,C∖{k}/∂zˉk\sum_{k\in C}(-1)^{|A|+\#\{j\in C:j<k\}}\,\partial\eta_{A,C\setminus\{k\}}/\partial\bar z_k∑k∈C​(−1)∣A∣+#{j∈C:j<k}∂ηA,C∖{k}​/∂zˉk​. A sorry-free check confirms that this sign convention makes the mixed second derivatives cancel in ∂ˉ∂ˉη\bar\partial\bar\partial\eta∂ˉ∂ˉη, and that ∂zˉ1/∂zˉ1=1\partial\bar z_1/\partial\bar z_1 = 1∂zˉ1​/∂zˉ1​=1.
  • H(p,q)(U)=0H^{(p,q)}(U)=0H(p,q)(U)=0 is stated as "every closed smooth (p,q)(p,q)(p,q)-form is exact"; the quotient space is not built. The solution ω\omegaω is required to be smooth.
  • Radii of a possibly unbounded polydisc lie in ℝ≥0∞, with ∞\infty∞ meaning the factor C\mathbb{C}C.
  • Holomorphic on an open set is DifferentiableOn ℂ. A domain is an open connected set. Cousin index types range over Type, which loses nothing.
  • Restriction: Lemma 4.4.6 is stated for UUU an open disc. The book allows any bounded open set with piecewise-C1C^1C1 boundary. The disc is the case that the Dolbeault–Grothendieck lemma uses. The measure dζ∧dζˉd\zeta\wedge d\bar\zetadζ∧dζˉ​ is −2i-2i−2i times Lebesgue measure.
  • The goal cannot be trivialized through the form layer. A definition of ∂ˉ\bar\partial∂ˉ with a wrong sign, or one that drops the smoothness of ω\omegaω or the ∂ˉ\bar\partial∂ˉ-closedness of η\etaη, states a different theorem and is ruled out. Hypotheses are satisfiable: η=0\eta = 0η=0 is closed, and Cn\mathbb{C}^nCn is a possibly unbounded polydisc (checked sorry-free).
  • Needed infrastructure: the Cauchy transform and Cauchy–Pompeiu formula, differentiation under the integral with parameters, smooth cutoffs, uniform approximation of holomorphic functions by polynomials on polydiscs, and partitions of unity. The form layer is reusable in later work on the ∂ˉ\bar\partial∂ˉ-problem (balls, Hartogs triangle, pseudoconvex domains). Proofs of ∂ˉ2=0\bar\partial^2 = 0∂ˉ2=0 for the dbar defined here, or of the one-variable lemma for general piecewise-C1C^1C1 domains, are welcome.

Selected references

  • J. Lebl, Tasty Bits of Several Complex Variables, version 4.4, 2026, §4.4–4.6. https://www.jirka.org/scv/
  • L. Hörmander, An Introduction to Complex Analysis in Several Variables, North-Holland Mathematical Library 7, 3rd ed., 1990.
  • P. Dolbeault, Sur la cohomologie des variétés analytiques complexes, C. R. Acad. Sci. Paris 236 (1953), 175–177.
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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 I: Exponential Decay under Delayed Boundary FeedbackResearch Paper

Motivation

Boundary feedback stabilization of the wave equation asks whether a vibrating body at rest on part of its boundary can be brought to rest by a damping law on the rest of its boundary. With the undelayed velocity feedback ∂u/∂ν=−μ1ut\partial u/\partial\nu = -\mu_1 u_t∂u/∂ν=−μ1​ut​, the energy decays exponentially under geometric conditions on the domain; results of this kind go back to Chen (1979, 1981), Lagnese (1983, 1988), Lasiecka and Triggiani (1987), and Komornik and Zuazua (1990).

Real controllers act with a delay, and delays can destroy stability. Datko, Lagnese and Polis (1986) and Datko (1988) showed that an arbitrarily small delay in a boundary feedback that stabilizes the one-dimensional wave equation can make the closed loop unstable. For a feedback made of an undelayed part and a delayed part, μ1ut(t)+μ2ut(t−τ)\mu_1 u_t(t) + \mu_2 u_t(t-\tau)μ1​ut​(t)+μ2​ut​(t−τ), Xu, Yung and Li (2006) proved, by spectral analysis in one space dimension, that the system is stable when μ2<μ1\mu_2 < \mu_1μ2​<μ1​. Nicaise and Pignotti (2006) extended the stability result to bounded domains in any dimension nnn. This mission formalizes that extension: Theorem 1.1 of their paper.

Setting

Let Ω⊂Rn\Omega \subset \mathbb R^nΩ⊂Rn (n≥1n \ge 1n≥1) be a bounded open set whose boundary Γ\GammaΓ is 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 \ne \emptysetΓD​=∅. Let ν\nuν be the outer unit normal and dΓd\GammadΓ the surface measure on Γ\GammaΓ. Fix the undelayed gain μ1>0\mu_1 > 0μ1​>0, the delayed gain μ2>0\mu_2 > 0μ2​>0 and the delay τ>0\tau > 0τ>0. The problem is

utt−Δu=0in Ω×(0,∞),(1.1)u=0on ΓD×(0,∞),(1.2)∂u∂ν(x,t)=−μ1ut(x,t)−μ2ut(x,t−τ)on ΓN×(0,∞),(1.3)\begin{aligned} u_{tt} - \Delta u &= 0 && \text{in } \Omega \times (0,\infty), &(1.1)\\ u &= 0 && \text{on } \Gamma_D \times (0,\infty), &(1.2)\\ \tfrac{\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), &(1.3) \end{aligned}utt​−Δuu∂ν∂u​(x,t)​=0=0=−μ1​ut​(x,t)−μ2​ut​(x,t−τ)​​in Ω×(0,∞),on ΓD​×(0,∞),on ΓN​×(0,∞),​(1.1)(1.2)(1.3)​

with initial data u(⋅,0)=u0u(\cdot,0) = u_0u(⋅,0)=u0​ and ut(⋅,0)=u1u_t(\cdot,0) = u_1ut​(⋅,0)=u1​ in Ω\OmegaΩ, and a history ut=f0u_t = f_0ut​=f0​ on ΓN×(−τ,0)\Gamma_N \times (-\tau, 0)ΓN​×(−τ,0) (1.4)–(1.5).

The geometric hypothesis requires a function v∈C2(Ω‾)v \in C^2(\overline\Omega)v∈C2(Ω) and a constant α>0\alpha > 0α>0 with two properties:

⟨D2v(x)ξ,ξ⟩≥2α∣ξ∣2(x∈Ω‾, ξ∈Rn),(1.6)\langle D^2 v(x)\xi,\xi\rangle \ge 2\alpha|\xi|^2 \quad (x \in \overline\Omega,\ \xi \in \mathbb R^n), \tag{1.6}⟨D2v(x)ξ,ξ⟩≥2α∣ξ∣2(x∈Ω, ξ∈Rn),(1.6) ∇v(x)⋅ν(x)≤0(x∈ΓD).(1.7)\nabla v(x)\cdot\nu(x) \le 0 \quad (x \in \Gamma_D). \tag{1.7}∇v(x)⋅ν(x)≤0(x∈ΓD​).(1.7)

For example, v(x)=∣x∣2v(x) = |x|^2v(x)=∣x∣2 satisfies both on an annulus whose inner sphere is ΓD\Gamma_DΓD​.

Assume the gain condition

μ2<μ1,(1.8)\mu_2 < \mu_1, \tag{1.8}μ2​<μ1​,(1.8)

and fix ξ\xiξ with

τμ2<ξ<τ(2μ1−μ2).(1.10)\tau\mu_2 < \xi < \tau(2\mu_1 - \mu_2). \tag{1.10}τμ2​<ξ<τ(2μ1​−μ2​).(1.10)

The energy of a solution is the standard wave energy plus a term that stores the delayed velocity:

E(t)=12∫Ω{ut2(x,t)+∣∇u(x,t)∣2} dx+ξ2∫ΓN∫01ut2(x,t−τρ) dρ dΓ.(1.9)E(t) = \frac12\int_\Omega \{u_t^2(x,t) + |\nabla u(x,t)|^2\}\,dx + \frac{\xi}{2}\int_{\Gamma_N}\int_0^1 u_t^2(x,t-\tau\rho)\,d\rho\,d\Gamma. \tag{1.9}E(t)=21​∫Ω​{ut2​(x,t)+∣∇u(x,t)∣2}dx+2ξ​∫ΓN​​∫01​ut2​(x,t−τρ)dρdΓ.(1.9)

Formalization targets

Goal: Theorem 1.1 (exponential decay)

There are constants C1,C2>0C_1, C_2 > 0C1​,C2​>0, depending on Ω,ΓD,ΓN,v,α,μ1,μ2,τ,ξ\Omega, \Gamma_D, \Gamma_N, v, \alpha, \mu_1, \mu_2, \tau, \xiΩ,ΓD​,ΓN​,v,α,μ1​,μ2​,τ,ξ but not on the solution, such that every regular solution satisfies

E(t)≤C1E(0) e−C2t∀t≥0.(1.11)E(t) \le C_1 E(0)\, e^{-C_2 t} \qquad \forall t \ge 0. \tag{1.11}E(t)≤C1​E(0)e−C2​t∀t≥0.(1.11)

The constants are existential and are not fixed numerically. Any valid pair proves the goal.

Milestones, in the order the paper's proof uses them

  1. (3.6): the energy identity, which expresses E′(t)E'(t)E′(t) through boundary integrals over ΓN\Gamma_NΓN​ only.
  2. Proposition 3.1: EEE is nonincreasing, and
E′(t)≤−C∫ΓN{ut2(x,t)+ut2(x,t−τ)} dΓ,C=min⁡{μ1−μ22−ξ2τ, −μ22+ξ2τ}>0.E'(t) \le -C\int_{\Gamma_N}\{u_t^2(x,t) + u_t^2(x,t-\tau)\}\,d\Gamma, \qquad C = \min\Big\{\mu_1 - \frac{\mu_2}{2} - \frac{\xi}{2\tau},\ -\frac{\mu_2}{2} + \frac{\xi}{2\tau}\Big\} > 0.E′(t)≤−C∫ΓN​​{ut2​(x,t)+ut2​(x,t−τ)}dΓ,C=min{μ1​−2μ2​​−2τξ​, −2μ2​​+2τξ​}>0.
  1. (3.22): the integrated form E(T)−E(0)≤−C∫0T∫ΓN{ut2(t)+ut2(t−τ)} dΓ dtE(T) - E(0) \le -C\int_0^T\int_{\Gamma_N}\{u_t^2(t) + u_t^2(t-\tau)\}\,d\Gamma\,dtE(T)−E(0)≤−C∫0T​∫ΓN​​{ut2​(t)+ut2​(t−τ)}dΓdt.
  2. Proposition 3.2 (observability): there is T‾>0\overline T > 0T>0 such that for every T>T‾T > \overline TT>T some C0>0C_0 > 0C0​>0 satisfies
E(0)≤C0∫0T∫ΓN{ut2(x,t)+ut2(x,t−τ)} dΓ dt.(3.10)E(0) \le C_0\int_0^T\int_{\Gamma_N}\{u_t^2(x,t) + u_t^2(x,t-\tau)\}\,d\Gamma\,dt. \tag{3.10}E(0)≤C0​∫0T​∫ΓN​​{ut2​(x,t)+ut2​(x,t−τ)}dΓdt.(3.10)
  1. Contraction: there are T>0T > 0T>0 and 0≤C~<10 \le \tilde C < 10≤C~<1 with E(T)≤C~E(0)E(T) \le \tilde C E(0)E(T)≤C~E(0) for every regular solution.

Significance

The theorem shows that adding a delayed component to a stabilizing boundary feedback preserves exponential decay if the delayed gain is dominated by the undelayed gain. It holds in every dimension, under the same geometric condition that governs the undelayed problem. The companion Theorem 1.2 of the same paper shows that the condition μ2<μ1\mu_2 < \mu_1μ2​<μ1​ cannot be removed: when it fails, there are delays for which some solutions keep constant, positive standard energy. The Lyapunov functional (1.9) became a standard device for delayed feedbacks in later work on wave, plate and Timoshenko systems.

The result was proved in 2006. It has no machine-checked proof. This mission produces:

  • a formal statement of the theorem on classical solutions;
  • the energy identity and dissipation inequality with explicit constants;
  • the observability inequality as a separate target, which is the deep analytic input and is reusable by any stabilization argument on the same geometry.

Difficulty

The dissipation inequality (Proposition 3.1) is a calculation: Green's formula, a change of variables in the delay variable ρ\rhoρ, and Young's inequality. The difficulty is entirely in the observability inequality (3.10). The obvious multiplier argument, which multiplies the equation by ∇v⋅∇u\nabla v\cdot\nabla u∇v⋅∇u and integrates, leaves a lower-order term ∥u∥\|u\|∥u∥ that the boundary observation does not control.

The paper removes that term in two steps. The first is a Carleman-type estimate of Lasiecka, Triggiani and Yao (1999), which is where hypotheses (1.6)–(1.7) enter. The second is a compactness–uniqueness argument closed by Holmgren's uniqueness theorem. None of these tools exists in Mathlib, and neither does Green's formula on a curved domain. The final step from a one-period contraction to exponential decay uses time-translation invariance and monotonicity of EEE.

Formalization scope

  • Domain. A MixedDomain n bundles the following:

    • a bounded open set 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);
    • the split ΓD∪ΓN=∂Ω\Gamma_D \cup \Gamma_N = \partial\OmegaΓD​∪ΓN​=∂Ω with disjoint closures and ΓD≠∅\Gamma_D \ne \emptysetΓD​=∅;
    • a finite measure σ\sigmaσ carried by ∂Ω\partial\Omega∂Ω satisfying the Gauss–Green formula for every C1C^1C1 vector field.

    The outer normal is ν=∇ψ/∣∇ψ∣\nu = \nabla\psi/|\nabla\psi|ν=∇ψ/∣∇ψ∣. The Gauss–Green requirement determines σ\sigmaσ uniquely as the surface measure, so the normalization of dΓd\GammadΓ in (1.9) and (1.10) is the paper's.

