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Dynamical Systems·Captain: mikedeng1

Ordinary Differential Equations and Dynamical Systems VI: The Poincaré–Bendixson TheoremTextbook

Motivation

Long-time behaviour is the central question about an autonomous differential equation x˙=f(x)\dot x = f(x)x˙=f(x): where does a trajectory go as t→±∞t \to \pm\inftyt→±∞? In the plane this question has an almost complete answer. The theory begun by Poincaré (Mémoire sur les courbes définies par une équation différentielle, 1881–1886) and completed by Bendixson (Sur les courbes définies par des équations différentielles, Acta Math. 24, 1901, doi:10.1007/BF02403068) shows that a bounded planar trajectory can only accumulate on equilibria, on a periodic orbit, or on a chain of equilibria joined by connecting orbits. Chaotic behaviour, which already occurs for three-dimensional flows such as the Lorenz system, is excluded. It is the standard tool for proving that a planar system has a limit cycle, and it underlies Hilbert's 16th problem.

This mission formalizes Section 7.3 of G. Teschl, Ordinary Differential Equations and Dynamical Systems (author's preliminary version of AMS Graduate Studies in Mathematics 140, 2012), pp. 220–224, which proves the classical theorem and the generalized version with finitely many fixed points.

Setting

Let M⊆R2M \subseteq \mathbb{R}^2M⊆R2 be open and f∈C1(M,R2)f \in C^1(M, \mathbb{R}^2)f∈C1(M,R2). An integral curve at xxx is a function φ\varphiφ on an open interval J∋0J \ni 0J∋0 with φ(0)=x\varphi(0) = xφ(0)=x, φ(J)⊆M\varphi(J) \subseteq Mφ(J)⊆M and φ˙(s)=f(φ(s))\dot\varphi(s) = f(\varphi(s))φ˙​(s)=f(φ(s)) on JJJ. The union of all such JJJ is the maximal interval Ix=(T−(x),T+(x))I_x = (T_-(x), T_+(x))Ix​=(T−​(x),T+​(x)). The flow Φ(t,x)\Phi(t, x)Φ(t,x), t∈Ixt \in I_xt∈Ix​, is the value at time ttt of the maximal integral curve at xxx. With σ∈{+,−}\sigma \in \{+,-\}σ∈{+,−}:

  • the orbit is γ(x)={Φ(t,x):t∈Ix}\gamma(x) = \{\Phi(t,x) : t \in I_x\}γ(x)={Φ(t,x):t∈Ix​}, and the half-orbit γσ(x)\gamma_\sigma(x)γσ​(x) keeps only t∈Ixt \in I_xt∈Ix​ with σt>0\sigma t > 0σt>0;
  • a fixed point is a point with f(x)=0f(x) = 0f(x)=0; a periodic point is a point with Φ(T,x)=x\Phi(T, x) = xΦ(T,x)=x for some T>0T > 0T>0 in IxI_xIx​ (fixed points included). A regular periodic orbit is the orbit of a periodic point that is not fixed, and a non-closed orbit is the orbit of a point that is not periodic;
  • the ωσ\omega_\sigmaωσ​-limit set ωσ(x)\omega_\sigma(x)ωσ​(x) is the set of y∈My \in My∈M with Φ(tk,x)→y\Phi(t_k, x) \to yΦ(tk​,x)→y for some times tk∈Ixt_k \in I_xtk​∈Ix​, tk→σ∞t_k \to \sigma\inftytk​→σ∞;
  • a set U⊆MU \subseteq MU⊆M is σ\sigmaσ invariant if γσ(x)⊆U\gamma_\sigma(x) \subseteq Uγσ​(x)⊆U for every x∈Ux \in Ux∈U;
  • a transversal arc Σ=s(J)\Sigma = s(J)Σ=s(J) is the image of a C1C^1C1 embedding sss of an open interval JJJ into MMM with s˙≠0\dot s \ne 0s˙=0 and s˙1f2(s)−s˙2f1(s)≠0\dot s_1 f_2(s) - \dot s_2 f_1(s) \neq 0s˙1​f2​(s)−s˙2​f1​(s)=0 on JJJ. The parameter orders the points of Σ\SigmaΣ.

In Lean, points are Fin 2 → ℝ (general Fin n → ℝ for the Chapter 6 notions), and σ\sigmaσ is a Bool with true for +++. The definitions are lifetime, flow, orbit, halfOrbit, omegaLimitSet, IsPeriodicPoint and IsTransversalArc, all in the namespace TeschlODE.Planar.

Formalization targets

Goal: the generalized Poincaré–Bendixson theorem (Theorem 7.16)

Fix x∈Mx \in Mx∈M and σ\sigmaσ, and suppose ωσ(x)≠∅\omega_\sigma(x) \neq \emptysetωσ​(x)=∅ is compact, connected and contains only finitely many fixed points. Then one of three cases holds:

(i) ωσ(x)={x0}, f(x0)=0;(ii) ωσ(x)=γ(y), y periodic, f(y)≠0;\text{(i) } \omega_\sigma(x) = \{x_0\},\ f(x_0) = 0; \qquad \text{(ii) } \omega_\sigma(x) = \gamma(y),\ y \text{ periodic},\ f(y) \neq 0;(i) ωσ​(x)={x0​}, f(x0​)=0;(ii) ωσ​(x)=γ(y), y periodic, f(y)=0; (iii) every y∈ωσ(x) with f(y)≠0 lies on a non-closed orbit γ(y)⊆ωσ(x) with ω+(y)={a}, ω−(y)={b},\text{(iii) every } y \in \omega_\sigma(x) \text{ with } f(y) \ne 0 \text{ lies on a non-closed orbit } \gamma(y) \subseteq \omega_\sigma(x) \text{ with } \omega_+(y) = \{a\},\ \omega_-(y) = \{b\},(iii) every y∈ωσ​(x) with f(y)=0 lies on a non-closed orbit γ(y)⊆ωσ​(x) with ω+​(y)={a}, ω−​(y)={b},

where a,ba, ba,b are fixed points in ωσ(x)\omega_\sigma(x)ωσ​(x).

Milestones

  1. Lemma 7.9. The successive intersections of γσ(x0)\gamma_\sigma(x_0)γσ​(x0​) with a transversal arc through a regular point x0x_0x0​ are monotone along the arc.
  2. Corollary 7.10. ωσ(x)\omega_\sigma(x)ωσ​(x) meets a transversal arc in at most one point.
  3. Corollary 7.11. If ωσ(x)∩γσ(x)≠∅\omega_\sigma(x) \cap \gamma_\sigma(x) \neq \emptysetωσ​(x)∩γσ​(x)=∅, then xxx is periodic and ω+(x)=ω−(x)=γ(x)\omega_+(x) = \omega_-(x) = \gamma(x)ω+​(x)=ω−​(x)=γ(x).
  4. Corollary 7.12. A minimal compact σ\sigmaσ invariant set is a periodic orbit.
  5. Lemma 7.13 (Poincaré–Bendixson). A nonempty compact ωσ(x)\omega_\sigma(x)ωσ​(x) without fixed points is a regular periodic orbit.
  6. Lemma 7.14. A connected ωσ(x)\omega_\sigma(x)ωσ​(x) that contains a regular periodic orbit γ(y)\gamma(y)γ(y) equals γ(y)\gamma(y)γ(y).
  7. Lemma 7.15. If ωσ(x)\omega_\sigma(x)ωσ​(x) is compact, at most one orbit in ωσ(x)\omega_\sigma(x)ωσ​(x) runs from a fixed point x−x_-x−​ to a distinct fixed point x+x_+x+​.

Significance

The theorem turns the existence of periodic solutions into a topological statement. It is enough to find a compact positively invariant region with no equilibria, often an annulus bounded by two curves on which the vector field points inward. This is how periodic orbits are established for the van der Pol and Liénard equations (Theorem 7.8 of the same chapter) and for many models in biology and chemistry. The generalized version also describes limit sets that contain equilibria, such as homoclinic and heteroclinic cycles. Corollary 7.12 records the dimensional boundary: in the plane every minimal set is a periodic orbit, while from dimension three on minimal sets can be invariant tori with dense orbits.

The results have been proved for over a century. None of them is formalized in Mathlib or on the platform. Mathlib has omegaLimit for global flows on topological spaces and existence and uniqueness of integral curves, but no local flow of a vector field on an open set, no transversal sections and no Jordan curve theorem. This mission produces a machine-checked planar limit-set theory. The local flow and limit-set layer it needs is reusable for every later chapter on dynamical systems.

Difficulty

The statements are topological, and the proofs rest on the Jordan curve theorem for piecewise C1C^1C1 curves: a closed curve made of an orbit segment and a piece of transversal arc separates the plane, and trajectories cannot cross it in the forbidden direction. That theorem is not in Mathlib, and the platform's Jordan-curve and Schoenflies statements are open. Everything that looks one-dimensional in a sketch, "the orbit enters the inside and is trapped", depends on it. The ingredients a sketch treats as obvious also need care: the flow-box straightening (Lemma 6.2), the local return map to a transversal arc (Lemma 6.9), and the invariance, closedness and connectedness of limit sets (Lemmas 6.5–6.6). Generic arguments about compact invariant sets do not suffice: the conclusions are false in R3\mathbb{R}^3R3, so any proof must use planarity.

Formalization scope

  • Points are Fin 2 → ℝ. Its sup norm induces the Euclidean topology, and no statement depends on the norm. fff is a total function with ContDiffOn ℝ 1 f M on the open set MMM.
  • The flow is defined, not assumed. lifetime f M x is the union of domains of integral curves at xxx, and flow f M t x is the value at ttt of such a curve, selected by choice (unique for C1C^1C1 fields). Outside IxI_xIx​ the flow has the junk value xxx, and no statement evaluates it there. Limit points must lie in MMM, as in the book.
  • σ∈{±}\sigma \in \{\pm\}σ∈{±} is a Bool; true means +++ (atTop), false means −-− (atBot).
  • "Periodic" includes fixed points (period zero), as in the book. "Regular periodic" is periodic with f(y)≠0f(y) \neq 0f(y)=0, and "non-closed" is not periodic.
  • A transversal arc is a C1C^1C1 topological embedding of an open interval into MMM. The book says "smooth", so these statements cover a wider class of arcs and are at least as strong as the book's. Lemma 7.9's "monotone sequence of intersections" is stated as: any parametrization uuu of the intersection points (s(u(t))=Φ(t,x0)s(u(t)) = \Phi(t, x_0)s(u(t))=Φ(t,x0​)) is monotone or antitone on the set of intersection times.
  • "Connected" is IsPreconnected; nonemptiness is a separate hypothesis. "Finitely many fixed points" is Set.Finite {y ∈ ω_σ(x) | f y = 0}. The book's "ω±(y)∈{xj}\omega_\pm(y) \in \{x_j\}ω±​(y)∈{xj​}" is ω±(y)={a}\omega_\pm(y) = \{a\}ω±​(y)={a} for a fixed point a∈ωσ(x)a \in \omega_\sigma(x)a∈ωσ​(x). No statement uses O(·), "sufficiently small" or an unspecified constant.
  • The four hypotheses on ωσ(x)\omega_\sigma(x)ωσ​(x) (nonempty, compact, connected, finitely many fixed points) are the book's and are all kept. A formalization that drops one of them, or reads "regular periodic orbit" to include a fixed point, is not the theorem.
  • Needed infrastructure: local existence, uniqueness and continuity of the flow (Chapter 2, 6.1), the flow box, the Jordan curve theorem for piecewise C1C^1C1 curves, and the basic limit-set lemmas of Chapter 6. Contributions of any of these as separate lemmas are welcome, and the Jordan curve theorem in particular is reusable far beyond this mission.

Selected references

  • G. Teschl, Ordinary Differential Equations and Dynamical Systems, Graduate Studies in Mathematics 140, AMS, 2012 (author's preliminary version, §7.3). doi:10.1090/gsm/140, author's copy
  • I. Bendixson, Sur les courbes définies par des équations différentielles, Acta Mathematica 24 (1901), 1–88. doi:10.1007/BF02403068
  • M. W. Hirsch, S. Smale, R. L. Devaney, Differential Equations, Dynamical Systems, and an Introduction to Chaos, 3rd ed., Academic Press, 2013, Ch. 10. doi:10.1016/C2009-0-61160-0
  • L. Perko, Differential Equations and Dynamical Systems, 3rd ed., Springer, 2001, §3.7. doi:10.1007/978-1-4613-0003-8
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Control TheoryDynamical Systems·Captain: mikedeng1

Ordinary Differential Equations and Dynamical Systems V: Limit Sets and the Krasovskii–LaSalle PrincipleTextbook

Motivation

Most differential equations that model physical, biological or engineered systems cannot be solved in closed form, yet the question asked about them is usually qualitative: does the system settle down to an equilibrium, and does it stay near the equilibrium when perturbed? Liapunov's direct method answers that question without solving the equation, by exhibiting a function that does not increase along solutions. It is the standard tool of nonlinear stability analysis and of control design, where a controller is typically certified by a Liapunov function for the closed-loop system (Khalil, Nonlinear Systems).

A Liapunov function whose values strictly decrease along every non-constant solution gives asymptotic stability directly. In practice the natural candidate, often the total energy of a damped mechanical system, only satisfies a non-strict inequality. The Krasovskii–LaSalle invariance principle closes that gap: if the function is not constant along any complete orbit other than the equilibrium, the equilibrium is still asymptotically stable. It was established by Barbashin and Krasovskii (1952) and by LaSalle (1960, IRE Trans. Circuit Theory 7).

This mission formalizes Chapter 6 of Teschl, Ordinary Differential Equations and Dynamical Systems (AMS Graduate Studies in Mathematics 140, 2012; author's preliminary version), from the local flow of an autonomous equation, through limit sets, to the principle itself.

Setting

Fix n∈Nn \in \mathbb{N}n∈N, an open set M⊆RnM \subseteq \mathbb{R}^nM⊆Rn (the phase space) and a vector field f:M→Rnf : M \to \mathbb{R}^nf:M→Rn of class C1C^1C1. The autonomous system is x˙=f(x)\dot x = f(x)x˙=f(x). An integral curve is a differentiable map φ\varphiφ from an open interval JJJ into MMM with φ˙(t)=f(φ(t))\dot\varphi(t) = f(\varphi(t))φ˙​(t)=f(φ(t)) for all t∈Jt \in Jt∈J.

For each x∈Mx \in Mx∈M there is a maximal interval Ix=(T−(x),T+(x))∋0I_x = (T_-(x), T_+(x)) \ni 0Ix​=(T−​(x),T+​(x))∋0 and a unique maximal integral curve t↦Φ(t,x)t \mapsto \Phi(t, x)t↦Φ(t,x) on IxI_xIx​ with Φ(0,x)=x\Phi(0, x) = xΦ(0,x)=x: every integral curve through xxx at time 000 is a restriction of it. The map Φ\PhiΦ on W={(t,x):x∈M, t∈Ix}W = \{(t, x) : x \in M,\ t \in I_x\}W={(t,x):x∈M, t∈Ix​} is the flow. It is a local flow: IxI_xIx​ may be bounded, because solutions can leave MMM or blow up in finite time.

The orbit of xxx is γ(x)={Φ(t,x):t∈Ix}\gamma(x) = \{\Phi(t, x) : t \in I_x\}γ(x)={Φ(t,x):t∈Ix​} and the forward orbit is γ+(x)={Φ(t,x):t∈Ix, t>0}\gamma_+(x) = \{\Phi(t, x) : t \in I_x,\ t > 0\}γ+​(x)={Φ(t,x):t∈Ix​, t>0} (γ−(x)\gamma_-(x)γ−​(x) with t<0t < 0t<0). The ω+\omega_+ω+​-limit set ω+(x)\omega_+(x)ω+​(x) is the set of y∈My \in My∈M with Φ(tk,x)→y\Phi(t_k, x) \to yΦ(tk​,x)→y for some times tk→+∞t_k \to +\inftytk​→+∞ in IxI_xIx​; ω−(x)\omega_-(x)ω−​(x) uses tk→−∞t_k \to -\inftytk​→−∞.

A point x0∈Mx_0 \in Mx0​∈M with f(x0)=0f(x_0) = 0f(x0​)=0 is a fixed point. It is stable if every neighborhood U′U'U′ of x0x_0x0​ contains a neighborhood VVV of x0x_0x0​ such that solutions starting in VVV exist and stay in U′U'U′ for all t≥0t \ge 0t≥0. It is asymptotically stable if moreover Φ(t,x)→x0\Phi(t, x) \to x_0Φ(t,x)→x0​ as t→∞t \to \inftyt→∞ for all xxx in some neighborhood of x0x_0x0​.

A Liapunov function at x0x_0x0​ is a continuous L:U→RL : U \to \mathbb{R}L:U→R on an open neighborhood U⊆MU \subseteq MU⊆M of x0x_0x0​ with L(x0)=0L(x_0) = 0L(x0​)=0, L>0L > 0L>0 on U∖{x0}U \setminus \{x_0\}U∖{x0​}, and L(φ(t0))≥L(φ(t1))L(\varphi(t_0)) \ge L(\varphi(t_1))L(φ(t0​))≥L(φ(t1​)) for every integral curve φ\varphiφ and all t0<t1t_0 < t_1t0​<t1​ with φ(t0),φ(t1)∈U∖{x0}\varphi(t_0), \varphi(t_1) \in U \setminus \{x_0\}φ(t0​),φ(t1​)∈U∖{x0​}. It is strict if the inequality is always strict. SδS_\deltaSδ​ denotes the connected component of {x∈U:L(x)≤δ}\{x \in U : L(x) \le \delta\}{x∈U:L(x)≤δ} containing x0x_0x0​.

Formalization targets

Goal: Theorem 6.14 (Krasovskii–LaSalle principle)

Let x0x_0x0​ be a fixed point and LLL a Liapunov function at x0x_0x0​ on UUU. Write (∗)(\ast)(∗) for: LLL is not constant on any orbit lying entirely in U∖{x0}U \setminus \{x_0\}U∖{x0​}, i.e. every y∈My \in My∈M with γ(y)⊆U∖{x0}\gamma(y) \subseteq U \setminus \{x_0\}γ(y)⊆U∖{x0​} has points a,b∈γ(y)a, b \in \gamma(y)a,b∈γ(y) with L(a)≠L(b)L(a) \ne L(b)L(a)=L(b). Then

(∗) ⟹ x0 is asymptotically stable;L strict ⟹ (∗);(\ast) \ \Longrightarrow\ x_0 \text{ is asymptotically stable}; \qquad L \text{ strict} \ \Longrightarrow\ (\ast);(∗) ⟹ x0​ is asymptotically stable;L strict ⟹ (∗);

and, under (∗)(\ast)(∗), every x∈Mx \in Mx∈M whose forward orbit lies in a compact subset of UUU satisfies Φ(t,x)→x0\Phi(t, x) \to x_0Φ(t,x)→x0​ as t→∞t \to \inftyt→∞.

Milestones

In attack order: Theorem 6.1 (the maximal flow exists, WWW is open, Φ\PhiΦ is CkC^kCk on WWW, and Φ(t+s,x)=Φ(t,Φ(s,x))\Phi(t+s, x) = \Phi(t, \Phi(s, x))Φ(t+s,x)=Φ(t,Φ(s,x))); Lemma 6.3 (a forward orbit in a compact subset of MMM forces T+(x)=∞T_+(x) = \inftyT+​(x)=∞); Lemma 6.6 (ω±(x)\omega_\pm(x)ω±​(x) is then nonempty, compact and connected); Lemma 6.7 (d(Φ(t,x),ω±(x))→0d(\Phi(t, x), \omega_\pm(x)) \to 0d(Φ(t,x),ω±​(x))→0); Theorem 6.15 (a function non-increasing along γ+(x)⊆U\gamma_+(x) \subseteq Uγ+​(x)⊆U is constant on ω+(x)∩U\omega_+(x) \cap Uω+​(x)∩U); Lemma 6.11 (a closed SδS_\deltaSδ​ is positively invariant); Lemma 6.12 (Sε⊆Bδ(x0)S_\varepsilon \subseteq B_\delta(x_0)Sε​⊆Bδ​(x0​) and Bε(x0)⊆SδB_\varepsilon(x_0) \subseteq S_\deltaBε​(x0​)⊆Sδ​); Theorem 6.13 (Liapunov: a Liapunov function makes x0x_0x0​ stable).

Significance

The result itself. The invariance principle is the form of Liapunov's method used in applications. It gives asymptotic stability of damped mechanical systems from their energy, of gradient systems from their potential, and of adaptive and passivity-based controllers, where the natural Liapunov function is only non-increasing. Its limit-set formulation (Theorem 6.15) is also the entry point to the Poincaré–Bendixson theory of the next chapter, which uses the same ω\omegaω-limit sets.

Formalizing it. Mathlib has local existence and uniqueness for ODEs and a theory of ω\omegaω-limit sets for global flows (omegaLimit, Flow). It has no maximal solution of an ODE, no local flow with its maximal intervals, and no Liapunov stability theory. The results are classical and proved in the book; none has a machine-checked proof on this platform. This mission builds the local-flow and limit-set layer and the Liapunov layer on top of it.

Difficulty

The central difficulty is that the flow is local. The book's arguments pass freely between "the solution stays in a compact set" and "the solution exists for all positive time" (Lemma 6.3). In a formal setting every statement about Φ(t,x)\Phi(t, x)Φ(t,x) must first establish t∈Ixt \in I_xt∈Ix​, and the maximal interval must be constructed from local solutions. Theorem 6.1 on its own requires gluing local solutions into a maximal one and proving that the domain WWW is open with CkC^kCk dependence on initial conditions.

A common first idea is to assume the vector field is complete, so that Mathlib's global Flow and omegaLimit apply directly. That assumption is not available: the goal concerns orbits that stay in the neighborhood UUU, and completeness of such orbits is a consequence of the argument, not a hypothesis. Similarly, LLL is only continuous, so a derivative-based criterion ∇L⋅f≤0\nabla L \cdot f \le 0∇L⋅f≤0 cannot replace condition (6.36).

Formalization scope

The state space is EuclideanSpace ℝ (Fin n), so ∣x∣|x|∣x∣ is the Euclidean norm, and Br(x0)B_r(x_0)Br​(x0​) is the open ball Metric.ball. The standing assumption f∈Ck(M,Rn)f \in C^k(M, \mathbb{R}^n)f∈Ck(M,Rn), k≥1k \ge 1k≥1, MMM open, is a binder of every theorem (as ContDiffOn ℝ 1 f M, the weakest case, and for general k≥1k \ge 1k≥1 in Theorem 6.1). The flow enters as a pair (I, Φ) satisfying IsMaximalFlow f M I Φ, which characterizes the maximal integral curves uniquely. Theorem 6.1 proves that such a pair exists, so no completeness or extra regularity is assumed. The two time directions σ∈{±}\sigma \in \{\pm\}σ∈{±} of Lemmas 6.3–6.7 are one statement with a real parameter σ = 1 ∨ σ = -1. The ω\omegaω-limit set contains only points of MMM, as in the book.

Stability conclusions include existence of the solution for all t≥0t \ge 0t≥0. The Liapunov condition quantifies over every integral curve and constrains only the two endpoint values, exactly as (6.36). LLL is a total function whose values off UUU are never read.

Correction to the printed statement. The book's final sentence of Theorem 6.14, "every orbit lying entirely in U(x0)U(x_0)U(x0​) converges to x0x_0x0​", is false as printed. With U=M=R2U = M = \mathbb{R}^2U=M=R2 and a strict Liapunov function, some orbits escape to infinity (Khalil, §4.1). The goal therefore asks for convergence of every forward orbit contained in a compact subset of UUU, which is what the book's argument uses. The other two parts are as printed.

A trivializing formalization is ruled out: stability and asymptotic stability are stated for the maximal flow, with existence for all t≥0t \ge 0t≥0 required, and not for an arbitrary map Φ or a flow assumed global. Asymptotic stability keeps both conjuncts, stability and attraction.

Needed infrastructure: maximal solutions of C1C^1C1 autonomous ODEs and their continuation (reusable across Chapters 6–13), openness of WWW and smooth dependence on initial data, compactness arguments for limit sets, and connected components of sublevel sets. Contributions of the local-flow layer as standalone lemmas are especially welcome, since later missions of this series rely on the same objects.

Selected references

  • G. Teschl, Ordinary Differential Equations and Dynamical Systems, Graduate Studies in Mathematics 140, AMS, 2012; author's preliminary version, Chapter 6, pp. 187–208. https://www.mat.univie.ac.at/~gerald/ftp/book-ode/ode.pdf (published book: https://doi.org/10.1090/gsm/140)
  • J. P. LaSalle, Some extensions of Liapunov's second method, IRE Transactions on Circuit Theory 7 (1960), 520–527. https://doi.org/10.1109/TCT.1960.1086720
  • E. A. Barbashin and N. N. Krasovskii, On global stability of motion, Doklady Akademii Nauk SSSR 86 (1952), 453–456.
  • H. K. Khalil, Nonlinear Systems, 3rd ed., Prentice Hall, 2002, §4.1–4.2. https://www.pearson.com/en-us/subject-catalog/p/nonlinear-systems/P200000003359
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Dynamical Systems·Captain: mikedeng1

Ordinary Differential Equations and Dynamical Systems I: Existence, Uniqueness and Peano's TheoremTextbook

Why initial value problems come first

Almost every quantitative statement about an ordinary differential equation, from the stability of an equilibrium to the existence of a periodic orbit, presupposes that the equation has a solution through each initial point and, usually, that this solution is unique and depends continuously on the data. Chapter 2 of Gerald Teschl's graduate textbook Ordinary Differential Equations and Dynamical Systems (author's preliminary version of AMS GSM 140, 2012) establishes these facts for first-order systems in Rn\mathbb{R}^nRn. It is the foundation for the rest of the series: the flows, limit sets, Poincaré maps and invariant manifolds of later chapters are all built on the existence, uniqueness and extension results proved here.

A short history. Local existence was first proved in the nineteenth century by polygonal approximation (Cauchy) under differentiability-type hypotheses. Lipschitz isolated the condition that bears his name. Picard and Lindelöf established existence and uniqueness by successive approximation, and Banach (1922) abstracted the argument into the contraction principle. Peano (1890) showed that continuity of the right-hand side alone suffices for existence, without uniqueness. Gronwall's inequality and its integral generalisations give the continuous dependence estimates. Teschl's chapter presents all of these in a uniform notation.

Setting

An initial value problem (IVP) is

x˙=f(t,x),x(t0)=x0,(2.10)\dot x = f(t, x), \qquad x(t_0) = x_0, \qquad (2.10)x˙=f(t,x),x(t0​)=x0​,(2.10)

where fff is a continuous map from an open set U⊆R×RnU \subseteq \mathbb{R} \times \mathbb{R}^nU⊆R×Rn to Rn\mathbb{R}^nRn and (t0,x0)∈U(t_0, x_0) \in U(t0​,x0​)∈U. Here ∣x∣|x|∣x∣ is the Euclidean norm on Rn\mathbb{R}^nRn. A solution on an interval III is a function x:I→Rnx : I \to \mathbb{R}^nx:I→Rn whose graph {(t,x(t)):t∈I}\{(t, x(t)) : t \in I\}{(t,x(t)):t∈I} lies in UUU and which is differentiable on III (one-sidedly at an endpoint that belongs to III) with x˙(t)=f(t,x(t))\dot x(t) = f(t, x(t))x˙(t)=f(t,x(t)). Such a solution is automatically continuously differentiable.

The function fff is locally Lipschitz in the second argument, uniformly with respect to the first, if for every compact V0⊆UV_0 \subseteq UV0​⊆U there is a constant LLL with ∣f(t,x)−f(t,y)∣≤L∣x−y∣|f(t,x) - f(t,y)| \le L|x - y|∣f(t,x)−f(t,y)∣≤L∣x−y∣ whenever (t,x),(t,y)∈V0(t,x), (t,y) \in V_0(t,x),(t,y)∈V0​ (the book's (2.18)).

For T,δ>0T, \delta > 0T,δ>0 let V=[t0,t0+T]×Bˉδ(x0)V = [t_0, t_0 + T] \times \bar B_\delta(x_0)V=[t0​,t0​+T]×Bˉδ​(x0​), where Bˉδ(x0)={x:∣x−x0∣≤δ}\bar B_\delta(x_0) = \{x : |x - x_0| \le \delta\}Bˉδ​(x0​)={x:∣x−x0​∣≤δ}, let M=max⁡V∣f∣M = \max_V |f|M=maxV​∣f∣, and define the existence time

T0=min⁡{T,δM},with δM=∞ when M=0.T_0 = \min\Bigl\{T, \frac{\delta}{M}\Bigr\}, \qquad \text{with } \frac{\delta}{M} = \infty \text{ when } M = 0 .T0​=min{T,Mδ​},with Mδ​=∞ when M=0.

The chapter also works in a real Banach space XXX, a complete normed real vector space, where a contraction of a closed set C⊆XC \subseteq XC⊆X is a map K:C→CK : C \to CK:C→C with ∥K(x)−K(y)∥≤θ∥x−y∥\|K(x) - K(y)\| \le \theta\|x - y\|∥K(x)−K(y)∥≤θ∥x−y∥ for some θ∈[0,1)\theta \in [0, 1)θ∈[0,1).

Formalization targets

Goal: Peano's existence theorem (Theorem 2.19)

If fff is continuous on V=[t0,t0+T]×Bˉδ(x0)V = [t_0, t_0 + T] \times \bar B_\delta(x_0)V=[t0​,t0​+T]×Bˉδ​(x0​) and M=max⁡V∣f∣M = \max_V |f|M=maxV​∣f∣, then there is a function xxx with x(t0)=x0x(t_0) = x_0x(t0​)=x0​ solving

x˙(t)=f(t,x(t)),∣x(t)−x0∣≤δ,t∈[t0,t0+T0],\dot x(t) = f(t, x(t)), \qquad |x(t) - x_0| \le \delta, \qquad t \in [t_0, t_0 + T_0],x˙(t)=f(t,x(t)),∣x(t)−x0​∣≤δ,t∈[t0​,t0​+T0​],

and the analogous statement holds on [t0−T0,t0][t_0 - T_0, t_0][t0​−T0​,t0​] with V=[t0−T,t0]×Bˉδ(x0)V = [t_0 - T, t_0] \times \bar B_\delta(x_0)V=[t0​−T,t0​]×Bˉδ​(x0​). No Lipschitz condition is assumed and the solution need not be unique.

Milestones

  1. Theorem 2.1 (contraction principle). A contraction of a nonempty closed subset of a Banach space has a unique fixed point xˉ\bar xxˉ, and ∥Km(x)−xˉ∥≤θm1−θ∥K(x)−x∥\|K^m(x) - \bar x\| \le \frac{\theta^m}{1-\theta}\|K(x) - x\|∥Km(x)−xˉ∥≤1−θθm​∥K(x)−x∥ for every x∈Cx \in Cx∈C.
  2. Theorem 2.2 (Picard–Lindelöf). Under the local Lipschitz condition, (2.10) has a solution on an open interval around t0t_0t0​; two solutions on any interval containing t0t_0t0​ coincide; and a solution exists on [t0,t0+T0][t_0, t_0 + T_0][t0​,t0​+T0​] with graph in VVV (and on [t0−T0,t0][t_0 - T_0, t_0][t0​−T0​,t0​]).
  3. Theorem 2.4 (Weissinger). If ∥Km(x)−Km(y)∥≤θm∥x−y∥\|K^m(x) - K^m(y)\| \le \theta_m\|x - y\|∥Km(x)−Km(y)∥≤θm​∥x−y∥ with ∑θm<∞\sum \theta_m < \infty∑θm​<∞, then KKK has a unique fixed point and ∥Km(x)−xˉ∥≤(∑j≥mθj)∥K(x)−x∥\|K^m(x) - \bar x\| \le \bigl(\sum_{j \ge m}\theta_j\bigr)\|K(x) - x\|∥Km(x)−xˉ∥≤(∑j≥m​θj​)∥K(x)−x∥.
  4. Lemma 2.7 (generalised Gronwall). ψ≤α+∫0tβψ\psi \le \alpha + \int_0^t \beta\psiψ≤α+∫0t​βψ with β≥0\beta \ge 0β≥0 implies ψ(t)≤α(t)+∫0tα(s)β(s)e∫stβ ds\psi(t) \le \alpha(t) + \int_0^t \alpha(s)\beta(s)e^{\int_s^t \beta}\,dsψ(t)≤α(t)+∫0t​α(s)β(s)e∫st​βds, and ψ(t)≤α(t)e∫0tβ\psi(t) \le \alpha(t)e^{\int_0^t\beta}ψ(t)≤α(t)e∫0t​β for nondecreasing α\alphaα.
  5. Theorem 2.8 (continuous dependence). ∣x(t)−y(t)∣≤∣x0−y0∣eL∣t−t0∣+ML(eL∣t−t0∣−1)|x(t) - y(t)| \le |x_0 - y_0|e^{L|t-t_0|} + \frac{M}{L}(e^{L|t-t_0|} - 1)∣x(t)−y(t)∣≤∣x0​−y0​∣eL∣t−t0​∣+LM​(eL∣t−t0​∣−1) for solutions of x˙=f(t,x)\dot x = f(t,x)x˙=f(t,x) and y˙=g(t,y)\dot y = g(t,y)y˙​=g(t,y).
  6. Theorem 2.17 (global existence). If ∣f(t,x)∣≤M(T)+L(T)∣x∣|f(t,x)| \le M(T) + L(T)|x|∣f(t,x)∣≤M(T)+L(T)∣x∣ on [−T,T]×Rn[-T, T] \times \mathbb{R}^n[−T,T]×Rn for every T>0T > 0T>0, every solution extends to all of R\mathbb{R}R.
  7. Theorem 2.18 (Arzelà–Ascoli). A bounded, equicontinuous sequence in C([a,b],Rn)C([a,b], \mathbb{R}^n)C([a,b],Rn) has a uniformly convergent subsequence.

Significance

Peano's theorem is the existence statement with the weakest regularity hypothesis on fff in the classical theory. It is what lets one speak of solutions of equations with non-Lipschitz right-hand sides, such as x˙=∣x∣\dot x = \sqrt{|x|}x˙=∣x∣​, and it is the starting point for the theory of non-unique solutions and differential inclusions. The explicit existence time T0=min⁡{T,δ/M}T_0 = \min\{T, \delta/M\}T0​=min{T,δ/M} is the quantitative form used whenever one needs a uniform lower bound on the lifetime of solutions starting in a compact set. Picard–Lindelöf, Gronwall and continuous dependence together make the IVP well posed. The global existence theorem under linear growth is used throughout the later chapters to define global flows.

Mathlib already contains a Picard–Lindelöf theorem (IsPicardLindelof), Gronwall's inequality in differential form, the Banach fixed point theorem for complete (extended) metric spaces, and an Arzelà–Ascoli theorem for bounded continuous functions. It does not contain Peano's theorem, the integral form of the generalised Gronwall inequality with variable α\alphaα, Weissinger's theorem, or global existence under linear growth. The statements here are phrased in the book's setting: one-sided intervals, the M=0M = 0M=0 convention for T0T_0T0​, local Lipschitz conditions on an open set, Rn\mathbb{R}^nRn-valued functions. Connecting them to the existing Mathlib results is part of the work.

Difficulty

For Peano's theorem the obvious approach, Picard iteration, does not apply. Without a Lipschitz condition the integral operator x↦x0+∫t0tf(s,x(s)) dsx \mapsto x_0 + \int_{t_0}^t f(s, x(s))\,dsx↦x0​+∫t0​t​f(s,x(s))ds need not be a contraction on any ball, its fixed points need not be unique, and a sequence of approximate solutions need not converge. Any argument has to produce a solution without a uniqueness mechanism and still reach the full interval [t0,t0+T0][t_0, t_0 + T_0][t0​,t0​+T0​] that the theorem specifies, not merely some shorter one. On the formal side, derivatives relative to closed intervals, the M=0M = 0M=0 corner of T0T_0T0​, and passing between the differential and the integral form of the IVP all need care.

For Theorem 2.17 the difficulty is that "every solution is defined on all of R\mathbb{R}R" is a statement about maximal solutions, and the book defines these only through a gluing construction. Without a Lipschitz condition that construction is no longer unique. An a-priori bound on ∣x(t)∣|x(t)|∣x(t)∣ alone does not give extension beyond a finite endpoint.