  • Solutions are real-valued and classical: uuu is one C2C^2C2 function on Rn×R\mathbb R^n \times \mathbb RRn×R. It satisfies (1.1)–(1.3) for t>0t > 0t>0, and its values at t≤0t \le 0t≤0 are the initial data and the history. Time derivatives are one-variable derivatives in ttt, and ∂u/∂ν=∇u⋅ν\partial u/\partial\nu = \nabla u \cdot \nu∂u/∂ν=∇u⋅ν. This is a subclass of the paper's solutions, so the formal theorems are the paper's restricted to smooth, compatible data.

  • Added hypothesis. In Proposition 3.2, the contraction step and the goal, every connected component of Ω\OmegaΩ has a boundary point in ΓD\Gamma_DΓD​ (true whenever Ω\OmegaΩ is connected). The paper's uniqueness step ("−Δw=0-\Delta w = 0−Δw=0, w=0w = 0w=0 on ΓD\Gamma_DΓD​, ∂w/∂ν=0\partial w/\partial\nu = 0∂w/∂ν=0 on ΓN\Gamma_NΓN​, so w≡0w \equiv 0w≡0") needs every component of Ω\OmegaΩ to meet ΓD\Gamma_DΓD​.

  • Strengthened statements. The identity (3.6) and Propositions 3.1 and (3.22) omit hypotheses they do not use. Proposition 3.1 states the explicit constant CCC from the end of its proof.

  • Conventions. Condition (1.10) is strict. The energy is EEE of (1.9), with the delay term, and not the standard energy. Derivatives of EEE are asserted with HasDerivAt.

  • Excluded trivializations. Three things would make the statements empty or different, and none of them is allowed:

    • a free measure in place of the surface measure;
    • the standard energy in place of EEE;
    • replacing (1.11) by E(t)→0E(t) \to 0E(t)→0.

    The degenerate case ΓN=∅\Gamma_N = \emptysetΓN​=∅ is already excluded by (1.6), (1.7) and Gauss–Green together.

  • Infrastructure needed and welcome:

    • Gauss–Green and Green's first identity on MixedDomain;
    • differentiation under the integral over Ω\OmegaΩ and ΓN\Gamma_NΓN​;
    • a Carleman or multiplier observability estimate for the wave equation with mixed boundary conditions;
    • unique continuation (Holmgren) for the wave equation;
    • the elementary lemma turning a one-period contraction plus monotonicity into exponential decay.

    The last lemma and Gauss–Green on C2C^2C2 domains are reusable far beyond this mission.

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) (2006), 1561–1585. https://doi.org/10.1137/060648891
  • 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 (2006), 770–785. https://doi.org/10.1051/cocv:2006021
  • 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 (1986), 152–156. 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 (1988), 697–713. https://doi.org/10.1137/0326040
  • I. Lasiecka, R. Triggiani, P. F. Yao, Inverse/observability estimates for second-order hyperbolic equations with variable coefficients, J. Math. Anal. Appl. 235 (1999), 13–57. https://doi.org/10.1006/jmaa.1999.6348
  • V. Komornik, E. Zuazua, A direct method for the boundary stabilization of the wave equation, J. Math. Pures Appl. 69 (1990), 33–54.
  • J. Lagnese, Decay of solutions of wave equations in a bounded region with boundary dissipation, J. Differential Equations 50 (1983), 163–182. https://doi.org/10.1016/0022-0396(83)90073-6
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AnalysisPure Mathematics·Captain: mikedeng1

Tasty Bits of Several Complex Variables VI: The Hartogs PhenomenonTextbook

Motivation

In one complex variable every open set is the natural domain of some holomorphic function: 1/z1/z1/z on a punctured disc cannot be continued across the puncture. In two or more variables this fails in a striking way. Hartogs observed in 1906 that a function holomorphic on the complement of a compact set inside a domain always extends across the hole (Hartogs, Math. Ann. 62, 1906). This Hartogs phenomenon is the first place where several complex variables departs from the one-variable theory, and it forces the notions of domain of holomorphy and pseudoconvexity that organize the rest of the subject.

Timeline. Hartogs's original argument (1906) had gaps. A complete proof was given by Fueter in 1939 for n=2n = 2n=2, and independently by Bochner and Martinelli for general nnn in the early 1940s. The proof now standard, via the compactly supported ∂ˉ\bar\partial∂ˉ-problem, is due to Ehrenpreis (Ehrenpreis, Bull. Amer. Math. Soc. 67, 1961). This mission follows the presentation in §4.1–4.3 of Lebl's textbook (Lebl, version 4.4, 2026).

Setting

Write Cn\mathbb{C}^nCn for nnn-tuples z=(z1,…,zn)z = (z_1, \dots, z_n)z=(z1​,…,zn​) of complex numbers, zk=xk+iykz_k = x_k + i y_kzk​=xk​+iyk​. A domain is a nonempty connected open set. A function on an open set is holomorphic if it is complex differentiable there (for open sets this agrees with the textbook's definition by local boundedness and separate holomorphy).

The Wirtinger derivatives of a differentiable function fff are

∂f∂zˉk=12(∂f∂xk+i ∂f∂yk),k=1,…,n,\frac{\partial f}{\partial \bar z_k} = \frac12\left(\frac{\partial f}{\partial x_k} + i\,\frac{\partial f}{\partial y_k}\right), \qquad k = 1, \dots, n,∂zˉk​∂f​=21​(∂xk​∂f​+i∂yk​∂f​),k=1,…,n,

and in one variable ∂f/∂zˉ=12(∂xf+i ∂yf)\partial f/\partial\bar z = \tfrac12(\partial_x f + i\,\partial_y f)∂f/∂zˉ=21​(∂x​f+i∂y​f). A C1C^1C1 function is holomorphic exactly when all ∂f/∂zˉk\partial f/\partial\bar z_k∂f/∂zˉk​ vanish.

A (0,1)(0,1)(0,1)-form is an expression g=g1 dzˉ1+⋯+gn dzˉng = g_1\,d\bar z_1 + \cdots + g_n\,d\bar z_ng=g1​dzˉ1​+⋯+gn​dzˉn​ with coefficient functions gjg_jgj​. For a smooth ψ\psiψ, ∂ˉψ=∑k∂ψ∂zˉk dzˉk\bar\partial\psi = \sum_k \frac{\partial\psi}{\partial\bar z_k}\,d\bar z_k∂ˉψ=∑k​∂zˉk​∂ψ​dzˉk​, so the equation ∂ˉψ=g\bar\partial\psi = g∂ˉψ=g is the system ∂ψ/∂zˉk=gk\partial\psi/\partial\bar z_k = g_k∂ψ/∂zˉk​=gk​ for all kkk. Since mixed partial derivatives commute, a solution can exist only if the compatibility conditions ∂gk/∂zˉℓ=∂gℓ/∂zˉk\partial g_k/\partial\bar z_\ell = \partial g_\ell/\partial\bar z_k∂gk​/∂zˉℓ​=∂gℓ​/∂zˉk​ hold.

In one variable, the area element is written dζ∧dζˉ=(−2i) dAd\zeta\wedge d\bar\zeta = (-2i)\,dAdζ∧dζˉ​=(−2i)dA, where dA=dx dydA = dx\,dydA=dxdy is Lebesgue measure on C\mathbb{C}C.

Formalization targets

Goal: the Hartogs phenomenon (Theorem 4.3.1)

Let n≥2n \ge 2n≥2, U⊂CnU \subset \mathbb{C}^nU⊂Cn a domain, K⊂UK \subset UK⊂U compact with U∖KU \setminus KU∖K connected, and fff holomorphic on U∖KU \setminus KU∖K. Then

∃! F∈O(U) with F∣U∖K=f,\exists!\, F \in \mathcal{O}(U) \text{ with } F|_{U \setminus K} = f,∃!F∈O(U) with F∣U∖K​=f,

where uniqueness means any two such extensions agree on UUU.

Milestones

  1. Cauchy–Pompeiu formula (Theorem 4.1.1), on a disc UUU: for fff continuous on U‾\overline UU with bounded continuous partial derivatives in UUU and z∈Uz \in Uz∈U,
f(z)=12πi∫∂Uf(ζ)ζ−z dζ+12πi∫U∂f/∂ζˉ(ζ)ζ−z dζ∧dζˉ.f(z) = \frac{1}{2\pi i}\int_{\partial U}\frac{f(\zeta)}{\zeta - z}\,d\zeta + \frac{1}{2\pi i}\int_U \frac{\partial f/\partial\bar\zeta(\zeta)}{\zeta - z}\,d\zeta\wedge d\bar\zeta.f(z)=2πi1​∫∂U​ζ−zf(ζ)​dζ+2πi1​∫U​ζ−z∂f/∂ζˉ​(ζ)​dζ∧dζˉ​.
  1. One-variable ∂ˉ\bar\partial∂ˉ (Lemma 4.4.6), on a disc UUU: for ggg smooth near U‾\overline UU, ψ(z)=12πi∫Ug(ζ)ζ−z dζ∧dζˉ\psi(z) = \frac{1}{2\pi i}\int_U \frac{g(\zeta)}{\zeta - z}\,d\zeta\wedge d\bar\zetaψ(z)=2πi1​∫U​ζ−zg(ζ)​dζ∧dζˉ​ is smooth on UUU with ∂ψ/∂zˉ=g\partial\psi/\partial\bar z = g∂ψ/∂zˉ=g.
  2. Compactly supported ∂ˉ\bar\partial∂ˉ-problem (Theorem 4.2.1): for n≥2n \ge 2n≥2 and compactly supported smooth g1,…,gng_1, \dots, g_ng1​,…,gn​ satisfying the compatibility conditions, there is a unique compactly supported smooth ψ\psiψ with ∂ˉψ=g\bar\partial\psi = g∂ˉψ=g.
  3. Zero sets (Corollary 4.3.2): for n≥2n \ge 2n≥2 and fff holomorphic on a domain, a nonempty zero set f−1(0)f^{-1}(0)f−1(0) is never compact.

Significance

The result. The Hartogs phenomenon shows that isolated singularities, and more generally compact singular sets, do not exist for holomorphic functions of several variables. Direct consequences include Corollary 4.3.2, the fact that the complement of a bounded domain of holomorphy is connected, and the extension of CR functions from the boundary of a bounded domain (the Hartogs–Bochner and Severi theorems). It is the reason the domain of a holomorphic function in Cn\mathbb{C}^nCn carries geometric information, which leads to pseudoconvexity and the Levi problem. Theorem 4.2.1 is the simplest solvability statement for the ∂ˉ\bar\partial∂ˉ-equation, a model for the Dolbeault and Hörmander L2L^2L2 theories.

Formalizing it. All results here are classical and proved in the book; none is formalized. Mathlib has the one-variable Cauchy integral formula on discs, but it has no Cauchy–Pompeiu formula, no Cauchy transform with a ∂ˉ\bar\partial∂ˉ identity, and no ∂ˉ\bar\partial∂ˉ-problem in Cn\mathbb{C}^nCn. A complete development would provide a reusable one-variable ∂ˉ\bar\partial∂ˉ solution operator, differentiation under a singular integral, and the removable-compact-set theorem for holomorphic functions of several variables.

Difficulty

The first idea, extending fff one complex line at a time by one-variable Cauchy integrals, works only for special shapes of KKK (Hartogs figures): for a general compact KKK with connected complement the one-variable slices of U∖KU \setminus KU∖K can be complicated, and patching slice-wise extensions into one holomorphic function is where the historical proofs had gaps. The milestones carry their own analytic difficulties. The kernel 1/(ζ−z)1/(\zeta - z)1/(ζ−z) is singular, so the area integrals must first be shown to converge, and a zˉ\bar zzˉ-derivative cannot be moved naively under the integral (doing so would give 000, contradicting Lemma 4.4.6). In Theorem 4.2.1 the delicate point is compact support of the solution, which is where n≥2n \ge 2n≥2 enters: for n=1n = 1n=1 the equation is solvable but in general has no compactly supported solution.

Formalization scope

  • Cn\mathbb{C}^nCn is Fin n → ℂ; functions are total, and only their values on the sets named in the hypotheses matter. Holomorphic is DifferentiableOn ℂ on an open set. A domain is IsOpen U ∧ IsConnected U. "K⊂⊂UK \subset\subset UK⊂⊂U compact" is IsCompact K ∧ K ⊆ U. The hypothesis n≥2n \ge 2n≥2 is 2 ≤ n and is essential.
  • wirtingerBar k f is 12(∂xkf+i ∂ykf)\tfrac12(\partial_{x_k}f + i\,\partial_{y_k}f)21​(∂xk​​f+i∂yk​​f) built from real one-variable derivs; dbar f is its one-variable analogue. Smooth means real C∞C^\inftyC∞ (ContDiff ℝ ∞), not analytic; compact support is HasCompactSupport.
  • In Theorem 4.1.1 and Lemma 4.4.6 the book allows any bounded open set with piecewise-C1C^1C1 boundary; the formalization restricts to open discs, since Mathlib has no boundary integral over such sets. The boundary integral is circleIntegral, and ∫U⋯dζ∧dζˉ\int_U \cdots d\zeta\wedge d\bar\zeta∫U​⋯dζ∧dζˉ​ is (−2i)(-2i)(−2i) times the Lebesgue (Bochner) integral over the disc. Integrability of the singular integrand is part of the conclusion, so a vanishing Bochner integral cannot make a statement hold vacuously.
  • Uniqueness in the goal is agreement on UUU of any two holomorphic extensions (values off UUU are unconstrained); in Theorem 4.2.1 it is ∃! among compactly supported smooth functions.
  • Trivializations ruled out: the goal is not stated for n=1n = 1n=1, it does not assume fff already holomorphic on UUU, and it does not replace "extends" by the existence of some function on UUU without the agreement F=fF = fF=f on U∖KU \setminus KU∖K.
  • Omitted: Corollary 4.3.3 (Severi), which needs real-analytic hypersurfaces and CR functions.
  • Needed infrastructure: Green's theorem on a disc or an equivalent polar-coordinate argument, local integrability of 1/∣ζ∣1/|\zeta|1/∣ζ∣ in the plane, differentiation under the integral sign, smooth cutoff functions, and the identity theorem in Cn\mathbb{C}^nCn. Reusable contributions in any of these are welcome.

Selected references

  • J. Lebl, Tasty Bits of Several Complex Variables, version 4.4, 2026, §4.1–4.3, pp. 130–137. https://www.jirka.org/scv/scv.pdf
  • F. Hartogs, Zur Theorie der analytischen Funktionen mehrerer unabhängiger Veränderlichen, insbesondere über die Darstellung derselben durch Reihen, welche nach Potenzen einer Veränderlichen fortschreiten, Math. Ann. 62 (1906), 1–88.
  • L. Ehrenpreis, A new proof and an extension of Hartog's theorem, Bull. Amer. Math. Soc. 67 (1961), 507–509.
  • L. Hörmander, An Introduction to Complex Analysis in Several Variables, 3rd ed., North-Holland, 1990, Theorem 2.3.2.
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Notes on Partial Differential Equations XII: Friedrichs Symmetric Systems — Weak Equals StrongTextbook

Motivation

Many systems of first-order partial differential equations arising in physics — linear acoustics, Maxwell's equations, linearized gas dynamics, the Tricomi equation of transonic flow — can be written as symmetric systems Ai∂iu+Cu=fA^i\partial_i u + Cu = fAi∂i​u+Cu=f with symmetric coefficient matrices AiA^iAi. K. O. Friedrichs showed in 1958 (Friedrichs 1958) that a single energy argument gives existence and uniqueness for boundary value problems of this form under positivity conditions on the equation and the boundary condition, regardless of whether the system is elliptic, hyperbolic or of mixed type. The theory is the subject of Chapter 8 of J. K. Hunter's Notes on Partial Differential Equations (UC Davis, revised 6/18/2014), which this mission follows.

The core analytic tool of the theory is older. In 1944 Friedrichs introduced mollifiers precisely to prove that weak and strong extensions of differential operators coincide (Friedrichs 1944); the key estimate is a bound on the commutator of a mollifier with a first-order operator with Lipschitz coefficients. Lax and Phillips (1960) developed the boundary version for dissipative symmetric operators.

Setting

Write points of Rn\mathbb{R}^nRn as x=(x1,…,xn)x = (x_1, \dots, x_n)x=(x1​,…,xn​) and give Rm\mathbb{R}^mRm its Euclidean norm ∣w∣|w|∣w∣. Let A1,…,An,C:Rn→Rm×mA^1, \dots, A^n, C : \mathbb{R}^n \to \mathbb{R}^{m\times m}A1,…,An,C:Rn→Rm×m be matrix-valued coefficients. The first-order operator and its formal adjoint are (summation over iii)

Lu=Ai∂iu+Cu,L∗v=−Ai∂iv+CTv−(∂iAi)v.Lu = A^i\partial_i u + Cu, \qquad L^*v = -A^i\partial_i v + C^Tv - (\partial_i A^i)v .Lu=Ai∂i​u+Cu,L∗v=−Ai∂i​v+CTv−(∂i​Ai)v.

A mollifier profile is a C∞C^\inftyC∞, compactly supported, non-negative, radially symmetric η:Rn→R\eta : \mathbb{R}^n \to \mathbb{R}η:Rn→R with ∫η=1\int \eta = 1∫η=1. For ε>0\varepsilon > 0ε>0 set ηε(x)=ε−nη(x/ε)\eta_\varepsilon(x) = \varepsilon^{-n}\eta(x/\varepsilon)ηε​(x)=ε−nη(x/ε) and define the smoothing operator Jεu=ηε∗uJ_\varepsilon u = \eta_\varepsilon * uJε​u=ηε​∗u. The commutator [Jε,L]u=Jε(Lu)−L(Jεu)[J_\varepsilon, L]u = J_\varepsilon(Lu) - L(J_\varepsilon u)[Jε​,L]u=Jε​(Lu)−L(Jε​u) is defined for u∈Cc1(Rn;Rm)u \in C^1_c(\mathbb{R}^n;\mathbb{R}^m)u∈Cc1​(Rn;Rm).

For the boundary value problem, Ω⊆Rn\Omega \subseteq \mathbb{R}^nΩ⊆Rn is a bounded open set with C2C^2C2-boundary, ν\nuν its outward unit normal, and the problem is

Ai∂iu+Cu=f  in Ω,B−u=0  on ∂Ω,A^i\partial_iu + Cu = f \ \text{ in } \Omega, \qquad B_-u = 0 \ \text{ on } \partial\Omega,Ai∂i​u+Cu=f  in Ω,B−​u=0  on ∂Ω,

with boundary matrix B=νiAiB = \nu_iA^iB=νi​Ai. The system is positive symmetric with constant c>0c > 0c>0 if the AiA^iAi are symmetric and C+CT−∂iAi≥2cIC + C^T - \partial_iA^i \ge 2cIC+CT−∂i​Ai≥2cI in Ω\OmegaΩ. The boundary condition is maximally positive if BBB is nonsingular on ∂Ω\partial\Omega∂Ω and there is a matrix function MMM on ∂Ω\partial\Omega∂Ω with B±=12(B±M)B_\pm = \tfrac12(B \pm M)B±​=21​(B±M), M+MT≥0M + M^T \ge 0M+MT≥0 and Rm=ker⁡B+⊕ker⁡B−\mathbb{R}^m = \ker B_+ \oplus \ker B_-Rm=kerB+​⊕kerB−​. A weak solution with data f∈L2(Ω;Rm)f \in L^2(\Omega;\mathbb{R}^m)f∈L2(Ω;Rm) is u∈L2(Ω;Rm)u \in L^2(\Omega;\mathbb{R}^m)u∈L2(Ω;Rm) with ∫ΩuTL∗v=∫ΩfTv\int_\Omega u^TL^*v = \int_\Omega f^Tv∫Ω​uTL∗v=∫Ω​fTv for every v∈D∗={v∈C1(Ω‾):B+Tv=0 on ∂Ω}v \in D^* = \{v \in C^1(\overline\Omega) : B_+^Tv = 0 \text{ on } \partial\Omega\}v∈D∗={v∈C1(Ω):B+T​v=0 on ∂Ω}.

Formalization targets

Goal: Friedrichs' commutator lemma (Lemma 8.11)

Let Ai∈Cc1(Rn;Rm×m)A^i \in C^1_c(\mathbb{R}^n;\mathbb{R}^{m\times m})Ai∈Cc1​(Rn;Rm×m) and C∈Cc(Rn;Rm×m)C \in C_c(\mathbb{R}^n;\mathbb{R}^{m\times m})C∈Cc​(Rn;Rm×m). For each ε>0\varepsilon > 0ε>0 the commutator [Jε,L]:Cc1→L2[J_\varepsilon, L] : C^1_c \to L^2[Jε​,L]:Cc1​→L2 extends to a bounded operator [Jε,L]‾\overline{[J_\varepsilon, L]}[Jε​,L]​ on L2(Rn;Rm)L^2(\mathbb{R}^n;\mathbb{R}^m)L2(Rn;Rm), and

sup⁡ε>0∥[Jε,L]‾∥L2→L2<∞,[Jε,L]‾ u→0  in L2 as ε→0+  for every u∈L2.\sup_{\varepsilon > 0}\big\|\overline{[J_\varepsilon, L]}\big\|_{L^2\to L^2} < \infty, \qquad \overline{[J_\varepsilon, L]}\,u \to 0 \ \text{ in } L^2 \text{ as } \varepsilon \to 0^+ \ \text{ for every } u \in L^2 .ε>0sup​​[Jε​,L]​​L2→L2​<∞,[Jε​,L]​u→0  in L2 as ε→0+  for every u∈L2.

The goal asserts only the shape: a uniform bound exists, with no value fixed.

Milestones: energy estimates and existence (Theorems 8.6, 8.9, Corollary 8.7)

Under the smoothness, positivity and maximal positivity conditions above, with ∥⋅∥\|\cdot\|∥⋅∥ the L2(Ω)L^2(\Omega)L2(Ω) norm,

c∥u∥≤∥Lu∥  (u∈C1(Ω‾), B−u=0),c∥v∥≤∥L∗v∥  (v∈C1(Ω‾), B+Tv=0);c\|u\| \le \|Lu\| \ \ (u \in C^1(\overline\Omega),\ B_-u = 0), \qquad c\|v\| \le \|L^*v\| \ \ (v \in C^1(\overline\Omega),\ B_+^Tv = 0);c∥u∥≤∥Lu∥  (u∈C1(Ω), B−​u=0),c∥v∥≤∥L∗v∥  (v∈C1(Ω), B+T​v=0);

smooth solutions are unique; and for every f∈L2(Ω)f \in L^2(\Omega)f∈L2(Ω) a weak solution exists.

Significance

The commutator lemma is what turns weak solutions into strong ones: mollifying a weak solution produces smooth functions that solve the equation up to an error [Jε,L]u[J_\varepsilon, L]u[Jε​,L]u, and the lemma says this error vanishes in the limit. Friedrichs' "weak equals strong" theorem (Theorem 8.12 of the notes), the uniqueness of weak solutions (Corollary 8.13), and much of the L2L^2L2 theory of hyperbolic systems and pseudo-differential commutator estimates rest on it. The energy estimates of Theorem 8.6 and the existence theorem 8.9 are the two halves of the Friedrichs theory that do not need mollification: an a priori bound for smooth functions satisfying the boundary condition, and existence by duality.

All of these results are classical and proved. As far as a search of the platform and of Mathlib shows, none is formalized: Mathlib has convolution, ContDiffBump mollifiers and LpL^pLp spaces, but no commutator estimates, no divergence theorem on C2C^2C2 domains, and no Friedrichs systems. The mission would produce the first machine-checked commutator estimate for mollifiers and first-order operators with Lipschitz coefficients, and the first formal treatment of positive symmetric boundary value problems.

Difficulty

The obvious argument for the goal — bound Jε(Ai∂iu)J_\varepsilon(A^i\partial_iu)Jε​(Ai∂i​u) and Ai∂i(Jεu)A^i\partial_i(J_\varepsilon u)Ai∂i​(Jε​u) separately — fails: each term involves ∂iu\partial_i u∂i​u, which is not controlled by ∥u∥L2\|u\|_{L^2}∥u∥L2​, and each is of size ε−1∥u∥\varepsilon^{-1}\|u\|ε−1∥u∥ after moving the derivative onto ηε\eta_\varepsilonηε​. Only the difference is bounded, and only because the coefficient difference Ai(y)−Ai(x)A^i(y) - A^i(x)Ai(y)−Ai(x) is of size ∣x−y∣≲ε|x - y| \lesssim \varepsilon∣x−y∣≲ε on the support of ηε(x−y)\eta_\varepsilon(x - y)ηε​(x−y). The cancellation between the two terms is the whole content of the uniform bound. Convergence to zero on smooth compactly supported uuu is easy, but it does not by itself give convergence on all of L2L^2L2.

For the milestones, the central difficulty is Green's theorem: the energy identity requires the divergence theorem on a bounded C2C^2C2 domain for C1C^1C1 vector fields, with the outward normal and surface measure, none of which Mathlib provides for general domains.

Formalization scope

  • Rn\mathbb{R}^nRn and Rm\mathbb{R}^mRm are EuclideanSpace ℝ (Fin n) and EuclideanSpace ℝ (Fin m), so ∣⋅∣|\cdot|∣⋅∣ is Euclidean and L2(Rn;Rm)L^2(\mathbb{R}^n;\mathbb{R}^m)L2(Rn;Rm) is Lp (EuclideanSpace ℝ (Fin m)) 2 volume. Coordinates are 0-based: A i is Ai+1A^{i+1}Ai+1.
  • The goal takes a family T : ℝ → (L² →L[ℝ] L²). "Extends" means: for ε>0\varepsilon > 0ε>0 and every u∈Cc1u \in C^1_cu∈Cc1​, T ε applied to the class of uuu agrees a.e. with the pointwise commutator. Because Cc1C^1_cCc1​ is dense in L2L^2L2, this pins down each T ε; a bound stated on Cc1C^1_cCc1​ only would be weaker than the lemma and is not what is asked.
  • The lemma is stated for every mollifier profile, which includes the bump (1.5) of the notes. C∞C^\inftyC∞ means ContDiff ℝ ∞ (smooth, not analytic).
  • A bounded open set with C2C^2C2-boundary is one with a global C2C^2C2 defining function ρ\rhoρ (Ω={ρ<0}\Omega = \{\rho < 0\}Ω={ρ<0}, ∇ρ≠0\nabla\rho \ne 0∇ρ=0 on {ρ=0}\{\rho = 0\}{ρ=0}); for bounded sets this is equivalent to the chart definition of the notes. The outward normal is ∇ρ/∣∇ρ∣\nabla\rho/|\nabla\rho|∇ρ/∣∇ρ∣, which does not depend on ρ\rhoρ. It is not a free function argument.
  • C1(Ω‾)C^1(\overline\Omega)C1(Ω) is modelled by C1C^1C1 functions on Rn\mathbb{R}^nRn. For C2C^2C2 domains their restrictions are exactly C1(Ω‾)C^1(\overline\Omega)C1(Ω).
  • The printed Definition 8.5 sets B±=B±MB_\pm = B \pm MB±​=B±M and also B=B++B−B = B_+ + B_-B=B+​+B−​, which would force B=0B = 0B=0. The formalization uses B±=12(B±M)B_\pm = \tfrac12(B \pm M)B±​=21​(B±M), Friedrichs' normalisation. This gives the same kernels ker⁡B±\ker B_\pmkerB±​, so the same boundary conditions.
  • L2L^2L2 norms are eLpNorm · 2 in [0,∞][0,\infty][0,∞], so no integrability condition is hidden in the estimates.