Formalization scope

  • State space. Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n), so ∣x∣|x|∣x∣ is the Euclidean norm. The right-hand side is a total function f:R×Rn→Rnf : \mathbb{R} \times \mathbb{R}^n \to \mathbb{R}^nf:R×Rn→Rn; hypotheses restrict attention to UUU or VVV. Banach spaces are real normed spaces with CompleteSpace.
  • Solutions. IsSolutionOn U f I x: for every t∈It \in It∈I, (t,x(t))∈U(t, x(t)) \in U(t,x(t))∈U and xxx has derivative f(t,x(t))f(t, x(t))f(t,x(t)) at ttt relative to III. Initial conditions are separate hypotheses.
  • Closed ball. The book writes the open ball Bδ(x0)B_\delta(x_0)Bδ​(x0​) in Theorems 2.2 and 2.19 but takes a maximum over VVV and uses ∣x(t)−x0∣≤δ|x(t) - x_0| \le \delta∣x(t)−x0​∣≤δ in the proofs. The statements use the closed ball: over the open ball the maximum may not exist, and the solution can reach the sphere at t0+T0t_0 + T_0t0​+T0​.
  • Quantifier readings. "The maximum of ∣f∣|f|∣f∣ on VVV" is a variable MMM with IsGreatest {|f(p)| : p ∈ V} M. T0T_0T0​ is if M = 0 then T else min T (δ / M). "Some interval around t0t_0t0​" in Theorem 2.2 is ∃ε>0\exists \varepsilon > 0∃ε>0 with (t0−ε,t0+ε)(t_0 - \varepsilon, t_0 + \varepsilon)(t0​−ε,t0​+ε), and "unique" means uniqueness on every interval containing t0t_0t0​. In Theorem 2.8 the suprema LLL, MMM of (2.41) become arbitrary constants L≥0L \ge 0L≥0, MMM bounding the same quantities, which is equivalent because the bound is monotone in both; the case L=0L = 0L=0 uses the limit M∣t−t0∣M|t - t_0|M∣t−t0​∣. In Theorem 2.17 the constants M(T),L(T)M(T), L(T)M(T),L(T) are existential inside ∀T>0\forall T > 0∀T>0, so they may depend on TTT but not on xxx. "All solutions are defined for all ttt" means that every solution on an open interval extends to a solution on R\mathbb{R}R.
  • Hypotheses of Theorem 2.17. Section 2.6 opens with a standing assumption of local uniqueness, but Theorem 2.17's own text needs only continuity and (2.66), and the book's remark after Theorem 2.13 covers maximal solutions without uniqueness. The statement assumes only continuity of fff and (2.66); it is therefore at least as strong as the book's.
  • Added regularity. Lemma 2.7 assumes ψ,α,β\psi, \alpha, \betaψ,α,β continuous on [0,T][0, T][0,T], which the book leaves implicit.
  • Ruling out trivial readings. An existence statement in which the interval collapses to a point would be trivially true. Here T,δ>0T, \delta > 0T,δ>0 are required, T0=TT_0 = TT0​=T when M=0M = 0M=0 (never Lean's δ/0=0\delta/0 = 0δ/0=0), and a solution must satisfy the differential equation at every point of [t0,t0+T0][t_0, t_0 + T_0][t0​,t0​+T0​] with the book's T0T_0T0​, not on some unspecified shorter interval.

A complete development needs derivatives within intervals, interval integrals, uniform convergence and compactness in C([a,b],Rn)C([a,b], \mathbb{R}^n)C([a,b],Rn). The definitions IsSolutionOn and LocallyLipschitzSecond are reused throughout the Teschl series. Contributions that connect these statements to Mathlib's IsPicardLindelof, ContractingWith and BoundedContinuousFunction.arzela_ascoli are welcome.

Selected references

  • G. Teschl, Ordinary Differential Equations and Dynamical Systems, Graduate Studies in Mathematics 140, American Mathematical Society, 2012. Author's preliminary version: https://www.mat.univie.ac.at/~gerald/ftp/book-ode/ode.pdf ; published version: https://doi.org/10.1090/gsm/140
  • G. Peano, Démonstration de l'intégrabilité des équations différentielles ordinaires, Mathematische Annalen 37 (1890), 182–228. https://doi.org/10.1007/BF01200235
  • S. Banach, Sur les opérations dans les ensembles abstraits et leur application aux équations intégrales, Fundamenta Mathematicae 3 (1922), 133–181. https://doi.org/10.4064/fm-3-1-133-181
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Pure Mathematics·Captain: mikedeng1

Tasty Bits of Several Complex Variables II: The Ball and the Polydisc Are Not BiholomorphicTextbook

Motivation

In one complex variable the Riemann mapping theorem classifies a whole class of domains by topology alone: every nonempty simply connected proper subdomain of C\mathbb{C}C is biholomorphic to the unit disc. Nothing of the kind holds in several variables. The two most obvious generalizations of the disc to Cn\mathbb{C}^nCn, the unit ball and the unit polydisc, are homeomorphic, yet no biholomorphic map carries one onto the other. This is the first result a student of several complex variables meets that has no one-variable shadow, and it is the standard illustration that the geometry of the boundary, not the topology of the domain, governs holomorphic equivalence.

As recounted in the source, Poincaré (1907) observed the inequivalence by computing the automorphism groups of D2\mathbb{D}^2D2 and B2\mathbb{B}_2B2​, assuming the maps extend past the boundary; H. Cartan gave the first complete proof in 1931; and Rothstein (1935) proved that there is not even a proper holomorphic map from the bidisc to the ball. This mission follows the presentation in §1.4–1.6 of J. Lebl, Tasty Bits of Several Complex Variables (version 4.4, 2026), where the inequivalence is derived from a general theorem on proper maps out of product domains, followed by Cartan's uniqueness theorem and the basic structure theory of zero sets and injective maps.

Setting

Write Cn\mathbb{C}^nCn for nnn-tuples z=(z1,…,zn)z = (z_1, \dots, z_n)z=(z1​,…,zn​) of complex numbers, D={ζ∈C:∣ζ∣<1}\mathbb{D} = \{\zeta \in \mathbb{C} : |\zeta| < 1\}D={ζ∈C:∣ζ∣<1} for the unit disc, and ∥z∥=(∣z1∣2+⋯+∣zn∣2)1/2\|z\| = (|z_1|^2 + \cdots + |z_n|^2)^{1/2}∥z∥=(∣z1​∣2+⋯+∣zn​∣2)1/2 for the Euclidean norm. The unit ball and unit polydisc are

Bn={z∈Cn:∣z1∣2+⋯+∣zn∣2<1},Dn={z∈Cn:∣zk∣<1 for k=1,…,n},\mathbb{B}_n = \{ z \in \mathbb{C}^n : |z_1|^2 + \cdots + |z_n|^2 < 1 \}, \qquad \mathbb{D}^n = \{ z \in \mathbb{C}^n : |z_k| < 1 \text{ for } k = 1, \dots, n \},Bn​={z∈Cn:∣z1​∣2+⋯+∣zn​∣2<1},Dn={z∈Cn:∣zk​∣<1 for k=1,…,n},

and the unit sphere is S2n−1=∂Bn={z:∣z1∣2+⋯+∣zn∣2=1}S^{2n-1} = \partial\mathbb{B}_n = \{ z : |z_1|^2 + \cdots + |z_n|^2 = 1 \}S2n−1=∂Bn​={z:∣z1​∣2+⋯+∣zn​∣2=1}. A domain is a nonempty connected open set. A map between open subsets of complex spaces is holomorphic if it is complex differentiable at every point.

A continuous map f:U→Vf : U \to Vf:U→V is proper if f−1(K)f^{-1}(K)f−1(K) is compact for every compact K⊂VK \subset VK⊂V. A biholomorphic map f:U→Vf : U \to Vf:U→V is a holomorphic bijection whose inverse is holomorphic; every biholomorphism is proper. An analytic disc is a nonconstant holomorphic map φ:D→Cn\varphi : \mathbb{D} \to \mathbb{C}^nφ:D→Cn, and a set SSS contains no analytic discs if no analytic disc has φ(D)⊂S\varphi(\mathbb{D}) \subset Sφ(D)⊂S. A circular domain is a domain UUU with eiθz∈Ue^{i\theta} z \in Ueiθz∈U whenever z∈Uz \in Uz∈U and θ∈R\theta \in \mathbb{R}θ∈R.

Formalization targets

Goal: Rothstein's theorem (Theorem 1.4.4)

there is no proper holomorphic map f:D2→B2.\text{there is no proper holomorphic map } f : \mathbb{D}^2 \to \mathbb{B}_2 .there is no proper holomorphic map f:D2→B2​.

The path to the goal

  • Proposition 1.4.6. S2n−1S^{2n-1}S2n−1 contains no analytic discs.
  • Lemma 1.4.7. For bounded domains U⊂RnU \subset \mathbb{R}^nU⊂Rn, V⊂RmV \subset \mathbb{R}^mV⊂Rm and continuous f:U→Vf : U \to Vf:U→V: fff is proper if and only if, whenever pk∈Up_k \in Upk​∈U and pk→p∈∂Up_k \to p \in \partial Upk​→p∈∂U, every limit point of {f(pk)}\{f(p_k)\}{f(pk​)} lies in ∂V\partial V∂V.
  • Theorem 1.4.8. If U=U′×U′′⊂Cn×CkU = U' \times U'' \subset \mathbb{C}^n \times \mathbb{C}^kU=U′×U′′⊂Cn×Ck (n,k≥1n, k \ge 1n,k≥1) and V⊂CmV \subset \mathbb{C}^mV⊂Cm are bounded domains and ∂V\partial V∂V contains no analytic discs, there is no proper holomorphic map U→VU \to VU→V.

Further results on the same definitions

  • Theorem 1.5.1 (Cartan). If U⊂CnU \subset \mathbb{C}^nU⊂Cn is a bounded domain, a∈Ua \in Ua∈U, f:U→Uf : U \to Uf:U→U holomorphic, f(a)=af(a) = af(a)=a and Df(a)=IDf(a) = IDf(a)=I, then f(z)=zf(z) = zf(z)=z on UUU.
  • Corollary 1.5.2. A biholomorphism f:U→Vf : U \to Vf:U→V of bounded circular domains with f(0)=0f(0) = 0f(0)=0 is the restriction of a linear map.
  • Theorem 1.6.1 (Riemann extension). If g∈O(U)g \in \mathcal{O}(U)g∈O(U) is not identically zero on a domain UUU and f∈O(U∖g−1(0))f \in \mathcal{O}(U \setminus g^{-1}(0))f∈O(U∖g−1(0)) is locally bounded in UUU, then fff extends uniquely to some F∈O(U)F \in \mathcal{O}(U)F∈O(U).
  • Theorem 1.6.2. The zero set of a holomorphic function that is not identically zero on a domain is, on an open dense subset of itself, locally a graph zn=g(z1,…,zn−1)z_n = g(z_1, \dots, z_{n-1})zn​=g(z1​,…,zn−1​) after reordering the variables.
  • Theorem 1.6.6. An injective holomorphic map U→CnU \to \mathbb{C}^nU→Cn on an open U⊂CnU \subset \mathbb{C}^nU⊂Cn has nowhere vanishing Jacobian determinant; a holomorphic bijection between open sets of Cn\mathbb{C}^nCn is biholomorphic.

The goal is chosen as the textbook's headline result of §1.4. Theorem 1.4.8 is strictly more general; it is a milestone, so a solver may prove the goal as its special case.

Significance

Rothstein's theorem implies the biholomorphic inequivalence of B2\mathbb{B}_2B2​ and D2\mathbb{D}^2D2, the basic example that the Riemann mapping theorem has no analogue in several variables. Theorem 1.4.8 isolates the reason: a boundary that contains analytic discs cannot be mapped properly into a boundary that contains none. Cartan's uniqueness theorem and its corollary are the standard tools for computing automorphism groups of the ball and the polydisc. The Riemann extension theorem, the local graph structure of zero sets and the Jacobian criterion for injective maps are used throughout the theory of analytic varieties and of holomorphic mappings.

All of these results are classical and proved in the source. None of them is formalized in Mathlib or on the platform for Cn\mathbb{C}^nCn with n≥2n \ge 2n≥2: Mathlib has one-variable Riemann removable singularities and the maximum modulus principle, and the platform has one-variable results on injective holomorphic maps. This mission produces machine-checked statements of the several-variable versions, and infrastructure (proper maps between subsets, analytic discs, holomorphic families) that later chapters of the series reuse.

Difficulty

The goal cannot be reached through topology: D2\mathbb{D}^2D2 and B2\mathbb{B}_2B2​ are homeomorphic, so any argument must use holomorphy essentially and must see the boundary. The step that needs genuine analysis is passing from properness, a statement about compact sets, to a statement about boundary values of holomorphic functions of one variable along slices of the product domain; this requires normal families (Montel's theorem) in several variables, which Mathlib does not provide in the needed form. Cartan's theorem rests on power-series expansions in homogeneous parts and vector-valued Cauchy estimates on polydiscs. Theorem 1.6.2 needs the holomorphic implicit function theorem and Rouché's theorem, and Theorem 1.6.6 an induction on dimension that runs through Theorem 1.6.2. The Riemann extension theorem needs holomorphy of parameter-dependent Cauchy integrals.

Formalization scope

Cn\mathbb{C}^nCn is Fin n → ℂ. Mathlib's norm on this type is the sup norm, so Metric.ball 0 1 is the polydisc, not the ball. The ball and the sphere are therefore defined with the explicit Euclidean condition, unitBall n = {z | ∑ k, ‖z k‖ ^ 2 < 1} and unitSphere n = {z | ∑ k, ‖z k‖ ^ 2 = 1}. The polydisc is written coordinatewise as unitPolydisc n. Reading the ball as the sup-norm ball would trivialize the goal (the identity of the bidisc is a proper holomorphic self-map); the definitions exclude that reading. Boundedness is Bornology.IsBounded, and boundaries are Mathlib's frontier; neither depends on the norm. A domain is IsOpen U ∧ IsConnected U, so it is nonempty.

Holomorphic means DifferentiableOn ℂ on an open set. On open sets this is equivalent to the book's Definition 1.1.2 (Proposition 1.1.3 and Theorem 1.2.1). Maps into Cm\mathbb{C}^mCm are Fin m → ℂ-valued. Df(a)Df(a)Df(a) is fderiv ℂ f a, and the Jacobian determinant is LinearMap.det of it. Maps are ambient functions whose values off the relevant set are irrelevant. Consequently:

  • Proper is IsProperMapOn f U V: f maps U into V, is continuous on U, and U ∩ f ⁻¹' K is compact for every compact K ⊆ V. This is Definition 1.4.3 for the restricted map. It is not IsProperMap of the ambient map.
  • Uniqueness in Theorem 1.6.1 is uniqueness on UUU.
  • The inverse of a biholomorphism is a function g holomorphic on VVV with Set.InvOn g f U V.

Lemma 1.4.7 works in Fin n → ℝ and reads "limit point of the sequence {f(pk)}\{f(p_k)\}{f(pk​)}" as a cluster point of the sequence (MapClusterPt). Theorem 1.4.8 uses the product type (Fin n → ℂ) × (Fin k → ℂ) for Cn×Ck\mathbb{C}^n \times \mathbb{C}^kCn×Ck. In Theorem 1.6.2, "after reordering the variables" means choosing the index j of the solved-for coordinate. The remaining coordinates are indexed by {i // i ≠ j}. Only the open-disc part of Definition 1.4.5 (analytic discs) is formalized, because closed analytic discs are not used here.

A complete development needs Montel's theorem for maps into bounded subsets of Cm\mathbb{C}^mCm, homogeneous expansions and Cauchy estimates on polydiscs, the holomorphic implicit function theorem, Rouché's theorem, and holomorphic parameter-dependent Cauchy integrals. All of it is reusable beyond this mission, and contributions of it are welcome.

Selected references

  • J. Lebl, Tasty Bits of Several Complex Variables: A Whirlwind Tour of the Subject, version 4.4, 2026, §1.4–1.6 (pp. 32–46). https://www.jirka.org/scv/scv.pdf
  • H. Poincaré, Les fonctions analytiques de deux variables et la représentation conforme, Rend. Circ. Mat. Palermo 23 (1907), 185–220. https://doi.org/10.1007/BF03013518
  • S. G. Krantz, Function Theory of Several Complex Variables, 2nd ed., AMS Chelsea, 2001 (cited by Lebl as [K]). https://doi.org/10.1090/chel/340
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Functional AnalysisPartial Differential Equations·Captain: mikedeng1

Notes on Partial Differential Equations X: Galerkin Existence of Weak Solutions of Parabolic PDEsTextbook

Motivation

Linear second-order parabolic equations such as ut+Lu=fu_t + Lu = fut​+Lu=f model diffusion with advection, growth or decay, and external sources. The heat equation is the prototype. For coefficients that are only bounded and measurable, classical solutions need not exist, and the natural well-posedness theory is the L2L^2L2 energy theory of weak solutions. In that theory the solution is a curve t↦u(t)t \mapsto u(t)t↦u(t) in a Sobolev space, and the equation holds in the dual space. This framework, developed by J.-L. Lions and others in the 1950s–60s (Lions–Magenes 1972), underlies the numerical analysis of parabolic problems through finite elements and spectral Galerkin methods. It also underlies the existence theory for nonlinear evolution equations such as the Navier–Stokes equations (Temam 1977).

This mission formalizes Chapter 6 of J. K. Hunter's Notes on Partial Differential Equations (UC Davis, revised 6/18/2014): the existence, uniqueness and energy estimate for weak solutions of the parabolic initial–boundary value problem, proved by the Galerkin method. It also formalizes the vector-valued calculus on Hilbert triples that the proof rests on, and the Ehrling and Aubin–Lions compactness results of §6.6.

Setting

Let Ω⊂Rn\Omega \subset \mathbb{R}^nΩ⊂Rn be a bounded open set and T>0T > 0T>0. H01(Ω)H^1_0(\Omega)H01​(Ω) is the closure of Cc∞(Ω)C_c^\infty(\Omega)Cc∞​(Ω) in the norm ∥u∥H012=∫Ω(u2+∣Du∣2) dx\|u\|_{H^1_0}^2 = \int_\Omega (u^2 + |Du|^2)\,dx∥u∥H01​2​=∫Ω​(u2+∣Du∣2)dx. H−1(Ω)H^{-1}(\Omega)H−1(Ω) is its dual, with pairing ⟨f,v⟩\langle f, v\rangle⟨f,v⟩. Every u∈L2(Ω)u \in L^2(\Omega)u∈L2(Ω) acts on H01(Ω)H^1_0(\Omega)H01​(Ω) by v↦∫Ωuv dxv \mapsto \int_\Omega uv\,dxv↦∫Ω​uvdx.

The operator is Lu=−∑i,j∂i(aij∂ju)+∑jbj∂ju+cuLu = -\sum_{i,j}\partial_i(a^{ij}\partial_j u) + \sum_j b^j\partial_j u + cuLu=−∑i,j​∂i​(aij∂j​u)+∑j​bj∂j​u+cu. Its coefficients satisfy Assumption 6.1: aij,bj,c∈L∞(Ω×(0,T))a^{ij}, b^j, c \in L^\infty(\Omega\times(0,T))aij,bj,c∈L∞(Ω×(0,T)), aij=ajia^{ij} = a^{ji}aij=aji, and uniform ellipticity ∑aijξiξj≥θ∣ξ∣2\sum a^{ij}\xi_i\xi_j \ge \theta|\xi|^2∑aijξi​ξj​≥θ∣ξ∣2 for some θ>0\theta > 0θ>0. The associated form is

a(u,v;t)=∑i,j∫Ωaij∂iu ∂jv dx+∑j∫Ωbj∂ju v dx+∫Ωc uv dx.a(u, v; t) = \sum_{i,j}\int_\Omega a^{ij}\partial_i u\,\partial_j v\,dx + \sum_j\int_\Omega b^j\partial_j u\,v\,dx + \int_\Omega c\,uv\,dx.a(u,v;t)=i,j∑​∫Ω​aij∂i​u∂j​vdx+j∑​∫Ω​bj∂j​uvdx+∫Ω​cuvdx.

A function u:[0,T]→H01(Ω)u : [0,T] \to H^1_0(\Omega)u:[0,T]→H01​(Ω) has weak time derivative ut=wu_t = wut​=w if ∫0Tϕ′(t)u(t) dt=−∫0Tϕ(t)w(t) dt\int_0^T \phi'(t)u(t)\,dt = -\int_0^T\phi(t)w(t)\,dt∫0T​ϕ′(t)u(t)dt=−∫0T​ϕ(t)w(t)dt for all ϕ∈Cc∞(0,T)\phi \in C_c^\infty(0,T)ϕ∈Cc∞​(0,T), with Bochner integrals in H−1(Ω)H^{-1}(\Omega)H−1(Ω). Given f∈L2(0,T;H−1(Ω))f \in L^2(0,T;H^{-1}(\Omega))f∈L2(0,T;H−1(Ω)) and g∈L2(Ω)g \in L^2(\Omega)g∈L2(Ω), uuu is a weak solution of

ut+Lu=f in Ω×(0,T),u=0 on ∂Ω,u(0)=gu_t + Lu = f \ \text{in } \Omega\times(0,T), \qquad u = 0 \ \text{on } \partial\Omega, \qquad u(0) = gut​+Lu=f in Ω×(0,T),u=0 on ∂Ω,u(0)=g

when three conditions hold. First, u∈L2(0,T;H01)u \in L^2(0,T;H^1_0)u∈L2(0,T;H01​) and ut∈L2(0,T;H−1)u_t \in L^2(0,T;H^{-1})ut​∈L2(0,T;H−1). Second, ⟨ut(t),v⟩+a(u(t),v;t)=⟨f(t),v⟩\langle u_t(t), v\rangle + a(u(t), v; t) = \langle f(t), v\rangle⟨ut​(t),v⟩+a(u(t),v;t)=⟨f(t),v⟩ for every v∈H01(Ω)v \in H^1_0(\Omega)v∈H01​(Ω) and a.e. ttt. Third, u(0)=gu(0) = gu(0)=g, where the value at 000 is that of the continuous representative in C([0,T];L2(Ω))C([0,T];L^2(\Omega))C([0,T];L2(Ω)).

The Galerkin approximations use an L2L^2L2-orthonormal basis {wk}\{w_k\}{wk​} of Dirichlet eigenfunctions and the spaces EN=⟨w1,…,wN⟩E_N = \langle w_1, \dots, w_N\rangleEN​=⟨w1​,…,wN​⟩. The approximation uN:[0,T]→ENu_N : [0,T] \to E_NuN​:[0,T]→EN​ solves the projected equation (uNt,v)L2+a(uN,v;t)=⟨f,v⟩(u_{Nt}, v)_{L^2} + a(u_N, v; t) = \langle f, v\rangle(uNt​,v)L2​+a(uN​,v;t)=⟨f,v⟩ for v∈ENv \in E_Nv∈EN​, with uN(0)=PNgu_N(0) = P_N guN​(0)=PN​g.

A Hilbert triple V↪H↪V′\mathcal{V} \hookrightarrow \mathcal{H} \hookrightarrow \mathcal{V}'V↪H↪V′ consists of two separable Hilbert spaces V\mathcal{V}V, H\mathcal{H}H and the dual V′\mathcal{V}'V′, with dense continuous injective embeddings and ⟨f,v⟩=(f,v)H\langle f, v\rangle = (f, v)_{\mathcal{H}}⟨f,v⟩=(f,v)H​ for f∈Hf \in \mathcal{H}f∈H. The model is H01↪L2↪H−1H^1_0 \hookrightarrow L^2 \hookrightarrow H^{-1}H01​↪L2↪H−1.

Formalization targets

Goal: Theorem 6.3

For every f∈L2(0,T;H−1(Ω))f \in L^2(0,T;H^{-1}(\Omega))f∈L2(0,T;H−1(Ω)) and g∈L2(Ω)g \in L^2(\Omega)g∈L2(Ω) there is a unique weak solution u∈C([0,T];L2)∩L2(0,T;H01)u \in C([0,T];L^2) \cap L^2(0,T;H^1_0)u∈C([0,T];L2)∩L2(0,T;H01​) with ut∈L2(0,T;H−1)u_t \in L^2(0,T;H^{-1})ut​∈L2(0,T;H−1). There is also a constant C=C(Ω,T,L)C = C(\Omega, T, L)C=C(Ω,T,L) such that

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

Milestones

  • Theorem 6.41. If u∈L2(0,T;V)u \in L^2(0,T;\mathcal{V})u∈L2(0,T;V) and ut∈L2(0,T;V′)u_t \in L^2(0,T;\mathcal{V}')ut​∈L2(0,T;V′), then u∈C([0,T];H)u \in C([0,T];\mathcal{H})u∈C([0,T];H). Moreover ddt(u,v)H=⟨ut,v⟩\frac{d}{dt}(u,v)_{\mathcal{H}} = \langle u_t, v\rangledtd​(u,v)H​=⟨ut​,v⟩, ddt∥u∥H2=2⟨ut,u⟩\frac{d}{dt}\|u\|^2_{\mathcal{H}} = 2\langle u_t, u\rangledtd​∥u∥H2​=2⟨ut​,u⟩, and ∥u∥L∞(H)≤C(∥u∥L2(V)+∥ut∥L2(V′))\|u\|_{L^\infty(\mathcal{H})} \le C(\|u\|_{L^2(\mathcal{V})} + \|u_t\|_{L^2(\mathcal{V}')})∥u∥L∞(H)​≤C(∥u∥L2(V)​+∥ut​∥L2(V′)​).
  • Theorem 6.42. ∫0T⟨ut,v⟩ dt=(u(T),v(T))H−(u(0),v(0))H−∫0T⟨u,vt⟩ dt\int_0^T\langle u_t, v\rangle\,dt = (u(T),v(T))_{\mathcal{H}} - (u(0),v(0))_{\mathcal{H}} - \int_0^T\langle u, v_t\rangle\,dt∫0T​⟨ut​,v⟩dt=(u(T),v(T))H​−(u(0),v(0))H​−∫0T​⟨u,vt​⟩dt.
  • Proposition 6.5. Each Galerkin problem has a unique solution uNu_NuN​.
  • Proposition 6.6. The energy estimate above holds for uNu_NuN​ with CCC independent of NNN.
  • Proposition 6.7. A subsequence of uNu_NuN​ converges weakly to a weak solution satisfying the estimate.
  • Lemma 6.10 (Ehrling) and Theorem 6.9 (Aubin–Lions). These are further results of the chapter, stated for Banach spaces X↪Y↪ZX \hookrightarrow Y \hookrightarrow ZX↪Y↪Z with XXX compactly embedded in YYY.

Significance

Theorem 6.3 is the basic well-posedness theorem for linear parabolic equations with rough coefficients. It gives existence and uniqueness, and continuous dependence on the data through the linear estimate. The same argument gives the Galerkin convergence that justifies spectral and finite-element semi-discretizations. The Hilbert-triple calculus of Theorems 6.41–6.42 is the standard setting for linear and nonlinear evolution equations. The Aubin–Lions lemma is the compactness tool for nonlinear problems, such as the semilinear heat equation of §6.6 and the Navier–Stokes equations of §6.7.

All of these results are classical and proved in the notes, except that Theorem 6.41's proof leans on vector-valued mollification. As far as a search of the platform shows, none of them is formalized there. Mathlib has the Bochner integral, LpL^pLp spaces of Banach-valued functions and Gronwall's inequality. It does not have weak derivatives of vector-valued functions, Hilbert triples, or evolution-equation existence theorems. The work here is therefore to formalize known proofs, and in doing so to build reusable infrastructure for time-dependent PDEs.

Difficulty

The main obstacle is that the natural objects are equivalence classes of vector-valued functions, not functions. The initial condition u(0)=gu(0) = gu(0)=g is meaningless for an element of L2(0,T;H01)L^2(0,T;H^1_0)L2(0,T;H01​) until Theorem 6.41 provides a continuous representative. Its proof needs extension across the endpoints and mollification of V\mathcal{V}V-valued functions. Passing to the limit in the Galerkin scheme needs weak compactness in L2(0,T;H01)L^2(0,T;H^1_0)L2(0,T;H01​) and L2(0,T;H−1)L^2(0,T;H^{-1})L2(0,T;H−1), identified with a dual Bochner space. Proposition 6.5 is a linear ODE system whose coefficients are only L∞L^\inftyL∞ in time, so the Picard–Lindelöf theorem for continuous right-hand sides does not apply directly. The H−1H^{-1}H−1 bound on uNtu_{Nt}uNt​ needs the projection PNP_NPN​ to be bounded on H01H^1_0H01​ as well as on L2L^2L2, which is why the basis is taken to be eigenfunctions. Uniqueness needs the energy identity (6.46) and a Gronwall argument in weak form.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n), with 0-based coordinates. H10 n Ω is the closure of the jets (ϕ,∇ϕ)(\phi, \nabla\phi)(ϕ,∇ϕ), ϕ∈Cc∞(Ω)\phi \in C_c^\infty(\Omega)ϕ∈Cc∞​(Ω), in L2(Ω;R×Rn)L^2(\Omega;\mathbb{R}\times\mathbb{R}^n)L2(Ω;R×Rn), so its norm is the full H1H^1H1 norm. Hm1 n Ω is StrongDual ℝ (H10 n Ω). l2Embed is the embedding H01↪L2↪H−1H^1_0 \hookrightarrow L^2 \hookrightarrow H^{-1}H01​↪L2↪H−1.
  • Lp(0,T;X)L^p(0,T;X)Lp(0,T;X) is MemLp for Lebesgue measure on (0,T)(0,T)(0,T), and norms are eLpNorm with values in [0,∞][0,\infty][0,∞]. Constants are finite nonnegative reals. Every constant is quantified before the data it must not depend on: before fff, ggg in Theorem 6.3, and before the basis, fff, ggg, NNN in Propositions 6.6–6.7.
  • The weak time derivative is (6.14) in its standard form ∫ϕ′u=−∫ϕw\int\phi' u = -\int\phi w∫ϕ′u=−∫ϕw. The page prints ϕ\phiϕ and ϕ′\phi'ϕ′ interchanged, which is a typo.
  • Weak solutions take g∈L2(Ω)g \in L^2(\Omega)g∈L2(Ω) as in Assumption 6.1(3). The printed Theorem 6.3 says g∈H01(Ω)g \in H^1_0(\Omega)g∈H01​(Ω), a special case. u(0)=gu(0) = gu(0)=g is read through a continuous representative u~∈C([0,T];L2)\tilde u \in C([0,T];L^2)u~∈C([0,T];L2), and uniqueness means equality for a.e. ttt.
  • Coefficient conditions and ellipticity hold almost everywhere on Ω×(0,T)\Omega\times(0,T)Ω×(0,T). The Galerkin basis is a hypothesis: an orthonormal basis of L2(Ω)L^2(\Omega)L2(Ω) of weak Dirichlet eigenfunctions.
  • Proposition 6.7 states weak convergence of uNku_{N_k}uNk​​ in L2(0,T;H01)L^2(0,T;H^1_0)L2(0,T;H01​) and of uNktu_{N_k t}uNk​t​ in L2(0,T;H−1)L^2(0,T;H^{-1})L2(0,T;H−1), in the explicit integral form of p. 186. This is at least as strong as the printed claim.
  • Hilbert triples are structures with two continuous injective dense-range embeddings, separability, and the compatibility identity. Reflexivity in Theorem 6.9 is surjectivity of the canonical map into the bidual.
  • Ruling out trivializations. Every Bochner integral in a definition has an integrable integrand under the stated L2L^2L2 hypotheses, so no weak-derivative or weak-solution condition holds through the integral's junk value 000. The initial condition is imposed on a continuous representative, so it is not vacuous on a null set.
  • Reusable infrastructure welcome: vector-valued mollification and extension, the Hilbert-triple calculus, and dual identification of L2(0,T;X)′L^2(0,T;X)'L2(0,T;X)′.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, Chapter 6. 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, §7.1. https://doi.org/10.1090/gsm/019
  • J.-L. Lions and E. Magenes, Non-Homogeneous Boundary Value Problems and Applications I, Springer, 1972. https://doi.org/10.1007/978-3-642-65161-8
  • R. Temam, Navier–Stokes Equations: Theory and Numerical Analysis, North-Holland, 1977; AMS Chelsea reprint 2001. https://doi.org/10.1090/chel/343
  • J. Simon, Compact sets in the space Lp(0,T;B)L^p(0,T;B)Lp(0,T;B), Ann. Mat. Pura Appl. 146 (1987), 65–96. https://doi.org/10.1007/BF01762360
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Notes on Partial Differential Equations VIII: Strongly Continuous Semigroups and the Lumer–Phillips TheoremTextbook

Motivation

Many linear partial differential equations of evolution type — the heat equation, the Schrödinger equation, linear wave and Klein–Gordon equations, linearized reaction–diffusion and Kuramoto–Sivashinsky equations — can be written as an ordinary differential equation

ut=Au,u(0)=f,u_t = Au, \qquad u(0) = f,ut​=Au,u(0)=f,

in a Banach space XXX of functions, where AAA is a spatial differential operator. When AAA is bounded, the solution is the operator exponential etAfe^{tA}fetAf. Differential operators are unbounded, however, and then the solution operators f↦u(t)f \mapsto u(t)f↦u(t) are only continuous in time in the strong sense and may exist only forward in time. Semigroup theory makes this picture rigorous: it characterizes exactly which operators AAA generate a well-posed evolution, and it is the standard route from energy estimates to existence and uniqueness for linear and semilinear evolution equations (Duhamel's formula, §5.4.5 of the notes, used for the semilinear heat equation in §5.5).

This mission formalizes §5.4 of J. K. Hunter's Notes on Partial Differential Equations (UC Davis, revised 6/18/2014): uniformly continuous groups, strongly continuous semigroups and their generators, the Hille–Yosida theorem, the Lumer–Phillips theorem and Stone's theorem.

Timeline. The generation theorem for contraction semigroups is due independently to E. Hille (1948) and K. Yosida (1948); the general version with constants MMM, aaa to Feller, Miyadera and Phillips (1952–53). G. Lumer and R. S. Phillips (1961) recast the contraction case in terms of dissipative operators. Stone's theorem on one-parameter unitary groups dates from 1930–32. Standard modern accounts are Pazy (1983) and Engel–Nagel (2000).

Setting

Let XXX be a Banach space over K=R\mathbb{K} = \mathbb{R}K=R or C\mathbb{C}C, and L(X)\mathcal{L}(X)L(X) the Banach space of bounded linear operators on XXX with the operator norm.

A uniformly continuous group is a family {T(t):t∈R}⊂L(X)\{T(t) : t \in \mathbb{R}\} \subset \mathcal{L}(X){T(t):t∈R}⊂L(X) with T(0)=IT(0) = IT(0)=I, T(s)T(t)=T(s+t)T(s)T(t) = T(s+t)T(s)T(t)=T(s+t), and T(h)→IT(h) \to IT(h)→I in operator norm as h→0h \to 0h→0. A strongly continuous (C₀) semigroup is a family {T(t):t≥0}⊂L(X)\{T(t) : t \ge 0\} \subset \mathcal{L}(X){T(t):t≥0}⊂L(X) with T(0)=IT(0) = IT(0)=I, T(s)T(t)=T(s+t)T(s)T(t) = T(s+t)T(s)T(t)=T(s+t) for s,t≥0s, t \ge 0s,t≥0, and T(h)f→fT(h)f \to fT(h)f→f as h→0+h \to 0^+h→0+ for every f∈Xf \in Xf∈X; it is a contraction semigroup if ∥T(t)∥≤1\|T(t)\| \le 1∥T(t)∥≤1 for all t≥0t \ge 0t≥0. A C₀ group has the same properties for all s,t∈Rs, t \in \mathbb{R}s,t∈R; on a complex Hilbert space it is unitary if every T(t)T(t)T(t) is unitary.

An operator A:D(A)⊂X→XA : \mathcal{D}(A) \subset X \to XA:D(A)⊂X→X is a linear map defined on a subspace D(A)\mathcal{D}(A)D(A). The generator of a C₀ semigroup is the operator AAA whose domain is the set of fff for which

Af=lim⁡h→0+T(h)f−fhAf = \lim_{h \to 0^+} \frac{T(h)f - f}{h}Af=h→0+lim​hT(h)f−f​

exists in norm, with AfAfAf this limit. AAA is closed if its graph {(f,Af):f∈D(A)}\{(f, Af) : f \in \mathcal{D}(A)\}{(f,Af):f∈D(A)} is closed in X×XX \times XX×X, and densely defined if D(A)\mathcal{D}(A)D(A) is dense. A scalar λ\lambdaλ is in the resolvent set of AAA if λI−A:D(A)→X\lambda I - A : \mathcal{D}(A) \to XλI−A:D(A)→X is a bijection, and then R(λ,A)=(λI−A)−1R(\lambda, A) = (\lambda I - A)^{-1}R(λ,A)=(λI−A)−1 is the resolvent. AAA is dissipative if λ∥f∥≤∥(λI−A)f∥\lambda\|f\| \le \|(\lambda I - A)f\|λ∥f∥≤∥(λI−A)f∥ for all real λ>0\lambda > 0λ>0 and f∈D(A)f \in \mathcal{D}(A)f∈D(A), and m-dissipative if in addition λI−A\lambda I - AλI−A is onto XXX for some λ>0\lambda > 0λ>0. On a complex Hilbert space H\mathcal{H}H, AAA is self-adjoint if D(A)\mathcal{D}(A)D(A) is dense, D(A)=D(A∗)\mathcal{D}(A) = \mathcal{D}(A^*)D(A)=D(A∗), and (x,Ay)=(Ax,y)(x, Ay) = (Ax, y)(x,Ay)=(Ax,y) for x,y∈D(A)x, y \in \mathcal{D}(A)x,y∈D(A).

Formalization targets

Goal: the Lumer–Phillips theorem (Theorem 5.38)

For an operator A:D(A)⊂X→XA : \mathcal{D}(A) \subset X \to XA:D(A)⊂X→X,

A generates a C₀ contraction semigroup on X  ⟺  A is closed, densely defined and m-dissipative.A \text{ generates a C₀ contraction semigroup on } X \iff A \text{ is closed, densely defined and m-dissipative.}A generates a C₀ contraction semigroup on X⟺A is closed, densely defined and m-dissipative.

Milestones

  1. Theorem 5.24. A uniformly continuous group is smooth in operator norm, A=T′(0)∈L(X)A = T'(0) \in \mathcal{L}(X)A=T′(0)∈L(X) exists, and T(t)=etAT(t) = e^{tA}T(t)=etA for all t∈Rt \in \mathbb{R}t∈R.
  2. Theorem 5.32. The generator of a C₀ semigroup is closed and densely defined.
  3. Theorem 5.35 (Hille–Yosida). AAA generates a C₀ semigroup if and only if, for some M≥1M \ge 1M≥1 and a∈Ra \in \mathbb{R}a∈R, AAA is closed and densely defined, (a,∞)(a, \infty)(a,∞) lies in the resolvent set, and
∥R(λ,A)n∥≤M(λ−a)n(λ>a, n∈N);\|R(\lambda, A)^n\| \le \frac{M}{(\lambda - a)^n} \qquad (\lambda > a,\ n \in \mathbb{N});∥R(λ,A)n∥≤(λ−a)nM​(λ>a, n∈N);

in that case ∥T(t)∥≤Meat\|T(t)\| \le M e^{at}∥T(t)∥≤Meat for t≥0t \ge 0t≥0. 4. Corollary 5.36. The contraction case: M=1M = 1M=1, a=0a = 0a=0, with ∥R(λ,A)∥≤1/λ\|R(\lambda, A)\| \le 1/\lambda∥R(λ,A)∥≤1/λ. 5. Theorem 5.42 (Stone). On a complex Hilbert space, iAiAiA generates a C₀ unitary group if and only if AAA is self-adjoint.

Significance

The result itself. The Lumer–Phillips theorem is the working form of generation theory for PDEs: to show that ut=Auu_t = Auut​=Au is well posed with ∥u(t)∥≤∥u(0)∥\|u(t)\| \le \|u(0)\|∥u(t)∥≤∥u(0)∥, it suffices to prove an energy inequality (dissipativity) and to solve a single resolvent equation λf−Af=g\lambda f - Af = gλf−Af=g. The notes apply it to the Laplacian on H2(Rn)⊂L2(Rn)H^2(\mathbb{R}^n) \subset L^2(\mathbb{R}^n)H2(Rn)⊂L2(Rn) and, after a shift, to the linearized Kuramoto–Sivashinsky operator; later chapters use the resulting semigroups in Duhamel's formula to construct solutions of semilinear heat and Schrödinger equations. Hille–Yosida gives the general growth bound ∥T(t)∥≤Meat\|T(t)\| \le Me^{at}∥T(t)∥≤Meat, and Stone's theorem identifies unitary quantum dynamics with self-adjoint Hamiltonians.

Formalizing it. All results are classical and proved in the literature; the notes themselves state 5.32, 5.35, 5.36, 5.38 and 5.42 without proof, referring to standard texts. Mathlib currently has the operator exponential on Banach algebras, partially defined linear maps (LinearPMap) with closedness, closures and adjoints, but no theory of C₀ semigroups or their generators. A complete development would give Lean a reusable generation theory for unbounded operators, on which parabolic and dispersive PDE existence results can rest.

Difficulty

The central obstacle is the passage from resolvent information to a semigroup. Formally T(t)=etAT(t) = e^{tA}T(t)=etA, but for unbounded AAA the exponential series is meaningless, and the necessity directions require showing that the resolvent is a Laplace transform of the semigroup, which needs integration of strongly (not norm) continuous operator-valued functions. The sufficiency directions must construct a semigroup from AAA by an approximation of the unbounded generator and a limit that converges only strongly, and then identify the generator of the limit with AAA — including its domain, which is where most careless arguments fail. In the Lumer–Phillips theorem, surjectivity of λI−A\lambda I - AλI−A is assumed for a single λ>0\lambda > 0λ>0 and must be propagated to every λ>0\lambda > 0λ>0. In Stone's theorem both directions need domain arguments for unbounded operators on Hilbert space; symmetry of AAA alone is not enough.

Formalization scope

  • Scalars: a field 𝕜 with [RCLike 𝕜] (ℝ or ℂ), and X a Banach space over it ([NormedAddCommGroup X] [NormedSpace 𝕜 X] [CompleteSpace X]). Stone's theorem is over ℂ on an InnerProductSpace ℂ H with [CompleteSpace H]. Theorem 5.24 additionally equips X with a compatible real structure ([NormedSpace ℝ X] [IsScalarTower ℝ 𝕜 X]) so that t↦T(t)t \mapsto T(t)t↦T(t) can be differentiated; etAe^{tA}etA is Mathlib's NormedSpace.exp, and C∞C^\inftyC∞ is ContDiff ℝ ∞.
  • Operators A:D(A)⊂X→XA : \mathcal{D}(A) \subset X \to XA:D(A)⊂X→X are X →ₗ.[𝕜] X (LinearPMap); closedness is LinearPMap.IsClosed (closed graph).
  • Semigroups are functions T : ℝ → X →L[𝕜] X; for semigroups only the values at t≥0t \ge 0t≥0 enter. Composition is multiplication in X →L[𝕜] X.
  • The generator relation IsGenerator T A states, for all f,gf, gf,g: the right difference quotient h−1(T(h)f−f)h^{-1}(T(h)f - f)h−1(T(h)f−f) tends to ggg as h→0+h \to 0^+h→0+ if and only if f∈D(A)f \in \mathcal{D}(A)f∈D(A) and Af=gAf = gAf=g. So "AAA generates a semigroup" means that AAA equals the generator including its domain; a formalization in which AAA merely agrees with the limit on some subspace, or in which the generator is a restriction, would make the theorems different (and false) statements, and is ruled out.
  • Resolvent norm bounds ∥R(λ,A)n∥≤c\|R(\lambda, A)^n\| \le c∥R(λ,A)n∥≤c are stated pointwise, ∥R(λ,A)ng∥≤c∥g∥\|R(\lambda,A)^n g\| \le c\|g\|∥R(λ,A)ng∥≤c∥g∥ for all ggg, which is equivalent. In (5.24) n=0n = 0n=0 is included, which adds nothing because M≥1M \ge 1M≥1. The "in that case" clause of Theorem 5.35 is a second conjunct: for every semigroup generated by AAA and every M,aM, aM,a satisfying the three conditions, ∥T(t)∥≤Meat\|T(t)\| \le Me^{at}∥T(t)∥≤Meat.
  • Closedness and density, which the notes build into the definitions of the resolvent set and of dissipativity, are stated explicitly wherever they are used (they appear as condition (1) in every theorem).
  • The generator of a C₀ group (Stone) is the generator of its forward part, as in Definition 5.30; the operator iAiAiA is Complex.I • A, with the same domain as AAA. Self-adjointness is Definition 5.41 as printed, not Mathlib's IsSelfAdjoint for LinearPMap, although the two agree.
  • Useful infrastructure, reusable beyond this mission: Riemann/Bochner integration of strongly continuous operator families, the Laplace-transform representation of the resolvent, Yosida approximations, and dissipativity–resolvent equivalences. Contributions of any of these as separate lemmas are welcome.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, §5.4. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • A. Pazy, Semigroups of Linear Operators and Applications to Partial Differential Equations, Springer, 1983. https://doi.org/10.1007/978-1-4612-5561-1
  • K.-J. Engel and R. Nagel, One-Parameter Semigroups for Linear Evolution Equations, Springer GTM 194, 2000. https://doi.org/10.1007/b97696
  • G. Lumer and R. S. Phillips, Dissipative operators in a Banach space, Pacific J. Math. 11 (1961), 679–698. https://doi.org/10.2140/pjm.1961.11.679
  • M. H. Stone, On one-parameter unitary groups in Hilbert space, Ann. of Math. 33 (1932), 643–648. https://doi.org/10.2307/1968538
  • K. Yosida, On the differentiability and the representation of one-parameter semigroup of linear operators, J. Math. Soc. Japan 1 (1948), 15–21. https://doi.org/10.2969/jmsj/00110015
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Harmonic AnalysisPartial Differential Equations·Captain: mikedeng1

Notes on Partial Differential Equations II: The Newtonian Potential and Hölder Estimates for Poisson's EquationTextbook

Motivation

Poisson's equation −Δu=f-\Delta u = f−Δu=f is the model elliptic partial differential equation. It describes the electrostatic potential of a charge density, the gravitational potential of a mass density, and the steady temperature of a body with internal heat sources. Its solution on the whole space by convolution with a point-source potential, and the fact that this solution has exactly two more derivatives than the data when smoothness is measured in Hölder norms, are the starting point of the regularity theory of second-order elliptic equations.

This mission formalizes §2.6–2.7 of J. K. Hunter's Notes on Partial Differential Equations (UC Davis, revised 6/18/2014), which follow the classical line: the fundamental solution, the Newtonian potential, an integral representation of its second derivatives, and the Hölder estimate. The estimate goes back to J. Schauder (1934), who used it to build an existence theory for elliptic equations with Hölder continuous coefficients, now called Schauder theory (Gilbarg–Trudinger, Ch. 4 and 6). The singular integral operators that appear in the second derivatives were later placed in a general framework by A. P. Calderón and A. Zygmund (1952), whose theory gives the LpL^pLp analogue.

Setting

Throughout, n≥2n \ge 2n≥2 and Rn\mathbb{R}^nRn carries the Euclidean norm ∣x∣|x|∣x∣ and Lebesgue measure. Let αn\alpha_nαn​ be the volume of the open unit ball. The fundamental solution of Laplace's equation is

Γ(x)=1n(n−2)αn 1∣x∣n−2(n≥3),Γ(x)=−12πlog⁡∣x∣(n=2),\Gamma(x) = \frac{1}{n(n-2)\alpha_n}\,\frac{1}{|x|^{n-2}} \quad (n \ge 3), \qquad \Gamma(x) = -\frac{1}{2\pi}\log|x| \quad (n = 2),Γ(x)=n(n−2)αn​1​∣x∣n−21​(n≥3),Γ(x)=−2π1​log∣x∣(n=2),

defined for x≠0x \neq 0x=0. With this sign convention (as in Evans, opposite to Gilbarg–Trudinger) Γ\GammaΓ is harmonic away from the origin and −ΔΓ=δ-\Delta\Gamma = \delta−ΔΓ=δ in the sense of distributions. Γ\GammaΓ is locally integrable, and so is its gradient, but its second derivatives behave like ∣x∣−n|x|^{-n}∣x∣−n and are not.

For a smooth function fff with compact support, f∈Cc∞(Rn)f \in C_c^\infty(\mathbb{R}^n)f∈Cc∞​(Rn), the Newtonian potential of fff is the convolution

u(x)=(Γ∗f)(x)=∫RnΓ(x−y) f(y) dy.u(x) = (\Gamma * f)(x) = \int_{\mathbb{R}^n} \Gamma(x - y)\, f(y)\, dy.u(x)=(Γ∗f)(x)=∫Rn​Γ(x−y)f(y)dy.

Partial derivatives are written ∂i\partial_i∂i​, with ∂ij=∂i∂j\partial_{ij} = \partial_i \partial_j∂ij​=∂i​∂j​, and δij\delta_{ij}δij​ is the Kronecker delta. For 0<α≤10 < \alpha \le 10<α≤1 the Hölder seminorm of v:Rn→Rv : \mathbb{R}^n \to \mathbb{R}v:Rn→R is

[v]0,α=sup⁡x≠y∣v(x)−v(y)∣∣x−y∣α∈[0,∞].[v]_{0,\alpha} = \sup_{x \neq y} \frac{|v(x) - v(y)|}{|x - y|^{\alpha}} \in [0, \infty].[v]0,α​=x=ysup​∣x−y∣α∣v(x)−v(y)∣​∈[0,∞].

In the Lean development these objects are fundamentalSolution n, unitBallVolume n, newtonianPotential n f, partialDeriv u i, secondPartial u i j and holderSeminorm α Set.univ v, all in the namespace HunterPDE.Newtonian.

Formalization targets

Goal: the Hölder estimate (Theorem 2.28)

For 0<α<10 < \alpha < 10<α<1 there is a constant CCC, depending only on α\alphaα and nnn, such that for every f∈Cc∞(Rn)f \in C_c^\infty(\mathbb{R}^n)f∈Cc∞​(Rn) and all indices i,ji, ji,j,

[∂ij(Γ∗f)]0,α≤C [f]0,α.[\partial_{ij}(\Gamma * f)]_{0,\alpha} \le C\,[f]_{0,\alpha}.[∂ij​(Γ∗f)]0,α​≤C[f]0,α​.

The constant is not specified: the goal asserts the shape of the estimate, not a numerical value.

Milestones

  1. Eq. (2.14). Γ\GammaΓ is C∞C^\inftyC∞ on Rn∖{0}\mathbb{R}^n \setminus \{0\}Rn∖{0} and ∂iΓ(x)=−1nαn1∣x∣n−1xi∣x∣\partial_i\Gamma(x) = -\dfrac{1}{n\alpha_n}\dfrac{1}{|x|^{n-1}}\dfrac{x_i}{|x|}∂i​Γ(x)=−nαn​1​∣x∣n−11​∣x∣xi​​ for x≠0x \neq 0x=0.
  2. Eq. (2.23). Γ∗(Δf)=−f\Gamma * (\Delta f) = -fΓ∗(Δf)=−f for f∈Cc∞(Rn)f \in C_c^\infty(\mathbb{R}^n)f∈Cc∞​(Rn).
  3. Theorem 2.25. u=Γ∗fu = \Gamma * fu=Γ∗f is well defined, u∈C∞(Rn)u \in C^\infty(\mathbb{R}^n)u∈C∞(Rn), and −Δu=f-\Delta u = f−Δu=f.
  4. Corollary 2.27. For every xxx and every open ball BR(x)B_R(x)BR​(x) containing the support of fff,
∂iju(x)=∫BR(x)∂ijΓ(x−y) [f(y)−f(x)] dy−1nf(x) δij,\partial_{ij} u(x) = \int_{B_R(x)} \partial_{ij}\Gamma(x - y)\,[f(y) - f(x)]\,dy - \frac{1}{n} f(x)\,\delta_{ij},∂ij​u(x)=∫BR​(x)​∂ij​Γ(x−y)[f(y)−f(x)]dy−n1​f(x)δij​,

with the integral absolutely convergent.

Significance

Theorem 2.25 is the existence theorem for Poisson's equation on the whole space. Corollary 2.27 expresses D2uD^2 uD2u as a singular integral operator applied to fff plus a multiple of fff; it is the prototype of the representations behind both the Hölder (Schauder) and the LpL^pLp (Calderón–Zygmund) theories. Theorem 2.28 is the first Schauder estimate. With it, a priori estimates for equations with variable Hölder coefficients follow by freezing the coefficients, and existence follows by the method of continuity. The notes point out that the Hölder scale is essential: there are continuous compactly supported fff for which Γ∗f\Gamma * fΓ∗f is not C2C^2C2, so no estimate of D2uD^2 uD2u by the maximum of ∣f∣|f|∣f∣ holds. The endpoint α=1\alpha = 1α=1 is excluded from the theorem.

All four statements are classical and proved in the notes; none is new mathematics. As far as the Prove2Me corpus and Mathlib show, none has been machine-checked. Mathlib has the Laplacian on inner product spaces, convolution, and the volume of Euclidean balls, but no fundamental solution of the Laplacian in general dimension, no Newtonian potential, and no Hölder estimates for it. A formalization would supply reusable infrastructure: the fundamental solution with its derivative formulas, differentiation under the integral sign with a locally integrable kernel, and estimates for kernels homogeneous of degree −n-n−n with mean zero on spheres.

Difficulty

The obvious route to the second derivatives, differentiating twice under the integral sign, fails: ∂ijΓ\partial_{ij}\Gamma∂ij​Γ is of order ∣x∣−n|x|^{-n}∣x∣−n near the origin and is not locally integrable, so ∫∂ijΓ(x−y)f(y) dy\int \partial_{ij}\Gamma(x-y) f(y)\,dy∫∂ij​Γ(x−y)f(y)dy need not exist. Corollary 2.27 is precisely the statement that the correct formula carries a subtracted value f(x)f(x)f(x) and a boundary contribution −1nf(x)δij-\frac1n f(x)\delta_{ij}−n1​f(x)δij​, and computing that contribution needs integrals over spheres, which Mathlib supports only indirectly. For the goal, a pointwise bound on the kernel is not enough. Estimating ∣∂ijΓ(x−y)∣ ∣f(y)−f(x)∣|\partial_{ij}\Gamma(x-y)|\,|f(y)-f(x)|∣∂ij​Γ(x−y)∣∣f(y)−f(x)∣ in absolute value gives a bound that grows with the radius of the ball containing the support of fff, while the theorem's constant must be uniform over all fff, all indices and all pairs of points. The estimate depends on cancellation in the kernel, and the maximum-norm version of the same statement is false.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n) with volume. Every theorem assumes 2 ≤ n; the definition of Γ\GammaΓ returns junk values for n=0,1n = 0, 1n=0,1, which the book excludes.
  • Γ(0)\Gamma(0)Γ(0) is undefined in the book; in Lean it equals 000 (from 1/0=01/0 = 01/0=0 and log⁡0=0\log 0 = 0log0=0), one point of measure zero.
  • Coordinates are 0-based (i : Fin n). ∂iu(x)\partial_i u(x)∂i​u(x) is fderiv ℝ u x (EuclideanSpace.single i 1), and ∂iju=∂i(∂ju)\partial_{ij} u = \partial_i(\partial_j u)∂ij​u=∂i​(∂j​u). fderiv is 000 where uuu is not differentiable, so ∂ijΓ(x−y)\partial_{ij}\Gamma(x-y)∂ij​Γ(x−y) in Corollary 2.27 has an arbitrary value at the single point y=xy = xy=x.
  • "Smooth" is ContDiff ℝ ∞ (C∞C^\inftyC∞). In this Mathlib ContDiff ℝ ⊤ means analytic, and it is not used. Compact support is HasCompactSupport, and "the support of fff" is the closed support tsupport f.
  • Δ\DeltaΔ is Mathlib's InnerProductSpace.laplacian.
  • The convolution Γ∗f\Gamma * fΓ∗f is the Lebesgue integral ∫Γ(x−y)f(y) dy\int \Gamma(x-y) f(y)\,dy∫Γ(x−y)f(y)dy, with no integrability assumed of Γ\GammaΓ. Lean's Bochner integral is 000 for a non-integrable integrand, so Theorem 2.25 asserts integrability of y↦Γ(x−y)f(y)y \mapsto \Gamma(x-y)f(y)y↦Γ(x−y)f(y) for every xxx, and Corollary 2.27 asserts integrability of its integrand on the ball. Both are true and are implicit in the book's formulas; they rule out reading an identity between junk values as the theorem.
  • The Hölder seminorm is a supremum in [0,∞][0,\infty][0,∞] over all pairs of distinct points of Rn\mathbb{R}^nRn, not Mathlib's HolderWith, which fixes a constant. In the goal CCC is a finite nonnegative real quantified before fff, iii and jjj. The inequality therefore also asserts that ∂iju\partial_{ij} u∂ij​u is uniformly α\alphaα-Hölder, because [f]0,α<∞[f]_{0,\alpha} < \infty[f]0,α​<∞ for f∈Cc∞f \in C_c^\inftyf∈Cc∞​. A formalization that takes CCC after fff, lets it depend on the support of fff, or includes the excluded endpoint α=1\alpha = 1α=1 is not the theorem.
  • Theorem 2.26 of the notes (the same representation over an arbitrary smooth domain, with a surface integral over ∂Ω\partial\Omega∂Ω) is not stated, because a faithful statement needs a surface measure on general smooth boundaries. The singular-integral discussion of §2.8 is commentary and is not stated.

Useful infrastructure, all reusable beyond this mission: differentiation of Γ\GammaΓ away from the origin; integration in polar coordinates and integrals of ∣x∣−a|x|^{-a}∣x∣−a over balls and annuli; surface integrals over spheres, or the divergence theorem on balls; differentiation under the integral sign for convolutions with a locally integrable kernel. Contributions of any of these as separate lemmas are welcome.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, §2.6–2.8 and Definition 1.1. 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, §2.2. https://doi.org/10.1090/gsm/019
  • D. Gilbarg and N. S. Trudinger, Elliptic Partial Differential Equations of Second Order, Springer, 2001 (reprint of the 1998 ed.), Ch. 4. https://doi.org/10.1007/978-3-642-61798-0
  • J. Schauder, Über lineare elliptische Differentialgleichungen zweiter Ordnung, Mathematische Zeitschrift 38 (1934), 257–282. https://doi.org/10.1007/BF01170635
  • A. P. Calderón and A. Zygmund, On the existence of certain singular integrals, Acta Mathematica 88 (1952), 85–139. https://doi.org/10.1007/BF02392130
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Partial Differential Equations·Captain: mikedeng1

Notes on Partial Differential Equations I: Mean Values, Maximum Principles and Analyticity of Harmonic FunctionsTextbook

Motivation

Laplace's equation Δu=0\Delta u = 0Δu=0 is the prototype of an elliptic partial differential equation. Its solutions, the harmonic functions, describe equilibrium states in potential theory (gravitation, electrostatics, steady heat flow), are the real and imaginary parts of holomorphic functions in the plane, and are the stationary states of Brownian motion. Many qualitative properties of general elliptic equations — interior smoothing, maximum principles, Harnack-type inequalities — are first seen, and most cleanly proved, for the Laplacian.

This mission covers §2.1–2.3 of J. K. Hunter's Notes on Partial Differential Equations (UC Davis lecture notes, revised 6/18/2014, author's copy), which follow Evans, Partial Differential Equations, §2.2 (AMS GSM 19) and Gilbarg–Trudinger, Elliptic Partial Differential Equations of Second Order, Ch. 2 (Springer). The chain runs from the mean value property to interior derivative estimates with explicit constants and ends with the real-analyticity of harmonic functions in any dimension; the maximum principles and Liouville's theorem are consequences on the same definitions. The results are classical (Gauss, Liouville, Weyl, Harnack; nineteenth and early twentieth century) and are in every graduate PDE course.

Setting

Fix n∈Nn \in \mathbb{N}n∈N and write Rn\mathbb{R}^nRn for Euclidean space with Lebesgue measure. For x∈Rnx \in \mathbb{R}^nx∈Rn and r>0r > 0r>0, Br(x)={y:∣y−x∣<r}B_r(x) = \{y : |y - x| < r\}Br​(x)={y:∣y−x∣<r} is the open ball and ∂Br(x)={y:∣y−x∣=r}\partial B_r(x) = \{y : |y - x| = r\}∂Br​(x)={y:∣y−x∣=r} the sphere. For an open set Ω⊆Rn\Omega \subseteq \mathbb{R}^nΩ⊆Rn write Br(x)⋐ΩB_r(x) \Subset \OmegaBr​(x)⋐Ω when the closed ball B‾r(x)\overline{B}_r(x)Br​(x) is contained in Ω\OmegaΩ.

The Laplacian of a twice differentiable u:Ω→Ru : \Omega \to \mathbb{R}u:Ω→R is Δu=∑i=1n∂i2u\Delta u = \sum_{i=1}^n \partial_i^2 uΔu=∑i=1n​∂i2​u. A function u∈C2(Ω)u \in C^2(\Omega)u∈C2(Ω) is harmonic in Ω\OmegaΩ if Δu=0\Delta u = 0Δu=0 there, subharmonic if Δu≥0\Delta u \ge 0Δu≥0 and superharmonic if Δu≤0\Delta u \le 0Δu≤0 (Definition 2.4).

The averages of uuu over a ball and a sphere are

⨍Br(x)u dx=1αnrn∫Br(x)u dx,⨍∂Br(x)u dS=1nαnrn−1∫∂Br(x)u dS,⨍_{B_r(x)} u\,dx = \frac{1}{\alpha_n r^n}\int_{B_r(x)} u\,dx, \qquad ⨍_{\partial B_r(x)} u\,dS = \frac{1}{n\alpha_n r^{n-1}}\int_{\partial B_r(x)} u\,dS,⨍Br​(x)​udx=αn​rn1​∫Br​(x)​udx,⨍∂Br​(x)​udS=nαn​rn−11​∫∂Br​(x)​udS,

where αn\alpha_nαn​ is the volume of the unit ball and dSdSdS is surface measure. A continuous uuu has the mean-value property (2.3) in Ω\OmegaΩ if u(x)u(x)u(x) equals both averages whenever Br(x)⋐ΩB_r(x) \Subset \OmegaBr​(x)⋐Ω.

For a multi-index α=(α1,…,αn)∈N0n\alpha = (\alpha_1, \dots, \alpha_n) \in \mathbb{N}_0^nα=(α1​,…,αn​)∈N0n​ of order ∣α∣=α1+⋯+αn|\alpha| = \alpha_1 + \cdots + \alpha_n∣α∣=α1​+⋯+αn​, ∂αu\partial^\alpha u∂αu differentiates uuu αi\alpha_iαi​ times in the iii-th coordinate. A function is real-analytic in Ω\OmegaΩ if near every point of Ω\OmegaΩ it equals the sum of a convergent power series.

Formalization targets

Goal: analyticity (Theorem 2.10)

If u∈C2(Ω)u \in C^2(\Omega)u∈C2(Ω) is harmonic in an open set Ω⊆Rn\Omega \subseteq \mathbb{R}^nΩ⊆Rn, then uuu is real-analytic in Ω\OmegaΩ.

Milestones

  • Theorem 2.1 (mean value property): if uuu is harmonic and Br(x)⋐ΩB_r(x) \Subset \OmegaBr​(x)⋐Ω, then u(x)=⨍Br(x)u dx=⨍∂Br(x)u dSu(x) = ⨍_{B_r(x)} u\,dx = ⨍_{\partial B_r(x)} u\,dSu(x)=⨍Br​(x)​udx=⨍∂Br​(x)​udS.
  • Theorem 2.2 (converse): a continuous function with the mean-value property is C∞C^\inftyC∞ and harmonic.
  • Theorem 2.7: ∣∂iu(x)∣≤nrmax⁡B‾r(x)∣u∣|\partial_i u(x)| \le \dfrac{n}{r}\max_{\overline{B}_r(x)}|u|∣∂i​u(x)∣≤rn​maxBr​(x)​∣u∣ for harmonic uuu and Br(x)⋐ΩB_r(x) \Subset \OmegaBr​(x)⋐Ω.
  • Theorem 2.9: for ∣α∣=k≥1|\alpha| = k \ge 1∣α∣=k≥1,
∣∂αu(x)∣≤nkek−1k!rkmax⁡B‾r(x)∣u∣.|\partial^\alpha u(x)| \le \frac{n^k e^{k-1} k!}{r^k}\max_{\overline{B}_r(x)}|u|.∣∂αu(x)∣≤rknkek−1k!​Br​(x)max​∣u∣.
  • Corollary 2.8 (Liouville): a bounded harmonic function on Rn\mathbb{R}^nRn is constant.
  • Theorem 2.5: u(x)≤u(x) \leu(x)≤ both averages for subharmonic uuu, ≥\ge≥ for superharmonic uuu.
  • Theorem 2.13 (strong maximum principle): a subharmonic function on a connected open set that attains a global maximum is constant.
  • Theorem 2.17 (weak maximum principle): on a bounded connected open set, a harmonic u∈C2(Ω)∩C(Ω‾)u \in C^2(\Omega) \cap C(\overline{\Omega})u∈C2(Ω)∩C(Ω) satisfies max⁡Ω‾u=max⁡∂Ωu\max_{\overline{\Omega}} u = \max_{\partial\Omega} umaxΩ​u=max∂Ω​u and min⁡Ω‾u=min⁡∂Ωu\min_{\overline{\Omega}} u = \min_{\partial\Omega} uminΩ​u=min∂Ω​u.

Theorems 2.1, 2.2, 2.7 and 2.9 lie on the path to the goal; the others are further results on the same definitions.

Significance

The result. Analyticity means that a harmonic function is determined on a connected domain by its germ at one point (Corollary 2.11). It is the model case of analytic hypoellipticity for elliptic operators with analytic coefficients. The derivative estimates of Theorem 2.9, with a constant growing like k!k!k!, are the quantitative content: they are Cauchy-type estimates in several real variables and underlie compactness of families of harmonic functions and interior regularity arguments. The maximum principles give uniqueness for the Dirichlet problem (Theorem 2.18), and Liouville's theorem in Rn\mathbb{R}^nRn is the classification of bounded entire harmonic functions.

Formalizing it. Mathlib defines the Laplacian and harmonicity on inner product spaces and proves that harmonic functions on C\mathbb{C}C are real parts of holomorphic functions, hence analytic; the Prove2Me corpus contains the mean value property and Liouville's theorem for functions on C\mathbb{C}C (two dimensions, circle averages). Nothing in Mathlib or on the platform covers harmonic functions on Rn\mathbb{R}^nRn for general nnn: no mean value property over balls and spheres in Rn\mathbb{R}^nRn, no derivative estimates, no maximum principle, no analyticity. All statements here are proved results; the work is formalizing the known proofs.

Difficulty

The two-dimensional route through holomorphic functions does not exist for n≥3n \ge 3n≥3: there is no complex structure to borrow, so analyticity must come from the real-variable estimates of Theorem 2.9 and a remainder estimate for the multivariable Taylor expansion. Those estimates need the mean value property on balls and spheres of Rn\mathbb{R}^nRn, which requires surface measure on spheres, polar coordinates and the divergence theorem on a ball — tools that Mathlib has only in part. Theorem 2.9 asks for the constant nkek−1k!/rkn^k e^{k-1}k!/r^knkek−1k!/rk exactly, not merely some constant: the kkk-dependence is the whole point, since a bound that grows faster than k!k!k! times a geometric factor does not make the Taylor series converge. The converse Theorem 2.2 needs mollification. The weak maximum principle needs that the boundary of a bounded nonempty open set in Rn\mathbb{R}^nRn is nonempty and that the closure is compact.

Formalization scope

  • Rn\mathbb{R}^nRn is EuclideanSpace ℝ (Fin n) with Lebesgue measure volume; an open set is Ω : Set (EuclideanSpace ℝ (Fin n)) with IsOpen Ω. Functions are u : EuclideanSpace ℝ (Fin n) → ℝ of which only the values on Ω\OmegaΩ (or Ω‾\overline{\Omega}Ω) matter.
  • "u∈C2(Ω)u \in C^2(\Omega)u∈C2(Ω) harmonic in Ω\OmegaΩ" is Mathlib's InnerProductSpace.HarmonicOnNhd u Ω; Δ\DeltaΔ is Mathlib's laplacian; C∞C^\inftyC∞ is ContDiffOn ℝ ∞ (smooth, not analytic); real-analytic in Ω\OmegaΩ is AnalyticOnNhd ℝ u Ω.
  • Br(x)⋐ΩB_r(x) \Subset \OmegaBr​(x)⋐Ω is 0 < r ∧ Metric.closedBall x r ⊆ Ω, never the open ball. The ball average is Mathlib's set average over Metric.ball x r; the sphere average is defined in polar form over the unit sphere with Mathlib's surface measure volume.toSphere. The mean-value property requires both identities of (2.3).
  • Coordinates are 0-based (i : Fin n); ∂iu(x)\partial_i u(x)∂i​u(x) is the Fréchet derivative applied to the iii-th basis vector, and ∂α\partial^\alpha∂α applies these repeatedly, αi\alpha_iαi​ times in coordinate iii.
  • max⁡B‾r(x)∣u∣\max_{\overline{B}_r(x)}|u|maxBr​(x)​∣u∣ in Theorems 2.7 and 2.9 is expressed by an arbitrary bound MMM of ∣u∣|u|∣u∣ on the closed ball; since the maximum is attained, this is equivalent. In Theorem 2.17 each equality of maxima is stated as attainment of the maximum over Ω‾\overline{\Omega}Ω at a point of ∂Ω\partial\Omega∂Ω.
  • Theorem 2.9 is stated for k=∣α∣≥1k = |\alpha| \ge 1k=∣α∣≥1: at k=0k = 0k=0 the printed bound reads ∣u(x)∣≤e−1max⁡∣u∣|u(x)| \le e^{-1}\max|u|∣u(x)∣≤e−1max∣u∣, which fails for constants. The hypothesis n≥1n \ge 1n≥1 is added where the statement mentions a sphere (Theorems 2.1, 2.5) or a boundary (Theorem 2.17), which are empty in R0\mathbb{R}^0R0.
  • A trivializing reading is excluded: the balls are closed balls of positive radius inside Ω\OmegaΩ, the averages are normalized integrals of continuous functions over sets of positive finite measure, and analyticity is required at every point of Ω\OmegaΩ rather than on one ball.

Needed infrastructure, reusable well beyond this mission: surface measure and polar coordinates on spheres of Rn\mathbb{R}^nRn, the divergence theorem on balls, mollification of continuous functions, and multivariable Taylor expansion with remainder in multi-index form. Contributions of any of these as separate lemmas are welcome.

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, Chapter 2. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • L. C. Evans, Partial Differential Equations, 2nd ed., AMS Graduate Studies in Mathematics 19, 2010, §2.2. https://doi.org/10.1090/gsm/019
  • D. Gilbarg and N. S. Trudinger, Elliptic Partial Differential Equations of Second Order, Springer Classics in Mathematics, 2001, Chapter 2. https://doi.org/10.1007/978-3-642-61798-0
  • Q. Han and F. Lin, Elliptic Partial Differential Equations, 2nd ed., Courant Lecture Notes 1, AMS, 2011. https://doi.org/10.1090/cln/001
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Generalized Gradients and Applications I: The Generalized Gradient of a Max FunctionResearch Paper

Motivation

Many objective functions in optimization are pointwise maxima: the worst case of a loss over an uncertainty set, the value of a minimax problem as a function of the outer variable, a penalty max⁡igi(x)\max_i g_i(x)maxi​gi​(x) for a system of constraints, or the largest eigenvalue of a symmetric matrix. Such a function

f(x)=max⁡{g(x,u):u∈U}f(x)=\max\{g(x,u):u\in U\}f(x)=max{g(x,u):u∈U}

is typically not differentiable even when every piece g(⋅,u)g(\cdot,u)g(⋅,u) is smooth, because the maximizing uuu jumps. Descent methods, optimality conditions and sensitivity analysis for these problems all need a substitute for the gradient of fff and a formula for its directional derivatives.

Danskin's theorem (Danskin 1966) answers this when ∇xg(x,u)\nabla_x g(x,u)∇x​g(x,u) exists and is continuous in (x,u)(x,u)(x,u) and UUU is compact: fff has one-sided directional derivatives f′(x;v)=max⁡{∇xg(x,u)⋅v:u∈M(x)}f'(x;v)=\max\{\nabla_x g(x,u)\cdot v:u\in M(x)\}f′(x;v)=max{∇x​g(x,u)⋅v:u∈M(x)}, where M(x)M(x)M(x) is the set of maximizers. Convex analysis gives the analogue when each g(⋅,u)g(\cdot,u)g(⋅,u) is convex (Rockafellar 1970). In Generalized gradients and applications (Clarke 1975) Frank Clarke introduced the generalized gradient of a locally Lipschitz function and proved, as his first application, a single theorem, Theorem (2.1), that contains both cases. The generalized gradient became the standard object of nonsmooth analysis (Clarke 1983), and Theorem (2.1) is the prototype of every "subdifferential of a max function" rule used in minimax optimization.

Setting

Work in Rn\mathbb R^nRn with the Euclidean norm ∣⋅∣|\cdot|∣⋅∣ and inner product ζ⋅v\zeta\cdot vζ⋅v. A function f:Rn→Rf:\mathbb R^n\to\mathbb Rf:Rn→R is locally Lipschitz if for every bounded set BBB there is KKK with ∣f(x1)−f(x2)∣≤K∣x1−x2∣|f(x_1)-f(x_2)|\le K|x_1-x_2|∣f(x1​)−f(x2​)∣≤K∣x1​−x2​∣ for x1,x2∈Bx_1,x_2\in Bx1​,x2​∈B. By Rademacher's theorem such fff is differentiable almost everywhere.

  • The generalized gradient ∂f(x)\partial f(x)∂f(x) (Definition (1.1)) is the convex hull of all limits lim⁡i∇f(x+hi)\lim_i\nabla f(x+h_i)limi​∇f(x+hi​), where hi→0h_i\to0hi​→0, fff is differentiable at each x+hix+h_ix+hi​, and the gradients converge.
  • The generalized directional derivative (Definition (1.3)) is
f∘(x;v)=lim sup⁡h→0, δ↓0f(x+h+δv)−f(x+h)δ,f^\circ(x;v)=\limsup_{h\to0,\ \delta\downarrow0}\frac{f(x+h+\delta v)-f(x+h)}{\delta},f∘(x;v)=h→0, δ↓0limsup​δf(x+h+δv)−f(x+h)​,

and the one-sided directional derivative is f′(x;v)=lim⁡δ↓0[f(x+δv)−f(x)]/δf'(x;v)=\lim_{\delta\downarrow0}[f(x+\delta v)-f(x)]/\deltaf′(x;v)=limδ↓0​[f(x+δv)−f(x)]/δ when the limit exists.

  • A multifunction Φ\PhiΦ into subsets of Rn\mathbb R^nRn is upper semicontinuous if xi→xx_i\to xxi​→x, vi→vv_i\to vvi​→v and vi∈Φ(xi)v_i\in\Phi(x_i)vi​∈Φ(xi​) imply v∈Φ(x)v\in\Phi(x)v∈Φ(x).

For the max function, UUU is a nonempty sequentially compact topological space and g:Rn×U→Rg:\mathbb R^n\times U\to\mathbb Rg:Rn×U→R. Write ∂xg(x,u)\partial_xg(x,u)∂x​g(x,u), gx∘(x,u;v)g^\circ_x(x,u;v)gx∘​(x,u;v), gx′(x,u;v)g'_x(x,u;v)gx′​(x,u;v) for the objects above applied to y↦g(y,u)y\mapsto g(y,u)y↦g(y,u) at xxx. Let f(x)=max⁡u∈Ug(x,u)f(x)=\max_{u\in U}g(x,u)f(x)=maxu∈U​g(x,u) and M(x)={u∈U:g(x,u)=f(x)}M(x)=\{u\in U:g(x,u)=f(x)\}M(x)={u∈U:g(x,u)=f(x)}. The hypotheses of Theorem (2.1) are:

  • (a) ggg is upper semicontinuous in (x,u)(x,u)(x,u);
  • (b) ggg is locally Lipschitz in xxx uniformly in uuu: for each bounded BBB one constant KKK serves for every u∈Uu\in Uu∈U;
  • (c) for all x,u,vx,u,vx,u,v, gx′(x,u;v)g'_x(x,u;v)gx′​(x,u;v) exists and equals gx∘(x,u;v)g^\circ_x(x,u;v)gx∘​(x,u;v);
  • (d) (x,u)↦∂xg(x,u)(x,u)\mapsto\partial_xg(x,u)(x,u)↦∂x​g(x,u) is upper semicontinuous on Rn×U\mathbb R^n\times URn×U.