Needed infrastructure: Young's convolution inequality on Rn\mathbb{R}^nRn, density of Cc1C^1_cCc1​ in L2L^2L2, differentiation under the convolution integral, and, for the milestones, the divergence theorem on bounded C2C^2C2 domains together with the Riesz representation theorem. The divergence theorem on C2C^2C2 domains, and the commutator estimate itself, are reusable well beyond this mission. Contributions of any of these are welcome.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, Chapter 8. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • K. O. Friedrichs, The identity of weak and strong extensions of differential operators, Trans. Amer. Math. Soc. 55 (1944), 132–151. https://doi.org/10.1090/S0002-9947-1944-0009701-0
  • K. O. Friedrichs, Symmetric positive linear differential equations, Comm. Pure Appl. Math. 11 (1958), 333–418. https://doi.org/10.1002/cpa.3160110306
  • P. D. Lax and R. S. Phillips, Local boundary conditions for dissipative symmetric linear differential operators, Comm. Pure Appl. Math. 13 (1960), 427–455. https://doi.org/10.1002/cpa.3160130307
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AnalysisFunctional Analysis·Captain: mikedeng1

Notes on Partial Differential Equations XI: Existence and Uniqueness of Weak Solutions of Hyperbolic PDEsTextbook

Motivation

Hyperbolic partial differential equations model waves: acoustic, elastic, electromagnetic and gravitational. Their qualitative behaviour differs sharply from that of parabolic equations. They have finite speed of propagation, they are reversible in time, and they do not smooth their data: a singularity in the initial state is transported, not damped. The analytical consequence is that energy estimates for hyperbolic equations are weaker than for parabolic ones, and the existence theory has to be run in spaces that carry exactly one derivative's worth of information.

This mission formalizes the energy-space well-posedness theory for linear second-order hyperbolic equations with time-dependent coefficients, following Chapter 7 of J. K. Hunter's lecture notes Notes on Partial Differential Equations (UC Davis, revised 6/18/2014). The same theory appears in L. C. Evans, Partial Differential Equations, §7.2, and goes back to the Galerkin and energy methods of J.-L. Lions and E. Magenes.

Setting

Let Ω⊂Rn\Omega \subset \mathbb{R}^nΩ⊂Rn be a bounded open set and T>0T > 0T>0. A test function is a smooth function with compact support in Ω\OmegaΩ; the Sobolev space H01(Ω)H^1_0(\Omega)H01​(Ω) is the closure of the test functions in the norm ∥u∥H01=(∫Ω(u2+∣Du∣2) dx)1/2\|u\|_{H^1_0} = \big(\int_\Omega (u^2 + |Du|^2)\,dx\big)^{1/2}∥u∥H01​​=(∫Ω​(u2+∣Du∣2)dx)1/2, where DuDuDu is the weak gradient. L2(Ω)L^2(\Omega)L2(Ω) carries the inner product (u,v)L2=∫Ωuv dx(u,v)_{L^2} = \int_\Omega uv\,dx(u,v)L2​=∫Ω​uvdx, and H−1(Ω)=H01(Ω)′H^{-1}(\Omega) = H^1_0(\Omega)'H−1(Ω)=H01​(Ω)′ is the dual space with pairing ⟨f,v⟩\langle f, v \rangle⟨f,v⟩. There are embeddings H01(Ω)↪L2(Ω)↪H−1(Ω)H^1_0(\Omega) \hookrightarrow L^2(\Omega) \hookrightarrow H^{-1}(\Omega)H01​(Ω)↪L2(Ω)↪H−1(Ω).

The operator is

Lu=−∑i,j=1n∂i(aij(x,t) ∂ju)+c(x,t) u,Lu = -\sum_{i,j=1}^n \partial_i\big(a^{ij}(x,t)\,\partial_j u\big) + c(x,t)\,u,Lu=−i,j=1∑n​∂i​(aij(x,t)∂j​u)+c(x,t)u,

with bilinear form a(u,v;t)=∑i,j∫Ωaij∂iu ∂jv dx+∫Ωc uv dxa(u,v;t) = \sum_{i,j}\int_\Omega a^{ij}\partial_i u\,\partial_j v\,dx + \int_\Omega c\,uv\,dxa(u,v;t)=∑i,j​∫Ω​aij∂i​u∂j​vdx+∫Ω​cuvdx on H01(Ω)H^1_0(\Omega)H01​(Ω), and ata_tat​ is the same form built from the time derivatives atija^{ij}_tatij​, ctc_tct​. Assumption 7.1 requires aij,c,atij,ct∈L∞(Ω×(0,T))a^{ij}, c, a^{ij}_t, c_t \in L^\infty(\Omega\times(0,T))aij,c,atij​,ct​∈L∞(Ω×(0,T)), aij=ajia^{ij} = a^{ji}aij=aji, and uniform ellipticity: ∑i,jaijξiξj≥θ∣ξ∣2\sum_{i,j} a^{ij}\xi_i\xi_j \ge \theta|\xi|^2∑i,j​aijξi​ξj​≥θ∣ξ∣2 for some θ>0\theta > 0θ>0.

A vector-valued function u:(0,T)→Xu : (0,T) \to Xu:(0,T)→X has weak time derivative www if ∫0Tφ′(t)u(t) dt=−∫0Tφ(t)w(t) dt\int_0^T \varphi'(t)u(t)\,dt = -\int_0^T \varphi(t)w(t)\,dt∫0T​φ′(t)u(t)dt=−∫0T​φ(t)w(t)dt for all test functions φ\varphiφ on (0,T)(0,T)(0,T), the integrals being Bochner integrals. The problem is

utt+Lu=f in Ω×(0,T),u=0 on ∂Ω×(0,T),u=g, ut=h at t=0.(7.5)u_{tt} + Lu = f \text{ in } \Omega\times(0,T), \qquad u = 0 \text{ on } \partial\Omega\times(0,T), \qquad u = g,\ u_t = h \text{ at } t = 0. \qquad (7.5)utt​+Lu=f in Ω×(0,T),u=0 on ∂Ω×(0,T),u=g, ut​=h at t=0.(7.5)

A weak solution (Definition 7.2) is a function u:[0,T]→H01(Ω)u : [0,T] \to H^1_0(\Omega)u:[0,T]→H01​(Ω) with weak derivatives utu_tut​, uttu_{tt}utt​ such that u∈C([0,T];H01)u \in C([0,T];H^1_0)u∈C([0,T];H01​), ut∈C([0,T];L2)u_t \in C([0,T];L^2)ut​∈C([0,T];L2), utt∈L2(0,T;H−1)u_{tt} \in L^2(0,T;H^{-1})utt​∈L2(0,T;H−1), and for every v∈H01(Ω)v \in H^1_0(\Omega)v∈H01​(Ω)

⟨utt(t),v⟩+a(u(t),v;t)=(f(t),v)L2for a.e. t,\langle u_{tt}(t), v\rangle + a(u(t), v; t) = (f(t), v)_{L^2} \quad \text{for a.e. } t,⟨utt​(t),v⟩+a(u(t),v;t)=(f(t),v)L2​for a.e. t,

with u(0)=gu(0) = gu(0)=g and ut(0)=hu_t(0) = hut​(0)=h.

Formalization targets

Goal: Theorem 7.3

Under Assumption 7.1 there is a constant CCC, depending only on Ω\OmegaΩ, TTT and the coefficients, such that for every f∈L2(0,T;L2(Ω))f \in L^2(0,T;L^2(\Omega))f∈L2(0,T;L2(Ω)), g∈H01(Ω)g \in H^1_0(\Omega)g∈H01​(Ω), h∈L2(Ω)h \in L^2(\Omega)h∈L2(Ω) there is a unique weak solution, and

∥u∥L∞(0,T;H01)+∥ut∥L∞(0,T;L2)+∥utt∥L2(0,T;H−1)≤C(∥f∥L2(0,T;L2)+∥g∥H01+∥h∥L2).\|u\|_{L^\infty(0,T;H^1_0)} + \|u_t\|_{L^\infty(0,T;L^2)} + \|u_{tt}\|_{L^2(0,T;H^{-1})} \le C\big(\|f\|_{L^2(0,T;L^2)} + \|g\|_{H^1_0} + \|h\|_{L^2}\big).∥u∥L∞(0,T;H01​)​+∥ut​∥L∞(0,T;L2)​+∥utt​∥L2(0,T;H−1)​≤C(∥f∥L2(0,T;L2)​+∥g∥H01​​+∥h∥L2​).

Milestones

  • Proposition 7.5. For every NNN, the Galerkin problem projected onto the span ENE_NEN​ of the first NNN Dirichlet eigenfunctions has a unique approximate solution uN∈C1([0,T];EN)u_N \in C^1([0,T];E_N)uN​∈C1([0,T];EN​) with uNtt∈L2(0,T;EN)u_{Ntt} \in L^2(0,T;E_N)uNtt​∈L2(0,T;EN​).
  • Proposition 7.6. The approximate solutions satisfy the energy estimate of Theorem 7.3 with a constant independent of NNN.
  • Lemma 7.8. If V↪H\mathcal{V} \hookrightarrow \mathcal{H}V↪H is a dense continuous embedding of Hilbert spaces, u∈L∞(0,T;V)u \in L^\infty(0,T;\mathcal{V})u∈L∞(0,T;V) and ut∈L2(0,T;H)u_t \in L^2(0,T;\mathcal{H})ut​∈L2(0,T;H), then uuu is weakly continuous into V\mathcal{V}V.
  • Lemma 7.10. If u∈L2(0,T;H01)u \in L^2(0,T;H^1_0)u∈L2(0,T;H01​), ut∈L2(0,T;L2)u_t \in L^2(0,T;L^2)ut​∈L2(0,T;L2), utt∈L2(0,T;H−1)u_{tt} \in L^2(0,T;H^{-1})utt​∈L2(0,T;H−1) and utt+Lu∈L2(0,T;L2)u_{tt} + Lu \in L^2(0,T;L^2)utt​+Lu∈L2(0,T;L2), then
12ddt(∥ut∥L22+a(u,u;t))=(utt+Lu,ut)L2+12at(u,u;t),\tfrac12 \tfrac{d}{dt}\big(\|u_t\|^2_{L^2} + a(u,u;t)\big) = (u_{tt}+Lu, u_t)_{L^2} + \tfrac12 a_t(u,u;t),21​dtd​(∥ut​∥L22​+a(u,u;t))=(utt​+Lu,ut​)L2​+21​at​(u,u;t),

and the energy is absolutely continuous.

  • Proposition 7.12. Weak solutions in the sense of Definition 7.2 are unique.

Significance

Theorem 7.3 is the basic well-posedness result for linear wave equations in inhomogeneous, time-dependent media in the natural energy space. It is the starting point for the regularity theory of such solutions, for finite-speed-of-propagation arguments in a weak setting, and for fixed-point constructions for semilinear wave equations, which linearize around a known solution and need exactly this estimate with a constant depending only on the coefficients. Lemma 7.8 and Lemma 7.10 are general tools that recur in evolution equations: the first converts uniform-in-time bounds into weak continuity, the second justifies an energy identity for solutions too rough to differentiate directly.

The results are classical and fully proved in the literature, and to our knowledge no machine-checked version exists. Formalizing them requires vector-valued Sobolev spaces in time, Bochner-integral weak derivatives and duality arguments. These are largely absent from Mathlib and would be reused by any formal treatment of evolution equations, parabolic ones included.

Difficulty

The obvious approach, testing the equation with utu_tut​ to obtain energy conservation, is not available for weak solutions: ut(t)u_t(t)ut​(t) lies only in L2(Ω)L^2(\Omega)L2(Ω), not in H01(Ω)H^1_0(\Omega)H01​(Ω), so the pairing a(u,ut;t)a(u, u_t; t)a(u,ut​;t) is undefined. This affects both halves of the theorem. For existence, the energy estimate holds only for the finite-dimensional approximations, and the limit is obtained in weak-star topologies of L∞L^\inftyL∞ in time, which give neither continuity in time nor the initial conditions directly. For uniqueness, a different test function is needed. The continuity requirements of Definition 7.2 are an essential part of the statement, not a technicality, and establishing them for the constructed solution is a large part of the work.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n) with Lebesgue measure; coordinates are 0-based. H01(Ω)H^1_0(\Omega)H01​(Ω) is modelled by jets (u,Du)(u, Du)(u,Du): the closure of {(φ,∇φ)}\{(\varphi, \nabla\varphi)\}{(φ,∇φ)} in L2(Ω;R×Rn)L^2(\Omega;\mathbb{R}\times\mathbb{R}^n)L2(Ω;R×Rn), with norm exactly (∫Ωu2+∣Du∣2)1/2\big(\int_\Omega u^2 + |Du|^2\big)^{1/2}(∫Ω​u2+∣Du∣2)1/2. H−1(Ω)H^{-1}(\Omega)H−1(Ω) is StrongDual ℝ (H10 n Ω), and f∈L2f \in L^2f∈L2 acts by v↦(f,v)L2v \mapsto (f, v)_{L^2}v↦(f,v)L2​.
  • Time-dependent objects are functions on R\mathbb{R}R. Only values on (0,T)(0,T)(0,T) (integrability, weak derivatives) or [0,T][0,T][0,T] (continuity, initial values) matter. utu_tut​ is the weak derivative of uuu regarded in L2L^2L2, and uttu_{tt}utt​ that of utu_tut​ regarded in H−1H^{-1}H−1. Local integrability is built into the weak derivative, so no Bochner integral takes the junk value 000.
  • Coefficients are functions of (x,t)(x,t)(x,t), bundled with their time derivatives. Assumption 7.1 requires those to be weak time derivatives on Ω×(0,T)\Omega\times(0,T)Ω×(0,T). Symmetry and ellipticity hold almost everywhere there, the meaning for L∞L^\inftyL∞ coefficients. The consequences (7.7) of Assumption 7.1 are not assumed.
  • Norms in the estimates are ℝ≥0∞-valued (eLpNorm, ‖·‖ₑ), and the constants are finite (ℝ≥0). Each constant is quantified before the data f,g,hf, g, hf,g,h; in Proposition 7.6 it also precedes the eigenbasis and NNN.
  • The Galerkin basis is any L2L^2L2-orthonormal basis of weak Dirichlet eigenfunctions, indexed from 000.
  • Two misprints are corrected. The first integral of (7.6) has ∂jv\partial_j v∂j​v, not ∂ju\partial_j u∂j​u. The energy (7.16) is ∥ut∥L22+a(u,u;t)\|u_t\|^2_{L^2} + a(u,u;t)∥ut​∥L22​+a(u,u;t), with the square that (7.19) uses.
  • Lemma 7.10 is stated in integrated form. The right-hand side of (7.19) is integrable, and the energy equals a constant plus its integral for a.e. ttt. This is the identity together with absolute continuity.
  • A trivializing formalization is excluded. Definition 7.2 keeps all three regularity classes and both initial conditions, and uniqueness and the estimate are asserted for the object of that definition. A definition without the continuity classes would admit non-solutions.