Formalization targets

Goal: Theorem (2.1)

Under (a)–(d):

  1. fff is locally Lipschitz;
  2. f′(x;v)f'(x;v)f′(x;v) exists for all x,vx,vx,v;
  3. f′(x;v)=f∘(x;v)=max⁡{ζ⋅v:ζ∈∂xg(x,u), u∈M(x)}f'(x;v)=f^\circ(x;v)=\max\{\zeta\cdot v:\zeta\in\partial_xg(x,u),\ u\in M(x)\}f′(x;v)=f∘(x;v)=max{ζ⋅v:ζ∈∂x​g(x,u), u∈M(x)};
  4. for every xxx,
∂f(x)=co⁡{∂xg(x,u):u∈M(x)}.\partial f(x)=\operatorname{co}\{\partial_xg(x,u):u\in M(x)\}.∂f(x)=co{∂x​g(x,u):u∈M(x)}.

Milestones

  • Proposition (1.4): f∘(x;v)=max⁡{ζ⋅v:ζ∈∂f(x)}f^\circ(x;v)=\max\{\zeta\cdot v:\zeta\in\partial f(x)\}f∘(x;v)=max{ζ⋅v:ζ∈∂f(x)} for locally Lipschitz fff.
  • Corollary (1.10): if ζ⋅v≤lim sup⁡δ↓0[f(x+δv)−f(x)]/δ\zeta\cdot v\le\limsup_{\delta\downarrow0}[f(x+\delta v)-f(x)]/\deltaζ⋅v≤limsupδ↓0​[f(x+δv)−f(x)]/δ for all vvv, then ζ∈∂f(x)\zeta\in\partial f(x)ζ∈∂f(x).
  • Theorem (2.1)(1): under (a), (b), fff is locally Lipschitz.
  • (2.2): co⁡{∂xg(x,u):u∈M(x)}⊆∂f(x)\operatorname{co}\{\partial_xg(x,u):u\in M(x)\}\subseteq\partial f(x)co{∂x​g(x,u):u∈M(x)}⊆∂f(x).
  • (2.3): if fff is differentiable at xˉ\bar xxˉ and u∈M(xˉ)u\in M(\bar x)u∈M(xˉ), then ∂xg(xˉ,u)={∇f(xˉ)}\partial_xg(\bar x,u)=\{\nabla f(\bar x)\}∂x​g(xˉ,u)={∇f(xˉ)}.
  • Theorem (2.1)(4): the equality above.

Significance

The result. Theorem (2.1) computes the directional derivatives and the generalized gradient of a max function from those of its active pieces. It yields Danskin's theorem when ∇xg\nabla_xg∇x​g is continuous, and the convex max rule when each g(⋅,u)g(\cdot,u)g(⋅,u) is convex, and it applies to nonsmooth, nonconvex families satisfying (c), a property later called regularity (Clarke 1983, §2.3). In the same paper it is applied to the distance function dE(x)=min⁡e∈E∣x−e∣d_E(x)=\min_{e\in E}|x-e|dE​(x)=mine∈E​∣x−e∣ to compute ∂dE\partial d_E∂dE​ (Proposition (2.4), Corollary (2.5)), which then drives the characterization of flow-invariant sets in §4. Proposition (1.4) and Corollary (1.10), which the theorem rests on, are the duality between ∂f\partial f∂f and f∘f^\circf∘ used throughout nonsmooth optimization: Clarke stationarity, bundle methods and subgradient methods for weakly convex functions all state their results against them.

Formalizing it. The results are classical and proved; none of them, to the platform's knowledge, has a machine-checked proof. Mathlib has Rademacher's theorem, gradients and convex hulls, but no Clarke generalized gradient. This mission builds the first layer of nonsmooth analysis: the definitions of ∂f\partial f∂f, f∘f^\circf∘, f′f'f′ and upper semicontinuity of multifunctions, the support-function duality, and the max rule.

Difficulty

The obvious approach reads ∂f(x)\partial f(x)∂f(x) off a single active piece. It fails because the active set M(x+h)M(x+h)M(x+h) changes as h→0h\to0h→0, may be infinite, and need not converge; fff can be differentiable at points where no individual piece is known to be. Hypothesis (c) cannot be dropped: for UUU a single point and g(x,u)=−∣x∣g(x,u)=-|x|g(x,u)=−∣x∣ on R\mathbb RR, f=gf=gf=g has f′(0;v)=−∣v∣f'(0;v)=-|v|f′(0;v)=−∣v∣ while f∘(0;v)=∣v∣f^\circ(0;v)=|v|f∘(0;v)=∣v∣, so conclusion (3) fails. Limits of maximizers exist only through the sequential compactness of UUU together with (a), and limits of gradients only through the joint closed-graph condition (d) in (x,u)(x,u)(x,u); continuity in xxx for each fixed uuu is not enough. Proposition (1.4), on which everything rests, is itself a measure-theoretic statement: it relates the upper limit of difference quotients over all nearby base points to gradients that exist only almost everywhere.

Formalization scope

  • Rn\mathbb R^nRn is EuclideanSpace ℝ (Fin n), ζ⋅v\zeta\cdot vζ⋅v is inner ℝ ζ v, ∇f\nabla f∇f is Mathlib's gradient, and "∇f(x)\nabla f(x)∇f(x) exists" is DifferentiableAt ℝ f x.
  • "Locally Lipschitz" is the paper's bounded-set form, LipschitzOnBounded. Hypothesis (b) is ∀ B bounded, ∃ K, ∀ u, LipschitzOnWith K (g · u) B: the constant is uniform in uuu.
  • ∂f(x)\partial f(x)∂f(x) is the plain convex hull (no closure) of limits of gradients taken only at differentiability points; without that restriction 000 would belong to every ∂f(x)\partial f(x)∂f(x), because gradient is 000 where fff is not differentiable.
  • f∘f^\circf∘ is Filter.limsup in R\mathbb RR along N(0)×N>(0)\mathcal N(0)\times\mathcal N_{>}(0)N(0)×N>​(0); this is a junk value for non-Lipschitz fff, so every statement using f∘f^\circf∘ assumes the Lipschitz hypothesis. The one-sided derivative is a Tendsto along N>(0)\mathcal N_{>}(0)N>​(0).
  • "max" in conclusions is IsGreatest, which asserts attainment. The max function is ⨆ u, g x u; UUU is nonempty ([Nonempty U]) and SeqCompactSpace, and (a) is Mathlib's UpperSemicontinuous on Rn×U\mathbb R^n\times URn×U. The paper uses U≠∅U\ne\emptysetU=∅ implicitly; with U=∅U=\emptysetU=∅ conclusion (4) would be false.
  • (d) is the sequential closed-graph property in (x,u)(x,u)(x,u) jointly, not Mathlib's UpperHemicontinuous.
  • A formalization in which ∂f\partial f∂f contains junk gradients, f∘f^\circf∘ is a limsup without the Lipschitz hypothesis, or "max" is sSup without attainment would make the statements trivial or false; these are ruled out as above.

Contributions welcome: proofs of the milestones, in particular Proposition (1.4) and Corollary (1.10), which are reusable for every later nonsmooth-analysis mission; lemmas that ∂f(x)\partial f(x)∂f(x) is nonempty and compact; the equivalence of LipschitzOnBounded with Mathlib's LocallyLipschitz.

Selected references

  • F. H. Clarke, Generalized gradients and applications, Trans. Amer. Math. Soc. 205 (1975), 247–262. https://doi.org/10.1090/s0002-9947-1975-0367131-6
  • J. M. Danskin, The theory of max-min, with applications, SIAM J. Appl. Math. 14 (1966), 641–664. https://doi.org/10.1137/0114053
  • R. T. Rockafellar, Convex Analysis, Princeton University Press, 1970. https://doi.org/10.1515/9781400873173
  • F. H. Clarke, Optimization and Nonsmooth Analysis, Wiley, 1983; SIAM Classics reprint 1990. https://doi.org/10.1137/1.9781611971309
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Analysis of Generalized Pattern Searches: Nonnegative Clarke Derivatives at Limits of Refining SubsequencesResearch Paper

Motivation

Generalized pattern search (GPS) is a class of derivative-free methods for minimizing a function that can only be evaluated, not differentiated. Such objectives arise in engineering design, where one evaluation is an expensive simulation that may fail and return no value at all. The helicopter rotor design problem of Booker et al. is one example: no value was returned for roughly 66% of the trial points (Booker et al., 1999). A method for such problems has to tolerate objectives that are discontinuous or take the value +∞+\infty+∞.

Earlier convergence theory for GPS assumed continuous differentiability of the objective on a neighbourhood of the level set. Torczon established it for unconstrained problems (SIAM J. Optim. 7, 1997), and Lewis and Torczon extended it to bound constraints (1999) and to finitely many linear constraints (SIAM J. Optim. 10, 2000). Audet and Dennis (SIAM J. Optim. 13, 2003) replaced these analyses with a single argument. Its conclusions are local and are graded by the smoothness of the objective at the limit point only, through Clarke's generalized directional derivative. That paper is the source of this mission. Its analysis is the basis of the later mesh adaptive direct search (MADS) theory (Audet, Dennis, SIAM J. Optim. 17, 2006).

Setting

The problem is

min⁡x∈Ωf(x),f:Rn→R∪{+∞},Ω={x∈Rn:ℓ≤Ax≤u},\min_{x\in\Omega} f(x),\qquad f:\mathbb R^n\to\mathbb R\cup\{+\infty\},\qquad \Omega=\{x\in\mathbb R^n:\ell\le Ax\le u\},x∈Ωmin​f(x),f:Rn→R∪{+∞},Ω={x∈Rn:ℓ≤Ax≤u},

with A∈Rm×nA\in\mathbb R^{m\times n}A∈Rm×n and ℓ≤u\ell\le uℓ≤u in (R∪{±∞})m(\mathbb R\cup\{\pm\infty\})^m(R∪{±∞})m. The algorithm works with the barrier function fΩf_\OmegafΩ​, equal to fff on Ω\OmegaΩ and to +∞+\infty+∞ elsewhere.

The algorithm uses a finite set of directions D=GZˉD=G\bar ZD=GZˉ, the columns dj=Gzˉjd_j=G\bar z_jdj​=Gzˉj​ of the product of a nonsingular G∈Rn×nG\in\mathbb R^{n\times n}G∈Rn×n and an integer matrix Zˉ∈Zn×p\bar Z\in\mathbb Z^{n\times p}Zˉ∈Zn×p. The directions form a positive spanning set: their nonnegative combinations give all of Rn\mathbb R^nRn. At iteration kkk, with iterate xkx_kxk​ and mesh size parameter Δk>0\Delta_k>0Δk​>0, the mesh is Mk={xk+ΔkDz:z∈Z+p}M_k=\{x_k+\Delta_k Dz: z\in\mathbb Z_+^{p}\}Mk​={xk​+Δk​Dz:z∈Z+p​}. A poll set {xk+Δkd:d∈Dk}\{x_k+\Delta_k d: d\in D_k\}{xk​+Δk​d:d∈Dk​} is drawn from a positive spanning subset Dk⊆DD_k\subseteq DDk​⊆D. Each iteration ends in one of two ways:

  1. Improved mesh point. Some xk+1∈Mk∩Ωx_{k+1}\in M_k\cap\Omegaxk+1​∈Mk​∩Ω with fΩ(xk+1)<fΩ(xk)f_\Omega(x_{k+1})<f_\Omega(x_k)fΩ​(xk+1​)<fΩ​(xk​) was found, by the free SEARCH step or by the poll. Then Δk+1=τwkΔk\Delta_{k+1}=\tau^{w_k}\Delta_kΔk+1​=τwk​Δk​ with 0≤wk≤w+0\le w_k\le w^+0≤wk​≤w+.
  2. Mesh local optimizer. fΩ(xk)≤fΩ(xk+Δkd)f_\Omega(x_k)\le f_\Omega(x_k+\Delta_k d)fΩ​(xk​)≤fΩ​(xk​+Δk​d) for every d∈Dkd\in D_kd∈Dk​. Then xk+1=xkx_{k+1}=x_kxk+1​=xk​ and Δk+1=τwkΔk\Delta_{k+1}=\tau^{w_k}\Delta_kΔk+1​=τwk​Δk​ with w−≤wk≤−1w^-\le w_k\le-1w−≤wk​≤−1.

Here τ>1\tau>1τ>1 is rational and w−≤−1≤0≤w+w^-\le-1\le 0\le w^+w−≤−1≤0≤w+ are integers. The assumptions are A1 fΩ(x0)<∞f_\Omega(x_0)<\inftyfΩ​(x0​)<∞, A2 AAA is rational, and A3 all iterates lie in a compact set. A refining subsequence is an infinite set of mesh local optimizers {xk}k∈K\{x_k\}_{k\in K}{xk​}k∈K​ along which Δk→0\Delta_k\to 0Δk​→0 (Definition 3.5). For fff Lipschitz near x^\hat xx^, Clarke's derivative is

f∘(x^;d)=lim sup⁡y→x^, t↓0f(y+td)−f(y)t.f^\circ(\hat x;d)=\limsup_{y\to\hat x,\ t\downarrow 0}\frac{f(y+td)-f(y)}{t}.f∘(x^;d)=y→x^, t↓0limsup​tf(y+td)−f(y)​.

Formalization targets

Goal: Theorem 3.7

Assume A1–A3. Let x^\hat xx^ be the limit of a refining subsequence, and let d∈Dd\in Dd∈D be a direction polled at a feasible point xk+Δkdx_k+\Delta_k dxk​+Δk​d for infinitely many kkk in the subsequence. If fff is Lipschitz near x^\hat xx^, then

f∘(x^;d) ≥ 0.f^\circ(\hat x;d)\ \ge\ 0 .f∘(x^;d) ≥ 0.

Milestones on the way

  • Theorem 3.1: the iterates have a limit point, lim⁡kf(xk)\lim_k f(x_k)limk​f(xk​) exists and dominates fff at lower semicontinuity limit points, and all continuity limit points share one value.
  • Lemma 3.2: min⁡u≠v∈Mk∥u−v∥≥Δk/∥G−1∥\min_{u\ne v\in M_k}\|u-v\|\ge\Delta_k/\|G^{-1}\|minu=v∈Mk​​∥u−v∥≥Δk​/∥G−1∥ for every norm giving nonzero integer vectors norm at least 111.
  • Lemma 3.3: Δk≤Δ0τr+\Delta_k\le\Delta_0\tau^{r^+}Δk​≤Δ0​τr+ for some positive integer r+r^+r+.
  • Proposition 3.4: lim inf⁡k→∞Δk=0\liminf_{k\to\infty}\Delta_k=0liminfk→∞​Δk​=0.
  • Theorem 3.6: a convergent refining subsequence exists.

Corollaries

  • Theorem 3.9: if Ω=Rn\Omega=\mathbb R^nΩ=Rn and fff is strictly differentiable at x^\hat xx^, then ∇f(x^)=0\nabla f(\hat x)=0∇f(x^)=0.
  • Theorem 3.14: if the poll sets conform to the boundary of Ω\OmegaΩ (Definition 3.13) and fff is strictly differentiable at x^\hat xx^, then ∇f(x^)Tw≥0\nabla f(\hat x)^Tw\ge 0∇f(x^)Tw≥0 on the tangent cone TΩ(x^)T_\Omega(\hat x)TΩ​(x^) and −∇f(x^)∈NΩ(x^)-\nabla f(\hat x)\in N_\Omega(\hat x)−∇f(x^)∈NΩ​(x^). So x^\hat xx^ is a KKT point.

Significance

Theorem 3.7 gives a first-order conclusion at a limit point from a local hypothesis at that point alone. It does not require smoothness elsewhere, finiteness of fff elsewhere, or continuity. It turns the heuristic "the method stopped improving on ever finer meshes" into a statement about generalized derivatives. The unconstrained stationarity result (Theorem 3.9) and the linearly constrained KKT result (Theorem 3.14) follow from it, and they recover the Torczon and Lewis–Torczon theorems under weaker smoothness assumptions. The chain Lemma 3.2 → Lemma 3.3 → Proposition 3.4 → Theorem 3.6 shows that the goal's hypothesis is always met. Every run satisfying A1 and A3 has a refining subsequence, which rests on the rationality of τ\tauτ and on the integer structure of DDD.

All results in this mission are proved in the source paper. None of them has, to the best of our knowledge, a machine-checked proof. The mission contributes a formal model of the GPS algorithm class as a class of runs, a formal Clarke directional derivative, and checked proofs of the mesh-refinement chain and the main theorem.

Difficulty

Given a refining subsequence, the goal is a comparison of limsups: the poll inequalities give nonnegative difference quotients at the points (xk,Δk)(x_k,\Delta_k)(xk​,Δk​), which converge to (x^,0+)(\hat x,0^+)(x^,0+). The difficulty lies in two places. First, the objective is extended-valued, and the barrier hides fff at infeasible poll points, where the poll inequality fΩ(xk)≤+∞f_\Omega(x_k)\le+\inftyfΩ​(xk​)≤+∞ says nothing. The hypothesis on ddd has to supply feasibility, and the Lipschitz hypothesis has to supply finiteness near x^\hat xx^. Second, the existence of refining subsequences is not a compactness argument alone. Coarsening is allowed, so Δk\Delta_kΔk​ need not decrease, and with an irrational τ\tauτ or a direction set that is not an integer lattice image (for instance D=[−1,+π]D=[-1,+\pi]D=[−1,+π] in R\mathbb RR) the meshes can be dense and lim inf⁡Δk\liminf\Delta_kliminfΔk​ can be positive. The lattice argument behind Proposition 3.4 is where the integrality hypotheses are used.

Formalization scope

Points of Rn\mathbb R^nRn are Fin n → ℝ, fff takes values in WithTop ℝ, and the bounds ℓ,u\ell,uℓ,u are EReal-valued, so m=0m=0m=0 gives Ω=Rn\Omega=\mathbb R^nΩ=Rn. The barrier is defined by cases, never by extended addition. Directions are the columns of G * Zbar indexed by Fin p, and DkD_kDk​ is a Finset (Fin p). A GPS run is a structure of sequences xk,Δk,Dk,wkx_k,\Delta_k,D_k,w_kxk​,Δk​,Dk​,wk​ and a per-iteration predicate "mesh local optimizer", subject to exactly the two update rules above, Δ0>0\Delta_0>0Δ0​>0, rational τ>1\tau>1τ>1 and the exponent bounds. The SEARCH step, the choice of DkD_kDk​ and the exponents are left free, since the paper allows any strategy. A subsequence is a strictly increasing map K:N→NK:\mathbb N\to\mathbb NK:N→N. The Clarke derivative of a real function is an EReal-valued limit superior along y→x^y\to\hat xy→x^, t→0+t\to 0^+t→0+. "fff Lipschitz near x^\hat xx^" means that fff agrees near x^\hat xx^ with a real function Lipschitz there, and the conclusions are stated for every such function. Strict differentiability is the directional notion of Section 3.4 of the paper.

The goal is not trivialized by an empty run class: Theorem 3.6, on the same class, asserts that refining subsequences exist. The mesh-local-optimizer branch requires the complete poll inequality over DkD_kDk​. The Clarke limit superior cannot take a default value. The direction ddd must be polled at feasible points infinitely often, which is the paper's "fff was evaluated".

Contributions welcome: proofs of any milestone, and reusable lemmas on positive spanning sets, lattice points in compact sets, and the Clarke derivative (for instance, that it equals ∇f(x^)Td\nabla f(\hat x)^Td∇f(x^)Td under strict differentiability).

Selected references

  • C. Audet, J. E. Dennis Jr., Analysis of Generalized Pattern Searches, SIAM J. Optim. 13(3):889–903, 2003. https://doi.org/10.1137/S1052623400378742
  • V. Torczon, On the Convergence of Pattern Search Algorithms, SIAM J. Optim. 7(1):1–25, 1997. https://doi.org/10.1137/S1052623493250780
  • R. M. Lewis, V. Torczon, Pattern Search Methods for Linearly Constrained Minimization, SIAM J. Optim. 10(3):917–941, 2000. https://doi.org/10.1137/S1052623497331373
  • F. H. Clarke, Optimization and Nonsmooth Analysis, Wiley, 1983; reprinted SIAM Classics in Applied Mathematics 5, 1990. https://doi.org/10.1137/1.9781611971309
  • A. J. Booker, J. E. Dennis Jr., P. D. Frank, D. B. Serafini, V. Torczon, M. W. Trosset, A rigorous framework for optimization of expensive functions by surrogates, Structural Optimization 17:1–13, 1999. https://doi.org/10.1007/BF01197559
  • C. Audet, J. E. Dennis Jr., Mesh Adaptive Direct Search Algorithms for Constrained Optimization, SIAM J. Optim. 17(1):188–217, 2006. https://doi.org/10.1137/040603371
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Numerical AnalysisOperations ResearchOptimization·Captain: mikedeng1

A Nonsmooth Version of Newton's Method I: local superlinear convergence of the generalized-Jacobian Newton method at a semismooth regular rootResearch Paper

Motivation

Many problems in optimization and equilibrium modelling reduce to a system of equations F(x)=0F(x) = 0F(x)=0 whose map F:Rn→RnF : \mathbb R^n \to \mathbb R^nF:Rn→Rn is Lipschitz but not differentiable: reformulations of nonlinear complementarity problems through the componentwise minimum or the Fischer–Burmeister function, Karush–Kuhn–Tucker systems of constrained programs, and gradients of augmented Lagrangians all have kinks. Newton's method, xk+1=xk−F′(xk)−1F(xk)x^{k+1} = x^k - F'(x^k)^{-1}F(x^k)xk+1=xk−F′(xk)−1F(xk), is the standard fast local solver for smooth systems, but it needs a derivative at every iterate.

Qi and Sun (Math. Programming 58, 1993) replaced the Jacobian by an arbitrary element of Clarke's generalized Jacobian and showed that the resulting method converges locally superlinearly under a regularity condition they called semismoothness, extending Mifflin's notion for functionals (Mifflin, SIAM J. Control Optim. 15, 1977) to vector-valued maps. This theorem is the foundation of the family of semismooth Newton methods used in complementarity, variational inequalities and PDE-constrained optimization.

Timeline. Robinson (1988) and Pang (Math. OR 15, 1990) studied Newton methods built on B-derivatives, with convergence proved under a strong Fréchet derivative at the solution; Kummer (1988) gave an abstract framework for Newton methods for nonsmooth equations; Qi and Sun (1993) proved local superlinear convergence for the generalized-Jacobian iteration under semismoothness and nonsingularity of ∂F(x∗)\partial F(x^*)∂F(x∗), with order 1+p1+p1+p under ppp-order semismoothness.

Setting

Let F:Rn→RmF : \mathbb R^n \to \mathbb R^mF:Rn→Rm be locally Lipschitz. By Rademacher's theorem FFF is differentiable on a set DFD_FDF​ of full measure; write JF(y)JF(y)JF(y) for the Jacobian at y∈DFy \in D_Fy∈DF​. The generalized Jacobian is

∂F(x)=co{lim⁡i→∞JF(xi):xi→x, xi∈DF},\partial F(x) = \mathrm{co}\Big\{\lim_{i\to\infty} JF(x_i) : x_i \to x,\ x_i \in D_F\Big\},∂F(x)=co{i→∞lim​JF(xi​):xi​→x, xi​∈DF​},

the convex hull of all limits of Jacobians along sequences of differentiability points converging to xxx. The one-sided directional derivative is F′(x;h)=lim⁡t↓0(F(x+th)−F(x))/tF'(x;h) = \lim_{t\downarrow 0}(F(x+th)-F(x))/tF′(x;h)=limt↓0​(F(x+th)−F(x))/t.

FFF is semismooth at xxx if it is Lipschitz near xxx and, for every hhh, the limit of Vh′Vh'Vh′ over V∈∂F(x+th′)V \in \partial F(x+th')V∈∂F(x+th′), h′→hh' \to hh′→h, t↓0t \downarrow 0t↓0 exists. For 0<p≤10 < p \le 10<p≤1, FFF is ppp-order semismooth at xxx if in addition Vh−F′(x;h)=O(∥h∥1+p)Vh - F'(x;h) = O(\|h\|^{1+p})Vh−F′(x;h)=O(∥h∥1+p) for V∈∂F(x+h)V \in \partial F(x+h)V∈∂F(x+h), h→0h \to 0h→0.

For m=nm = nm=n, the nonsmooth Newton method is

xk+1=xk−Vk−1F(xk),Vk∈∂F(xk),(3.2)x^{k+1} = x^k - V_k^{-1}F(x^k), \qquad V_k \in \partial F(x^k), \tag{3.2}xk+1=xk−Vk−1​F(xk),Vk​∈∂F(xk),(3.2)

where any element of ∂F(xk)\partial F(x^k)∂F(xk) may be chosen at each step. A run is a pair of sequences (xk)(x^k)(xk), (Vk)(V_k)(Vk​) with Vk∈∂F(xk)V_k \in \partial F(x^k)Vk​∈∂F(xk) and Vk(xk+1−xk)=−F(xk)V_k(x^{k+1}-x^k) = -F(x^k)Vk​(xk+1−xk)=−F(xk) for all kkk. A root x∗x^*x∗ (F(x∗)=0F(x^*) = 0F(x∗)=0) is regular when every V∈∂F(x∗)V \in \partial F(x^*)V∈∂F(x∗) is nonsingular.

Formalization targets

Goal: Theorem 3.2, local superlinear convergence

Let FFF be locally Lipschitz, F(x∗)=0F(x^*) = 0F(x∗)=0, FFF semismooth at x∗x^*x∗, and every V∈∂F(x∗)V \in \partial F(x^*)V∈∂F(x∗) nonsingular. Then there is δ>0\delta > 0δ>0 such that every V∈∂F(y)V \in \partial F(y)V∈∂F(y) with ∥y−x∗∥<δ\|y - x^*\| < \delta∥y−x∗∥<δ is nonsingular, a Newton step from such a yyy stays within δ\deltaδ of x∗x^*x∗, and every run with ∥x0−x∗∥<δ\|x^0 - x^*\| < \delta∥x0−x∗∥<δ satisfies

xk→x∗,∥xk+1−x∗∥=o(∥xk−x∗∥).x^k \to x^*, \qquad \|x^{k+1} - x^*\| = o(\|x^k - x^*\|).xk→x∗,∥xk+1−x∗∥=o(∥xk−x∗∥).

The goal asserts only the shape of the convergence (superlinear) and fixes no constants.

Stronger: Theorem 3.2, order 1+p1 + p1+p

If moreover FFF is ppp-order semismooth at x∗x^*x∗, 0<p≤10 < p \le 10<p≤1, there are δ>0\delta > 0δ>0 and CCC with

∥xk+1−x∗∥≤C∥xk−x∗∥1+p\|x^{k+1} - x^*\| \le C\|x^k - x^*\|^{1+p}∥xk+1−x∗∥≤C∥xk−x∗∥1+p

for every run started within δ\deltaδ of x∗x^*x∗.

Milestones

The milestones follow the paper's route: Proposition 2.1 (the limit in the definition of semismoothness is the directional derivative), Lemma 2.2 (Lipschitz continuity of F′(x;⋅)F'(x;\cdot)F′(x;⋅) and its realisation by an element of ∂F(x)\partial F(x)∂F(x)), Theorem 2.3 (semismoothness is equivalent to Vh−F′(x;h)=o(∥h∥)Vh - F'(x;h) = o(\|h\|)Vh−F′(x;h)=o(∥h∥) and to the corresponding condition at differentiability points), the Remark's expansion (2.17), Proposition 3.1 (uniform invertibility near a regular point), the order-(1+p)(1+p)(1+p) sentence of Theorem 3.2, and Corollary 2.5 (strong Fréchet differentiability implies semismoothness).

Significance

The theorem gives a locally superlinearly convergent method for Lipschitz equations with no smoothness beyond semismoothness at the root. Convex, smooth and subsmooth functions are semismooth, as are sums and scalar products of semismooth functions (the paper, citing Mifflin), and later work showed that the complementarity and KKT reformulations on which semismooth Newton solvers are built are semismooth as well; the order-(1+p)(1+p)(1+p) variant gives local quadratic convergence for strongly semismooth maps. Mission II of this series treats the paper's global convergence theorem on a ball, and Mission III the semismoothness of augmented Lagrangian gradients, which supplies the application.

The results are proved in the paper. No machine-checked version of the generalized Jacobian, of semismoothness or of the nonsmooth Newton method is known to exist in Mathlib or on this platform; the platform's formalized Newton results concern one-dimensional C2C^2C2 functions (MetodosNumericos.newton_local_convergence) and smooth convex minimization. A complete development would provide the first formal library for Clarke's generalized Jacobian and semismooth maps.

Difficulty

The classical Newton proof compares F(xk)F(x^k)F(xk) with its linearization JF(x∗)(xk−x∗)JF(x^*)(x^k - x^*)JF(x∗)(xk−x∗) and uses continuity of the Jacobian at x∗x^*x∗. Here neither is available: FFF need not be differentiable at x∗x^*x∗ or at any iterate, the element VkV_kVk​ is chosen arbitrarily from a set, and VkV_kVk​ need not be close to any fixed linear map. The comparison has to go through the directional derivative F′(x∗;⋅)F'(x^*; \cdot)F′(x∗;⋅), which is only positively homogeneous, not linear. The analytic content therefore sits in Section 2: showing that semismoothness, defined through a limit over a set-valued map, controls Vh−F′(x;h)Vh - F'(x;h)Vh−F′(x;h) uniformly in the direction, and that F(x+h)−F(x)−F′(x;h)F(x+h) - F(x) - F'(x;h)F(x+h)−F(x)−F′(x;h) is small. Both rest on Clarke's mean-value inclusion and on compactness and upper semicontinuity of ∂F\partial F∂F, none of which is in Mathlib. The superlinear rate also requires a uniform bound on ∥V−1∥\|V^{-1}\|∥V−1∥ in a whole neighbourhood, not just at x∗x^*x∗.

Formalization scope

Everything lives in the namespace NonsmoothNewton.Local. Section 2 results are stated for maps between finite-dimensional real normed spaces E→GE \to GE→G (the paper's Rn→Rm\mathbb R^n \to \mathbb R^mRn→Rm is the Euclidean instance); Section 3 results use EuclideanSpace ℝ (Fin n). Conventions fixed by the Lean statements:

  • JFJFJF is fderiv; the generalized Jacobian is the convex hull (no closure) of limits of fderiv along sequences xi→xx_i \to xxi​→x of differentiability points.
  • F′(x;h)F'(x;h)F′(x;h) is the one-sided limit over t↓0t \downarrow 0t↓0, never the two-sided lineDeriv; its value is a limUnder, used only where existence is a hypothesis or a consequence.
  • Nonsingular means IsUnit in the ring of continuous linear endomorphisms; ∥V−1∥≤C\|V^{-1}\| \le C∥V−1∥≤C is a two-sided inverse of operator norm at most CCC.
  • A run of (3.2) is encoded by the linear equation Vk(xk+1−xk)=−F(xk)V_k(x^{k+1} - x^k) = -F(x^k)Vk​(xk+1−xk)=−F(xk) with Vk∈∂F(xk)V_k \in \partial F(x^k)Vk​∈∂F(xk); all choices of VkV_kVk​ are quantified, and δ\deltaδ is chosen before the run.
  • Pinned asymptotics. The goal's rate is the proof's display (3.3), stated as IsLittleO along atTop; the printed Theorem 3.2 states only well-definedness and convergence. "Order 1+p1+p1+p" is pinned as ∥xk+1−x∗∥≤C∥xk−x∗∥1+p\|x^{k+1}-x^*\| \le C\|x^k-x^*\|^{1+p}∥xk+1−x∗∥≤C∥xk−x∗∥1+p with δ\deltaδ and CCC uniform over runs. Every o(∥h∥)o(\|h\|)o(∥h∥) in (2.8), (2.9) and (2.17) is its ε\varepsilonε–δ\deltaδ form with a non-strict inequality ≤ε∥h∥\le \varepsilon\|h\|≤ε∥h∥, and every O(∥h∥1+p)O(\|h\|^{1+p})O(∥h∥1+p) is an explicit constant and radius.
  • The standing assumptions "FFF locally Lipschitzian" of Sections 2 and 3 are hypotheses of every statement.
  • The strong Fréchet derivative of Corollary 2.5 is Mathlib's HasStrictFDerivAt, which corrects the misprint F(x)F(x)F(x) for F(z)F(z)F(z) in the paper's display (2.16).

A trivializing formalization is ruled out: the update is not written with a junk inverse (which would make a singular step "well defined"), the generalized Jacobian is the paper's nonempty set rather than one that could be empty, and the theorem quantifies over every run rather than asserting that some run converges.

A complete development needs Clarke's mean-value inclusion (2.2), compactness and upper semicontinuity of ∂F\partial F∂F for locally Lipschitz maps (via Rademacher's theorem, available in Mathlib), and perturbation bounds for inverses of linear maps. The generalized-Jacobian and semismoothness layer is reusable beyond this mission, in particular for Missions II and III of this series. Contributions of proofs of any milestone, and of general lemmas about ∂F\partial F∂F, are welcome.

Selected references

  • L. Qi, J. Sun, A nonsmooth version of Newton's method, Mathematical Programming 58 (1993) 353–367. https://doi.org/10.1007/BF01581275
  • F. H. Clarke, Optimization and Nonsmooth Analysis, Wiley, 1983 (SIAM reprint 1990). https://doi.org/10.1137/1.9781611971309
  • R. Mifflin, Semismooth and semiconvex functions in constrained optimization, SIAM Journal on Control and Optimization 15 (1977) 959–972. https://doi.org/10.1137/0315061
  • J.-S. Pang, Newton's method for B-differentiable equations, Mathematics of Operations Research 15 (1990) 311–341. https://doi.org/10.1287/moor.15.2.311
  • J. M. Ortega, W. C. Rheinboldt, Iterative Solution of Nonlinear Equations in Several Variables, Academic Press, 1970 (SIAM reprint 2000). https://doi.org/10.1137/1.9780898719468
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Mathematical PhysicsNumber Theory·Captain: Lucas

String Theory (Tong) III: Modular Invariance of the One-Loop Partition FunctionTextbook

Motivation

At one loop, the worldsheet of a closed string is a torus, and the one-loop vacuum amplitude of the bosonic string is an integral over all conformally inequivalent tori. Two tori with modular parameters τ\tauτ and τ′\tau'τ′ are equivalent exactly when τ′=(aτ+b)/(cτ+d)\tau'=(a\tau+b)/(c\tau+d)τ′=(aτ+b)/(cτ+d) for an integer matrix of determinant one, so a consistent string amplitude must be built from SL(2,Z)SL(2,\mathbb Z)SL(2,Z)-invariant data. In David Tong's Cambridge Part III lecture notes (Section 6.4), the partition function of the bosonic string is computed in lightcone gauge and written in terms of the Dedekind eta function; the notes then observe that the measure and the integrand are individually modular invariant. This invariance is the mechanism by which string theory avoids the ultraviolet divergences of point-particle loops: the integration region is a fundamental domain that never reaches Im⁡τ→0\operatorname{Im}\tau\to0Imτ→0 (Polchinski 1986).

Setting

Write H={τ∈C:Im⁡τ>0}\mathbb H=\{\tau\in\mathbb C:\operatorname{Im}\tau>0\}H={τ∈C:Imτ>0}. A modular transformation is the map

τ⟼γτ=aτ+bcτ+d,a,b,c,d∈Z,ad−bc=1,(6.19)\tau\longmapsto \gamma\tau=\frac{a\tau+b}{c\tau+d},\qquad a,b,c,d\in\mathbb Z,\quad ad-bc=1, \qquad (6.19)τ⟼γτ=cτ+daτ+b​,a,b,c,d∈Z,ad−bc=1,(6.19)

generated by T:τ↦τ+1T:\tau\mapsto\tau+1T:τ↦τ+1 and S:τ↦−1/τS:\tau\mapsto-1/\tauS:τ↦−1/τ. With q=e2πiτq=e^{2\pi i\tau}q=e2πiτ the Dedekind eta function is

η(τ)=q1/24∏n=1∞(1−qn)=e2πiτ/24∏n=1∞(1−e2πinτ),\eta(\tau)=q^{1/24}\prod_{n=1}^\infty(1-q^n)=e^{2\pi i\tau/24}\prod_{n=1}^\infty\bigl(1-e^{2\pi i n\tau}\bigr),η(τ)=q1/24n=1∏∞​(1−qn)=e2πiτ/24n=1∏∞​(1−e2πinτ),

convergent and non-vanishing on H\mathbb HH. The partition function of a single free scalar field on the torus is, up to constant factors, (6.20)

Zscalar(τ)=1Im⁡τ 1∣η(τ)∣2,Z_{\text{scalar}}(\tau)=\frac{1}{\sqrt{\operatorname{Im}\tau}}\,\frac{1}{|\eta(\tau)|^{2}},Zscalar​(τ)=Imτ​1​∣η(τ)∣21​,

and the bosonic string partition function is

Zstring=∫Fd2τ(Im⁡τ)2  F(τ),F(τ)=(1Im⁡τ1η(τ) η(τ)‾)24=1(Im⁡τ)12 ∣η(τ)∣48,Z_{\text{string}}=\int_{\mathcal F}\frac{d^2\tau}{(\operatorname{Im}\tau)^2}\;F(\tau),\qquad F(\tau)=\left(\frac{1}{\sqrt{\operatorname{Im}\tau}}\frac{1}{\eta(\tau)\,\overline{\eta(\tau)}}\right)^{24}=\frac{1}{(\operatorname{Im}\tau)^{12}\,|\eta(\tau)|^{48}},Zstring​=∫F​(Imτ)2d2τ​F(τ),F(τ)=(Imτ​1​η(τ)η(τ)​1​)24=(Imτ)12∣η(τ)∣481​,

where F={∣τ∣≥1, ∣Re⁡τ∣≤12}\mathcal F=\{|\tau|\ge1,\ |\operatorname{Re}\tau|\le\tfrac12\}F={∣τ∣≥1, ∣Reτ∣≤21​} is the standard fundamental domain.