A complete development needs Bochner-valued Sobolev spaces on an interval, Banach–Alaoglu in L∞(0,T;X)=L1(0,T;X′)′L^\infty(0,T;X) = L^1(0,T;X')'L∞(0,T;X)=L1(0,T;X′)′, linear ODE systems with L∞L^\inftyL∞ coefficients, Gronwall's inequality, and the spectral theory of the Dirichlet Laplacian. The time-dependent function-space layer is reusable for parabolic and Schrödinger-type equations. Contributions of general lemmas on vector-valued weak derivatives are welcome.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, Chapter 7. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • L. C. Evans, Partial Differential Equations, 2nd ed., Graduate Studies in Mathematics 19, AMS, 2010, §7.2. https://doi.org/10.1090/gsm/019
  • J.-L. Lions and E. Magenes, Non-Homogeneous Boundary Value Problems and Applications, Vol. I, Springer, 1972, Chapter 3. https://doi.org/10.1007/978-3-642-65161-8
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AnalysisHarmonic Analysis·Captain: mikedeng1

Notes on Partial Differential Equations IX: Local Existence for a Semilinear Heat Equation and the Nonlinear Schrödinger EquationTextbook

Motivation

Reaction–diffusion equations ut=Δu+f(u)u_t = \Delta u + f(u)ut​=Δu+f(u) are the standard model for the interplay of diffusion with local growth or decay: chemical kinetics, population dynamics, and the bifurcation of equilibria of partial differential equations. The special case

ut=Δu+λu−γumu_t = \Delta u + \lambda u - \gamma u^mut​=Δu+λu−γum

(the Chafee–Infante equation on bounded domains, Chafee and Infante 1974) is the model equation for loss of stability: u=0u = 0u=0 is linearly stable for λ<0\lambda < 0λ<0 and unstable for λ>0\lambda > 0λ>0, and for m=3m = 3m=3, γ>0\gamma > 0γ>0 the reaction term produces a supercritical pitchfork bifurcation. Before any of that dynamics can be studied, one needs solutions to exist. §5.5 of J. K. Hunter's Notes on Partial Differential Equations (UC Davis, revised 6/18/2014) proves local existence by rewriting the equation as an integral equation and applying the contraction mapping theorem. This argument, the "mild solution" method of Kato and Segal, is the template for local well-posedness of semilinear parabolic and dispersive equations (Pazy 1983, Henry 1981).

Setting

Write Rn\mathbb{R}^nRn for Euclidean space with Lebesgue measure. For f∈L2(Rn)f \in L^2(\mathbb{R}^n)f∈L2(Rn) the Fourier transform is f^(k)=(2π)−n∫f(x)e−ik⋅x dx\hat f(k) = (2\pi)^{-n}\int f(x)e^{-ik\cdot x}\,dxf^​(k)=(2π)−n∫f(x)e−ik⋅xdx, defined by this formula on Schwartz functions and extended to L2L^2L2 by Plancherel's theorem. For s≥0s \ge 0s≥0, the Sobolev space Hs(Rn)H^s(\mathbb{R}^n)Hs(Rn) consists of the f∈L2f \in L^2f∈L2 with finite norm

∥f∥Hs=((2π)n∫Rn(1+∣k∣2)s ∣f^(k)∣2 dk)1/2.\|f\|_{H^s} = \Big((2\pi)^n \int_{\mathbb{R}^n} (1+|k|^2)^{s}\,|\hat f(k)|^2\,dk\Big)^{1/2}.∥f∥Hs​=((2π)n∫Rn​(1+∣k∣2)s∣f^​(k)∣2dk)1/2.

The heat semigroup e−tAe^{-tA}e−tA, A=−ΔA = -\DeltaA=−Δ, is the Fourier multiplier e−tAh^(k)=e−t∣k∣2h^(k)\widehat{e^{-tA}h}(k) = e^{-t|k|^2}\hat h(k)e−tAh(k)=e−t∣k∣2h^(k). For t>0t > 0t>0 it is convolution with the heat kernel Γt(x)=(4πt)−n/2e−∣x∣2/4t\Gamma_t(x) = (4\pi t)^{-n/2}e^{-|x|^2/4t}Γt​(x)=(4πt)−n/2e−∣x∣2/4t.

Fix λ,γ∈R\lambda, \gamma \in \mathbb{R}λ,γ∈R and an integer m≥1m \ge 1m≥1, and let F(h)=λh−γhmF(h) = \lambda h - \gamma h^mF(h)=λh−γhm act pointwise on functions. The initial value problem is

ut=Δu+λu−γum,u(x,0)=g(x).(5.34)u_t = \Delta u + \lambda u - \gamma u^m, \qquad u(x,0) = g(x). \tag{5.34}ut​=Δu+λu−γum,u(x,0)=g(x).(5.34)

Write C([0,T];Hs)C([0,T];H^s)C([0,T];Hs) for the curves t↦u(t)∈Hst \mapsto u(t) \in H^st↦u(t)∈Hs that are continuous on [0,T][0,T][0,T] in the HsH^sHs norm, normed by sup⁡0≤t≤T∥u(t)∥Hs\sup_{0\le t\le T}\|u(t)\|_{H^s}sup0≤t≤T​∥u(t)∥Hs​. A mild solution on [0,T][0,T][0,T] with values in H2αH^{2\alpha}H2α is a curve u∈C([0,T];H2α)u \in C([0,T];H^{2\alpha})u∈C([0,T];H2α) satisfying the Duhamel formula

u(t)=e−tAg+∫0te−(t−s)AF(u(s)) ds(0≤t≤T).u(t) = e^{-tA}g + \int_0^t e^{-(t-s)A}F(u(s))\,ds \qquad (0 \le t \le T).u(t)=e−tAg+∫0t​e−(t−s)AF(u(s))ds(0≤t≤T).

The right-hand side, viewed as a function of uuu, is the map Φ(u)\Phi(u)Φ(u).

Formalization targets

Goal: local existence and uniqueness (Theorem 5.49)

Let 1≤n≤31 \le n \le 31≤n≤3 and n/4<α<1n/4 < \alpha < 1n/4<α<1. For every R>0R > 0R>0 there is T>0T > 0T>0, depending only on α,n,R,λ,γ,m\alpha, n, R, \lambda, \gamma, mα,n,R,λ,γ,m, such that for every ggg with ∥g∥H2α≤R\|g\|_{H^{2\alpha}} \le R∥g∥H2α​≤R, (5.34) has a mild solution u∈C([0,T];H2α)u \in C([0,T];H^{2\alpha})u∈C([0,T];H2α), and any two mild solutions on [0,T][0,T][0,T] coincide.

Milestones

  • Smoothing (Lemma 5.50). For α>0\alpha > 0α>0 there is C=C(α,n)C = C(\alpha,n)C=C(α,n) with
∥e−tAh∥H2α≤Cettα∥h∥L2(t>0, h∈L2).\|e^{-tA}h\|_{H^{2\alpha}} \le \frac{Ce^t}{t^\alpha}\|h\|_{L^2} \qquad (t > 0,\ h \in L^2).∥e−tAh∥H2α​≤tαCet​∥h∥L2​(t>0, h∈L2).
  • Fractional Sobolev embedding (Theorem 5.79). If 0<s<n/20 < s < n/20<s<n/2 and 1/q=1/2−s/n1/q = 1/2 - s/n1/q=1/2−s/n, then ∥f∥Lq≤C∥f∥Hs\|f\|_{L^q} \le C\|f\|_{H^s}∥f∥Lq​≤C∥f∥Hs​. If s>n/2s > n/2s>n/2, then every f∈Hsf \in H^sf∈Hs is a.e. equal to a continuous function vanishing at infinity, and ∥f∥L∞≤C∥f∥Hs\|f\|_{L^\infty} \le C\|f\|_{H^s}∥f∥L∞​≤C∥f∥Hs​.
  • Local Lipschitz bound for Φ\PhiΦ (Lemma 5.51). For n/4<α<1n/4 < \alpha < 1n/4<α<1, Φ\PhiΦ maps C([0,T];H2α)C([0,T];H^{2\alpha})C([0,T];H2α) to itself, and for 0<T≤T00 < T \le T_00<T≤T0​
∥Φ(u)−Φ(v)∥≤CT1−α(1+∥u∥m−1+∥v∥m−1)∥u−v∥,\|\Phi(u)-\Phi(v)\| \le C T^{1-\alpha}\big(1 + \|u\|^{m-1} + \|v\|^{m-1}\big)\|u - v\|,∥Φ(u)−Φ(v)∥≤CT1−α(1+∥u∥m−1+∥v∥m−1)∥u−v∥,

where all norms are in C([0,T];H2α)C([0,T];H^{2\alpha})C([0,T];H2α) and CCC depends on α,m,n,λ,γ,T0\alpha, m, n, \lambda, \gamma, T_0α,m,n,λ,γ,T0​.

Significance

The theorem is the base case of the semigroup approach to nonlinear evolution equations. The existence time depends only on the size of the data, so an a priori bound on ∥u(t)∥H2α\|u(t)\|_{H^{2\alpha}}∥u(t)∥H2α​ upgrades local existence to global existence. The same scheme, with X=D(Aα)X = \mathcal D(A^\alpha)X=D(Aα) for a sectorial operator AAA, covers general semilinear parabolic problems. The smoothing estimate and the fractional Sobolev embedding are also used separately, in parabolic regularity theory and in the analysis of dispersive equations.

The results are classical and proved in the notes. None of them has a machine-checked proof on this platform. Mathlib has the L2L^2L2 Fourier transform and Plancherel's theorem, tempered distributions, and a Bessel-potential definition of Sobolev spaces, but no fractional Sobolev embedding on Rn\mathbb{R}^nRn and no mild-solution theory for semilinear heat equations. The mission asks for complete formal proofs of the three milestones and the goal, stated for the concrete objects above.

Difficulty

The obvious fixed-point argument needs three separate analytic inputs. The first is that the L2→H2αL^2 \to H^{2\alpha}L2→H2α operator norm of e−tAe^{-tA}e−tA blows up like t−αt^{-\alpha}t−α, which is integrable only because α<1\alpha < 1α<1. The second is that FFF is locally Lipschitz from H2αH^{2\alpha}H2α to L2L^2L2, which needs the embedding H2α↪L∞H^{2\alpha} \hookrightarrow L^\inftyH2α↪L∞ and fails for α≤n/4\alpha \le n/4α≤n/4. The third is that the Duhamel integral defines a continuous H2αH^{2\alpha}H2α-valued curve even though its integrand is singular at s=ts = ts=t. With these in hand, the contraction must be run on a ball whose radius is fixed by the data, with TTT chosen uniformly over that ball. Uniqueness is claimed in all of C([0,T];H2α)C([0,T];H^{2\alpha})C([0,T];H2α), not only in the ball where the contraction runs, so an extra argument is needed to exclude solutions that leave the ball.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n) with volume. The solution and the data are real-valued. Theorem 5.79 and Lemma 5.50 are stated for complex-valued functions. A curve is a map ℝ → (ℝⁿ → ℝ), and only its values on [0,T][0,T][0,T] matter.
  • Fourier normalization. The book's f^(k)=(2π)−n∫fe−ik⋅x\hat f(k) = (2\pi)^{-n}\int f e^{-ik\cdot x}f^​(k)=(2π)−n∫fe−ik⋅x is obtained from Mathlib's L2L^2L2 transform Lp.fourierTransformₗᵢ (kernel e−2πi⟨x,ξ⟩e^{-2\pi i\langle x,\xi\rangle}e−2πi⟨x,ξ⟩, no prefactor) as f^(k)=(2π)−nFf(k/2π)\hat f(k) = (2\pi)^{-n}\mathcal F f(k/2\pi)f^​(k)=(2π)−nFf(k/2π). Mathlib's constants are never used for the book's.
  • HsH^sHs norm. hsNorm is valued in [0,∞][0,\infty][0,∞] and is ∞\infty∞ off L2L^2L2, so f∈Hsf \in H^sf∈Hs means hsNorm n s f < ⊤. The factor (2π)n(2\pi)^n(2π)n is inside the square root, as in the book's inner product and in its proof of Lemma 5.50. Definition 5.74 prints it outside, which is inconsistent with both. With this choice ∥f∥H0=∥f∥L2\|f\|_{H^0} = \|f\|_{L^2}∥f∥H0​=∥f∥L2​.
  • Semigroup. e−tAe^{-tA}e−tA is convolution with the heat kernel for t>0t > 0t>0, which agrees with the multiplier (5.37) on L2L^2L2, and the identity at t=0t = 0t=0. No abstract semigroup theory is used.
  • Duhamel integral. It is taken pointwise in xxx, and (5.39) is required for almost every xxx at each t∈[0,T]t \in [0,T]t∈[0,T]. For curves in C([0,T];H2α)C([0,T];H^{2\alpha})C([0,T];H2α) with α>n/4\alpha > n/4α>n/4, the integrand is bounded, so this is the book's L2L^2L2-valued integral.
  • Constants and corrections. The data dependence of TTT is read as uniform over the ball ∥g∥H2α≤R\|g\|_{H^{2\alpha}} \le R∥g∥H2α​≤R. In Lemma 5.51 the constant, announced as C(α,m,n)C(\alpha,m,n)C(α,m,n), is allowed to depend on λ,γ\lambda, \gammaλ,γ and on an upper bound T0T_0T0​ for TTT. The hypothesis α<1\alpha < 1α<1 is added. Both corrections are used by the notes' own proof, and without them the printed inequality fails for large TTT. Theorem 5.79 prints its inequalities without the constant CCC it announces, and the constant is restored. Throughout, m≥1m \ge 1m≥1.
  • Trivializing readings excluded. The norms are [0,∞][0,\infty][0,∞]-valued and ∞\infty∞ off L2L^2L2, so no bound holds through a junk value 000. A mild solution must satisfy the Duhamel identity and be continuous in H2αH^{2\alpha}H2α, so existence cannot be met by an unconstrained curve. Uniqueness is stated over all mild solutions on [0,T][0,T][0,T], not over a ball.
  • Infrastructure. A complete development needs Plancherel in the book's normalization, the heat-kernel/multiplier identity on L2L^2L2, Bochner or pointwise integration of L2L^2L2-valued curves, the Banach fixed-point theorem on a closed ball of C([0,T];H2α)C([0,T];H^{2\alpha})C([0,T];H2α), and the fractional Sobolev embedding. The embedding and the smoothing estimate can be reused beyond this mission. Contributions of the HsH^sHs theory as a normed space are welcome.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, §5.5 and Appendices 5.C–5.D. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • N. Chafee and E. F. Infante, A bifurcation problem for a nonlinear partial differential equation of parabolic type, Applicable Analysis 4 (1974), 17–37. https://doi.org/10.1080/00036817408839081
  • A. Pazy, Semigroups of Linear Operators and Applications to Partial Differential Equations, Springer, 1983. https://doi.org/10.1007/978-1-4612-5561-1
  • D. Henry, Geometric Theory of Semilinear Parabolic Equations, Lecture Notes in Mathematics 840, Springer, 1981. https://doi.org/10.1007/BFb0089647
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Symplectic Geometry·Captain: Mazecto