Formalization targets

Goal: the string integrand is modular invariant

For every τ∈H\tau\in\mathbb Hτ∈H and all a,b,c,d∈Za,b,c,d\in\mathbb Za,b,c,d∈Z with ad−bc=1ad-bc=1ad−bc=1,

F ⁣(aτ+bcτ+d)=F(τ).F\!\left(\frac{a\tau+b}{c\tau+d}\right)=F(\tau).F(cτ+daτ+b​)=F(τ).

Milestones (Section 6.4, in the order of the notes)

  1. SSS and TTT generate SL(2,Z)SL(2,\mathbb Z)SL(2,Z).
  2. Every τ∈H\tau\in\mathbb Hτ∈H is mapped into F\mathcal FF by some modular transformation.
  3. Im⁡(γτ)=Im⁡τ/∣cτ+d∣2\operatorname{Im}(\gamma\tau)=\operatorname{Im}\tau/|c\tau+d|^2Im(γτ)=Imτ/∣cτ+d∣2 and d(γτ)/dτ=1/(cτ+d)2d(\gamma\tau)/d\tau=1/(c\tau+d)^2d(γτ)/dτ=1/(cτ+d)2 (so d2τ↦d2τ/∣cτ+d∣4d^2\tau\mapsto d^2\tau/|c\tau+d|^4d2τ↦d2τ/∣cτ+d∣4).
  4. The measure d2τ/(Im⁡τ)2d^2\tau/(\operatorname{Im}\tau)^2d2τ/(Imτ)2 on H\mathbb HH is SL(2,Z)SL(2,\mathbb Z)SL(2,Z)-invariant.
  5. η(τ+1)=e2πi/24η(τ)\eta(\tau+1)=e^{2\pi i/24}\eta(\tau)η(τ+1)=e2πi/24η(τ).
  6. η(−1/τ)=−iτ η(τ)\eta(-1/\tau)=\sqrt{-i\tau}\,\eta(\tau)η(−1/τ)=−iτ​η(τ).
  7. ZscalarZ_{\text{scalar}}Zscalar​ is modular invariant.

Significance

The result. Modular invariance of the integrand is what makes the one-loop string amplitude well defined as an integral over the moduli space of tori, rather than over the whole upper half-plane: restricting to F\mathcal FF is only consistent because nothing depends on the representative. It is the first instance of a consistency condition that, in the superstring, constrains the allowed gauge groups and spectra.

Formalizing it. The eta transformation laws are classical (Apostol 1990, Ch. 3); Mathlib contains the definition of the eta function and results on SL(2,Z)SL(2,\mathbb Z)SL(2,Z) and its fundamental domain, but, to the mission author's knowledge, not the SSS-transformation law of η\etaη. The mission produces a self-contained formal statement of the physics claim "both the measure and the integrand are individually modular invariant" and asks for its proof; milestones 1–2 are expected to follow from existing Mathlib results, milestone 6 is the analytic core.

Difficulty

The TTT-law is immediate from the product. The SSS-law η(−1/τ)=−iτ η(τ)\eta(-1/\tau)=\sqrt{-i\tau}\,\eta(\tau)η(−1/τ)=−iτ​η(τ) is not visible from the product formula at all: it requires either Poisson summation / the Jacobi triple product for theta functions, or a Mellin-transform / Eisenstein-series argument (log⁡η\log\etalogη is an Eichler integral of E2E_2E2​), together with care about the branch of the square root. Passing from generators to all of SL(2,Z)SL(2,\mathbb Z)SL(2,Z) requires an induction on words in SSS and TTT in which the multiplier ∣cτ+d∣|c\tau+d|∣cτ+d∣ must be tracked.

Formalization scope

Points of H\mathbb HH are represented as complex numbers τ\tauτ with the hypothesis 0<Im⁡τ0<\operatorname{Im}\tau0<Imτ; a modular transformation is given by four integers with ad−bc=1ad-bc=1ad−bc=1 and acts by TongString.modularAction a b c d τ = (aτ+b)/(cτ+d). The eta function is defined directly by Tong's product formula as TongString.dedekindEta, using Mathlib's unconditional infinite product tprod. The square root in the SSS-law is the principal branch, (−iτ)1/2(-i\tau)^{1/2}(−iτ)1/2, which is the one intended since Re⁡(−iτ)>0\operatorname{Re}(-i\tau)>0Re(−iτ)>0. The invariant measure is formalized as the measure on C\mathbb CC with density (Im⁡τ)−2(\operatorname{Im}\tau)^{-2}(Imτ)−2 with respect to Lebesgue measure restricted to H\mathbb HH, and invariance as equality of push-forward measures. Constant prefactors that Tong explicitly drops (powers of α′\alpha'α′, 4π24\pi^24π2) are omitted. Because every statement is restricted to Im⁡τ>0\operatorname{Im}\tau>0Imτ>0, where η\etaη has no zeros, the reciprocal 1/∣η∣1/|\eta|1/∣η∣ is never a division by zero, so no statement is vacuous.

Selected references

  • D. Tong, String Theory, Cambridge Part III lecture notes, 2009, Sections 6.4.1–6.4.2. http://www.damtp.cam.ac.uk/user/tong/string.html (arXiv:0908.0333)
  • J. Polchinski, Evaluation of the one loop string path integral, Commun. Math. Phys. 104 (1986) 37. https://doi.org/10.1007/BF01210927
  • T. M. Apostol, Modular Functions and Dirichlet Series in Number Theory, 2nd ed., Springer GTM 41, 1990, Chapter 3. https://doi.org/10.1007/978-1-4612-0999-7
  • J.-P. Serre, A Course in Arithmetic, Springer GTM 7, 1973, Chapter VII.
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Mathematical Physics·Captain: Lucas

Weinberg 1965: Infrared Photons and Gravitons — the soft exponents A and BResearch Paper

Motivation

When a charged particle scatters, it can radiate photons of arbitrarily low energy. In perturbative quantum electrodynamics this shows up as infrared divergences: loop integrals over very soft virtual photons diverge logarithmically, and so do the rates for emitting soft real photons. The standard resolution, due to Bloch and Nordsieck and systematized by Yennie, Frautschi and Suura, is that the divergences cancel in any rate that sums over undetectable soft emissions below an energy resolution EEE.

S. Weinberg's paper Infrared Photons and Gravitons (Phys. Rev. 140, B516 (1965)) shows that the same mechanism works for gravitons, derives explicit formulas for the exponents that control the soft factors, and proves that the extra "collinear" divergences produced by massless hard particles cancel for gravitons but not for photons. The soft-graviton factor (2.5)–(2.7) used there is the factor that appears in Weinberg's soft graviton theorem, and the spectrum formula is used in the paper to estimate the gravitational radiation from thermal collisions in the sun.

Timeline.

  • 1937 — Bloch and Nordsieck: soft-photon divergences cancel between virtual and real emission.
  • 1961 — Yennie, Frautschi and Suura: all-orders exponentiation of soft-photon factors in QED.
  • 1965 — Weinberg: the analogous treatment for gravitons, closed forms (2.16) and (2.26) for the exponents AAA and BBB, cancellation of collinear divergences for gravitons (Sec. III), and the Coulomb-phase result conjectured by Dalitz (Sec. V).

Setting

Work in units ℏ=c=1\hbar=c=1ℏ=c=1 with the paper's metric: for four-vectors p=(p,p0)p=(\mathbf p,p^0)p=(p,p0) and q=(q,q0)q=(\mathbf q,q^0)q=(q,q0), p⋅q=p⋅q−p0q0p\cdot q=\mathbf p\cdot\mathbf q-p^0q^0p⋅q=p⋅q−p0q0. A process α→β\alpha\to\betaα→β has finitely many external lines nnn; line nnn has mass mnm_nmn​, three-momentum pn∈R3\mathbf p_n\in\mathbb R^3pn​∈R3, on-shell energy En=∣pn∣2+mn2E_n=\sqrt{|\mathbf p_n|^2+m_n^2}En​=∣pn​∣2+mn2​​, charge ene_nen​, and sign ηn=+1\eta_n=+1ηn​=+1 (outgoing) or −1-1−1 (incoming). The relative velocity of lines n,mn,mn,m is

βnm=[1−mn2mm2(pn⋅pm)2]1/2.\beta_{nm}=\Bigl[1-\frac{m_n^2m_m^2}{(p_n\cdot p_m)^2}\Bigr]^{1/2}.βnm​=[1−(pn​⋅pm​)2mn2​mm2​​]1/2.

For a unit vector q^\hat qq^​ (the direction of a soft quantum) define the photon and graviton angular functions

A(q^)=12(2π)3∑n,menemηnηm(pn⋅pm)[En−pn⋅q^][Em−pm⋅q^],B(q^)=8πG2(2π)3∑n,mηnηm{(pn⋅pm)2−12mn2mm2}[En−pn⋅q^][Em−pm⋅q^],A(\hat q)=\frac{1}{2(2\pi)^3}\sum_{n,m}\frac{e_ne_m\eta_n\eta_m(p_n\cdot p_m)}{[E_n-\mathbf p_n\cdot\hat q][E_m-\mathbf p_m\cdot\hat q]},\qquad B(\hat q)=\frac{8\pi G}{2(2\pi)^3}\sum_{n,m}\frac{\eta_n\eta_m\{(p_n\cdot p_m)^2-\frac12m_n^2m_m^2\}}{[E_n-\mathbf p_n\cdot\hat q][E_m-\mathbf p_m\cdot\hat q]},A(q^​)=2(2π)31​n,m∑​[En​−pn​⋅q^​][Em​−pm​⋅q^​]en​em​ηn​ηm​(pn​⋅pm​)​,B(q^​)=2(2π)38πG​n,m∑​[En​−pn​⋅q^​][Em​−pm​⋅q^​]ηn​ηm​{(pn​⋅pm​)2−21​mn2​mm2​}​,

and the infrared exponents A=∫d2Ω A(q^)A=\int d^2\Omega\,A(\hat q)A=∫d2ΩA(q^​) and B=∫d2Ω B(q^)B=\int d^2\Omega\,B(\hat q)B=∫d2ΩB(q^​), integrals over the unit sphere against surface measure. With infrared cutoff λ\lambdaλ and dividing point Λ\LambdaΛ, virtual soft quanta multiply a rate by (λ/Λ)A(\lambda/\Lambda)^A(λ/Λ)A or (λ/Λ)B(\lambda/\Lambda)^B(λ/Λ)B, and summing over real soft emission of total energy at most EEE gives the cutoff-free factors (E/Λ)Ab(A)(E/\Lambda)^Ab(A)(E/Λ)Ab(A) and (E/Λ)Bb(B)(E/\Lambda)^Bb(B)(E/Λ)Bb(B) of Eqs. (2.51)–(2.52).

Formalization targets

Goal — Eq. (2.26)

For masses mn>0m_n>0mn​>0,

B=G2π∑n,mηnηmmnmm1+βnm2βnm(1−βnm2)1/2ln⁡(1+βnm1−βnm)=Gπ∑n,mηnmnηmmmf(βnm),B=\frac{G}{2\pi}\sum_{n,m}\eta_n\eta_mm_nm_m\frac{1+\beta_{nm}^2}{\beta_{nm}(1-\beta_{nm}^2)^{1/2}}\ln\Bigl(\frac{1+\beta_{nm}}{1-\beta_{nm}}\Bigr)=\frac{G}{\pi}\sum_{n,m}\eta_nm_n\eta_mm_mf(\beta_{nm}),B=2πG​n,m∑​ηn​ηm​mn​mm​βnm​(1−βnm2​)1/21+βnm2​​ln(1−βnm​1+βnm​​)=πG​n,m∑​ηn​mn​ηm​mm​f(βnm​),

with f(0)=1f(0)=1f(0)=1 for the diagonal terms. This is the formula for graviton bremsstrahlung in an arbitrary collision.

Milestones

  1. Sec. II.2 — summed over the N!N!N! orderings, the multiple pole factors of NNN soft emissions from one line factorize into single-emission factors.
  2. Eq. (2.13) — the real part of the virtual-photon exponent equals −Aln⁡(Λ/λ)-A\ln(\Lambda/\lambda)−Aln(Λ/λ).
  3. Eq. (2.16) — A=−18π2∑n,mηnηmenemβnm−1ln⁡1+βnm1−βnmA=-\frac{1}{8\pi^2}\sum_{n,m}\eta_n\eta_me_ne_m\beta_{nm}^{-1}\ln\frac{1+\beta_{nm}}{1-\beta_{nm}}A=−8π21​∑n,m​ηn​ηm​en​em​βnm−1​ln1−βnm​1+βnm​​.
  4. Eq. (2.14) — A≥0A\ge0A≥0 under charge conservation.
  5. Eq. (2.24) — B≥0B\ge0B≥0 under energy–momentum conservation.
  6. Eqs. (3.4)–(3.5) — if one line becomes massless, BBB stays finite (the ln⁡m1\ln m_1lnm1​ terms cancel by energy–momentum conservation).
  7. Eq. (3.3) — for photons the corresponding limit is A→+∞A\to+\inftyA→+∞ when the massless line is charged.
  8. Eq. (4.9) — f(β)=1+116β2+6340β4+O(β6)f(\beta)=1+\frac{11}{6}\beta^2+\frac{63}{40}\beta^4+O(\beta^6)f(β)=1+611​β2+4063​β4+O(β6).

Significance

The exponents AAA and BBB are the only process-dependent quantities in the soft factors: once they are known in closed form, the infrared behaviour of any rate, the shape EAE^AEA or EBE^BEB of the soft spectrum, and the soft power spectrum E dΓ=B Γ0 dEE\,d\Gamma=B\,\Gamma^0\,dEEdΓ=BΓ0dE (2.53) follow. The Sec. III cancellation is the statement that gravitation, unlike massless electrodynamics or Yang–Mills theory, is free of unremovable collinear divergences at this level; the paper uses the contrast to argue that charged massless particles are problematic. The expansion (4.9) feeds the nonrelativistic quadrupole formula (4.13) behind the solar estimate.

The paper's arguments are informal physics derivations. This mission makes the mathematical content of those derivations precise and machine-checkable: the angular integrals, the sign statements, the limiting behaviour as a mass goes to zero, and the combinatorial factorization.

Difficulty

The closed forms need the solid-angle integral of a product of two denominators [En−pn⋅q^]−1[Em−pm⋅q^]−1[E_n-\mathbf p_n\cdot\hat q]^{-1}[E_m-\mathbf p_m\cdot\hat q]^{-1}[En​−pn​⋅q^​]−1[Em​−pm​⋅q^​]−1 for two arbitrary, non-collinear momenta; the one-denominator case is a textbook integral in polar coordinates, but the two-denominator case does not reduce to it by an obvious choice of axis. The positivity statements are false without the conservation laws, so any proof must use them in an essential way. The massless-limit statements concern the interplay of a logarithmically divergent term with a coefficient that vanishes only at the limiting configuration, so a termwise limit fails.

Formalization scope

Three-momenta live in EuclideanSpace ℝ (Fin 3); energies are the on-shell values ∣p∣2+m2\sqrt{|\mathbf p|^2+m^2}∣p∣2+m2​ and are not free variables. Solid-angle integrals are Bochner integrals on the unit sphere against Mathlib's volume.toSphere (total mass 4π4\pi4π). External lines are indexed by an arbitrary Fintype; the signs ηn\eta_nηn​ are real numbers constrained to ±1\pm1±1 by hypothesis. Sums over n,mn,mn,m run over all ordered pairs, including n=mn=mn=m, where βnn=0\beta_{nn}=0βnn​=0; the kernels β−1ln⁡1+β1−β\beta^{-1}\ln\frac{1+\beta}{1-\beta}β−1ln1−β1+β​ and fff are extended by their limits 222 and 111 at β=0\beta=0β=0, so the formulas are not trivialized by Lean's convention x/0=0x/0=0x/0=0. The printed Eq. (4.6) has an exponent 1/21/21/2 on the logarithm's argument that contradicts (2.26), (4.5) and (4.9); the definition of fff drops it. The −iηϵ-i\eta\epsilon−iηϵ prescriptions are suppressed. The δ(q2)\delta(q^2)δ(q2) integration in (2.13) is carried out, leaving an integral over the shell λ≤∣q∣≤Λ\lambda\le|\mathbf q|\le\Lambdaλ≤∣q∣≤Λ. Positivity is stated as ≥0\ge0≥0, because A=B=0A=B=0A=B=0 in degenerate configurations. Sec. IV beyond (4.9) (the velocity expansion (4.8), the quadrupole formula (4.13), the solar estimate) and the Coulomb phases of Sec. V are out of scope for this mission.

A complete development needs solid-angle integration on S2S^2S2 (a spherical-coordinates change of variables for volume.toSphere), integration in polar coordinates on R3\mathbb R^3R3, and elementary inequalities for Minkowski products of timelike and null vectors. These are reusable beyond this mission, and contributions of them as separate lemmas are welcome.

Selected references

  • S. Weinberg, Infrared Photons and Gravitons, Phys. Rev. 140, B516 (1965). https://doi.org/10.1103/PhysRev.140.B516
  • F. Bloch and A. Nordsieck, Note on the Radiation Field of the Electron, Phys. Rev. 52, 54 (1937). https://doi.org/10.1103/PhysRev.52.54
  • D. R. Yennie, S. C. Frautschi and H. Suura, The infrared divergence phenomena and high-energy processes, Ann. Phys. 13, 379 (1961). https://doi.org/10.1016/0003-4916(61)90151-8
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Missing baryons from stacked SZ filaments: the model and statistics of de Graaff et al. (2019)Research Paper

Motivation

Big-bang nucleosynthesis and the acoustic peaks of the cosmic microwave background fix the baryon density of the universe to about 5% of its total energy density, but in the low-redshift universe only some 10% of those baryons are seen in galaxies, with another 10% in the circumgalactic and intracluster medium. Simulations place the remainder — the missing baryons — in a diffuse warm-hot intergalactic medium (WHIM) at 10510^5105–10710^7107 K, spread along the filaments of the cosmic web. Absorption-line studies and X-ray emission from individual filaments probe the cool and the hot ends of that range respectively, leaving the bulk poorly constrained.

de Graaff, Cai, Heymans & Peacock (2019) attack the problem statistically, by stacking the Planck Compton-yyy map over 1 020 3341\,020\,3341020334 pairs of CMASS galaxies and measuring the residual signal in the bridge between each pair. Interpreting that residual requires an analytic model of a filament, and that model — a cylinder with a Gaussian cross-section, convolved with the instrument beam — is what this mission formalizes. The same model, applied to the CMB lensing convergence map, converts the measured signals into a gas density and temperature, and hence into a baryon fraction.

Setting

A filament is modelled as an infinite cylinder seen side-on. In the plane perpendicular to the filament axis, write ℓ\ellℓ for the line-of-sight coordinate and r⊥r_\perpr⊥​ for the transverse coordinate on the sky. The electron density is taken to be a two-dimensional Gaussian

ne(ℓ,r⊥)=n0exp⁡ ⁣(−ℓ22σ2)exp⁡ ⁣(−r⊥22(σ2+σB2)),n_e(\ell, r_\perp) = n_0 \exp\!\left(-\frac{\ell^2}{2\sigma^2}\right)\exp\!\left(-\frac{r_\perp^2}{2(\sigma^2+\sigma_B^2)}\right),ne​(ℓ,r⊥​)=n0​exp(−2σ2ℓ2​)exp(−2(σ2+σB2​)r⊥2​​),

with central density n0n_0n0​, intrinsic width σ\sigmaσ and beam width σB\sigma_BσB​; the transverse direction, unlike the line of sight, is smoothed by the instrument beam, which is why σB\sigma_BσB​ appears only there.

The Compton yyy parameter of a line of sight is the optical-depth-weighted temperature of the scattering electrons,

y=kBTeσTmec2∫ne dℓ,y = \frac{k_B T_e \sigma_T}{m_e c^2}\int n_e \, d\ell,y=me​c2kB​Te​σT​​∫ne​dℓ,

with kBk_BkB​ the Boltzmann constant, σT\sigma_TσT​ the Thomson cross-section, mec2m_e c^2me​c2 the electron rest energy and TeT_eTe​ the electron temperature, assumed constant across the filament. The convergence κ\kappaκ of CMB lensing is the analogous projection of the total matter density contrast δ=ρ/ρˉ−1\delta = \rho/\bar\rho - 1δ=ρ/ρˉ​−1,

κ=3H02Ωm2c2∫0DSDL(DS−DL)DS δa dDL,\kappa = \frac{3H_0^2\Omega_m}{2c^2}\int_0^{D_S} \frac{D_L(D_S-D_L)}{D_S}\,\frac{\delta}{a}\, dD_L,κ=2c23H02​Ωm​​∫0DS​​DS​DL​(DS​−DL​)​aδ​dDL​,

with H0H_0H0​ the Hubble constant, Ωm\Omega_mΩm​ the matter density parameter, aaa the scale factor and DL,DSD_L, D_SDL​,DS​ the comoving distances of lens and source. For a structure thin compared with the lensing kernel, the geometric factor is constant across it and κ\kappaκ reduces to a line-of-sight integral of δ\deltaδ against a fixed prefactor.

The significance of the measurement is assessed with a second, statistical layer. A stack of NNN binned profiles yiky^k_iyik​ (kkk the map index, iii the bin index) has mean profile yˉi=1N∑kyik\bar y_i = \frac1N\sum_k y^k_iyˉ​i​=N1​∑k​yik​ and covariance estimator Ci,j=1N∑k(yik−yˉi)(yjk−yˉj)C_{i,j} = \frac1N\sum_k (y^k_i-\bar y_i)(y^k_j-\bar y_j)Ci,j​=N1​∑k​(yik​−yˉ​i​)(yjk​−yˉ​j​); the deviation of the mean profile from zero is measured by χ2=∑i,jyˉi(C−1)i,jyˉj\chi^2 = \sum_{i,j}\bar y_i (C^{-1})_{i,j}\bar y_jχ2=∑i,j​yˉ​i​(C−1)i,j​yˉ​j​. Because the stacked maps overlap on the sky, the paper replaces CCC by a jackknife covariance built from NsubN_{\mathrm{sub}}Nsub​ sky sub-samples, Ci,jJK=Nsub−1Nsub∑k(yik−yˉi)(yjk−yˉj)C^{JK}_{i,j} = \frac{N_{\mathrm{sub}}-1}{N_{\mathrm{sub}}}\sum_k (y^k_i-\bar y_i)(y^k_j-\bar y_j)Ci,jJK​=Nsub​Nsub​−1​∑k​(yik​−yˉ​i​)(yjk​−yˉ​j​), and multiplies the inverse by the Hartlap factor (Nsub−n−2)/(Nsub−1)(N_{\mathrm{sub}}-n-2)/(N_{\mathrm{sub}}-1)(Nsub​−n−2)/(Nsub​−1), with nnn the number of bins.

Measurements enter through two numbers: the mean Compton parameter yˉ\bar{y}yˉ​ and the mean convergence κˉ\bar{\kappa}κˉ over the boxed filament region, together with the empirical observation that the peak of each profile is close to 1/0.91/0.91/0.9 times its mean. Every statement in this mission imposes that calibration as a hypothesis on the model.

Formalization targets

Goal — total electron content, Eq. (A.4)

Ne  =  L∬ne dℓ dr⊥  =  yˉ0.9 mec2kBTeσT 2π L σ2+σB2.N_e \;=\; L \iint n_e\, d\ell\, dr_\perp \;=\; \frac{\bar y}{0.9}\,\frac{m_e c^2}{k_B T_e \sigma_T}\,\sqrt{2\pi}\, L\, \sqrt{\sigma^2+\sigma_B^2}.Ne​=L∬ne​dℓdr⊥​=0.9yˉ​​kB​Te​σT​me​c2​2π​Lσ2+σB2​​.

This is the quantity the paper's baryon budget is computed from: given the measured yˉ\bar yyˉ​, an assumed temperature TeT_eTe​ and the beam width, it fixes the number of electrons in a filament of length LLL.

Milestone — projected profile, Eq. (A.2)

y(r⊥)=2π n0σ kBTeσTmec2exp⁡ ⁣(−r⊥22(σ2+σB2)).y(r_\perp) = \sqrt{2\pi}\, n_0\sigma\,\frac{k_B T_e \sigma_T}{m_e c^2}\exp\!\left(-\frac{r_\perp^2}{2(\sigma^2+\sigma_B^2)}\right).y(r⊥​)=2π​n0​σme​c2kB​Te​σT​​exp(−2(σ2+σB2​)r⊥2​​).

Milestone — central density, Eq. (A.3)

n0=yˉ/0.92π σ⋅mec2kBTeσT.n_0 = \frac{\bar y/0.9}{\sqrt{2\pi}\,\sigma}\cdot\frac{m_e c^2}{k_B T_e \sigma_T}.n0​=2π​σyˉ​/0.9​⋅kB​Te​σT​me​c2​.

Milestone — lensing counterpart, Eq. (A.5)

δ0=κˉ/0.92π σ⋅2ac23H02Ωm⋅DSDL(DS−DL).\delta_0 = \frac{\bar\kappa/0.9}{\sqrt{2\pi}\,\sigma}\cdot\frac{2ac^2}{3H_0^2\Omega_m}\cdot\frac{D_S}{D_L(D_S-D_L)}.δ0​=2π​σκˉ/0.9​⋅3H02​Ωm​2ac2​⋅DL​(DS​−DL​)DS​​.

Milestone — beam dominance, the remark after Eq. (A.4)

σB≤σ2+σB2≤σB(1+σ22σB2).\sigma_B \le \sqrt{\sigma^2+\sigma_B^2}\le \sigma_B\left(1+\frac{\sigma^2}{2\sigma_B^2}\right).σB​≤σ2+σB2​​≤σB​(1+2σB2​σ2​).

Milestone — the covariance estimators, Eqs. (3) and (5)-(6)

Both CCC and CJKC^{JK}CJK are symmetric and positive semidefinite, for every data set and every sample size.

Milestone — the significance statistic, Eq. (4)

C positive definite  ⟹  χ2=∑i,jyˉi(C−1)i,jyˉj≥0.C \text{ positive definite} \implies \chi^2 = \sum_{i,j}\bar y_i (C^{-1})_{i,j}\bar y_j \ge 0.C positive definite⟹χ2=i,j∑​yˉ​i​(C−1)i,j​yˉ​j​≥0.

Milestone — the Hartlap correction, Eq. (7)

∑i,jyˉi[Nsub−n−2Nsub−1C−1]i,jyˉj=Nsub−n−2Nsub−1∑i,jyˉi(C−1)i,jyˉj.\sum_{i,j}\bar y_i\left[\frac{N_{\mathrm{sub}}-n-2}{N_{\mathrm{sub}}-1}C^{-1}\right]_{i,j}\bar y_j = \frac{N_{\mathrm{sub}}-n-2}{N_{\mathrm{sub}}-1}\sum_{i,j}\bar y_i (C^{-1})_{i,j}\bar y_j.i,j∑​yˉ​i​[Nsub​−1Nsub​−n−2​C−1]i,j​yˉ​j​=Nsub​−1Nsub​−n−2​i,j∑​yˉ​i​(C−1)i,j​yˉ​j​.

Significance

The four displayed identities are the entire inferential chain from two stacked maps to a baryon fraction. Eq. (A.2) says what the model predicts for the observable; Eq. (A.3) inverts it at the filament axis; Eq. (A.4) turns the inversion into a total electron count, from which the paper obtains gas at (5.5±2.9) ρˉb(5.5\pm2.9)\,\bar\rho_b(5.5±2.9)ρˉ​b​ and T=(2.7±1.7)×106T=(2.7\pm1.7)\times10^6T=(2.7±1.7)×106 K, accounting for 11±7%11\pm7\%11±7% of the cosmic baryon budget; Eq. (A.5) supplies the independent lensing constraint that breaks the density–temperature degeneracy of the SZ measurement alone. The statistical milestones cover the other half of the analysis: the covariance estimators of Eqs. (3) and (5)-(6) that turn a stack into an error bar, the nonnegativity of the χ2\chi^2χ2 of Eq. (4) that is converted into the quoted 2.9σ2.9\sigma2.9σ, and the Hartlap rescaling of Eq. (7). The beam-dominance milestone quantifies the paper's claim that the result barely depends on the one free shape parameter, the intrinsic width σ\sigmaσ, which is taken from simulations rather than measured.

Formalizing them contributes a machine-checked derivation layer for a widely used observational technique: the projection of a Gaussian cylinder onto a Compton-yyy or convergence map, and the inversion of that projection, recur throughout stacked-SZ and stacked-lensing analyses. What this mission adds over the paper is a statement of each identity with all its hypotheses exposed — which positivity conditions are needed, which parameters genuinely drop out — rather than a new physical result. The physics is not re-derived and the measurement is not re-analysed; the empirical inputs yˉ\bar yyˉ​, κˉ\bar\kappaκˉ and the peak-to-mean ratio 1/0.91/0.91/0.9 enter as hypotheses, not as claims.

Difficulty

The identities are Gaussian integrals, so the mathematical depth is modest; the difficulty is bookkeeping and faithfulness. Three specific traps. First, the line-of-sight and transverse directions have different widths — σ\sigmaσ against σ2+σB2\sqrt{\sigma^2+\sigma_B^2}σ2+σB2​​ — and the asymmetry is what makes the final answer depend on the beam; a formalization that symmetrizes them is a different theorem. Second, the paper's n0n_0n0​ is not free: it is pinned by the calibration ypeak=yˉ/0.9y_{\text{peak}} = \bar y/0.9ypeak​=yˉ​/0.9, so the goal must carry that equation as a hypothesis rather than substituting a closed form for n0n_0n0​ silently. Third, the total electron count is an iterated integral over the plane, and the inner and outer variables must be kept in the paper's order.

Formalization scope

Everything is stated over R\mathbb{R}R with no units, so every physical constant is an explicit real variable; integrals are Bochner integrals over the whole real line with Lebesgue measure, which return 000 on a non-integrable integrand. The definition bundle fixes the model once — the SZ prefactor, the Gaussian cylinder profile, the Compton parameter, the thin-lens convergence prefactor, the convergence and the total electron content — and every statement is phrased against it. The convergence definition is the thin-lens specialization of Eq. (2): the geometric kernel is a constant prefactor, not an integral over lens distance, and the mission does not claim the reduction from the full Eq. (2) to that form.

Degenerate readings are ruled out as follows. The calibration hypotheses are satisfiable for every admissible choice of constants, so no statement is vacuous; conversely they genuinely constrain the central amplitude, so no statement holds for a trivial reason. The positivity hypotheses are the minimal ones that make the denominators nonzero, and the widths enter as σ>0\sigma > 0σ>0 with σB\sigma_BσB​ unrestricted, so the beam-free case σB=0\sigma_B = 0σB​=0 is included rather than excluded. The statistical layer is finite-dimensional: profiles are real arrays indexed by a finite bin type, covariances are real matrices, and matrix inversion is the nonsingular inverse, which returns the zero matrix on a singular argument — hence the positive-definiteness hypothesis in the χ2\chi^2χ2 milestone. Counts are natural numbers but all arithmetic in the prefactors is performed after casting to the reals, so Nsub−n−2N_{\mathrm{sub}} - n - 2Nsub​−n−2 is a genuine real subtraction and may be negative. The statistical statements assert the structural properties of the estimators as written; they do not assert unbiasedness, nor the reduction C→C/NC \to C/NC→C/N for the covariance of a mean, nor any property of the resampling scheme. Only Mathlib's Gaussian-integral, measure-theory and positive-semidefinite-matrix API is needed; no new infrastructure is required, and the resulting projection lemmas are reusable for any other stacked-profile analysis.

Selected references

  • A. de Graaff, Y.-C. Cai, C. Heymans, J. A. Peacock, Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments, Astronomy & Astrophysics 624, A48 (2019). doi:10.1051/0004-6361/201935159
  • R. A. Sunyaev, Y. B. Zeldovich, The Observations of Relic Radiation as a Test of the Nature of X-Ray Radiation from the Clusters of Galaxies, Comments on Astrophysics and Space Physics 4, 173 (1972).
  • Planck Collaboration XXII, Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect, A&A 594, A22 (2016). doi:10.1051/0004-6361/201525826
  • Planck Collaboration XV, Planck 2015 results. XV. Gravitational lensing, A&A 594, A15 (2016). doi:10.1051/0004-6361/201525941
  • J. Hartlap, P. Simon, P. Schneider, Why your model parameter confidences might be too optimistic: unbiased estimation of the inverse covariance matrix, A&A 464, 399 (2007). doi:10.1051/0004-6361:20066170
  • H. Tanimura et al., A search for warm/hot gas filaments between pairs of SDSS Luminous Red Galaxies, MNRAS 483, 223 (2019). doi:10.1093/mnras/sty3118
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Hubble's Law: The Kinematics of a Uniformly Expanding UniverseTextbook

Motivation

Hubble's law — officially the Hubble–Lemaître law — is the observation that galaxies recede from us at a speed proportional to their distance, v=H0Dv = H_0 Dv=H0​D. It is the first observational basis for the expansion of the universe and one of the standard pieces of evidence cited for the Big Bang model. Georges Lemaître derived the proportionality from relativistic cosmology in 1927; Edwin Hubble published the observational relation in 1929, building on Vesto Slipher's redshifts and Henrietta Swan Leavitt's Cepheid distance scale. Alexander Friedmann had already shown in 1922 that the Einstein field equations admit expanding solutions, with an expansion rate governed by what is now called the scale factor.

Behind the astronomy sits a piece of elementary mathematics that is rarely written out in full: in a spatially homogeneous expansion, the linear velocity–distance relation is forced, it holds with the same constant for every observer, and the Hubble "constant" is in fact a function of time whose evolution is fixed by a single dimensionless parameter. This mission formalizes that kinematic core: the statements are about the scale factor and its derivatives, and involve no Einstein equations.

Setting

A scale factor is a function a:R→Ra : \mathbb{R} \to \mathbb{R}a:R→R of cosmic time ttt. A comoving point is labelled by a fixed coordinate x∈R3\mathbf{x} \in \mathbb{R}^3x∈R3 (with the Euclidean norm), and its proper position at time ttt is

Xx(t)  =  a(t) x.\mathbf{X}_{\mathbf{x}}(t) \;=\; a(t)\,\mathbf{x}.Xx​(t)=a(t)x.

The proper distance between the comoving points x\mathbf{x}x and y\mathbf{y}y is

Dx,y(t)  =  ∥a(t)x−a(t)y∥.D_{\mathbf{x},\mathbf{y}}(t) \;=\; \lVert a(t)\mathbf{x} - a(t)\mathbf{y}\rVert .Dx,y​(t)=∥a(t)x−a(t)y∥.

The Hubble parameter and the dimensionless deceleration parameter are

H(t)  =  a˙(t)a(t),q(t)  =  − a¨(t) a(t)a˙(t)2.H(t) \;=\; \frac{\dot a(t)}{a(t)},\qquad q(t) \;=\; -\,\frac{\ddot a(t)\,a(t)}{\dot a(t)^{2}} .H(t)=a(t)a˙(t)​,q(t)=−a˙(t)2a¨(t)a(t)​.

H0H_0H0​ denotes the present-day value of HHH; the name "Hubble constant" refers to the fact that HHH is constant in space at a fixed time, not in time.

Target

The goal theorem is the idealized Hubble law, stated in the source as a theorem of Euclidean geometry: any two points moving away from the origin, each along a straight line and with speed proportional to its distance from the origin, move away from each other with a speed proportional to their distance apart. Formally, for H≥0H \ge 0H≥0, a time ttt and curves p,q:R→R3p, q : \mathbb{R} \to \mathbb{R}^3p,q:R→R3 with

p′(t)=H p(t),q′(t)=H q(t),p'(t) = H\,p(t), \qquad q'(t) = H\,q(t),p′(t)=Hp(t),q′(t)=Hq(t),

the separation satisfies

dds∣s=t(p(s)−q(s))  =  H (p(t)−q(t)),∥H (p(t)−q(t))∥  =  H ∥p(t)−q(t)∥.\frac{d}{ds}\Big|_{s=t}\big(p(s) - q(s)\big) \;=\; H\,\big(p(t) - q(t)\big), \qquad \big\lVert H\,(p(t)-q(t))\big\rVert \;=\; H\,\lVert p(t)-q(t)\rVert .dsd​​s=t​(p(s)−q(s))=H(p(t)−q(t)),​H(p(t)−q(t))​=H∥p(t)−q(t)∥.

The relative velocity is parallel to the separation vector and its magnitude is HHH times the separation, with the same HHH for every pair — so no comoving observer occupies a distinguished centre of the expansion.

The milestones supply the cosmological content that surrounds this geometric fact:

  1. proper distances scale as D(t)=(a(t)/a(t0))D(t0)D(t) = \big(a(t)/a(t_0)\big) D(t_0)D(t)=(a(t)/a(t0​))D(t0​);
  2. a comoving point has velocity H(t)H(t)H(t) times its proper position vector;
  3. Hubble's law itself, D˙(t)=H(t) D(t)\dot D(t) = H(t)\,D(t)D˙(t)=H(t)D(t);
  4. the evolution law H˙=−(1+q)H2\dot H = -(1+q)H^{2}H˙=−(1+q)H2;
  5. the zero-deceleration case: if q≡0q \equiv 0q≡0 then H(t)=1/tH(t) = 1/tH(t)=1/t, with ttt the time since the Big Bang, so the Hubble time 1/H1/H1/H is exactly the age;
  6. a constant Hubble parameter forces exponential growth a(t)=a(t0)eH0(t−t0)a(t) = a(t_0)e^{H_0(t-t_0)}a(t)=a(t0​)eH0​(t−t0​);
  7. the small-redshift limit: with 1+z=a(t0)/a(te)1 + z = a(t_0)/a(t_\mathrm{e})1+z=a(t0​)/a(te​), the ratio z/(t0−te)z/(t_0 - t_\mathrm{e})z/(t0​−te​) tends to H(t0)H(t_0)H(t0​) as te→t0t_\mathrm{e} \to t_0te​→t0​, which is the z≈H0D/cz \approx H_0 D/cz≈H0​D/c form of the law used observationally.

Significance

The result itself is elementary but load-bearing: it is what licenses reading a linear redshift–distance diagram as evidence for uniform expansion rather than for a privileged position in space, and items 4–6 are the statements through which cosmological observations (the sign of qqq, the approach of qqq to −1-1−1 in Λ\LambdaΛCDM) are turned into claims about the past and future behaviour of HHH and aaa.

Formalizing it produces a small, reusable Lean layer for expansion kinematics: the scale factor, the Hubble and deceleration parameters, proper position and proper distance, with the differentiation lemmas that connect them. The platform already carries Friedmann-equation missions that fix the dynamics of aaa; this mission is the kinematic complement, and its Hubble parameter is the same function a˙/a\dot a/aa˙/a that those developments use. Nothing here is an open research problem: every statement is a known textbook fact, and the work is the formalization.

Difficulty

The mathematical content is a few lines of calculus, so the difficulty is entirely in the encoding. Three places are easy to get wrong. First, proper distance is defined through a norm, so the identity ∥a(t)v∥=a(t)∥v∥\lVert a(t)v\rVert = a(t)\lVert v\rVert∥a(t)v∥=a(t)∥v∥ needs positivity of aaa, and differentiating it needs positivity on a neighbourhood, not just at the point. Second, qqq is defined by a quotient with a˙2\dot a^{2}a˙2 in the denominator: in Lean division by zero returns zero, so a statement about qqq that forgets a˙(t)≠0\dot a(t) \ne 0a˙(t)=0 silently changes meaning. Third, milestone 5 propagates a hypothesis stated on (0,∞)(0,\infty)(0,∞) down to the endpoint t=0t=0t=0, where the Big Bang condition a(0)=0a(0)=0a(0)=0 lives; the continuity argument at the endpoint is the only step with any technical content.

Formalization scope

Time is R\mathbb{R}R and space is EuclideanSpace ℝ (Fin 3); derivatives are Mathlib's deriv / HasDerivAt, so "velocity" is always a derivative at a point rather than a difference quotient. Smoothness is assumed exactly where it is used: differentiability at a single time for the first-order statements, ContDiff ℝ 2 for the statements involving a¨\ddot aa¨. Positivity of the scale factor is stated explicitly wherever it is needed, as is a˙(t)≠0\dot a(t) \ne 0a˙(t)=0 in the statements mentioning qqq.

Degenerate readings are excluded: the goal's hypotheses are satisfiable (any pair of comoving points in an expanding universe satisfies them, as milestone 2 shows), and the milestones are non-vacuous for concrete scale factors such as a(t)=ta(t) = ta(t)=t and a(t)=eH0ta(t) = e^{H_0 t}a(t)=eH0​t. The goal theorem's second clause is a norm identity that is true for every H≥0H \ge 0H≥0; it carries the "speed proportional to distance" half of the source's statement, while the first clause carries the "moving away from each other along the separation" half.

The definition layer is a single self-contained file (scale factor derived quantities, proper position, proper distance); it is reusable by any mission about expansion kinematics. Contributions of the milestone proofs, and of variants such as the redshift relation 1+z=a(t0)/a(te)1+z = a(t_0)/a(t_\mathrm{e})1+z=a(t0​)/a(te​) derived from null geodesics rather than assumed, are welcome.

Selected references

  • Wikipedia, "Hubble's law" (Hubble–Lemaître law), https://en.wikipedia.org/wiki/Hubble%27s_law — the source text for this mission, in particular the sections "Recessional velocity", "Time-dependence of Hubble parameter", "Idealized Hubble's law" and "Ultimate fate and age of the universe".
  • E. Hubble, "A relation between distance and radial velocity among extra-galactic nebulae", PNAS 15 (1929) 168–173, https://doi.org/10.1073/pnas.15.3.168.
  • G. Lemaître, "Un univers homogène de masse constante et de rayon croissant rendant compte de la vitesse radiale des nébuleuses extra-galactiques", Annales de la Société Scientifique de Bruxelles A47 (1927) 49–59.
  • A. Friedmann, "Über die Krümmung des Raumes", Zeitschrift für Physik 10 (1922) 377–386, https://doi.org/10.1007/BF01332580.
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Mathematical PhysicsStatistics·Captain: Lucas

CODATA 2022: exactly known constants of the revised SI and the least-squares adjustmentResearch Paper

Motivation

Since the 2019 revision of the SI, seven constants of nature have fixed, exact numerical values: the caesium hyperfine frequency ΔνCs\Delta\nu_{\mathrm{Cs}}ΔνCs​, the speed of light ccc, the Planck constant hhh, the elementary charge eee, the Boltzmann constant kkk, the Avogadro constant NAN_ANA​ and the luminous efficacy KcdK_{\mathrm{cd}}Kcd​. Every other constant is either measured, and then carries an uncertainty, or is a closed-form expression in the seven, and is then known exactly. The CODATA 2022 adjustment (Mohr, Newell, Taylor and Tiesinga, Rev. Mod. Phys. 97, 025002, 2025) is the authoritative statement of which constants fall on which side of that line, and of the statistical procedure that produces the recommended values of the measured ones.

The exactly known side of the line is pure mathematics: the tabulated value of the Stefan-Boltzmann constant, of the radiation constants, of the molar gas constant and of the Faraday constant are theorems about π\piπ, an integral, and rational arithmetic - not measurements. The measured side rests on one statistical object, the weighted linear least-squares fit of N=133N=133N=133 input data to M=79M=79M=79 adjusted constants, together with the diagnostics (χ2\chi^2χ2, the Birge ratio, normalized residuals, expansion factors) the task group uses to decide that the fit is acceptable. This mission formalizes both.

Setting

Write hhh, ccc, kkk, eee, NAN_ANA​ for the numerical values of the defining constants in coherent SI units, and ℏ=h/2π\hbar = h/2\piℏ=h/2π. The spectral radiance of a blackbody at thermodynamic temperature TTT, per unit frequency, is Planck's function

Bν(T,ν)  =  2hν3c2 1ehν/kT−1,B_\nu(T,\nu) \;=\; \frac{2h\nu^3}{c^2}\,\frac{1}{e^{h\nu/kT}-1},Bν​(T,ν)=c22hν3​ehν/kT−11​,

and per unit wavelength

Bλ(T,λ)  =  2hc2λ5 1ehc/(λkT)−1.B_\lambda(T,\lambda) \;=\; \frac{2hc^2}{\lambda^5}\,\frac{1}{e^{hc/(\lambda k T)}-1}.Bλ​(T,λ)=λ52hc2​ehc/(λkT)−11​.

The derived constants named in Tables XXXII and XXXIII of the paper are σ=(π2/60)k4/ℏ3c2\sigma = (\pi^2/60)k^4/\hbar^3c^2σ=(π2/60)k4/ℏ3c2 (Stefan-Boltzmann), c1=2πhc2c_1 = 2\pi hc^2c1​=2πhc2 and c2=hc/kc_2 = hc/kc2​=hc/k (radiation constants), R=NAkR = N_AkR=NA​k (molar gas), F=NAeF = N_AeF=NA​e (Faraday), KJ=2e/hK_J = 2e/hKJ​=2e/h (Josephson) and RK=h/e2R_K = h/e^2RK​=h/e2 (von Klitzing).

For the adjustment, let A∈RN×MA \in \mathbb{R}^{N\times M}A∈RN×M be the design matrix of the linearized observational equations, z∈RNz \in \mathbb{R}^Nz∈RN the input data and W∈RN×NW \in \mathbb{R}^{N\times N}W∈RN×N the weight matrix - the inverse of the covariance matrix of the data, symmetric and positive definite. The fit minimizes

χ2(x)  =  (z−Ax)TW(z−Ax),x∈RM,\chi^2(x) \;=\; (z - Ax)^{\mathsf T} W (z - Ax), \qquad x \in \mathbb{R}^M,χ2(x)=(z−Ax)TW(z−Ax),x∈RM,

with ν=N−M\nu = N - Mν=N−M degrees of freedom, Birge ratio RB=(χ2/ν)1/2R_B = (\chi^2/\nu)^{1/2}RB​=(χ2/ν)1/2 and normalized residuals ri=(Xi−⟨Xi⟩)/u(Xi)r_i = (X_i - \langle X_i\rangle)/u(X_i)ri​=(Xi​−⟨Xi​⟩)/u(Xi​).

Formalization targets

Goal

∫0∞π Bν(T,ν) dν  =  σT4(T>0),σ=π260k4ℏ3c2.\int_0^{\infty} \pi\,B_\nu(T,\nu)\,\mathrm{d}\nu \;=\; \sigma T^4 \qquad (T>0), \qquad \sigma = \frac{\pi^2}{60}\frac{k^4}{\hbar^3c^2}.∫0∞​πBν​(T,ν)dν=σT4(T>0),σ=60π2​ℏ3c2k4​.

The goal fixes no digits: it asserts that the constant appearing in the tabulated closed form is exactly the one produced by integrating Planck's law over the spectrum and over a Lambertian hemisphere. The numerical enclosure of σ\sigmaσ is a separate, weaker milestone, so that the goal survives any change of tabulated digits.

Supporting targets

∫0∞x3ex−1 dx=π415,σ=2π5k415h3c2,R=NAk,F=NAe,\int_0^\infty \frac{x^3}{e^x-1}\,\mathrm{d}x = \frac{\pi^4}{15}, \qquad \sigma = \frac{2\pi^5k^4}{15h^3c^2}, \qquad R = N_Ak, \qquad F = N_Ae,∫0∞​ex−1x3​dx=15π4​,σ=15h3c22π5k4​,R=NA​k,F=NA​e,

together with the numerical enclosures of σ\sigmaσ, of Wien's displacement constants b=c2/x5b = c_2/x_5b=c2​/x5​ and b′=x3k/hb' = x_3k/hb′=x3​k/h (where x5x_5x5​, x3x_3x3​ solve x=5(1−e−x)x = 5(1-e^{-x})x=5(1−e−x) and x=3(1−e−x)x = 3(1-e^{-x})x=3(1−e−x)), and the identity KJ2RK=4/hK_J^2R_K = 4/hKJ2​RK​=4/h.

On the statistical side:

χ2(x)  =  χ2(x^)+(x−x^)TATWA (x−x^)wheneverATWA x^=ATWz,\chi^2(x) \;=\; \chi^2(\hat x) + (x-\hat x)^{\mathsf T}A^{\mathsf T}WA\,(x-\hat x) \quad\text{whenever}\quad A^{\mathsf T}WA\,\hat x = A^{\mathsf T}Wz,χ2(x)=χ2(x^)+(x−x^)TATWA(x−x^)wheneverATWAx^=ATWz,

the equivalence of minimality with the normal equations, the closed form x^=(ATWA)−1ATWz\hat x = (A^{\mathsf T}WA)^{-1}A^{\mathsf T}Wzx^=(ATWA)−1ATWz when ATWAA^{\mathsf T}WAATWA is invertible, and the behaviour of χ2\chi^2χ2, RBR_BRB​ and rir_iri​ under an expansion factor fff applied to the uncertainties.

Significance

The exact-constant statements are what makes the tabulated values checkable rather than authoritative: a reader who accepts the SI definitions can, in principle, re-derive R=8.314 462 618 153 24 J mol−1K−1R = 8.314\,462\,618\,153\,24\ \mathrm{J\,mol^{-1}K^{-1}}R=8.31446261815324 Jmol−1K−1 and F=96 485.332 123 310 0184 C mol−1F = 96\,485.332\,123\,310\,0184\ \mathrm{C\,mol^{-1}}F=96485.3321233100184 Cmol−1 by arithmetic, and σ=5.670 374 419…×10−8 W m−2K−4\sigma = 5.670\,374\,419\ldots\times10^{-8}\ \mathrm{W\,m^{-2}K^{-4}}σ=5.670374419…×10−8 Wm−2K−4 from Planck's law and ζ(4)\zeta(4)ζ(4). Formalizing them turns "in principle" into a machine-checked derivation from the seven fixed numbers.

The least-squares statements make precise what the adjustment is, independently of the 133 data of this particular round: that the recommended values are the unique minimizer of a quadratic form, that the normal equations characterize it, and that multiplying a group of uncertainties by an expansion factor fff - the device used in 2022 with f=1.7f = 1.7f=1.7, 2.52.52.5 and 3.93.93.9 - rescales χ2\chi^2χ2 by f−2f^{-2}f−2, the Birge ratio by f−1f^{-1}f−1 and the residuals by f−1f^{-1}f−1, without moving the fitted values. None of these statements is new mathematics; none of them, as far as the catalog shows, is currently available as a machine-checked statement about the CODATA quantities.

Difficulty

Two hard points. First, ∫0∞x3/(ex−1) dx=π4/15\int_0^\infty x^3/(e^x-1)\,\mathrm{d}x = \pi^4/15∫0∞​x3/(ex−1)dx=π4/15: the obvious route expands 1/(ex−1)1/(e^x-1)1/(ex−1) as a geometric series and integrates term by term, which needs a dominated convergence or monotone convergence argument plus the value ζ(4)=π4/90\zeta(4)=\pi^4/90ζ(4)=π4/90; interchanging the sum and the integral is the step that must be justified, not assumed. The goal then needs this together with a change of variables x=hν/kTx = h\nu/kTx=hν/kT on (0,∞)(0,\infty)(0,∞) and an integrability argument for the original integrand.

Second, the numerical enclosures. 5.670 374 419×10−8<σ5.670\,374\,419\times10^{-8} < \sigma5.670374419×10−8<σ requires certified rational bounds on π5\pi^5π5; the Wien constants require certified bounds on a transcendental root, obtained from interval evaluation of e−xe^{-x}e−x at rational points plus monotonicity of x−n(1−e−x)x - n(1-e^{-x})x−n(1−e−x). Floating-point evaluation proves nothing here.

The least-squares milestones are routine linear algebra, with one subtlety: the decomposition identity needs symmetry of WWW, and the characterization of minimizers needs positive definiteness, so both hypotheses are carried explicitly.

Formalization scope

All physical quantities are plain real numbers: each constant is the numerical value of the quantity in the coherent SI unit named in its docstring, and the code carries no units. The defining constants are given by the exact decimal literals of Table XXXII, so they are exact rationals; ℏ\hbarℏ is defined as h/2πh/2\pih/2π and is therefore irrational.

Planck's function is a total function of two real arguments. Outside the physical regime it returns junk rather than failing - at T=0T = 0T=0 the exponent is 000, the denominator e0−1=0e^0 - 1 = 0e0−1=0, and Lean's division returns 000 - so every statement about it carries 0<T0 < T0<T and a positivity hypothesis on the spectral variable. The goal's integral is the Bochner integral over (0,∞)(0,\infty)(0,∞) with respect to Lebesgue measure; it is not trivially true by non-integrability, since the integrand is integrable for T>0T>0T>0.

The adjustment is formalized over Fin N\mathrm{Fin}\,NFinN and Fin M\mathrm{Fin}\,MFinM with an arbitrary design matrix AAA and an arbitrary weight matrix WWW, hypotheses on WWW (Hermitian, positive definite) stated where they are used rather than baked into the definition; ν=N−M\nu = N-Mν=N−M is an integer, not a truncated natural number.

Contributions welcome: the ζ(4)\zeta(4)ζ(4) integral and the interval-arithmetic enclosures are reusable well beyond this mission, as are the least-squares statements.

Selected references

  • P. J. Mohr, D. B. Newell, B. N. Taylor, E. Tiesinga, CODATA recommended values of the fundamental physical constants: 2022, Rev. Mod. Phys. 97, 025002 (2025). https://doi.org/10.1103/RevModPhys.97.025002
  • Bureau International des Poids et Mesures, The International System of Units (SI), 9th edition (2019). https://www.bipm.org/en/publications/si-brochure
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Numerical Analysis·Captain: Lucas

Métodos Numéricos (Freitas) I: Zeros de Funções e Convergência do Método de NewtonTextbook

Motivation

Most equations that arise in applications cannot be solved in closed form: the age of the Moon from a radioactive-decay balance, the deflection of a clamped beam, the equilibrium of a catenary, all reduce to solving f(x)=0f(x) = 0f(x)=0 for a function fff with no algebraic inverse. A first course in numerical methods therefore opens with root finding: constructive procedures that produce a sequence of approximations x0,x1,x2,dotsx_0, x_1, x_2, \\dotsx0​,x1​,x2​,dots together with a theorem saying that the sequence converges to a root and how fast.

This mission is the first in a series formalizing the lecture notes Métodos Numéricos by Sergio Roberto de Freitas (Departamento de Computação e Estatística, UFMS, 2000). It covers Chapter 3, Zeros de Funções, whose capstone is the local convergence of Newton's method.

Setting

Let f:mathbbRtomathbbRf : \\mathbb{R} \\to \\mathbb{R}f:mathbbRtomathbbR and let barx\\bar{x}barx be a zero of fff, i.e. f(barx)=0f(\\bar{x}) = 0f(barx)=0. The chapter studies three constructions.

Bisection. Starting from an interval (a0,b0)(a_0, b_0)(a0​,b0​) with f(a0)<0<f(b0)f(a_0) < 0 < f(b_0)f(a0​)<0<f(b0​), put xk+1=(ak+bk)/2x_{k+1} = (a_k + b_k)/2xk+1​=(ak​+bk​)/2 and keep the half of (ak,bk)(a_k, b_k)(ak​,bk​) on whose endpoints fff still changes sign. The width of the bracketing interval is halved at every step.

Linear iteration (MIL). Rewrite f(x)=0f(x) = 0f(x)=0 as a fixed-point equation x=g(x)x = g(x)x=g(x) and iterate xn+1=g(xn)x_{n+1} = g(x_n)xn+1​=g(xn​) from an arbitrary x0x_0x0​.

Newton's method. Take the particular iteration function

g(x)=x−fracf(x)f′(x),qquadxn+1=xn−fracf(xn)f′(xn),g(x) = x - \\frac{f(x)}{f'(x)}, \\qquad x_{n+1} = x_n - \\frac{f(x_n)}{f'(x_n)},g(x)=x−fracf(x)f′(x),qquadxn+1​=xn​−fracf(xn​)f′(xn​),

obtained by truncating the Taylor expansion of fff at xnx_nxn​ after the linear term.

A sequence xntoalphax_n \\to \\alphaxn​toalpha has order of convergence ppp when ∣en+1∣/∣en∣p|e_{n+1}| / |e_n|^p∣en+1​∣/∣en​∣p tends to a finite constant, where en=xn−alphae_n = x_n - \\alphaen​=xn​−alpha; p=1p = 1p=1 is linear and p=2p = 2p=2 quadratic convergence.

Target

The goal theorem is the local convergence of Newton's method at a simple zero. If fff is twice differentiable on an open interval (a,b)(a, b)(a,b) containing barx\\bar{x}barx, its second derivative is continuous there, and f′f'f′ never vanishes on (a,b)(a, b)(a,b), then there is h>0h > 0h>0 such that

x0in[barx−h,barx+h]impliesxntobarx,x_0 \\in [\\bar{x} - h, \\bar{x} + h] \\implies x_n \\to \\bar{x},x0​in[barx−h,barx+h]impliesxn​tobarx,

where xnx_nxn​ is the Newton sequence started at x0x_0x0​. This is the formal content of the chapter's statement that Newton's method converges provided the initial guess is chosen close enough to the root.

The milestones are the supporting results of the chapter: the error bound and convergence of bisection, the convergence of the linear iterative method under a derivative bound ∣g′∣leL<1|g'| \\le L < 1∣g′∣leL<1, the a posteriori estimate ∣barx−xn∣lefracL1−L∣xn−xn−1∣|\\bar{x} - x_n| \\le \\frac{L}{1-L}|x_n - x_{n-1}|∣barx−xn​∣lefracL1−L∣xn​−xn−1​∣, and the quadratic order of Newton's method at a simple zero.

Significance

Bisection, fixed-point iteration and Newton's method are the three root finders every numerical-analysis course starts with, and the three convergence theorems above are what justifies using them. The a posteriori estimate is what turns the iteration into an algorithm with a stopping criterion: it bounds the distance to the root by a quantity the program can measure. The quadratic order statement explains the observed doubling of correct digits per step at a simple zero and its loss at a multiple zero.

On the formalization side, Mathlib already has a fixed-point theorem for contractions on complete spaces and the mean value theorem, but not the statements in the form used in numerical analysis: bisection with its explicit 2−n2^{-n}2−n bracket, the fracL1−L\\frac{L}{1-L}fracL1−L a posteriori bound, or Newton's local convergence and quadratic rate stated for the concrete iteration sequence. This mission asks for those.

Difficulty

The delicate point in all three theorems is that the iterates must be known to stay in the region where the hypotheses hold; the informal proofs assume this silently. For the linear iterative method the mission therefore states the invariance hypothesis explicitly (ggg maps the closed interval into itself). For Newton's method, no such hypothesis is given: the existence of a neighbourhood of barx\\bar{x}barx that the iteration preserves is part of what must be proved, and it comes from the continuity of g′g'g′ together with g′(barx)=0g'(\\bar{x}) = 0g′(barx)=0. The quadratic-order milestone also has to handle the degenerate possibility xn=barxx_n = \\bar{x}xn​=barx, which would put a zero in the denominator; it is excluded by hypothesis.

Formalization scope

Everything is over the real numbers. The iterations are given as explicit recursive sequences: the bisection construction returns the bracketing pair (an,bn)(a_n, b_n)(an​,bn​) and its midpoint, and there are separate sequences for the fixed-point and Newton iterations. Newton's method takes the derivative as a separate function argument f′f'f′, tied to fff by a hypothesis of the form "fff has derivative f′(x)f'(x)f′(x) at every xxx of the interval"; this avoids relying on any junk value of a derivative operator where fff fails to be differentiable. Division is total, so a step at a point where f′f'f′ vanishes would leave the iterate unchanged; the hypotheses exclude this inside the interval.

Two deliberate deviations from the source are worth flagging for the auditor. First, Proposição 3.5.1 assumes f′(x)neq0f'(x) \\neq 0f′(x)neq0 only for xneqbarxx \\neq \\bar{x}xneqbarx, but its proof divides by f′(barx)2f'(\\bar{x})^2f′(barx)2; the formal statement assumes f′neq0f' \\neq 0f′neq0 on the whole interval, so barx\\bar{x}barx is a simple zero. Second, the convergence statement for the linear iterative method adds the hypothesis that ggg maps the closed interval into itself, without which the iterates may leave the region where the derivative bound is assumed.

Selected references

  • S. R. Freitas, Métodos Numéricos, Departamento de Computação e Estatística, Centro de Ciências Exatas e Tecnologia, Universidade Federal de Mato Grosso do Sul, 2000. Chapter 3, Zeros de Funções, pp. 33–70. (Course notes supplied with this mission.)
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Numerical Analysis·Captain: Lucas

Métodos Numéricos (Freitas) V: Interpolação Polinomial e o Erro da Fórmula de LagrangeTextbook

Motivation

A table of values is all one has of many functions: measurements, tabulated physical constants, the output of an expensive simulation. Interpolation reconstructs a function between tabulated points by passing a polynomial through them, and it underlies much of the rest of numerical analysis — quadrature rules, finite-difference formulas and predictor-corrector schemes for differential equations are all obtained by integrating or differentiating an interpolating polynomial. What makes the reconstruction trustworthy is a formula for the error committed away from the nodes.

This mission is the fifth in a series formalizing the lecture notes Métodos Numéricos by Sergio Roberto de Freitas (UFMS, 2000). It covers Chapter 7, Interpolação.

Setting

Let x0<x1<dots<xnx_0 < x_1 < \\dots < x_nx0​<x1​<dots<xn​ be distinct nodes and fi=f(xi)f_i = f(x_i)fi​=f(xi​) the tabulated values of a function fff. The Lagrange form of the interpolating polynomial is

Pn(t)=sumi=0nfiLi(t),qquadLi(t)=prodjneqifract−xjxi−xj,P_n(t) = \\sum_{i=0}^{n} f_i L_i(t), \\qquad L_i(t) = \\prod_{j \\neq i}\\frac{t - x_j}{x_i - x_j},Pn​(t)=sumi=0n​fi​Li​(t),qquadLi​(t)=prodjneqi​fract−xj​xi​−xj​,

so that Pn(xi)=fiP_n(x_i) = f_iPn​(xi​)=fi​ for every iii, and PnP_nPn​ is the unique polynomial of degree at most nnn with this property.

The interpolation error at a point xxx that is not a node is the difference f(x)−Pn(x)f(x) - P_n(x)f(x)−Pn​(x).

Target

The goal theorem is Proposição 7.3.1: if fff is n+1n+1n+1 times differentiable on (a,b)(a,b)(a,b) and all nodes lie in (a,b)(a,b)(a,b), then for every xin(a,b)x \\in (a,b)xin(a,b) different from all nodes there exists xiin(a,b)\\xi \\in (a,b)xiin(a,b) with

f(x)=Pn(x)+left(prodk=0n(x−xk)right)fracf(n+1)(xi)(n+1)!.f(x) = P_n(x) + \\left(\\prod_{k=0}^{n}(x - x_k)\\right)\\frac{f^{(n+1)}(\\xi)}{(n+1)!}.f(x)=Pn​(x)+left(prodk=0n​(x−xk​)right)fracf(n+1)(xi)(n+1)!.

The milestones are the other results of the chapter needed to make sense of it: the existence and uniqueness of the interpolating polynomial of degree at most nnn through n+1n+1n+1 points with distinct abscissas (Proposição 7.2.1), the fact that the Lagrange formula does interpolate the data, and the practical error bound of Proposição 7.3.2, ∣f(x)−Pn(x)∣lefracM(n+1)!prodk∣x−xk∣|f(x) - P_n(x)| \\le \\frac{M}{(n+1)!}\\prod_k |x - x_k|∣f(x)−Pn​(x)∣lefracM(n+1)!prodk​∣x−xk​∣ when ∣f(n+1)∣leM|f^{(n+1)}| \\le M∣f(n+1)∣leM.

Significance

The error formula is the reason interpolation is a numerical method and not just a curve-drawing device: it shows that the error is governed by two independent factors, the smoothness of fff through f(n+1)f^{(n+1)}f(n+1) and the geometry of the nodes through the product prodk(x−xk)\\prod_k(x - x_k)prodk​(x−xk​). Everything downstream follows from it — the h2h^2h2 and h4h^4h4 error terms of the trapezoidal and Simpson rules in the next mission are obtained by integrating exactly this expression, and the choice of Chebyshev nodes is the attempt to make the product factor small.

Difficulty

The standard proof introduces the auxiliary function F(t)=f(t)−Pn(t)−Kprodk(t−xk)F(t) = f(t) - P_n(t) - K\\prod_k(t - x_k)F(t)=f(t)−Pn​(t)−Kprodk​(t−xk​) with KKK chosen so that F(x)=0F(x) = 0F(x)=0, and then applies Rolle's theorem n+1n+1n+1 times to conclude that F(n+1)F^{(n+1)}F(n+1) vanishes somewhere. Formalizing the repeated application of Rolle's theorem, keeping track of the n+2n+2n+2 distinct zeros and the nested intervals they generate, is the substance of the work; it is an induction that has to be organized carefully rather than a computation.

Formalization scope

The nodes are given as a strictly increasing family x0<dots<xnx_0 < \\dots < x_nx0​<dots<xn​ of n+1n+1n+1 reals lying in the open interval (a,b)(a,b)(a,b), and the interpolating polynomial is the explicit Lagrange sum rather than an abstract polynomial: at a node it is defined by the same formula, whose factors then include 0/00/00/0 contributions unless the nodes are distinct, which is why the distinctness hypothesis appears in the interpolation milestone. Smoothness is expressed as continuous differentiability of order n+1n+1n+1 on the open interval (a,b)(a,b)(a,b), and the derivative appearing in the error term is the iterated derivative computed within that set; since the set is open this agrees with the ordinary (n+1)(n+1)(n+1)-st derivative. The evaluation point xxx is assumed to lie in (a,b)(a,b)(a,b) and to differ from every node; the point xi\\xixi is asserted to exist in (a,b)(a,b)(a,b), with no claim of uniqueness or of any relation to xxx beyond membership in the interval. The uniqueness milestone is stated with Mathlib's polynomial type and the degree bound deglen\\deg \\le ndeglen, which includes the zero polynomial.

Selected references

  • S. R. Freitas, Métodos Numéricos, Departamento de Computação e Estatística, Universidade Federal de Mato Grosso do Sul, 2000. Chapter 7, Interpolação, pp. 133–161. (Course notes supplied with this mission.)
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Mathematical Physics·Captain: Lucas

Stability and Symmetry Breaking in the General Two-Higgs-Doublet ModelResearch Paper

Motivation

In the Standard Model the scalar sector consists of a single complex SU(2)LSU(2)_LSU(2)L​ doublet. The general Two-Higgs-Doublet Model (THDM) replaces it by two complex doublets φ1,φ2\varphi_1,\varphi_2φ1​,φ2​ of the same weak hypercharge y=1/2y=1/2y=1/2. This is the minimal extension of the scalar sector that is still renormalisable and gauge invariant, and it is forced on any supersymmetric completion: the Minimal Supersymmetric Standard Model has exactly two Higgs doublets. Before any phenomenology can be done with such a model, two questions have to be answered for the given parameter point: is the scalar potential stable, i.e. bounded from below, and does its global minimum break SU(2)L×U(1)YSU(2)_L\times U(1)_YSU(2)L​×U(1)Y​ down to the electromagnetic U(1)emU(1)_{\text{em}}U(1)em​?

The general THDM potential has 141414 real parameters, and answering these questions directly in field space — eight real scalar degrees of freedom, of which three are gauge — is unwieldy. Maniatis, von Manteuffel, Nachtmann and Nagel (2006) proposed a reformulation in terms of gauge-invariant bilinears, in which the gauge orbits of the Higgs fields are parametrised by a Minkowski-type four-vector confined to the closed forward light cone, and the potential becomes a quadratic polynomial on that cone. In these variables the stability question reduces to a one-variable problem: the sign of an explicit rational function f(u)f(u)f(u) on a finite set III of at most ten real numbers. This mission formalizes that analysis: the gauge-orbit parametrisation (their Theorem 4), the classification of the stationary points of the potential (their Theorem 2), and the stability criterion itself (their Theorem 1).

Setting

Write the two doublets as rows of a 2×22\times 22×2 complex matrix,

ϕ=(φ1+φ10φ2+φ20),\phi=\begin{pmatrix}\varphi_1^+&\varphi_1^0\\ \varphi_2^+&\varphi_2^0\end{pmatrix},ϕ=(φ1+​φ2+​​φ10​φ20​​),

and form the hermitian matrix of gauge-invariant scalar products Kij=φj†φiK^{ij}=\varphi_j^\dagger\varphi_iKij=φj†​φi​, i.e. K=ϕ ϕ†K=\phi\,\phi^\daggerK=ϕϕ†. Decomposing KKK in the Pauli basis gives four real functions

K0=tr⁡K,Ka=tr⁡ ⁣(Kσa),a=1,2,3.K_0=\operatorname{tr}K,\qquad K_a=\operatorname{tr}\!\left(K\sigma^a\right),\quad a=1,2,3 .K0​=trK,Ka​=tr(Kσa),a=1,2,3.

Positive semi-definiteness of KKK is equivalent to K0≥0K_0\ge 0K0​≥0 and K02−∣K∣2≥0K_0^2-|K|^2\ge 0K02​−∣K∣2≥0: the four-vector (K0,K)(K_0,K)(K0​,K) lies on or inside the forward light cone. A gauge transformation acts as ϕ↦ϕ UT\phi\mapsto \phi\,U^{\mathsf T}ϕ↦ϕUT with U∈U(2)U\in U(2)U∈U(2), and leaves KKK invariant.

The most general gauge-invariant renormalisable potential is

V=ξ0K0+ξTK⏟V2+η00K02+2K0 ηTK+KTEK⏟V4,V=\underbrace{\xi_0K_0+\xi^{\mathsf T}K}_{V_2}+\underbrace{\eta_{00}K_0^2+2K_0\,\eta^{\mathsf T}K+K^{\mathsf T}EK}_{V_4},V=V2​ξ0​K0​+ξTK​​+V4​η00​K02​+2K0​ηTK+KTEK​​,

with real parameters ξ0,η00∈R\xi_0,\eta_{00}\in\mathbb Rξ0​,η00​∈R, ξ,η∈R3\xi,\eta\in\mathbb R^3ξ,η∈R3 and a real symmetric 3×33\times33×3 matrix EEE. For K0>0K_0>0K0​>0 one sets k=K/K0k=K/K_0k=K/K0​, so that ∣k∣≤1|k|\le 1∣k∣≤1, and

J2(k)=ξ0+ξTk,J4(k)=η00+2ηTk+kTEk,V=K0J2(k)+K02J4(k).J_2(k)=\xi_0+\xi^{\mathsf T}k,\qquad J_4(k)=\eta_{00}+2\eta^{\mathsf T}k+k^{\mathsf T}Ek,\qquad V=K_0J_2(k)+K_0^2J_4(k).J2​(k)=ξ0​+ξTk,J4​(k)=η00​+2ηTk+kTEk,V=K0​J2​(k)+K02​J4​(k).

Stationary points of J4J_4J4​ on the ball ∣k∣≤1|k|\le1∣k∣≤1 are governed by the functions

f(u)=u+η00−ηT(E−u)−1η,f′(u)=1−ηT(E−u)−2η,g(u)=ξ0−ξT(E−u)−1η,f(u)=u+\eta_{00}-\eta^{\mathsf T}(E-u)^{-1}\eta,\qquad f'(u)=1-\eta^{\mathsf T}(E-u)^{-2}\eta,\qquad g(u)=\xi_0-\xi^{\mathsf T}(E-u)^{-1}\eta,f(u)=u+η00​−ηT(E−u)−1η,f′(u)=1−ηT(E−u)−2η,g(u)=ξ0​−ξT(E−u)−1η,

where uuu is a Lagrange multiplier for the constraint ∣k∣=1|k|=1∣k∣=1. The finite set III collects: every regular uuu with f′(u)=0f'(u)=0f′(u)=0; the point u=0u=0u=0 when f′(0)>0f'(0)>0f′(0)>0; and every eigenvalue μ\muμ of EEE at which fff stays finite and f′(μ)≥0f'(\mu)\ge0f′(μ)≥0. It has at most ten elements, and {f(u):u∈I}\{f(u):u\in I\}{f(u):u∈I} is exactly the set of stationary values of J4J_4J4​.

For the stationary points of the full potential one uses four-vector notation K~=(K0,K)\tilde K=(K_0,K)K~=(K0​,K), ξ~=(ξ0,ξ)\tilde\xi=(\xi_0,\xi)ξ~​=(ξ0​,ξ), E~=(η00ηTηE)\tilde E=\begin{pmatrix}\eta_{00}&\eta^{\mathsf T}\\ \eta&E\end{pmatrix}E~=(η00​η​ηTE​) and the metric g~=diag(1,−1,−1,−1)\tilde g=\mathrm{diag}(1,-1,-1,-1)g~​=diag(1,−1,−1,−1), so that V=K~Tξ~+K~TE~K~V=\tilde K^{\mathsf T}\tilde\xi+\tilde K^{\mathsf T}\tilde E\tilde KV=K~Tξ~​+K~TE~K~ on the domain K~Tg~K~≥0\tilde K^{\mathsf T}\tilde g\tilde K\ge0K~Tg~​K~≥0, K0≥0K_0\ge0K0​≥0, with f~(u)=−14ξ~T(E~−ug~)−1ξ~\tilde f(u)=-\tfrac14\tilde\xi^{\mathsf T}(\tilde E-u\tilde g)^{-1}\tilde\xif~​(u)=−41​ξ~​T(E~−ug~​)−1ξ~​.

Formalization targets

Goal — Theorem 1 (stability criterion)

For V4≡0V_4\equiv0V4​≡0 the potential is stable for ξ0>∣ξ∣\xi_0>|\xi|ξ0​>∣ξ∣, marginal for ξ0=∣ξ∣\xi_0=|\xi|ξ0​=∣ξ∣ and unstable for ξ0<∣ξ∣\xi_0<|\xi|ξ0​<∣ξ∣. For V4≢0V_4\not\equiv0V4​≡0,

f(ui)>0  ∀ui∈I ⟹ J4>0 on ∣k∣≤1(stability in the strong sense),f(u_i)>0\ \ \forall u_i\in I\ \Longrightarrow\ J_4>0 \text{ on } |k|\le1 \quad\text{(stability in the strong sense)},f(ui​)>0  ∀ui​∈I ⟹ J4​>0 on ∣k∣≤1(stability in the strong sense), ∃ui∈I: f(ui)<0 ⟹ V unbounded below,\exists u_i\in I:\ f(u_i)<0\ \Longrightarrow\ V \text{ unbounded below},∃ui​∈I: f(ui​)<0 ⟹ V unbounded below,

and if f≥0f\ge0f≥0 on III with equality somewhere, the sign of g(ui)g(u_i)g(ui​) — replaced by g(ui)−∣ξ⊥(ui)∣f′(ui)g(u_i)-|\xi_\perp(u_i)|\sqrt{f'(u_i)}g(ui​)−∣ξ⊥​(ui​)∣f′(ui​)​ when uiu_iui​ is an eigenvalue of EEE — decides between stability in the weak sense and instability.