Lectures on Symplectic Field Theory VIII: Asymptotic Analysis of Finite-Energy Pseudoholomorphic CurvesTextbook

Motivation

A finite-energy pseudoholomorphic curve in the symplectization R×S\mathbb{R}\times SR×S of a strictly star-shaped hypersurface S⊂R2n+2S\subset\mathbb{R}^{2n+2}S⊂R2n+2 approaches, near a non-removable puncture, a periodic Reeb orbit P=(x,T)P=(x,T)P=(x,T). The previous mission in this series formalizes this in the form of C. Wendl's Lectures on Symplectic Field Theory, Theorem 9.8: along suitable sequences of loops around the puncture the curve converges to the orbit. Most applications need much more precise information about the end. H. Hofer, K. Wysocki and E. Zehnder showed in 1996 (Ann. IHP 13) that at a nondegenerate orbit the convergence holds for the whole end and is exponentially fast, and that the leading term of the difference is eμse^{\mu s}eμs times an eigenvector of the asymptotic operator APA_PAP​; R. Siefring sharpened the formula to its present form. The asymptotic eigenvector is the input for winding numbers, fast planes and the intersection theory of punctured curves, for example in U. Hryniewicz's characterization of the Reeb orbits that bound disk-like global surfaces of section (arXiv:1105.2077).

This mission formalizes these asymptotic results in general dimension, in the setting of the previous mission. It follows Hryniewicz, Systems of global surfaces of section for dynamically convex Reeb flows on the 3-sphere, § 2.2.3 (Definitions 2.5 and 2.9, Theorem 2.11, Lemma 2.12), and the linear theory of C. Wendl's Lectures on Symplectic Field Theory (2026 notes, §§ 4.6 and 4.8). It is the eighth mission in a series on symplectic field theory.

Setting

All objects are those of FiniteEnergyPlane_Setting: V=R2n+2V=\mathbb{R}^{2n+2}V=R2n+2, a strictly star-shaped level S=H−1(1)S=H^{-1}(1)S=H−1(1) with Reeb field RRR and contact planes ξ\xiξ, a compatible complex structure JJJ on ξ\xiξ, the symplectization structure J~\tilde JJ~ on V∖{0}≅R×SV\setminus\{0\}\cong\mathbb{R}\times SV∖{0}≅R×S, and finite-energy curves.

  • Linearized Reeb flow. Along a periodic Reeb orbit P=(x,T)P=(x,T)P=(x,T), Φ(0)=id\Phi(0)=\mathrm{id}Φ(0)=id and Φ′(τ)=DR(x(τ)) Φ(τ)\Phi'(\tau)=DR(x(\tau))\,\Phi(\tau)Φ′(τ)=DR(x(τ))Φ(τ). PPP is nondegenerate if Φ(T)\Phi(T)Φ(T) fixes no nonzero vector of ξx(0)\xi_{x(0)}ξx(0)​.
  • Asymptotic operator. On smooth 111-periodic loops η\etaη with η(t)∈ξx(Tt)\eta(t)\in\xi_{x(Tt)}η(t)∈ξx(Tt)​, APη(t)=J(x(Tt))(−η′(t)+T DR(x(Tt)) η(t))A_P\eta(t)=J(x(Tt))\big(-\eta'(t)+T\,DR(x(Tt))\,\eta(t)\big)AP​η(t)=J(x(Tt))(−η′(t)+TDR(x(Tt))η(t)) (Hryniewicz, Definition 2.5).
  • Cylindrical ends. At the puncture 000 of a curve on the punctured disk, (s,t)↦e−2π(s+it)(s,t)\mapsto e^{-2\pi(s+it)}(s,t)↦e−2π(s+it); at ∞\infty∞ for a plane, (s,t)↦e2π(s+it)(s,t)\mapsto e^{2\pi(s+it)}(s,t)↦e2π(s+it). Along an end, a(s,t)a(s,t)a(s,t) and w(s,t)∈Sw(s,t)\in Sw(s,t)∈S are the two components of the curve.
  • Nondegenerate puncture (Hryniewicz, Definition 2.9): for a sign ε=±1\varepsilon=\pm1ε=±1 and constants c,dc,dc,d and b>0b>0b>0, a(s,t)−εTs−d→0a(s,t)-\varepsilon Ts-d\to0a(s,t)−εTs−d→0 and ebs(w(s,t)−x(εTt+c))→0e^{bs}\big(w(s,t)-x(\varepsilon Tt+c)\big)\to0ebs(w(s,t)−x(εTt+c))→0 uniformly in ttt. The orbit PPP itself need not be nondegenerate.
  • Asymptotic eigenvector. An eigenvalue μ\muμ of APA_PAP​ with εμ<0\varepsilon\mu<0εμ<0 and an eigenvector vvv such that, in the tube (τ,h)↦proj(x(τ)+h)(\tau,h)\mapsto\mathrm{proj}(x(\tau)+h)(τ,h)↦proj(x(τ)+h) with h∈ξx(τ)h\in\xi_{x(\tau)}h∈ξx(τ)​, the end is w=proj(x(τ)+eεμs(v(τ/T)+r))w=\mathrm{proj}\big(x(\tau)+e^{\varepsilon\mu s}(v(\tau/T)+r)\big)w=proj(x(τ)+eεμs(v(τ/T)+r)) with τ−εTt−c→0\tau-\varepsilon Tt-c\to0τ−εTt−c→0 and r→0r\to0r→0 in C∞C^\inftyC∞.

Formalization targets

Goal: asymptotic eigenvalue and eigenvector at a nondegenerate puncture

Let uuu be a finite-energy J~\tilde JJ~-holomorphic curve on the punctured unit disk D∖{0}D\setminus\{0\}D∖{0}, and let 000 be a nondegenerate puncture of uuu, asymptotic to a periodic Reeb orbit PPP with sign ε\varepsilonε. Then uuu converges to the trivial cylinder over PPP exponentially fast in C∞C^\inftyC∞. If moreover π du\pi\,duπdu does not vanish identically near 000, then uuu has an asymptotic eigenvalue μ\muμ with εμ<0\varepsilon\mu<0εμ<0 and an asymptotic eigenvector of APA_PAP​ at 000 (Hryniewicz, Theorem 2.11 and Lemma 2.12).

Milestones

  1. Linearized Reeb flow. It exists, is unique, maps ξ\xiξ to ξ\xiξ preserving ω0\omega_0ω0​, and Φ(τ+T)=Φ(τ)Φ(T)\Phi(\tau+T)=\Phi(\tau)\Phi(T)Φ(τ+T)=Φ(τ)Φ(T).
  2. Isolation. Nondegenerate orbits are isolated among the orbits of the same period.
  3. Symmetry. APA_PAP​ maps ξ\xiξ-loops to ξ\xiξ-loops and is symmetric for ⟨η,ζ⟩=∫01ω0(η,Jζ) dt\langle\eta,\zeta\rangle=\int_0^1\omega_0(\eta,J\zeta)\,dt⟨η,ζ⟩=∫01​ω0​(η,Jζ)dt (Hryniewicz, Definition 2.5).
  4. Kernel. APη=0A_P\eta=0AP​η=0 if and only if η(t)=Φ(Tt)η(0)\eta(t)=\Phi(Tt)\eta(0)η(t)=Φ(Tt)η(0); so PPP is nondegenerate if and only if APA_PAP​ has trivial kernel.
  5. Unitary frames. In a unitary frame of ξ\xiξ along PPP, APA_PAP​ becomes −J0∂t−S∞(t)-J_0\partial_t-S_\infty(t)−J0​∂t​−S∞​(t) with S∞S_\inftyS∞​ symmetric, with matching nondegeneracy (Hryniewicz, Remark 2.6).
  6. Linear exponential decay. Solutions of ∂sζ+J0∂tζ+Sζ=0\partial_s\zeta+J_0\partial_t\zeta+S\zeta=0∂s​ζ+J0​∂t​ζ+Sζ=0 on a half-cylinder that tend to 000, with S→S∞S\to S_\inftyS→S∞​ in C∞C^\inftyC∞ and −J0∂t−S∞-J_0\partial_t-S_\infty−J0​∂t​−S∞​ nondegenerate, decay exponentially (Wendl, Theorem 4.6.6).
  7. Linear asymptotic formula. If S−S∞S-S_\inftyS−S∞​ decays exponentially, a nontrivial solution of at most exponential growth is eμs(e(t)+r(s,t))e^{\mu s}(e(t)+r(s,t))eμs(e(t)+r(s,t)) with eee an eigenfunction and r→0r\to0r→0 in C∞C^\inftyC∞ (Wendl, Theorem 4.8.2).
  8. No zeros at infinity for such solutions when S→S∞S\to S_\inftyS→S∞​ in C∞C^\inftyC∞ (Wendl, Corollary 4.8.3).
  9. Asymptotically cylindrical ends. If loops along one sequence of radii converge to a nondegenerate orbit, the end is asymptotically cylindrical in C∞C^\inftyC∞ (Hofer–Wysocki–Zehnder, Theorem 1.3).
  10. Exponential convergence of asymptotically cylindrical ends at nondegenerate orbits (Hryniewicz, Theorem 2.10).
  11. Zeros of π du\pi\,duπdu. At a nondegenerate puncture, if π du\pi\,duπdu does not vanish identically near the puncture, it has no zeros near it (Hryniewicz, Definition 2.9 (3)).
  12. Planes. A nonconstant finite-energy plane whose loops at ∞\infty∞ converge along one sequence to a nondegenerate orbit has exponential asymptotics and an asymptotic eigenvector there.
  13. Bridge to R4\mathbb{R}^4R4. For n=1n=1n=1, nondegeneracy agrees with the nondegeneracy condition of the HryniewiczCriterion setting.

Significance

The results. The goal is the standard description of a finite-energy end used throughout symplectic field theory: it is what makes the asymptotic eigenvalue, the winding of the asymptotic eigenvector, the asymptotic Conley–Zehnder index and the asymptotic intersection theory of punctured curves meaningful. The goal does not assume that the limit orbit is nondegenerate, only that the end decays exponentially; this hypothesis is part of the definition of fast planes over possibly degenerate orbits (Hryniewicz, Definition 2.14). Milestone 12 is the form in which planes asymptotic to nondegenerate orbits are used, and milestone 13 connects it to the open HryniewiczCriterion mission. Milestones 6–8 are results about linear Cauchy–Riemann equations on a half-cylinder, independent of the geometry.

Formalizing them. All results are classical and proved in the cited sources (the linear results in Wendl's notes and in R. Siefring, Relative asymptotic behavior of pseudoholomorphic half-cylinders, CPAM 61 (2008)). None of them has been formalized in a proof assistant, as far as a literature search shows; Mathlib has no asymptotic operators of Reeb orbits and no theory of Cauchy–Riemann equations on cylinders.

Difficulty

The asymptotic operator acts on sections of ξ\xiξ along the orbit, defined intrinsically in R2n+2\mathbb{R}^{2n+2}R2n+2 with no preferred frame, and its spectral theory lives on loops in a moving subspace. The hypothesis of the goal is only exponential C0C^0C0 convergence, while the conclusion is C∞C^\inftyC∞ convergence and a precise leading term with a single eigenvector. The eigenvector formula is stated in a tube around the orbit with its own phase function τ(s,t)\tau(s,t)τ(s,t), so the leading term is measured transversally to the orbit rather than against the parametrization x(εTt+c)x(\varepsilon Tt+c)x(εTt+c). For multiply covered orbits the tube is only a covering of a neighbourhood of the orbit, and the phase τ\tauτ is a real lift.

Formalization scope

  • Namespace FiniteEnergyPlane; the definition module FiniteEnergyPlane_Asymptotics imports FiniteEnergyPlane_Setting (previous mission) and CauchyRiemannIndex_Setting (fifth mission) for Mat n, J₀ n, Vec n, IsSymLoop, IsNondegenerate and crOp. The bridge item also imports HryniewiczCriterion_ConleyZehnder.
  • Decay on an end is stated for maps on R×R\mathbb{R}\times\mathbb{R}R×R, uniformly in ttt as s→+∞s\to+\inftys→+∞; C∞C^\inftyC∞ statements bound every iteratedFDeriv and require smoothness on some (s0,∞)×R(s_0,\infty)\times\mathbb{R}(s0​,∞)×R. Matrix-valued convergence is entrywise.
  • Eigenvectors are smooth 111-periodic ξ\xiξ-loops that are not identically zero.
  • Not included. Winding numbers of eigenvectors, the relation between the Conley–Zehnder index and windings, windπ\mathrm{wind}_\piwindπ​ and wind∞\mathrm{wind}_\inftywind∞​, fast planes, and the Morse–Bott case are left to later missions.