Milestones

Theorem 4 (gauge orbits); the four stability cases (a), (b.2), (b.3), (b.4) of Section 4 including the criterion J22≤CJ4J_2^2\le CJ_4J22​≤CJ4​ for the marginal case; equation (4.39) identifying the stationary values of J4J_4J4​ with {f(u):u∈I}\{f(u):u\in I\}{f(u):u∈I}; equations (4.42)–(4.44) giving J2J_2J2​ at those stationary points; and Theorem 2, the classification of the stationary points of VVV.

Significance

The criterion is a decision procedure: given the 141414 parameters of a THDM, stability is settled by evaluating one rational function at the roots of another, without any search in field space. The authors use it to re-derive the known stability conditions for the MSSM potential and to settle the stability and symmetry-breaking properties of the THDM potential of Gunion et al., for which λ1+λ3>0\lambda_1+\lambda_3>0λ1​+λ3​>0, λ2+λ3>0\lambda_2+\lambda_3>0λ2​+λ3​>0 and λ4,κ>−2λ3−2(λ1+λ3)(λ2+λ3)\lambda_4,\kappa>-2\lambda_3-2\sqrt{(\lambda_1+\lambda_3)(\lambda_2+\lambda_3)}λ4​,κ>−2λ3​−2(λ1​+λ3​)(λ2​+λ3​)​ come out as the strong-stability conditions. Theorem 4 is what makes the whole approach legitimate: it says that nothing is lost in passing from fields to the invariants (K0,K)(K_0,K)(K0​,K), because the fibres of that map are exactly the gauge orbits.

The results are established in the published literature; what this mission adds is machine-checked proofs. The statements are not present in Mathlib in any form, and the note added in version 3 of the paper — a condition for the marginal case that was missing in the original version — is a concrete reminder that the case analysis here is easy to get subtly wrong.

Difficulty

The obvious route to stability is to minimise VVV directly; it fails because the domain is a cone with a boundary, and the minimisation over the boundary ∣k∣=1|k|=1∣k∣=1 introduces a Lagrange multiplier whose admissible values are the roots of f′f'f′, including the degenerate "exceptional" solutions where E−uE-uE−u is singular. Those exceptional solutions are not a technicality: they are where the eigenvalue clauses of III, the ξ⊥\xi_\perpξ⊥​ correction in (4.43), and the junk-value behaviour of matrix inverses all live. The marginal case (J4J_4J4​ and J2J_2J2​ vanishing simultaneously somewhere) is not decided by the signs alone and needs the quantitative bound J22≤CJ4J_2^2\le CJ_4J22​≤CJ4​.

Formalization scope

Vectors in R3\mathbb R^3R3 are plain functions Fin 3 → ℝ with an explicitly defined dot product; EEE is a Matrix (Fin 3) (Fin 3) ℝ and its symmetry is carried as a hypothesis. Four-vectors are indexed by Unit ⊕ Fin 3 so that E~\tilde EE~ and g~\tilde gg~​ are block matrices, with the first component being K0K_0K0​. Higgs configurations are 2×22\times22×2 complex matrices and K=ϕϕ†K=\phi\phi^\daggerK=ϕϕ†; a gauge transformation is ϕ↦ϕUT\phi\mapsto\phi U^{\mathsf T}ϕ↦ϕUT with U†U=1U^\dagger U=1U†U=1.

Stability is formalized as the honest statement that V(K0,k)V(K_0,k)V(K0​,k) is bounded from below on the physical domain K0≥0K_0\ge0K0​≥0, ∣k∣≤1|k|\le1∣k∣≤1 — not as any of the sign conditions that the theorem derives — so none of the implications is true by definition. Matrix inversion in Lean returns the zero matrix at a singular argument; every occurrence of (E−u)−1(E-u)^{-1}(E−u)−1 is therefore guarded by a regularity hypothesis, and the values of f,f′,gf,f',gf,f′,g at an eigenvalue of EEE are defined as limits, with the existence of those limits part of the membership condition for III. The projection ξ⊥(μ)\xi_\perp(\mu)ξ⊥​(μ) is characterised by its defining property (it lies in the eigenspace and ξ−ξ⊥\xi-\xi_\perpξ−ξ⊥​ is orthogonal to it) rather than by a choice of eigenbasis.

A complete development needs linear algebra over R\mathbb RR (resolvents, symmetric matrices, eigenspaces), U(2)U(2)U(2) and the spectral decomposition of positive semi-definite 2×22\times22×2 complex matrices for Theorem 4, and elementary real analysis (compactness of the ball, limits of rational functions) for Section 4. The gauge-orbit statement and the light-cone parametrisation are reusable for any multi-doublet scalar sector; contributions of the nnn-doublet generalisation (Appendix B, Theorem 5) are welcome as follow-ups.

Selected references

  • M. Maniatis, A. von Manteuffel, O. Nachtmann, F. Nagel, Stability and symmetry breaking in the general two-Higgs-doublet model, Eur. Phys. J. C 48 (2006) 805–823. https://arxiv.org/abs/hep-ph/0605184
  • J. F. Gunion, H. E. Haber, G. L. Kane, S. Dawson, The Higgs Hunter's Guide, Addison-Wesley, 1990.
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Probability·Captain: naimengye

Probability Theory and Examples I: Kolmogorov's Three-Series TheoremTextbook

Motivation

Given independent random variables X1,X2,…X_1,X_2,\dotsX1​,X2​,…, when does ∑nXn\sum_n X_n∑n​Xn​ converge? Not absolutely — that question is settled by ∑nE∣Xn∣<∞\sum_n\mathbb{E}|X_n|<\infty∑n​E∣Xn​∣<∞ and is usually too strong. The interesting question is when the partial sums converge for almost every outcome, and here independence buys something that holds for no general sequence: convergence is not a delicate matter of cancellation but is decided, once and for all, by three numerical series.

Chapter 2 of Rick Durrett's Probability: Theory and Examples (Version 5, 2019) reaches this in section 2.5. Kolmogorov's three-series theorem fixes a truncation level A>0A>0A>0, replaces each XnX_nXn​ by Yn=Xn1(∣Xn∣≤A)Y_n=X_n\mathbb{1}(|X_n|\le A)Yn​=Xn​1(∣Xn​∣≤A), and asserts that ∑nXn\sum_n X_n∑n​Xn​ converges almost surely if and only if

∑nP(∣Xn∣>A)<∞,∑nEYn converges,∑nvar⁡(Yn)<∞.\sum_n\mathbb{P}(|X_n|>A)<\infty,\qquad \sum_n\mathbb{E}Y_n \text{ converges},\qquad \sum_n\operatorname{var}(Y_n)<\infty .n∑​P(∣Xn​∣>A)<∞,n∑​EYn​ converges,n∑​var(Yn​)<∞.

Three deterministic conditions on the distributions decide an almost-sure question about paths, and the answer does not depend on which AAA is chosen. Through Kronecker's lemma this is also the route to the strong law of large numbers, which is how the chapter uses it.

Setting

Let X1,X2,…X_1,X_2,\dotsX1​,X2​,… be independent real random variables on a probability space, with partial sums SN=∑n<NXnS_N=\sum_{n<N}X_nSN​=∑n<N​Xn​. Say that ∑nXn\sum_n X_n∑n​Xn​ converges almost surely when for almost every ω\omegaω the sequence SN(ω)S_N(\omega)SN​(ω) has a real limit; following Durrett, "∑an\sum a_n∑an​ converges" means lim⁡N∑n≤Nan\lim_N\sum_{n\le N}a_nlimN​∑n≤N​an​ exists, not that it converges absolutely.

Three tools from the same section support the theorem. Kolmogorov's maximal inequality strengthens Chebyshev from P(∣Sn∣≥x)\mathbb{P}(|S_n|\ge x)P(∣Sn​∣≥x) to the maximum of the whole path,

P(max⁡1≤k≤n∣Sk∣≥x)≤x−2var⁡(Sn),\mathbb{P}\Bigl(\max_{1\le k\le n}|S_k|\ge x\Bigr)\le x^{-2}\operatorname{var}(S_n),P(1≤k≤nmax​∣Sk​∣≥x)≤x−2var(Sn​),

for independent, centred, square-integrable summands. From it comes the convergence criterion: if EXn=0\mathbb{E}X_n=0EXn​=0 and ∑nvar⁡(Xn)<∞\sum_n\operatorname{var}(X_n)<\infty∑n​var(Xn​)<∞ then ∑nXn\sum_n X_n∑n​Xn​ converges almost surely. Kronecker's lemma is the deterministic bridge to averages: if an↑∞a_n\uparrow\inftyan​↑∞ and ∑nxn/an\sum_n x_n/a_n∑n​xn​/an​ converges then an−1∑m≤nxm→0a_n^{-1}\sum_{m\le n}x_m\to0an−1​∑m≤n​xm​→0. And the Hewitt–Savage 0-1 law says that for an i.i.d. sequence every permutable event — one unchanged by rearranging finitely many coordinates — has probability 000 or 111.

Formalization targets

Goal — Theorem 2.5.8, Kolmogorov's three-series theorem

∑nXn converges a.s.  ⟺  {∑nP(∣Xn∣>A)<∞,∑nE[Xn1(∣Xn∣≤A)] converges,∑nvar⁡(Xn1(∣Xn∣≤A))<∞.\sum_n X_n \text{ converges a.s.} \iff \begin{cases} \sum_n\mathbb{P}(|X_n|>A)<\infty,\\ \sum_n\mathbb{E}\bigl[X_n\mathbb{1}(|X_n|\le A)\bigr]\ \text{converges},\\ \sum_n\operatorname{var}\bigl(X_n\mathbb{1}(|X_n|\le A)\bigr)<\infty . \end{cases}n∑​Xn​ converges a.s.⟺⎩⎨⎧​∑n​P(∣Xn​∣>A)<∞,∑n​E[Xn​1(∣Xn​∣≤A)] converges,∑n​var(Xn​1(∣Xn​∣≤A))<∞.​

Both directions are asserted, as Durrett states the theorem. The truncation level A>0A>0A>0 is arbitrary and fixed in the statement; that the three conditions hold for one AAA exactly when they hold for every AAA is a consequence, not an assumption.

Supporting levels

Kolmogorov's maximal inequality (2.5.5); the convergence criterion under summable variances (2.5.6); Kronecker's lemma (2.5.9); and the Hewitt–Savage 0-1 law (2.5.4).

Significance

The result itself. The three-series theorem is the complete answer to a question that has no complete answer without independence, and the shape of the answer is the interesting part: a pathwise, almost-sure property is equivalent to three conditions each computable from the marginal distributions alone. Each of the three does a separate job — the first says XnX_nXn​ and its truncation differ only finitely often, so Borel–Cantelli lets them be exchanged; the second controls the drift of the truncated sums; the third controls their fluctuation. The theorem is also the standard route to the strong law: applying it to Xn/nX_n/nXn​/n and then Kronecker's lemma gives Sn/n→μS_n/n\to\muSn​/n→μ, which is why section 2.5 sits where it does.

Formalizing it. Mathlib has the strong law of large numbers (strong_law_ae), both Borel–Cantelli lemmas, and Kolmogorov's 0-1 law for the tail σ-field. It has none of the following: Kolmogorov's maximal inequality, the almost-sure convergence criterion for random series with summable variances, Kronecker's lemma, the Hewitt–Savage 0-1 law, or the three-series theorem. The mission therefore contributes the whole of section 2.5, and the pieces are reusable well beyond it — the maximal inequality and Kronecker's lemma in particular are standard tools with no probabilistic content in the second case at all.

Difficulty

The maximal inequality is the step where the argument stops being routine. Chebyshev bounds P(∣Sn∣≥x)\mathbb{P}(|S_n|\ge x)P(∣Sn​∣≥x) and no more; controlling the maximum over the whole path needs the first passage decomposition Ak={∣Sk∣≥x, ∣Sj∣<x for j<k}A_k=\{|S_k|\ge x,\ |S_j|<x \text{ for } j<k\}Ak​={∣Sk​∣≥x, ∣Sj​∣<x for j<k} and the observation that Sk1AkS_k\mathbb{1}_{A_k}Sk​1Ak​​ is measurable with respect to the first kkk variables while Sn−SkS_n-S_kSn​−Sk​ is independent of them, so the cross terms vanish. That is a stopping-time argument in disguise, and it is what makes the whole section work.

The sufficiency half of the goal is then assembly: the third series and the convergence criterion give ∑(Yn−EYn)\sum(Y_n-\mathbb{E}Y_n)∑(Yn​−EYn​) convergent, the second adds the means back, and the first plus Borel–Cantelli replaces YnY_nYn​ by XnX_nXn​. Necessity is the harder direction, and Durrett does not prove it in Chapter 2 at all — he defers it to Example 3.4.12, where it follows from the Lindeberg–Feller central limit theorem. A solver attacking the goal should expect the reverse implication to need machinery from outside this section.

The Hewitt–Savage law has a difficulty of its own kind: the natural statement is about a σ-field of events on a sequence space, and the proof approximates a permutable event by cylinder events and then applies the permutation that swaps the first nnn coordinates with the next nnn.

Formalization scope

Random variables are measurable real-valued functions on a probability space and independence is Mathlib's iIndepFun. Variance is Mathlib's variance, and square-integrability is stated as membership in L2L^2L2 where the maximal inequality and the convergence criterion need it. The three-series theorem itself assumes no integrability: the truncated variables are bounded, so their means and variances exist automatically, which is exactly why the truncation is there.

"∑nan\sum_n a_n∑n​an​ converges" is formalized as convergence of the sequence of partial sums to a real limit, not as Summable, which in Mathlib means unconditional and hence absolute convergence for real series. This distinction is not pedantic here: condition (ii) of the theorem is convergence of ∑EYn\sum\mathbb{E}Y_n∑EYn​ in Durrett's sense and would be a strictly stronger condition if read as summability. Conditions (i) and (iii) are series of non-negative terms, where the two notions agree, and are stated as Summable.

Almost-sure convergence of ∑nXn\sum_n X_n∑n​Xn​ is "for almost every ω\omegaω there exists a real LLL with SN(ω)→LS_N(\omega)\to LSN​(ω)→L" — the limit is not asserted to be measurable in ω\omegaω, and does not need to be for the statement to say what it should.

For the Hewitt–Savage law the sequence space is the countable product N→S\mathbb{N}\to SN→S carrying the infinite product of copies of one law, which is Mathlib's Measure.infinitePi, and a permutable event is a measurable set invariant under every finitely supported permutation of the coordinates. That is Durrett's exchangeable σ-field stated directly rather than constructed as a σ-field object.

Contributions welcome beyond the listed items: the converse direction via Lindeberg–Feller (Example 3.4.12); the derivation of the strong law from the three-series theorem and Kronecker's lemma; the Marcinkiewicz–Zygmund law (2.5.12); and the rates of convergence of section 2.5.1.

Selected references

  • Rick Durrett, Probability: Theory and Examples, Version 5 (January 11, 2019), section 2.5 (pp. 81–90); Theorems 2.5.4, 2.5.5, 2.5.6, 2.5.8, 2.5.9. Published as Cambridge Series in Statistical and Probabilistic Mathematics, 5th edition, 2019, DOI 10.1017/9781108591034
  • A. N. Kolmogorov, Grundbegriffe der Wahrscheinlichkeitsrechnung, Springer, 1933.
  • E. Hewitt and L. J. Savage, Symmetric measures on Cartesian products, Transactions of the American Mathematical Society 80 (1955), 470–501. DOI 10.1090/S0002-9947-1955-0076206-8
  • P. Billingsley, Probability and Measure, 3rd ed., Wiley, 1995, section 22.
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Number Theory·Captain: Lucas

The de Bruijn–Newman Constant is Non-negativeResearch Paper

Motivation

The Riemann hypothesis asserts that all nontrivial zeros of the Riemann zeta function lie on the critical line. A classical way to measure how far the hypothesis is from failing runs through a one-parameter deformation of the Riemann ξ\xiξ function by the backward heat flow. De Bruijn (1950) introduced a family of entire functions HtH_tHt​, t∈Rt \in \mathbb{R}t∈R, with H0H_0H0​ essentially the ξ\xiξ function, and showed that HtH_tHt​ has only real zeros for t≥1/2t \ge 1/2t≥1/2. Newman (1976) proved that there is a finite constant Λ\LambdaΛ, now called the de Bruijn–Newman constant, such that HtH_tHt​ has only real zeros precisely when t≥Λt \ge \Lambdat≥Λ. The Riemann hypothesis is exactly the statement Λ≤0\Lambda \le 0Λ≤0, and Newman conjectured the complementary bound Λ≥0\Lambda \ge 0Λ≥0 — in his phrase, that if the Riemann hypothesis is true, then it is only barely so.

Timeline of lower bounds on Λ\LambdaΛ, all obtained before 2018 by exhibiting Lehmer pairs, that is, pairs of adjacent zeros of ζ\zetaζ that are unusually close together: Λ>−∞\Lambda > -\inftyΛ>−∞ (Newman 1976), Λ≥−50\Lambda \ge -50Λ≥−50 (Csordas–Norfolk–Varga 1988), Λ≥−5\Lambda \ge -5Λ≥−5 (te Riele 1991), Λ≥−0.385\Lambda \ge -0.385Λ≥−0.385 (Norfolk–Ruttan–Varga 1992), Λ≥−0.0991\Lambda \ge -0.0991Λ≥−0.0991 (Csordas–Ruttan–Varga 1991), Λ≥−4.379×10−6\Lambda \ge -4.379 \times 10^{-6}Λ≥−4.379×10−6 (Csordas–Smith–Varga 1994), Λ≥−5.895×10−9\Lambda \ge -5.895 \times 10^{-9}Λ≥−5.895×10−9 (Csordas–Odlyzko–Smith–Varga 1993), Λ≥−2.63×10−9\Lambda \ge -2.63 \times 10^{-9}Λ≥−2.63×10−9 (Odlyzko 2000), Λ≥−1.15×10−11\Lambda \ge -1.15 \times 10^{-11}Λ≥−1.15×10−11 (Saouter–Gourdon–Demichel 2011). Rodgers and Tao closed the gap in 2020 by proving Λ≥0\Lambda \ge 0Λ≥0. In the other direction, de Bruijn's bound Λ≤1/2\Lambda \le 1/2Λ≤1/2 was sharpened to Λ<1/2\Lambda < 1/2Λ<1/2 by Ki–Kim–Lee (2009) and to Λ≤0.22\Lambda \le 0.22Λ≤0.22 by the Polymath 15 project (2019).

Setting

For a real number uuu put

Φ(u):=∑n=1∞(2π2n4e9u−3πn2e5u)exp⁡(−πn2e4u),\Phi(u) := \sum_{n=1}^{\infty}\bigl(2\pi^2 n^4 e^{9u} - 3\pi n^2 e^{5u}\bigr)\exp\bigl(-\pi n^2 e^{4u}\bigr),Φ(u):=n=1∑∞​(2π2n4e9u−3πn2e5u)exp(−πn2e4u),

a function that decays super-exponentially as ∣u∣→∞|u| \to \infty∣u∣→∞ and satisfies Φ(u)=Φ(−u)\Phi(u) = \Phi(-u)Φ(u)=Φ(−u). For each t∈Rt \in \mathbb{R}t∈R define the entire function

Ht(z):=∫0∞etu2 Φ(u) cos⁡(zu) du.H_t(z) := \int_0^{\infty} e^{t u^2}\,\Phi(u)\,\cos(z u)\,du .Ht​(z):=∫0∞​etu2Φ(u)cos(zu)du.

Each HtH_tHt​ is even and satisfies Ht(zˉ)=Ht(z)‾H_t(\bar z) = \overline{H_t(z)}Ht​(zˉ)=Ht​(z)​; the function H0H_0H0​ is 18ξ(12+iz2)\tfrac18 \xi\bigl(\tfrac12 + \tfrac{iz}{2}\bigr)81​ξ(21​+2iz​), so the Riemann hypothesis says exactly that every zero of H0H_0H0​ is real. Write

S:={ t∈R:every zero of Ht is real },Λ:=inf⁡S.S := \{\, t \in \mathbb{R} : \text{every zero of } H_t \text{ is real} \,\},\qquad \Lambda := \inf S .S:={t∈R:every zero of Ht​ is real},Λ:=infS.

By Pólya and Newman, SSS is the ray [Λ,∞)[\Lambda, \infty)[Λ,∞) with −∞<Λ≤1/2-\infty < \Lambda \le 1/2−∞<Λ≤1/2.

When Λ<t≤0\Lambda < t \le 0Λ<t≤0 the zeros of HtH_tHt​ are real, simple, symmetric about the origin and avoid the origin, so they can be listed as (xj(t))j∈Z∗(x_j(t))_{j \in \mathbb{Z}^*}(xj​(t))j∈Z∗​, indexed by the nonzero integers, with 0<x1(t)<x2(t)<⋯0 < x_1(t) < x_2(t) < \cdots0<x1​(t)<x2​(t)<⋯ and x−j(t)=−xj(t)x_{-j}(t) = -x_j(t)x−j​(t)=−xj​(t). The classical locations ξj\xi_jξj​ are defined for j≥1j \ge 1j≥1 by Ψ(ξj)=j\Psi(\xi_j) = jΨ(ξj​)=j with

Ψ(T):=T4πlog⁡T4π−T4π,\Psi(T) := \frac{T}{4\pi}\log\frac{T}{4\pi} - \frac{T}{4\pi},Ψ(T):=4πT​log4πT​−4πT​,

extended by ξ−j=−ξj\xi_{-j} = -\xi_jξ−j​=−ξj​; they are the positions the zeros would occupy if the Riemann–von Mangoldt counting formula were exact. Throughout, log⁡+x:=log⁡(2+∣x∣)\log_+ x := \log(2 + |x|)log+​x:=log(2+∣x∣).

Formalization targets

Goal — Newman's conjecture

Λ≥0,equivalentlyevery t with Ht having only real zeros satisfies t≥0.\Lambda \ge 0, \qquad\text{equivalently}\qquad \text{every } t \text{ with } H_t \text{ having only real zeros satisfies } t \ge 0 .Λ≥0,equivalentlyevery t with Ht​ having only real zeros satisfies t≥0.

The goal is stated in both forms simultaneously, so that it does not depend on any convention for the infimum of a set that might be empty or unbounded below.

Milestones

The milestone list follows the architecture of Rodgers–Tao, which is a proof by contradiction: every milestone is stated under the standing hypothesis Λ<0\Lambda < 0Λ<0 of that paper, in the time ranges the paper uses (Λ<t≤0\Lambda < t \le 0Λ<t≤0, then Λ/2≤t≤0\Lambda/2 \le t \le 0Λ/2≤t≤0, then Λ/4≤t≤0\Lambda/4 \le t \le 0Λ/4≤t≤0). In order: an upper bound for HtH_tHt​ near the real axis (Lemma 4); Riemann–von Mangoldt type counting formulae for the zeros of HtH_tHt​ (Theorem 9); the resulting macroscopic description of the zeros (Corollary 10); the equations of motion ∂txk=2∑j≠k(xk−xj)−1\partial_t x_k = 2\sum_{j \ne k} (x_k - x_j)^{-1}∂t​xk​=2∑j=k​(xk​−xj​)−1 (Theorem 11); a quantitative lower bound on gaps between zeros (Proposition 13); a bound on the time-integrated renormalized energy (Theorem 17); and a bound on that energy at time t=0t = 0t=0 (Proposition 26). The last of these says that at time zero the zeros are, on average, locally in the equilibrium configuration of an arithmetic progression, which contradicts known results on the local distribution of zeros of ζ\zetaζ.

Significance

Λ≥0\Lambda \ge 0Λ≥0 settles Newman's conjecture, and together with the Riemann hypothesis it would force Λ=0\Lambda = 0Λ=0. Unconditionally, it says that the zeros of ξ\xiξ are not in local equilibrium: infinitely often, gaps between consecutive zeros deviate from the mean spacing, which is what makes the pair correlation phenomenology of Montgomery and of Conrey–Ghosh–Goldston–Gonek–Heath-Brown incompatible with Λ<0\Lambda < 0Λ<0. Any proof of the Riemann hypothesis must therefore be compatible with the hypothesis being tight in this sense.

The theorem has a complete published proof (Rodgers–Tao, Forum of Mathematics, Pi, 2020); it is not an open problem. What is missing is a machine-checked proof. To the extent the material has been formalized at all, the underlying objects — the ξ\xiξ function, the heat flow HtH_tHt​, the counting function for zeros, the zero dynamics, the renormalized energies — are not available in Mathlib, so the mission produces reusable analytic infrastructure: bounds for a Fourier–Laplace type integral by the saddle point method, a Riemann–von Mangoldt counting argument via the argument principle, and a gradient-flow monotonicity framework for an infinite particle system with logarithmic interaction.

Difficulty

The obvious route to Λ≥0\Lambda \ge 0Λ≥0 is the one used for every previous lower bound: exhibit Lehmer pairs of ever higher quality, since if Λ\LambdaΛ were very negative the zeros of H0H_0H0​ would repel each other and unusually close pairs of zeta zeros could not exist. Producing an infinite sequence of Lehmer pairs of arbitrarily high quality is possible under the GUE hypothesis, but the known unconditional upper bounds for small gaps between zeta zeros are too weak, even assuming the Riemann hypothesis. The proof instead upgrades repulsion to relaxation to local equilibrium: it must control the zeros of HtH_tHt​ uniformly for Λ<t≤0\Lambda < t \le 0Λ<t≤0 at length scales as fine as log⁡T\log TlogT, with only the weaker counting formulae available for negative ttt (an error term O(log⁡+2T)O(\log_+^2 T)O(log+2​T) rather than O(log⁡+T)O(\log_+ T)O(log+​T)), and must make sense of a Hamiltonian and an energy that are given by divergent series, which requires truncation, renormalization, and careful control of all the resulting boundary terms.

Formalization scope

The Lean development commits to the following conventions. Φ\PhiΦ is a tsum over the positive integers and Ht(z)H_t(z)Ht​(z) is the Bochner integral over (0,∞)(0, \infty)(0,∞) of etu2Φ(u)cos⁡(zu)e^{tu^2}\Phi(u)\cos(zu)etu2Φ(u)cos(zu); no convergence or entireness statement is built into the definition. Λ\LambdaΛ is sInf of the set of admissible times, and the goal theorem also states the quantifier form "every admissible ttt is nonnegative", so it cannot be satisfied by a junk value of the infimum. The zero families (xj(t))(x_j(t))(xj​(t)) and the classical locations (ξj)(\xi_j)(ξj​) are not defined by choice functions: they enter the milestones as universally quantified functions Z→R\mathbb{Z} \to \mathbb{R}Z→R subject to explicit predicates saying exactly which sequences they are, so a milestone asserts something about every valid enumeration. Asymptotic notation is unfolded: O(⋅)O(\cdot)O(⋅) becomes an explicit existential constant, oT→∞(⋅)o_{T \to \infty}(\cdot)oT→∞​(⋅) an explicit ε\varepsilonε–T0T_0T0​ statement, and a principal value sum a limit of symmetric partial sums. Where a statement asserts the value of a time integral, absolute integrability is part of the conclusion, so the statement cannot be satisfied by the convention that a non-integrable function has integral zero.

One degeneracy is inherent to the source and is stated here explicitly: since the paper argues by contradiction, each milestone carries the hypothesis Λ<0\Lambda < 0Λ<0 (directly, or through a time range such as Λ<t≤0\Lambda < t \le 0Λ<t≤0). Once the goal theorem is proved, those hypotheses are unsatisfiable and the milestones become vacuously true. They are the intended attack path on the goal, not independent targets, and a solver who derives one of them from the goal theorem contributes nothing.

Contributions welcome: the analytic estimates for HtH_tHt​ (Lemma 4) and the counting formulae (Theorem 9) are independent of the dynamical part and are the natural entry points; Mathlib-level infrastructure on the argument principle, the saddle point method, and Stirling asymptotics for Γ\GammaΓ in vertical strips is reusable well beyond this mission.

Selected references

  • B. Rodgers and T. Tao, The de Bruijn–Newman constant is non-negative, Forum of Mathematics, Pi 8 (2020), e6. https://doi.org/10.1017/fmp.2020.6
  • N. G. de Bruijn, The roots of trigonometric integrals, Duke Math. J. 17 (1950), 197–226. https://doi.org/10.1215/S0012-7094-50-01720-0
  • C. M. Newman, Fourier transforms with only real zeros, Proc. Amer. Math. Soc. 61 (1976), 246–251. https://doi.org/10.1090/S0002-9939-1976-0434982-5
  • G. Csordas, W. Smith and R. S. Varga, Lehmer pairs of zeros, the de Bruijn–Newman constant Λ\LambdaΛ, and the Riemann hypothesis, Constr. Approx. 10 (1994), 107–129. https://doi.org/10.1007/BF01205170
  • H. L. Montgomery, The pair correlation of zeros of the zeta function, Proc. Sympos. Pure Math. XXIV (1973), 181–193. https://doi.org/10.1090/pspum/024
  • J. B. Conrey, A. Ghosh, D. Goldston, S. M. Gonek and D. R. Heath-Brown, On the distribution of gaps between zeros of the zeta-function, Q. J. Math. 36 (1985), 43–51. https://doi.org/10.1093/qmath/36.1.43
  • D. H. J. Polymath, Effective approximation of heat flow evolution of the Riemann ξ\xiξ function, and a new upper bound for the de Bruijn–Newman constant, Res. Math. Sci. 6 (2019), 31. https://doi.org/10.1007/s40687-019-0193-1
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Captain: Lucas

Rudin PMA VI: The Riemann-Stieltjes IntegralTextbook

Motivation

Chapter 6 of Walter Rudin's Principles of Mathematical Analysis (3rd edition, McGraw-Hill, 1976) constructs the Riemann–Stieltjes integral ∫abf dα\int_a^b f\,d\alpha∫ab​fdα: the Riemann integral with the increments Δxi\Delta x_iΔxi​ of the variable replaced by the increments Δαi=α(xi)−α(xi−1)\Delta \alpha_i = \alpha(x_i) - \alpha(x_{i-1})Δαi​=α(xi​)−α(xi−1​) of a monotonically increasing integrator α\alphaα. Taking α(x)=x\alpha(x) = xα(x)=x recovers the ordinary Riemann integral; taking α\alphaα a step function turns integrals into sums, so series and integrals become special cases of one construction. This is the reason Rudin develops the theory in this generality: it unifies Chapter 3's series with the integral, and it is the natural setting for the Fourier coefficients of Chapter 8.

The chapter's capstone is the fundamental theorem of calculus (Theorem 6.21): an integrable function which is the derivative of some FFF integrates to F(b)−F(a)F(b) - F(a)F(b)−F(a).

This mission is the sixth in a series formalizing Rudin Chapters 1–11; it uses the uniform continuity of Mission IV and the mean value theorem of Mission V.

Setting

A partition PPP of [a,b][a,b][a,b] is a finite set of points a=x0≤x1≤⋯≤xn=ba = x_0 \le x_1 \le \dots \le x_n = ba=x0​≤x1​≤⋯≤xn​=b, with increments Δαi=α(xi)−α(xi−1)\Delta \alpha_i = \alpha(x_i) - \alpha(x_{i-1})Δαi​=α(xi​)−α(xi−1​) for a monotonically increasing α\alphaα. For a bounded real fff put Mi=sup⁡[xi−1,xi]fM_i = \sup_{[x_{i-1},x_i]} fMi​=sup[xi−1​,xi​]​f, mi=inf⁡[xi−1,xi]fm_i = \inf_{[x_{i-1},x_i]} fmi​=inf[xi−1​,xi​]​f, and

U(P,f,α)=∑i=1nMi Δαi,L(P,f,α)=∑i=1nmi Δαi.U(P,f,\alpha) = \sum_{i=1}^n M_i\,\Delta\alpha_i, \qquad L(P,f,\alpha) = \sum_{i=1}^n m_i\,\Delta\alpha_i .U(P,f,α)=i=1∑n​Mi​Δαi​,L(P,f,α)=i=1∑n​mi​Δαi​.

The upper and lower integrals are inf⁡PU(P,f,α)\inf_P U(P,f,\alpha)infP​U(P,f,α) and sup⁡PL(P,f,α)\sup_P L(P,f,\alpha)supP​L(P,f,α); fff is integrable with respect to α\alphaα, written f∈R(α)f \in \mathcal{R}(\alpha)f∈R(α), when they agree, and the common value is ∫abf dα\int_a^b f\,d\alpha∫ab​fdα. P′P'P′ refines PPP when every division point of PPP is one of P′P'P′. Writing R\mathcal{R}R for R(α)\mathcal{R}(\alpha)R(α) with α(x)=x\alpha(x) = xα(x)=x gives the Riemann integral ∫abf dx\int_a^b f\,dx∫ab​fdx.

Formalization targets

Goal — the fundamental theorem of calculus (Theorem 6.21)

f∈R on [a,b],F′=f on [a,b]  ⟹  ∫abf(x) dx=F(b)−F(a).f \in \mathcal{R} \text{ on } [a,b], \quad F' = f \text{ on } [a,b] \;\Longrightarrow\; \int_a^b f(x)\,dx = F(b) - F(a).f∈R on [a,b],F′=f on [a,b]⟹∫ab​f(x)dx=F(b)−F(a).

Milestones

P′ refines P⇒L(P,f,α)≤L(P′,f,α), U(P′,f,α)≤U(P,f,α)(6.4)P' \text{ refines } P \Rightarrow L(P,f,\alpha) \le L(P',f,\alpha),\ U(P',f,\alpha) \le U(P,f,\alpha) \qquad (6.4)P′ refines P⇒L(P,f,α)≤L(P′,f,α), U(P′,f,α)≤U(P,f,α)(6.4) ∫‾f dα≤∫‾f dα(6.5)\underline{\int} f\,d\alpha \le \overline{\int} f\,d\alpha \qquad (6.5)∫​fdα≤∫​fdα(6.5) f∈R(α)  ⟺  ∀ε>0 ∃P, U(P,f,α)−L(P,f,α)<ε(6.6)f \in \mathcal{R}(\alpha) \iff \forall \varepsilon>0\ \exists P,\ U(P,f,\alpha) - L(P,f,\alpha) < \varepsilon \qquad (6.6)f∈R(α)⟺∀ε>0 ∃P, U(P,f,α)−L(P,f,α)<ε(6.6) f continuous⇒f∈R(α)(6.8)f \text{ continuous} \Rightarrow f \in \mathcal{R}(\alpha) \qquad (6.8)f continuous⇒f∈R(α)(6.8) f monotone, α continuous⇒f∈R(α)(6.9)f \text{ monotone},\ \alpha \text{ continuous} \Rightarrow f \in \mathcal{R}(\alpha) \qquad (6.9)f monotone, α continuous⇒f∈R(α)(6.9) linearity of the integral(6.12a)\text{linearity of the integral} \qquad (6.12\mathrm{a})linearity of the integral(6.12a) monotonicity, additivity in the interval, and ∣ ⁣∫f dα∣≤M(α(b)−α(a))(6.12b,c,d)\text{monotonicity, additivity in the interval, and } \big|\!\int f\,d\alpha\big| \le M(\alpha(b)-\alpha(a)) \qquad (6.12\mathrm{b,c,d})monotonicity, additivity in the interval, and ​∫fdα​≤M(α(b)−α(a))(6.12b,c,d) α′∈R⇒(f∈R(α)  ⟺  fα′∈R), ∫f dα=∫fα′ dx(6.17)\alpha' \in \mathcal{R} \Rightarrow \big(f \in \mathcal{R}(\alpha) \iff f\alpha' \in \mathcal{R}\big),\ \int f\,d\alpha = \int f\alpha'\,dx \qquad (6.17)α′∈R⇒(f∈R(α)⟺fα′∈R), ∫fdα=∫fα′dx(6.17) change of variable through a strictly increasing φ(6.19)\text{change of variable through a strictly increasing } \varphi \qquad (6.19)change of variable through a strictly increasing φ(6.19) F(x)=∫axf dt is continuous, and F′(x0)=f(x0) where f is continuous(6.20)F(x) = \int_a^x f\,dt \text{ is continuous, and } F'(x_0) = f(x_0) \text{ where } f \text{ is continuous} \qquad (6.20)F(x)=∫ax​fdt is continuous, and F′(x0​)=f(x0​) where f is continuous(6.20) integration by parts(6.22)\text{integration by parts} \qquad (6.22)integration by parts(6.22)

Significance

The fundamental theorem is what makes the integral computable: it reduces integration to antidifferentiation and so links Chapters 5 and 6. Theorem 6.20 is its companion — it says the integral of a continuous function is an antiderivative — and together they show the two operations are mutually inverse to the extent that the hypotheses allow. Theorem 6.17 explains when a Stieltjes integral collapses to a Riemann integral with the density α′\alpha'α′, and it is the computational tool for integrators that are differentiable; the step-function case at the other extreme (Rudin's 6.15–6.16) is what turns sums into integrals.

Mathlib has no Riemann–Stieltjes integral: it has the Bochner integral, the interval integral, and a Lebesgue–Stieltjes measure, but the upper-and-lower-sum construction of Chapter 6 is absent. This mission therefore builds the object from Rudin's definitions and develops its basic theory; that development is reusable beyond this mission — Chapter 7's interchange theorem (7.16) and Chapter 8's Fourier coefficients are stated with respect to it.

Difficulty

Two obstacles are specific to formalizing this chapter. First, the upper and lower integrals are an infimum and a supremum over the set of all partitions, which is not a lattice-friendly index; every comparison between partitions goes through the common refinement, and Theorem 6.4 is the workhorse that makes such comparisons possible. Second, the fundamental theorem is proved by choosing a partition on which U−L<εU - L < \varepsilonU−L<ε and applying the mean value theorem on each subinterval, so the proof requires selecting an intermediate point per subinterval — a finite choice that is easy on paper and must be organized explicitly in Lean.

The integrator α\alphaα is only assumed monotone, so it may be discontinuous, and the theory must not assume otherwise: Theorem 6.9 needs continuity of α\alphaα precisely because it is not available in general.