Contributions welcome: general lemmas on linear ODEs along periodic orbits and on smooth families of subspaces over the circle.

Selected references

  • U. Hryniewicz, Systems of global surfaces of section for dynamically convex Reeb flows on the 3-sphere, J. Symplectic Geom. 12 (2014), § 2.2.3. https://arxiv.org/abs/1105.2077
  • U. Hryniewicz, Fast finite-energy planes in symplectizations and applications, Trans. Amer. Math. Soc. 364 (2012), 1859–1931, § 3.6 and Appendix B. https://arxiv.org/abs/0812.4076
  • H. Hofer, K. Wysocki, E. Zehnder, Properties of pseudoholomorphic curves in symplectisations I: Asymptotics, Ann. Inst. H. Poincaré Anal. Non Linéaire 13 (1996), 337–379, and Correction, 15 (1998), 535–538. https://doi.org/10.1016/S0294-1449(16)30108-1
  • C. Wendl, Lectures on Symplectic Field Theory, lecture notes, Humboldt-Universität zu Berlin (2026 version), §§ 3.1, 4.6, 4.8, 6.4, 6.7; earlier version arXiv:1612.01009. https://arxiv.org/abs/1612.01009
  • R. Siefring, Relative asymptotic behavior of pseudoholomorphic half-cylinders, Comm. Pure Appl. Math. 61 (2008), Appendix A. https://arxiv.org/abs/math/0702356
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EconomicsOperations Research·Captain: mikedeng1

High Discounts and Low Fundamental Surplus: An Equivalence Result for Unemployment Fluctuations: Tightness with Risk Premia Equals Tightness of an Artificial Economy Without Risk PremiaResearch Paper

Motivation

In the search-and-matching model of the labor market (Diamond–Mortensen–Pissarides), firms post vacancies until the expected value of a vacancy is zero, so how many jobs exist depends on how firms value future match cashflows. Shimer (2005) showed that the standard calibration produces unemployment fluctuations far smaller than in the data. Two explanations have been proposed for the gap. Ljungqvist and Sargent (2017) argue that what matters is a small fundamental surplus, the part of output that the labor market can allocate to vacancy creation. Hall (2017) argues instead for time-varying discount rates: when risk premia rise, firms discount future match surplus more heavily and post fewer vacancies.

Mitra, Seo and Xu (FRB Atlanta WP 2021-22; Management Science 2024) show that the two explanations are formally related. An economy with risk premia has the same labor-market tightness as an artificial economy without risk premia, in which the productivity process and the structural parameters are changed. In the artificial economy, the value of leisure and the vacancy cost are scaled up relative to average productivity, and discount-rate shocks appear as shocks to long-run productivity. This mission formalizes that equivalence, Proposition 1 of the paper.

Setting

The state of the economy is a pair of reals. In the economy without risk premia (§2.1), log productivity yyy mean-reverts toward a long-run level μ\muμ:

dyt=κy(μt−yt) dt+σy dBty,P,dμt=−κμμt dt+σμ dBtμ,P,dy_t=\kappa_y(\mu_t-y_t)\,dt+\sigma_y\,dB^{y,\mathcal P}_t,\qquad d\mu_t=-\kappa_\mu\mu_t\,dt+\sigma_\mu\,dB^{\mu,\mathcal P}_t,dyt​=κy​(μt​−yt​)dt+σy​dBty,P​,dμt​=−κμ​μt​dt+σμ​dBtμ,P​,

with κy>0\kappa_y>0κy​>0, κμ≥0\kappa_\mu\ge0κμ​≥0, σμ≥0\sigma_\mu\ge0σμ​≥0. Further parameters are the risk-free rate rfr_frf​, the separation rate sss, the workers' bargaining power β∈(0,1)\beta\in(0,1)β∈(0,1), the flow vacancy cost ccc and the value of leisure zzz. Matching is summarized by a vacancy-filling rate q(θ)q(\theta)q(θ) as a function of tightness θ\thetaθ (vacancies per unemployed worker), and the job-finding rate is f(θ)=θq(θ)f(\theta)=\theta q(\theta)f(θ)=θq(θ). The generator of the productivity process is

LP[κy,σy,κμ,σμ]F=κy(μ−y)∂1F+12σy2∂11F−κμμ ∂2F+12σμ2∂22F.\mathscr L^{\mathcal P}[\kappa_y,\sigma_y,\kappa_\mu,\sigma_\mu]F=\kappa_y(\mu-y)\partial_1F+\tfrac12\sigma_y^2\partial_{11}F-\kappa_\mu\mu\,\partial_2F+\tfrac12\sigma_\mu^2\partial_{22}F.LP[κy​,σy​,κμ​,σμ​]F=κy​(μ−y)∂1​F+21​σy2​∂11​F−κμ​μ∂2​F+21​σμ2​∂22​F.

An equilibrium is a match surplus S(y,μ)S(y,\mu)S(y,μ) and a tightness θ(y,μ)\theta(y,\mu)θ(y,μ) with

(rf+s)S=ey−z−βc1−βθ+LPS,c=(1−β)q(θ)S.(8)(r_f+s)S=e^y-z-\tfrac{\beta c}{1-\beta}\theta+\mathscr L^{\mathcal P}S,\qquad c=(1-\beta)q(\theta)S.\qquad(8)(rf​+s)S=ey−z−1−ββc​θ+LPS,c=(1−β)q(θ)S.(8)

The paper derives (8) from four value-function equations by free entry and Nash bargaining.

In the economy with risk premia (§2.2), productivity is dyt=−κyyt dt+σy dBty,Pdy_t=-\kappa_yy_t\,dt+\sigma_y\,dB^{y,\mathcal P}_tdyt​=−κy​yt​dt+σy​dBty,P​. Cashflows are discounted by a stochastic discount factor whose market price of risk η\etaη follows dηt=κη(ηˉ−ηt) dt+ση dBtη,Pd\eta_t=\kappa_\eta(\bar\eta-\eta_t)\,dt+\sigma_\eta\,dB^{\eta,\mathcal P}_tdηt​=κη​(ηˉ​−ηt​)dt+ση​dBtη,P​ with κη,ση>0\kappa_\eta,\sigma_\eta>0κη​,ση​>0. Under the risk-neutral measure, productivity has drift −(σyη+κyy)-(\sigma_y\eta+\kappa_yy)−(σy​η+κy​y) and is driven by Bty,Q=∫0tηu du+Bty,PB^{y,\mathcal Q}_t=\int_0^t\eta_u\,du+B^{y,\mathcal P}_tBty,Q​=∫0t​ηu​du+Bty,P​. The equilibrium (19) is (8) with the risk-neutral generator

LQF=−(σyη+κyy)∂1F+12σy2∂11F+κη(ηˉ−η)∂2F+12ση2∂22F.\mathscr L^{\mathcal Q}F=-(\sigma_y\eta+\kappa_yy)\partial_1F+\tfrac12\sigma_y^2\partial_{11}F+\kappa_\eta(\bar\eta-\eta)\partial_2F+\tfrac12\sigma_\eta^2\partial_{22}F.LQF=−(σy​η+κy​y)∂1​F+21​σy2​∂11​F+κη​(ηˉ​−η)∂2​F+21​ση2​∂22​F.

The dictionary uses the shift a=σyηˉ/κy=−EQ[yt]a=\sigma_y\bar\eta/\kappa_y=-\mathbb E^{\mathcal Q}[y_t]a=σy​ηˉ​/κy​=−EQ[yt​]. The artificial states are yQ=y+ay^{\mathcal Q}=y+ayQ=y+a and μQ=σy(ηˉ−η)/κy\mu^{\mathcal Q}=\sigma_y(\bar\eta-\eta)/\kappa_yμQ=σy​(ηˉ​−η)/κy​. The artificial parameters are zQ=eazz^{\mathcal Q}=e^azzQ=eaz, cQ=eacc^{\mathcal Q}=e^accQ=eac, κyQ=κy\kappa^{\mathcal Q}_y=\kappa_yκyQ​=κy​, σyQ=σy\sigma^{\mathcal Q}_y=\sigma_yσyQ​=σy​, κμQ=κη\kappa^{\mathcal Q}_\mu=\kappa_\etaκμQ​=κη​, σμQ=σησy/κy\sigma^{\mathcal Q}_\mu=\sigma_\eta\sigma_y/\kappa_yσμQ​=ση​σy​/κy​, and rf,s,β,qr_f,s,\beta,qrf​,s,β,q are unchanged.

Formalization targets

Goal: Proposition 1

For surpluses and tightnesses related by SQ(yQ,μQ)=eaS(y,η)S^{\mathcal Q}(y^{\mathcal Q},\mu^{\mathcal Q})=e^aS(y,\eta)SQ(yQ,μQ)=eaS(y,η) and θQ(yQ,μQ)=θ(y,η)\theta^{\mathcal Q}(y^{\mathcal Q},\mu^{\mathcal Q})=\theta(y,\eta)θQ(yQ,μQ)=θ(y,η),

(S,θ) solves (19)  ⟺  (SQ,θQ) solves (8) for the artificial parameters.(S,\theta)\ \text{solves (19)}\iff(S^{\mathcal Q},\theta^{\mathcal Q})\ \text{solves (8) for the artificial parameters}.(S,θ) solves (19)⟺(SQ,θQ) solves (8) for the artificial parameters.

The goal also states that the artificial parameters satisfy the standing assumptions of §2.1, and that the transformed productivity paths solve the artificial dynamics (26), driven by By,QB^{y,\mathcal Q}By,Q and −Bη,P-B^{\eta,\mathcal P}−Bη,P.

Milestones

  1. The surplus characterization (8) from the value-function equations (4), with the wage formula (§2.1).
  2. The risk-neutral productivity equation (15)–(16), along paths.
  3. The chain-rule facts expressing Sy,Syy,Sη,SηηS_y,S_{yy},S_\eta,S_{\eta\eta}Sy​,Syy​,Sη​,Sηη​ through derivatives of SQS^{\mathcal Q}SQ.
  4. The forward direction (19) ⇒ (25).
  5. The artificial productivity process (26)–(27).

Significance

The result. Proposition 1 lets every tool built for search models with risk-neutral firms be applied to models with time-varying risk premia. In particular, the Ljungqvist–Sargent decomposition of unemployment volatility through the fundamental surplus carries over. The paper uses it to show that high discounts in the original economy are equivalent to low fundamental surpluses in the artificial economy, and that discount-rate shocks act like long-run productivity shocks. Equilibrium moments of tightness-based statistics can then be computed in the artificial economy.

Formalizing it. The result is proved in the paper at the level of PDEs and change of variables. It has not been machine-checked. The mission produces a checked statement of the dictionary with every sign and scaling made explicit, together with the converse direction, which the paper leaves implicit. It also produces a small reusable layer: two-factor Ornstein–Uhlenbeck generators written as partial-derivative operators, and pathwise integral forms of the dynamics.

Difficulty

The algebra is elementary, but the bookkeeping is where errors occur. Three signs or scalings are easy to get wrong:

  • The long-run factor μQ\mu^{\mathcal Q}μQ decreases in η\etaη, so its shock is −Bη,P-B^{\eta,\mathcal P}−Bη,P.
  • The drift −σyη-\sigma_y\eta−σy​η must be absorbed into κy(μQ−yQ)\kappa_y(\mu^{\mathcal Q}-y^{\mathcal Q})κy​(μQ−yQ) with exactly the shift aaa.
  • eae^{a}ea rescales ccc and zzz but not β\betaβ, sss or rfr_frf​.

The converse direction needs the change of variables to be onto. The PDE identities need second derivatives of composed functions to be transported in both directions while regularity is preserved. A tempting shortcut is to define the artificial equilibrium as the pullback of (19). That makes the statement empty, and it is excluded here.

Formalization scope

All quantities are real numbers. States are curried functions R→R→R\mathbb R\to\mathbb R\to\mathbb RR→R→R with productivity first, and partial derivatives are deriv of one-variable sections. Both equilibrium predicates require the surplus to be C2C^2C2, because deriv returns 000 at non-differentiable points. The vacancy-filling rate qqq is an arbitrary function; no Cobb–Douglas form is imposed. No sign is imposed on rfr_frf​, sss, ccc or zzz.

The hypothesis σy>0\sigma_y>0σy​>0 is added to the standing assumptions of the economy with risk premia. The map (21b) is invertible only when σy≠0\sigma_y\neq0σy​=0, and the paper's estimate is σy=0.0179\sigma_y=0.0179σy​=0.0179.

Probability is not formalized. The stochastic differential equations are written as pathwise integral equations for t≥0t\ge0t≥0, driven by given paths through their increments Bt−B0B_t-B_0Bt​−B0​, and the paths y,ηy,\etay,η are continuous. The following are outside the mission's scope:

  • Girsanov's theorem, which makes By,QB^{y,\mathcal Q}By,Q a Brownian motion under the risk-neutral measure;
  • the Feynman–Kac representation linking value functions to the PDEs;
  • the stationary mean (22) under Q\mathcal QQ, whose value is used as the shift.

An equilibrium is its PDE characterization, as in the paper's derivation. The artificial equilibrium is the §2.1 predicate with the explicit generator LP\mathscr L^{\mathcal P}LP, evaluated at the artificial parameters. It is defined independently of (19) and of the dictionary, so the goal is not true by definition.

Contributions are welcome on the chain-rule lemmas for deriv under affine changes of variables in two dimensions and on regularity transfer for C2C^2C2 functions under affine maps. Both are reusable beyond this mission.

Selected references

  • I. Mitra, T. Seo, Y. Xu, High Discounts and Low Fundamental Surplus: An Equivalence Result for Unemployment Fluctuations, FRB Atlanta Working Paper 2021-22, 2021. https://doi.org/10.29338/wp2021-22 (published in Management Science 70(6), 4051–4068, 2024, https://doi.org/10.1287/mnsc.2022.03712)
  • R. E. Hall, High Discounts and High Unemployment, American Economic Review 107(2), 305–330, 2017. https://doi.org/10.1257/aer.20141297
  • L. Ljungqvist, T. J. Sargent, The Fundamental Surplus, American Economic Review 107(9), 2630–2665, 2017. https://doi.org/10.1257/aer.20150233
  • R. Shimer, The Cyclical Behavior of Equilibrium Unemployment and Vacancies, American Economic Review 95(1), 25–49, 2005. https://doi.org/10.1257/0002828053828572
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Operations ResearchProbabilityStochastic Systems·Captain: mikedeng1

Exact Optimal Stopping for Multidimensional Linear Switching Diffusions: The Optimal Stopping Boundaries Are the Unique Admissible Solution of a Nonlinear Integral EquationResearch Paper

Motivation

Optimal stopping of a diffusion whose coefficients switch with an exogenous Markov chain is the standard model for decisions taken in a random environment: an investment or abandonment decision when the economy alternates between regimes, a quickest-detection problem whose drift is driven by a hidden chain, a maintenance decision whose degradation rate depends on an operating mode. For one-dimensional problems without switching the optimal rule is a threshold, and the threshold is characterized by a nonlinear integral equation (Peskir and Shiryaev, Optimal Stopping and Free-Boundary Problems, 2006). In two dimensions with regime switching, the stopping region on each layer of the chain is bounded by a curve, the curves differ from layer to layer, and neither the optimality of the first entry time nor a characterization of the curves follows from the classical theory.

Ernst and Mei (arXiv:2107.14441, Mathematics of Operations Research, 2023) study such a problem for a two-dimensional linear diffusion driven by a two-state chain. They show that the first entry time into the stopping region is optimal although the running cost need not be integrable on [0,∞)[0,\infty)[0,∞), derive the regularity of the value function, and characterize the optimal stopping boundaries as the unique solution of a coupled system of nonlinear integral equations. Section 6 of the paper applies the results to quickest detection of a Markovian drift.

Setting

Let M={1,2}M=\{1,2\}M={1,2} be the regimes and let α\alphaα be a continuous-time Markov chain on MMM with generator Q=(qικ)Q=(q_{\iota\kappa})Q=(qικ​). Let W=(W1,W2)W=(W^1,W^2)W=(W1,W2) be a standard two-dimensional Brownian motion independent of α\alphaα. For x∈[0,∞)2x\in[0,\infty)^2x∈[0,∞)2 the state X=(X1,X2)X=(X^1,X^2)X=(X1,X2) solves

dXti=(ai(αt)+∑j=12bij(αt)Xtj)dt+σi(αt)Xti dWti,X0=x,i=1,2,dX^i_t=\Big(a^i(\alpha_t)+\sum_{j=1}^2 b^{ij}(\alpha_t)X^j_t\Big)dt+\sigma^i(\alpha_t)X^i_t\,dW^i_t,\qquad X_0=x,\quad i=1,2,dXti​=(ai(αt​)+j=1∑2​bij(αt​)Xtj​)dt+σi(αt​)Xti​dWti​,X0​=x,i=1,2,

with λ(ι)>0\lambda(\iota)>0λ(ι)>0, ai(ι)≥0a^i(\iota)\ge0ai(ι)≥0, σi(ι)≠0\sigma^i(\iota)\ne0σi(ι)=0 and bij(ι)≥0b^{ij}(\iota)\ge0bij(ι)≥0 for i≠ji\ne ji=j (Assumption 2.1). The running cost H(ι,⋅)H(\iota,\cdot)H(ι,⋅) is concave, locally Lipschitz up to the boundary, and increasing on [0,∞)2[0,\infty)^2[0,∞)2, with H(ι,(z,0))→∞H(\iota,(z,0))\to\inftyH(ι,(z,0))→∞ and H(ι,(0,z))→∞H(\iota,(0,z))\to\inftyH(ι,(0,z))→∞ (Assumption 2.2), and H‾=min⁡ιH(ι,(0,0))<0\underline H=\min_\iota H(\iota,(0,0))<0H​=minι​H(ι,(0,0))<0. The value function is

V(ι,x)=inf⁡τEι,x∫0τe−∫0tλ(αs)dsH(αt,Xt) dt,V(\iota,x)=\inf_{\tau}\mathsf E_{\iota,x}\int_0^{\tau}e^{-\int_0^t\lambda(\alpha_s)ds}H(\alpha_t,X_t)\,dt,V(ι,x)=τinf​Eι,x​∫0τ​e−∫0t​λ(αs​)dsH(αt​,Xt​)dt,

the infimum over stopping times of the augmented natural filtration of (α,X)(\alpha,X)(α,X). The continuation and stopping regions are Cι={V(ι,⋅)<0}C_\iota=\{V(\iota,\cdot)<0\}Cι​={V(ι,⋅)<0} and Dι={V(ι,⋅)=0}D_\iota=\{V(\iota,\cdot)=0\}Dι​={V(ι,⋅)=0} in (0,∞)2(0,\infty)^2(0,∞)2, the optimal stopping boundary is bι(x1)=inf⁡{x2>0:V(ι,x1,x2)=0}b_\iota(x_1)=\inf\{x_2>0:V(\iota,x_1,x_2)=0\}bι​(x1​)=inf{x2​>0:V(ι,x1​,x2​)=0}, and τD\tau_DτD​ is the first entry time of (α,X)(\alpha,X)(α,X) into DDD. Assumption 2.3 asks that each one-dimensional process dX~ti=(ai(αt)+bii(αt)X~ti)dt+σi(αt)X~ti dWtid\tilde X^i_t=(a^i(\alpha_t)+b^{ii}(\alpha_t)\tilde X^i_t)dt+\sigma^i(\alpha_t)\tilde X^i_t\,dW^i_tdX~ti​=(ai(αt​)+bii(αt​)X~ti​)dt+σi(αt​)X~ti​dWti​ be recurrent to (c,∞)(c,\infty)(c,∞) for every c>0c>0c>0. The truncated problem VNV^NVN replaces HHH by HN=min⁡(H,N)H^N=\min(H,N)HN=min(H,N).

Formalization targets

Goal: Theorem 5.1

With a constant discount rate λ≡λ0>0\lambda\equiv\lambda_0>0λ≡λ0​>0, the family {bι}\{b_\iota\}{bι​} is the unique solution, among bounded continuous c=(cι)c=(c_\iota)c=(cι​) with H(ι,(z,cι(z)))≥0H(\iota,(z,c_\iota(z)))\ge0H(ι,(z,cι​(z)))≥0, of

∫0∞∑κ∈M∫0∞∫0cκ(y1)e−λ0t pt(ι,x1,cι(x1);κ,y)H(κ,y) dy2 dy1 dt=0,x1>0,\int_0^\infty\sum_{\kappa\in M}\int_0^\infty\int_0^{c_\kappa(y_1)}e^{-\lambda_0t}\,p_t\big(\iota,x_1,c_\iota(x_1);\kappa,y\big)H(\kappa,y)\,dy_2\,dy_1\,dt=0,\qquad x_1>0,∫0∞​κ∈M∑​∫0∞​∫0cκ​(y1​)​e−λ0​tpt​(ι,x1​,cι​(x1​);κ,y)H(κ,y)dy2​dy1​dt=0,x1​>0,

and V(ι,x)=∫0∞∑κ∫0∞∫0bκ(y1)e−λ0tpt(ι,x;κ,y)H(κ,y) dy2 dy1 dtV(\iota,x)=\int_0^\infty\sum_\kappa\int_0^\infty\int_0^{b_\kappa(y_1)}e^{-\lambda_0t}p_t(\iota,x;\kappa,y)H(\kappa,y)\,dy_2\,dy_1\,dtV(ι,x)=∫0∞​∑κ​∫0∞​∫0bκ​(y1​)​e−λ0​tpt​(ι,x;κ,y)H(κ,y)dy2​dy1​dt.

Milestones

  1. Proposition 2.4: the one-dimensional truncated problem stops above finite positive thresholds xˉι1\bar x^1_\iotaxˉι1​.
  2. Lemmas 3.2 and 3.3: entry times of the truncated stopping regions are finite, and a criterion for optimality of τD\tau_DτD​.
  3. Lemmas 3.5 and 3.6, Proposition 3.7: VVV is increasing, concave and continuous; bιb_\iotabι​ is decreasing, convex, continuous and bounded.
  4. Theorem 3.8: V(ι,x)=Eι,x∫0τDe−∫0tλ(αs)dsH(αt,Xt) dtV(\iota,x)=\mathsf E_{\iota,x}\int_0^{\tau_D}e^{-\int_0^t\lambda(\alpha_s)ds}H(\alpha_t,X_t)\,dtV(ι,x)=Eι,x​∫0τD​​e−∫0t​λ(αs​)dsH(αt​,Xt​)dt.
  5. Lemmas 3.9 and 3.11, Proposition 3.13: V∈C2(Cι)V\in C^2(C_\iota)V∈C2(Cι​) solves LV−λV=−H\mathbb LV-\lambda V=-HLV−λV=−H there, V∈C1((0,∞)2)V\in C^1((0,\infty)^2)V∈C1((0,∞)2), and its gradient is Lipschitz on (1/K,K)2(1/K,K)^2(1/K,K)2.

Significance

Theorem 3.8 settles the optimality of the first entry time for a cost that is bounded below but not integrable, a case outside the standard criterion. The concavity and smooth-fit results give the free-boundary characterization of VVV (Theorem 4.1 of the paper), and the integral equation turns the unknown curves b1,b2b_1,b_2b1​,b2​ into the solution of a system that can be discretized and solved numerically, as is done for one-dimensional problems.

None of these results is formalized anywhere. A complete development would give a machine-checked account of an optimal stopping problem for a multidimensional diffusion with regime switching, including the passage from the truncated costs HNH^NHN to HHH, the regularity theory, and the integral equation. The uniqueness part of Theorem 5.1 is stated in the paper, but its proof is omitted ("we will omit further details", p. 18); a formal proof would also settle that argument in the presence of transition regions.

Difficulty

The obvious route to Theorem 3.8 is the classical criterion that the first entry time into {V=0}\{V=0\}{V=0} is optimal when E∫0∞e−Λt∣H(αt,Xt)∣ dt<∞\mathsf E\int_0^\infty e^{-\Lambda_t}|H(\alpha_t,X_t)|\,dt<\inftyE∫0∞​e−Λt​∣H(αt​,Xt​)∣dt<∞. That integrability fails here, because HHH grows without bound. Without it, the value need not be attained by any entry time a priori, and the entry time τD\tau_DτD​ need not even be finite.

The second obstacle is the chain. On a layer ι\iotaι, points of Cι∩DκC_\iota\cap D_\kappaCι​∩Dκ​ form transition regions where the process can jump from continuation into stopping without crossing a boundary, so the regularity theory for a Dirichlet problem with one common boundary does not apply, and any characterization of the curves must account for boundaries that differ by layer.

Formalization scope

Regimes and coordinates are Fin 2, 0-based: regime 0 is the paper's state 1 and x 0 is x1x_1x1​. The model is a structure of coefficients; the probabilistic setting is one probability space carrying the chain, the Brownian motions, the flow x↦Xxx\mapsto X^xx↦Xx of strong solutions of (2.2) for every x∈[0,∞)2x\in[0,\infty)^2x∈[0,∞)2, the one-dimensional flows X~i\tilde X^iX~i, and the filtrations. The SDEs are required in integral form with continuous paths; the stochastic integrals are the published relation EthierKurtz.HasBrownianItoIntegral. PPP is complete, both initial regimes have positive probability, and Pι,x\mathsf P_{\iota,x}Pι,x​ is PPP conditioned on α0=ι\alpha_0=\iotaα0​=ι, applied to XxX^xXx. Stopping times take values in [0,∞][0,\infty][0,∞] and the stopping cost is computed in extended reals from positive and negative parts, so a non-integrable cost is never silently replaced by 000. The standing H‾<0\underline H<0H​<0 of p. 4 is a hypothesis of every statement.

The integrals against the transition density in (5.1)–(5.2) are written as expectations, ∫0∞e−λ0t E[H(αt,Xt)1{Xt below the curve}]dt\int_0^\infty e^{-\lambda_0t}\,\mathsf E\big[H(\alpha_t,X_t)\mathbf 1\{X_t\text{ below the curve}\}\big]dt∫0∞​e−λ0​tE[H(αt​,Xt​)1{Xt​ below the curve}]dt, with absolute convergence required; this equals the density form whenever the density exists. A formalization that drops the integrability requirement, or that quantifies over an abstract Markov family instead of the solution of (2.2), would make the uniqueness statement false or vacuous, and is ruled out. Admissible functions take values in [0,∞)[0,\infty)[0,∞), where HHH is defined. Green regularity (used only in Lemma 3.3) is read in probability. W2,∞((1/K,K)2)W^{2,\infty}((1/K,K)^2)W2,∞((1/K,K)2) is read, as on p. 11 of the paper, as Lipschitz continuity of the first partial derivatives on the square.

Two printed slips are corrected: Lemma 3.6's bι(z)<bιN(z)b_\iota(z)<b^N_\iota(z)bι​(z)<bιN​(z) becomes ≤\le≤ (both vanish for large zzz), and Proposition 3.7(4)'s undefined xˉι2\bar x^2_\iotaxˉι2​ becomes the threshold xˉι1\bar x^1_\iotaxˉι1​ of the one-dimensional problem.

A complete development needs Itô's formula for switching diffusions, the strong Markov property of (α,X)(\alpha,X)(α,X), comparison for the linear SDE, Snell envelope arguments in continuous time, and interior elliptic regularity. The chain and filtration definitions and the extended-real stopping value are reusable for other regime-switching stopping problems. Proofs of any milestone, of the existence of the setting, and of reusable lemmas on the two-state chain are welcome.

Selected references

  • P. A. Ernst, H. Mei, Exact optimal stopping for multidimensional linear switching diffusions, Mathematics of Operations Research, 2023. arXiv:2107.14441
  • G. Peskir, A. Shiryaev, Optimal Stopping and Free-Boundary Problems, Birkhäuser, 2006. doi:10.1007/978-3-7643-7390-0
  • G. G. Yin, C. Zhu, Hybrid Switching Diffusions: Properties and Applications, Springer, 2010. doi:10.1007/978-1-4419-1105-6
  • J. du Toit, G. Peskir, The trap of complacency in predicting the maximum, Annals of Probability 35, 2007. doi:10.1214/009117906000000638
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