Formalization scope

Conventions fixed by this mission:

  • A partition of [a, b] is Rudin.Partition a b: the number n of subintervals together with a monotone placement function x with x 0 = a and x n = b. Rudin allows xi−1=xix_{i-1} = x_ixi−1​=xi​, and so does this structure.
  • Rudin.upperSum, Rudin.lowerSum, Rudin.upperIntegral, Rudin.lowerIntegral, Rudin.RSIntegrable, Rudin.RSIntegral follow Definitions 6.1–6.2 literally, with sSup and sInf over the images f([xi−1,xi])f([x_{i-1},x_i])f([xi−1​,xi​]).
  • Since sSup/sInf on ℝ return 0 on unbounded sets, every statement carries Rudin's boundedness hypothesis for fff explicitly; likewise monotonicity of α\alphaα is assumed as MonotoneOn α (Set.Icc a b) rather than built into a type.
  • Rudin.RiemannIntegrable and Rudin.RiemannIntegral are the case α=id\alpha = \mathrm{id}α=id, in which the goal theorem and Theorems 6.20–6.22 are stated, matching Rudin.
  • Derivatives are HasDerivAt, so F' = f is stated pointwise on [a, b] with the value f x supplied, as in Rudin's hypothesis.

The goal is not vacuous, and not a restatement of a library lemma: the integral in it is the one defined in this mission, so a solution must connect the upper/lower sum construction to differentiation rather than quoting Mathlib's interval integral.

Selected references

  • Walter Rudin, Principles of Mathematical Analysis, 3rd edition, McGraw-Hill, 1976, Chapter 6 (pp. 120–142).
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Harmonic AnalysisMachine LearningProbability+1·Captain: Shuze Chen

The Nature of Statistical Learning Theory VI: Kernels Generating Regularized Fourier ExpansionsTextbook

Motivation

A support vector machine never computes its feature map. It only evaluates a kernel K(x,y)K(x, y)K(x,y), the inner product of the feature vectors of xxx and yyy. When the features are the first NNN terms of an expansion, or infinitely many terms damped by regularizing weights, the learning algorithm is practical only if that inner product has a closed form. Chapter 6 of V. N. Vapnik, The Nature of Statistical Learning Theory (2nd ed., Springer 2000, doi:10.1007/978-1-4757-3264-1), §6.3–6.5, gives such closed forms for the kernels generating orthogonal-polynomial, spline and Fourier expansions. It also states Theorem 6.1, which lifts any one-dimensional kernel to nnn dimensions. The book prints these identities without proof and cites classical sources (Mikhlin 1964; Gradshtein and Ryzhik 1980). Several of them, as printed, are off by a constant factor, which a formal check settles.

Setting

Kernels in this mission are real functions of two real variables (or of two vectors of Rn\mathbb R^nRn) of the form K(x,y)=∑iri ψi(x) ψi(y)K(x, y) = \sum_i r_i\, \psi_i(x)\, \psi_i(y)K(x,y)=∑i​ri​ψi​(x)ψi​(y), a finite or convergent sum over basis functions ψi\psi_iψi​ with weights ri≥0r_i \ge 0ri​≥0.

  • Orthonormal polynomials. P1,P2,…P_1, P_2, \dotsP1​,P2​,… are real polynomials with deg⁡Pk=k−1\deg P_k = k - 1degPk​=k−1 that are orthonormal for a measure μ\muμ on R\mathbb RR with finite moments. Kn(x,y)=∑k=1nPk(x)Pk(y)K_n(x, y) = \sum_{k=1}^n P_k(x) P_k(y)Kn​(x,y)=∑k=1n​Pk​(x)Pk​(y) is the kernel of the first nnn of them.
  • Hermite. Pk(x)=(−1)kex2(d/dx)ke−x2P_k(x) = (-1)^k e^{x^2} (d/dx)^k e^{-x^2}Pk​(x)=(−1)kex2(d/dx)ke−x2, and Hk(x)=μkPk(x)e−x2H_k(x) = \mu_k P_k(x) e^{-x^2}Hk​(x)=μk​Pk​(x)e−x2 with normalization constants μk\mu_kμk​ (6.23). The regularized kernel is ∑i≥0qiHi(x)Hi(y)\sum_{i \ge 0} q^i H_i(x) H_i(y)∑i≥0​qiHi​(x)Hi​(y) with 0≤q<10 \le q < 10≤q<1.
  • Tensor products. Given coordinatewise basis functions bib_ibi​ on a set XXX, the nnn-dimensional basis is bi1…in(x)=bi1(x1)⋯bin(xn)b_{i_1 \dots i_n}(x) = b_{i_1}(x^1) \cdots b_{i_n}(x^n)bi1​…in​​(x)=bi1​​(x1)⋯bin​​(xn) (6.25).
  • Splines. The truncated power (x−t)+d(x - t)^d_+(x−t)+d​ is 000 for x≤tx \le tx≤t and (x−t)d(x - t)^d(x−t)d for x>tx > tx>t. The spline kernel with infinitely many nodes on (0,a)(0, a)(0,a) is ∫0a(xj−t)+d(xi−t)+d dt+∑r=0dxjrxir\int_0^a (x_j - t)^d_+ (x_i - t)^d_+\, dt + \sum_{r=0}^d x_j^r x_i^r∫0a​(xj​−t)+d​(xi​−t)+d​dt+∑r=0d​xjr​xir​ for xj,xi∈[0,a]x_j, x_i \in [0, a]xj​,xi​∈[0,a].
  • Fourier. KN(x,xi)=12+∑k=1N(sin⁡kxsin⁡kxi+cos⁡kxcos⁡kxi)K_N(x, x_i) = \tfrac12 + \sum_{k=1}^N (\sin kx \sin kx_i + \cos kx \cos kx_i)KN​(x,xi​)=21​+∑k=1N​(sinkxsinkxi​+coskxcoskxi​) is the kernel of the trigonometric polynomials of degree NNN. Its regularized versions damp the kkk-th harmonic by qkq^kqk (0<q<10 < q < 10<q<1) or by 1/(1+γ2k2)1/(1 + \gamma^2 k^2)1/(1+γ2k2) (γ>0\gamma > 0γ>0).

Formalization targets

Goal: Eq. (6.33)

For γ>0\gamma > 0γ>0 and real xi,xjx_i, x_jxi​,xj​ with 0≤∣xi−xj∣≤2π0 \le |x_i - x_j| \le 2\pi0≤∣xi​−xj​∣≤2π, the series converges and

12+∑k=1∞cos⁡kxicos⁡kxj+sin⁡kxisin⁡kxj1+γ2k2=π2γ cosh⁡π−∣xi−xj∣γsinh⁡πγ.\frac12 + \sum_{k=1}^{\infty} \frac{\cos kx_i \cos kx_j + \sin kx_i \sin kx_j}{1 + \gamma^2 k^2} = \frac{\pi}{2\gamma}\, \frac{\cosh\frac{\pi - |x_i - x_j|}{\gamma}}{\sinh\frac{\pi}{\gamma}} .21​+k=1∑∞​1+γ2k2coskxi​coskxj​+sinkxi​sinkxj​​=2γπ​sinhγπ​coshγπ−∣xi​−xj​∣​​.

The only numbered theorem of the section, Theorem 6.1, is close to an unfolding of the definitions. The goal is therefore the deepest identity of the section that is correct as printed.

Milestones

  1. (6.21), Christoffel–Darboux. There is a constant ana_nan​ such that Kn(x,y)=anPn+1(x)Pn(y)−Pn(x)Pn+1(y)x−yK_n(x, y) = a_n \frac{P_{n+1}(x)P_n(y) - P_n(x)P_{n+1}(y)}{x - y}Kn​(x,y)=an​x−yPn+1​(x)Pn​(y)−Pn​(x)Pn+1​(y)​ for x≠yx \ne yx=y and Kn(x,x)=an[Pn+1′(x)Pn(x)−Pn′(x)Pn+1(x)]K_n(x, x) = a_n[P'_{n+1}(x)P_n(x) - P'_n(x)P_{n+1}(x)]Kn​(x,x)=an​[Pn+1′​(x)Pn​(x)−Pn′​(x)Pn+1​(x)].
  2. (6.24), Hermite kernel. For some constants μk\mu_kμk​: ∑i≥0qiHi(x)Hi(y)=1π(1−q2)exp⁡{2xyq1+q−(x−y)2q21−q2}\sum_{i \ge 0} q^i H_i(x)H_i(y) = \frac{1}{\sqrt{\pi(1-q^2)}} \exp\{\frac{2xyq}{1+q} - \frac{(x-y)^2q^2}{1-q^2}\}∑i≥0​qiHi​(x)Hi​(y)=π(1−q2)​1​exp{1+q2xyq​−1−q2(x−y)2q2​} for all 0≤q<10 \le q < 10≤q<1 and real x,yx, yx,y.
  3. Theorem 6.1. ∑(i1,…,in)bi1…in(x) bi1…in(y)=∏k=1n∑ibi(xk)bi(yk)\sum_{(i_1, \dots, i_n)} b_{i_1 \dots i_n}(x)\, b_{i_1 \dots i_n}(y) = \prod_{k=1}^n \sum_i b_i(x^k) b_i(y^k)∑(i1​,…,in​)​bi1​…in​​(x)bi1​…in​​(y)=∏k=1n​∑i​bi​(xk)bi​(yk), for finite bases or bases whose one-dimensional kernel converges.
  4. (6.26). ∏i=1n1π(1−q2)exp⁡{⋯ }=1(1−q2)n/2exp⁡{2(x∗y)q1+q−∣x−y∣2q21−q2}\prod_{i=1}^n \frac{1}{\sqrt{\pi(1-q^2)}} \exp\{\cdots\} = \frac{1}{(1-q^2)^{n/2}} \exp\{\frac{2(x*y)q}{1+q} - \frac{|x-y|^2q^2}{1-q^2}\}∏i=1n​π(1−q2)​1​exp{⋯}=(1−q2)n/21​exp{1+q2(x∗y)q​−1−q2∣x−y∣2q2​}.
  5. (6.30), splines. For d≥0d \ge 0d≥0, the spline kernel equals ∑r=0dCdr2d−r+1(xj∧xi)2d−r+1∣xj−xi∣r+∑r=0dxjrxir\sum_{r=0}^d \frac{C_d^r}{2d - r + 1} (x_j \wedge x_i)^{2d-r+1} |x_j - x_i|^r + \sum_{r=0}^d x_j^r x_i^r∑r=0d​2d−r+1Cdr​​(xj​∧xi​)2d−r+1∣xj​−xi​∣r+∑r=0d​xjr​xir​. For d=1d = 1d=1 this is 1+xjxi+12∣xj−xi∣(xj∧xi)2+(xj∧xi)3/31 + x_jx_i + \frac12|x_j - x_i|(x_j \wedge x_i)^2 + (x_j \wedge x_i)^3/31+xj​xi​+21​∣xj​−xi​∣(xj​∧xi​)2+(xj​∧xi​)3/3.
  6. Dirichlet kernel (p. 197). KN(x,xi)=12+∑k=1Ncos⁡k(x−xi)=sin⁡(2N+1)(x−xi)2/sin⁡x−xi2K_N(x, x_i) = \frac12 + \sum_{k=1}^N \cos k(x - x_i) = \sin\frac{(2N+1)(x - x_i)}{2} \big/ \sin\frac{x - x_i}{2}KN​(x,xi​)=21​+∑k=1N​cosk(x−xi​)=sin2(2N+1)(x−xi​)​/sin2x−xi​​ for x−xi∉2πZx - x_i \notin 2\pi\mathbb Zx−xi​∈/2πZ.
  7. (6.32), Poisson kernel. For 0<q<10 < q < 10<q<1: 12+∑k≥1qkcos⁡k(xi−xj)=1−q22(1−2qcos⁡(xi−xj)+q2)\frac12 + \sum_{k \ge 1} q^k \cos k(x_i - x_j) = \frac{1 - q^2}{2(1 - 2q\cos(x_i - x_j) + q^2)}21​+∑k≥1​qkcosk(xi​−xj​)=2(1−2qcos(xi​−xj​)+q2)1−q2​.

Milestones 2, 4 and 6 are stated exactly as printed and are believed false (see Formalization scope). A disproof of each is a complete answer.

Significance

The result itself. Each closed form replaces an infinite or high-dimensional inner product by a constant number of elementary operations. That is what makes the regularized Fourier, Hermite and spline kernels usable in an SVM. Theorem 6.1 is the mechanism by which every multidimensional kernel of Chapter 6 is obtained from a one-dimensional one. The constants matter in practice. A wrong prefactor rescales the kernel matrix, and so the effective regularization of the SVM solution.

Formalizing it. The identities themselves are classical (Christoffel 1858, Darboux 1878, Mehler 1866, and the Fourier series of cosh⁡\coshcosh on [0,2π][0, 2\pi][0,2π]). As far as a search of the platform shows, none is stated on Prove2Me in these forms. SpikedWishart.Separated.eq_299 (Open) is one Christoffel–Darboux instance for a specific Hermite family. AronszajnRK.Product.direct_product_kernel concerns reproducing-kernel Hilbert spaces, not finite or summable feature sums. The mission produces machine-checked versions of the book's catalogue, together with a formal verdict on the three displays that are off by a constant.

Difficulty

The goal and (6.32) are infinite-series identities with no ready-made counterpart in the library, and the goal holds only on ∣xi−xj∣≤2π|x_i - x_j| \le 2\pi∣xi​−xj​∣≤2π. Outside that range the left side is 2π2\pi2π-periodic and the right side is not, so no argument that ignores the range can succeed. The Christoffel–Darboux formula needs a theory of orthogonal polynomials for a general measure, which Mathlib does not yet provide. (6.24) involves the iterated derivatives of e−x2e^{-x^2}e−x2 and a doubly infinite parameter family. The spline identity requires evaluating a piecewise-polynomial integral exactly. Theorem 6.1 for infinite bases requires summability over a product index set ιn\iota^nιn. The three false displays (2, 4, 6) hide their error in a constant factor. Two of them still reduce to an identity a solver may expect to hold.

Formalization scope

Everything is over R\mathbb RR. Series are stated with HasSum, or as Summable together with an equation for tsum. A divergent series therefore never reads as 000. Sums over k≥1k \ge 1k≥1 are written over k∈Nk \in \mathbb Nk∈N with k+1k + 1k+1 in place of kkk. The Christoffel–Darboux polynomials are indexed as in the book (P1P_1P1​ is the constant), they are orthonormal up to Pn+1P_{n+1}Pn+1​, and the measure has all moments finite. The Hermite PkP_kPk​ is the physicists' family, defined through iteratedDeriv. It is not Mathlib's probabilists' Polynomial.hermite. The normalization constants of (6.24) are existentially quantified, since the book does not give them. The range of qqq in (6.24) and (6.26) is 0≤q<10 \le q < 10≤q<1: the book's 0≤q≤10 \le q \le 10≤q≤1 without the singular point q=1q = 1q=1. The Dirichlet display is stated where sin⁡x−xi2≠0\sin\frac{x - x_i}{2} \ne 0sin2x−xi​​=0. The goal adds γ>0\gamma > 0γ>0, which the page leaves unstated. Spline points lie in [0,a][0, a][0,a] with a>0a > 0a>0. In Theorem 6.1, the multidimensional kernel is the sum over multi-indices of products of basis functions, a statement to be proved and not the product of kernels by definition. A formalization that defined the nnn-dimensional kernel as ∏kK(xk,yk)\prod_k K(x^k, y^k)∏k​K(xk,yk) would make the theorem trivial, and is ruled out.

Beyond the paper. Three corrected variants sit beside the faithful statements. Each changes one clause only. dirichlet_kernel_corrected (finding F1) uses the denominator 2sin⁡x−xi22\sin\frac{x - x_i}{2}2sin2x−xi​​, since at N=0N = 0N=0 and x−xi=πx - x_i = \pix−xi​=π the printed display reads 12=1\frac12 = 121​=1. hermite_kernel_corrected (F2) takes Hk=μkPkH_k = \mu_k P_kHk​=μk​Pk​ without the Gaussian factor. At q=0q = 0q=0 the printed (6.24) forces μ02e−x2−y2=π−1/2\mu_0^2 e^{-x^2-y^2} = \pi^{-1/2}μ02​e−x2−y2=π−1/2 for all x,yx, yx,y, and the corrected form is Mehler's formula. hermite_kernel_multidim_corrected (F3) uses the prefactor (π(1−q2))−n/2(\pi(1 - q^2))^{-n/2}(π(1−q2))−n/2, since at n=1n = 1n=1, x=y=0x = y = 0x=y=0, q=0q = 0q=0 the printed (6.26) reads π−1/2=1\pi^{-1/2} = 1π−1/2=1. One further observation is recorded without a variant: (6.33) also holds for γ<0\gamma < 0γ<0, because both sides are even in γ\gammaγ.

Reusable beyond this mission are the two definitions (the physicists' Hermite functions and the truncated power) and any proof of the summable form of Theorem 6.1. Proofs, disproofs of the three false milestones, and general lemmas on Fourier series of cosh⁡\coshcosh and qkcos⁡kθq^k\cos k\thetaqkcoskθ are all welcome.

Selected references

  • V. N. Vapnik, The Nature of Statistical Learning Theory, 2nd ed., Springer, 2000. doi:10.1007/978-1-4757-3264-1
  • I. S. Gradshteyn and I. M. Ryzhik, Table of Integrals, Series, and Products, Academic Press, 1980 (7th ed. 2007). doi:10.1016/C2009-0-22516-5
  • G. Szegő, Orthogonal Polynomials, AMS Colloquium Publications 23, 1939 (Christoffel–Darboux formula, §3.2). doi:10.1090/coll/023
  • F. G. Mehler, Ueber die Entwicklung einer Function von beliebig vielen Variablen nach Laplaceschen Functionen höherer Ordnung, J. reine angew. Math. 66 (1866), 161–176. doi:10.1515/crll.1866.66.161
  • S. G. Mikhlin, Variational Methods in Mathematical Physics, Pergamon, 1964.
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Control TheoryEconomicsOperations Research·Captain: mikedeng1

Knowledge Accumulation, Privacy, and Growth in a Data Economy: The Decentralized Economy Grows at the Socially Optimal Rate on the Balanced Growth PathResearch Paper

Motivation

Data have become an input to innovation: firms use consumer data, together with research labor, to develop new products. Data differ from labor and capital in two ways. They are a by-product of consumption, so their supply is endogenous, and selling them costs consumers privacy. Cong, Xie and Zhang (arXiv:2109.10028, published in Management Science) put both features into a continuous-time semi-endogenous growth model in the tradition of Romer (1990) and Jones (1995). They then ask whether a decentralized market economy with data trading grows at the rate a social planner would choose.

The paper's headline has two halves. The first, which this mission formalizes, is analytical: on the balanced growth path the decentralized economy and the social planner grow at the same rates (Proposition 3). The second, that the market economy underemploys R&D labor and overuses data, is shown only numerically (§3.3, Figure 1) and is not part of the mission.

Setting

Time is continuous. The population is L(t)=L0entL(t)=L_0e^{nt}L(t)=L0​ent with n>0n>0n>0. Parameters: discount rate ρ>0\rho>0ρ>0; inverse elasticity of intertemporal substitution γ>0\gamma>0γ>0, γ≠1\gamma\neq1γ=1; privacy-disutility curvature σ>1\sigma>1σ>1; labor elasticity 0<β<10<\beta<10<β<1; marginal cost ψ>0\psi>0ψ>0 of intermediate goods; innovation efficiency η>0\eta>0η>0; data share 0<ξ<10<\xi<10<ξ<1; knowledge spillover 0<ζ<10<\zeta<10<ζ<1.

Varieties of intermediate goods N(t)N(t)N(t) accumulate through the innovation possibility frontier

N˙(t)=ηN(t)ζϕ(t)ξlR(t)1−ξL(t),\dot N(t)=\eta N(t)^\zeta\phi(t)^\xi l_R(t)^{1-\xi}L(t),N˙(t)=ηN(t)ζϕ(t)ξlR​(t)1−ξL(t),

where ϕ(t)\phi(t)ϕ(t) is the data each consumer sells and lR(t)l_R(t)lR​(t), lE(t)=1−lR(t)l_E(t)=1-l_R(t)lE​(t)=1−lR​(t) are the labor shares of R&D and final-good production.

The decentralized economy (§2). Per-capita consumption ccc obeys the Euler equation c˙/c=(r−ρ)/γ\dot c/c=(r-\rho)/\gammac˙/c=(r−ρ)/γ. The data price pϕp_\phipϕ​ obeys p˙ϕ/pϕ−(σ−1)ϕ˙/ϕ=r−ρ\dot p_\phi/p_\phi-(\sigma-1)\dot\phi/\phi=r-\rhop˙​ϕ​/pϕ​−(σ−1)ϕ˙​/ϕ=r−ρ. Data are bounded by consumption: ϕ˙/ϕ≤c˙/c\dot\phi/\phi\le\dot c/cϕ˙​/ϕ≤c˙/c. Monopolistic intermediate producers earn the profit π=KπlEL\pi=K_\pi l_ELπ=Kπ​lE​L and pay the wage w=KwNw=K_wNw=Kw​N. A patent is worth the present value

V(t)=∫t∞exp⁡(−∫tsr(τ) dτ)π(s) ds.V(t)=\int_t^\infty \exp\Big(-\int_t^s r(\tau)\,d\tau\Big)\pi(s)\,ds .V(t)=∫t∞​exp(−∫ts​r(τ)dτ)π(s)ds.

Free entry equates the marginal value of data and of labor in R&D with their prices: ηξNζϕξ−1lR1−ξV=pϕ\eta\xi N^\zeta\phi^{\xi-1}l_R^{1-\xi}V=p_\phiηξNζϕξ−1lR1−ξ​V=pϕ​ and η(1−ξ)NζϕξlR−ξV=w\eta(1-\xi)N^\zeta\phi^\xi l_R^{-\xi}V=wη(1−ξ)NζϕξlR−ξ​V=w.

The social planner (§3.2) maximizes the consumer's utility subject to the frontier, the resource constraint c=AβNlEc=A\beta Nl_Ec=AβNlE​ with A=(ψ/(1−β))1−1/βA=(\psi/(1-\beta))^{1-1/\beta}A=(ψ/(1−β))1−1/β, and lR+lE=1l_R+l_E=1lR​+lE​=1. The paper solves this problem through the necessary conditions of the current-value Hamiltonian, with shadow prices λ\lambdaλ and μ\muμ ((A.7)–(A.10)).

A balanced growth path (BGP) is a path on which every variable grows at a constant rate of its own, and the interest rate is a constant r∗r^*r∗. With D=(1−ζ)σ−ξ(1−γ)D=(1-\zeta)\sigma-\xi(1-\gamma)D=(1−ζ)σ−ξ(1−γ), write

g∗=σnD,gϕ∗=(1−γ)nD.g^*=\frac{\sigma n}{D},\qquad g^*_\phi=\frac{(1-\gamma)n}{D}.g∗=Dσn​,gϕ∗​=D(1−γ)n​.

Formalization targets

Goal: Proposition 3 (p. 11)

With γ>1\gamma>1γ>1, for a balanced growth path of the decentralized economy and one of the planner's system with the same parameters,

gcS=gc,gNS=gN,gϕS=gϕ,glRS=glR,glES=glE,g^S_c=g_c,\quad g^S_N=g_N,\quad g^S_\phi=g_\phi,\quad g^S_{l_R}=g_{l_R},\quad g^S_{l_E}=g_{l_E},gcS​=gc​,gNS​=gN​,gϕS​=gϕ​,glR​S​=glR​​,glE​S​=glE​​,

and the planner's per-capita output ANlEAN l_EANlE​ grows at gcg_cgc​. The goal states equality of rates, not their closed form.

Milestones

  1. Lemma A.1 (PDF p. 24): two positive shares with constant growth rates that sum to one have rate zero.
  2. (A.2) (PDF p. 24): on a decentralized BGP, V=π/(r∗−n)V=\pi/(r^*-n)V=π/(r∗−n) and V˙/V=n\dot V/V=nV˙/V=n.
  3. (A.3) and (A.5) (PDF p. 25): (ζ−1)gN+ξgϕ+n=0(\zeta-1)g_N+\xi g_\phi+n=0(ζ−1)gN​+ξgϕ​+n=0 and (ζ−γ)gN+(ξ−σ)gϕ+n=0(\zeta-\gamma)g_N+(\xi-\sigma)g_\phi+n=0(ζ−γ)gN​+(ξ−σ)gϕ​+n=0.
  4. Proposition 1 (p. 9): decentralized rates gc=gN=g∗g_c=g_N=g^*gc​=gN​=g∗, gϕ=gϕ∗g_\phi=g^*_\phigϕ​=gϕ∗​; the data constraint never binds; gϕ<0g_\phi<0gϕ​<0 when γ>1\gamma>1γ>1.
  5. (A.11) and (A.13) (PDF p. 27): on a planner BGP, gc=1γ(gN−σgϕ)g_c=\frac1\gamma(g_N-\sigma g_\phi)gc​=γ1​(gN​−σgϕ​) and (ζ−1)gN+ξgϕ+n=0(\zeta-1)g_N+\xi g_\phi+n=0(ζ−1)gN​+ξgϕ​+n=0.
  6. (A.15) (PDF p. 28): planner rates gc=gN=g∗g_c=g_N=g^*gc​=gN​=g∗, gϕ=gϕ∗g_\phi=g^*_\phigϕ​=gϕ∗​.

Significance

The result. The equilibrium is inefficient: monopoly pricing and the knowledge spillover drive a wedge between private and social returns to R&D. Proposition 3 says that this wedge acts on levels (the R&D labor share and data intensity), not on long-run growth rates. Those rates are pinned by population growth, preferences and the frontier's returns to scale, and are free of scale effects. This puts the paper in the semi-endogenous growth family and isolates where data policy can matter. Privacy regulation and data ownership change allocations, not the long-run growth rate.

Formalizing it. The proofs in the paper are short and use growth-form identities freely. The mission makes the model precise: what a balanced growth path is, which equations hold in levels, and where integrability and positivity enter. The definition layer (constant-growth paths, present values of profit streams, Hamiltonian necessary-condition systems for growth models) does not exist on the platform and is reusable for other continuous-time growth models. None of these results has been machine-checked before.

Difficulty

The individual steps are short, but each has a gap the paper leaves open:

  • The decentralized patent value is an improper integral. The identity V=π/(r∗−n)V=\pi/(r^*-n)V=π/(r∗−n) needs r∗>nr^*>nr∗>n, which the paper does not state at that point and which must be derived from convergence of (9).
  • Growth-form identities come from differentiating products of real powers of positive functions; "a product of powers is constant" must be turned into "its growth rate vanishes".
  • Lemma A.1 needs a genuine argument: a positive function with a nonzero constant growth rate leaves (0,1)(0,1)(0,1).
  • Proposition 1 solves a 2×22\times22×2 linear system. Its determinant is DDD; the BGP hypotheses must rule out D≤0D\le0D≤0.

The tempting shortcut is to work with the growth rates directly. That skips the content: the rates of a balanced growth path are not given numbers, they are derived from the level equations.

Formalization scope

  • Paths and time. All paths are functions R→R\mathbb R\to\mathbb RR→R; every condition is imposed for t>0t>0t>0 (the paper's [0,∞)[0,\infty)[0,∞); the endpoint does not affect growth rates). Constant growth means x(t)>0x(t)>0x(t)>0 and x˙(t)=g x(t)\dot x(t)=g\,x(t)x˙(t)=gx(t) for t>0t>0t>0.
  • Decentralized economy. Encoded by its equilibrium conditions in level form: (4), (5), (3) with s=0s=0s=0, (9) with integrability of the integrand, (13), (15), (17)–(19), positivity, and lE+lR=1l_E+l_R=1lE​+lR​=1. The consumer's and producers' optimization problems are not formalized; the paper itself uses only these first-order conditions and closed forms. Data processing cost θ=0\theta=0θ=0 (baseline).
  • Planner. Encoded by the Hamiltonian necessary conditions (25)–(27), (A.7)–(A.10). The optimal control problem (24) is not formalized (no Pontryagin principle in Mathlib); the planner's BGP is a BGP of this system.
  • Disclosed readings of the text.
    • The BGP is read as "each variable at its own constant rate", although p. 9 says "the same constant rate"; Proposition 1 itself has gϕ∗≠g∗g^*_\phi\ne g^*gϕ∗​=g∗.
    • "Consumption grows with output" (PDF p. 25) is part of the decentralized BGP definition, since the paper never derives it.
    • Labor-market clearing is the equality used in every proof, not the inequality of p. 7.
    • The sign gϕ∗<0g^*_\phi<0gϕ∗​<0 in (21) is stated only under γ>1\gamma>1γ>1; for 0<γ<10<\gamma<10<γ<1 it is positive.
    • γ>1\gamma>1γ>1 is kept in Proposition 3 as printed, though the rate comparison does not use it.
  • Ruled-out trivialization. A formalization in which a BGP is a tuple of numbers satisfying (A.3), (A.5), (A.11), (A.13) would make the goal a linear-algebra exercise. Here the hypotheses are the level equations with derivatives. Positivity and integrability are part of the definitions, so junk values of Real.rpow and of the Bochner integral are excluded. Both BGP notions were checked to be inhabited at the paper's Table 2 calibration.
  • Welcome contributions. Lemmas on products of real powers of constant-growth functions, present values of exponentially growing streams, and proofs of the milestones in order.

Selected references

  • L. W. Cong, D. Xie, L. Zhang, Knowledge Accumulation, Privacy, and Growth in a Data Economy, arXiv:2109.10028v1, 2021; later published in Management Science. https://arxiv.org/abs/2109.10028
  • P. M. Romer, Endogenous Technological Change, Journal of Political Economy 98(5), S71–S102, 1990. https://doi.org/10.1086/261725
  • C. I. Jones, R&D-Based Models of Economic Growth, Journal of Political Economy 103(4), 759–784, 1995. https://doi.org/10.1086/262002
  • C. I. Jones, C. Tonetti, Nonrivalry and the Economics of Data, American Economic Review 110(9), 2819–2858, 2020. https://doi.org/10.1257/aer.20191330
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Category TheoryDifferential GeometryMathematical Physics·Captain: Alien60

Continuum Weatherall: Poincaré Lemma and Potentials vs. Field Strengths on a Vector SpaceResearch Paper

Motivation

Philosophers of physics use category theory to decide when a formulation of a theory carries excess structure. Weatherall (2016) represents each formulation of electromagnetism as a category of models and the passage from potentials to field strengths as the functor A↦F=dAA \mapsto F = dAA↦F=dA. A functor that is not full forgets structure, one that is not essentially surjective forgets properties, and one that is not faithful forgets stuff. Weatherall's §4 argues on Minkowski space that the potential formulation with gauge transformations as arrows is related to the field-strength formulation by a functor that is full and essentially surjective. His footnote 9 sets topology aside, and the erratum to his Proposition 2 (arXiv v2, p. 15) records that the gauge-theoretic functor is not faithful, because constant gauge transformations act trivially on fields.

On a contractible spacetime these facts all rest on one theorem: the Poincaré lemma, which says closed differential forms are exact. A companion mission (Weatherall 2016: Potentials vs. Field Strengths on a Finite 2-Complex) proves the discrete version, in which fullness, faithfulness and essential surjectivity are equivalent to the vanishing of H1H^1H1, H0H^0H0 and H2H^2H2 of a cell complex. This mission is the continuum version on a vector space, built on Mathlib's exterior derivative.

Timeline. The explicit radial homotopy operator proof of the Poincaré lemma is standard in textbooks; it is the proof of Theorem 4-11 in Spivak's Calculus on Manifolds (1965). Antiexact forms and the same operator are studied in Kycia (2020). Mathlib has the exterior derivative extDeriv with d2=0d^2 = 0d2=0. In 2025 Kudryashov proved the degree-1 case for convex sets, stated for 1-forms written as E → E →L F with a symmetric derivative. Mathlib has no Poincaré lemma in higher degree, no de Rham cohomology and no Hodge star.

Setting

Let EEE be a real normed space, for example Rn\mathbb R^nRn, and FFF a real Banach space of field values. A differential kkk-form is a map ω:E→E[∧k]→LF\omega : E \to E[\wedge^k]\to_L Fω:E→E[∧k]→L​F that assigns to each point a continuous alternating kkk-linear map. Smooth means C∞C^\inftyC∞ (ContDiff ℝ ∞). The exterior derivative is Mathlib's extDeriv:

dω(x)(v0,…,vk)=∑i=0k(−1)i Dω(x)(vi)(v0,…,vi^,…,vk).d\omega(x)(v_0,\dots,v_k) = \sum_{i=0}^{k} (-1)^i\, D\omega(x)(v_i)(v_0,\dots,\widehat{v_i},\dots,v_k).dω(x)(v0​,…,vk​)=i=0∑k​(−1)iDω(x)(vi​)(v0​,…,vi​​,…,vk​).

A function χ:E→F\chi : E \to Fχ:E→F is a 0-form, and dχd\chidχ is its derivative viewed as a 1-form (grad). The radial homotopy operator sends a (k+1)(k+1)(k+1)-form ω\omegaω to the kkk-form

(Kω)(x)(v1,…,vk)=∫01tk ω(tx)(x,v1,…,vk) dt.(K\omega)(x)(v_1,\dots,v_k) = \int_0^1 t^k\, \omega(tx)(x, v_1,\dots,v_k)\, dt .(Kω)(x)(v1​,…,vk​)=∫01​tkω(tx)(x,v1​,…,vk​)dt.

Field equations enter through an arbitrary predicate PPP on 2-forms. For example P(F)  ⟺  ⋆d⋆F=JP(F) \iff {\star d \star F} = JP(F)⟺⋆d⋆F=J once a metric is chosen, and P≡TrueP \equiv \mathrm{True}P≡True in vacuum. The categories are:

  • Fld P (Weatherall's EM1): smooth closed 2-forms BBB with P(B)P(B)P(B), with only identity arrows.
  • Pot P (EM2 with gauge arrows, fn. 15): smooth 1-forms AAA with P(dA)P(dA)P(dA). An arrow A→A′A \to A'A→A′ is a smooth χ:E→F\chi : E \to Fχ:E→F with A+dχ=A′A + d\chi = A'A+dχ=A′, and arrows compose by adding gauge functions.
  • fieldStrength P : Pot P ⥤ Fld P: the functor A↦dAA \mapsto dAA↦dA, which sends every gauge arrow to an identity.

The cohomology conditions are elementary Props:

  • H0=0H^0 = 0H0=0: smooth χ\chiχ with dχ=0d\chi = 0dχ=0 implies χ=0\chi = 0χ=0.
  • H1=0H^1 = 0H1=0: every smooth closed 1-form is dχd\chidχ for a smooth χ\chiχ.
  • H2=0H^2 = 0H2=0 on the PPP-sector: every smooth closed 2-form BBB with P(B)P(B)P(B) is dAdAdA for a smooth AAA.

Formalization targets

Goal: the continuum classification

For every PPP that admits at least one potential:

fieldStrength P is full and essentially surjective,faithful  ⟺  F is trivial,\texttt{fieldStrength}\ P \text{ is full and essentially surjective},\qquad \text{faithful} \iff F \text{ is trivial},fieldStrength P is full and essentially surjective,faithful⟺F is trivial, H1=0,H2=0,H0=0  ⟺  F is trivial.H^1 = 0,\qquad H^2 = 0,\qquad H^0 = 0 \iff F \text{ is trivial}.H1=0,H2=0,H0=0⟺F is trivial.

So the potential description with gauge arrows forgets only stuff, namely the constant gauge transformations, and nothing else on a vector space.

Milestones

  1. The radial homotopy operator preserves smoothness.
  2. The homotopy formula d(Kω)+K(dω)=ωd(K\omega) + K(d\omega) = \omegad(Kω)+K(dω)=ω for smooth ω\omegaω of degree k+1≥1k+1 \ge 1k+1≥1.
  3. The Poincaré lemma: a smooth closed form of degree ≥1\ge 1≥1 has a smooth primitive.
  4. Degree 0: for differentiable χ\chiχ, dχ=0d\chi = 0dχ=0 holds iff χ\chiχ is constant.
  5. H1=0H^1 = 0H1=0 and H2=0H^2 = 0H2=0 in the potentials language.
  6. Constants act freely and transitively on gauge arrows AoA′A o A'AoA′ by χ↦χ+c\chi \mapsto \chi + cχ↦χ+c, so Hom(A,A′)\mathrm{Hom}(A, A')Hom(A,A′) is empty or an FFF-torsor.
  7. The structural equivalences, which mirror the discrete mission: full   ⟺  H1=0\iff H^1 = 0⟺H1=0, faithful   ⟺  H0=0\iff H^0 = 0⟺H0=0, essentially surjective   ⟺  H2=0\iff H^2 = 0⟺H2=0.

Four supporting statements isolate the reusable ingredients of Milestone 2:

  • An alternating-sum identity for alternating maps.
  • An interior-product identity for Mathlib's alternatizeUncurryFin.
  • Differentiation of KωK\omegaKω under the integral sign.
  • The radial fundamental theorem of calculus.

Significance

The result. The goal makes precise, on Rn\mathbb R^nRn and with any field equation, the claim behind Weatherall's §4: up to the constants H0=FH^0 = FH0=F, potentials modulo gauge carry no more information than field strengths. With the discrete mission, it shows that the three ways of forgetting information correspond to H1H^1H1, H0H^0H0 and H2H^2H2 in both settings. The continuum version is metric-free. Maxwell's equations, sources or any other field equation enter only through PPP, so the classification holds for all of them at once.

Formalizing it. The homotopy formula and the Poincaré lemma for Mathlib's extDeriv in arbitrary degree are not in Mathlib. They are prerequisites for de Rham cohomology of manifolds, for the homotopy invariance of de Rham cohomology, and for any formal treatment of gauge potentials, Chern–Simons terms or Hamiltonian mechanics that uses local primitives. The classical proof is a textbook argument; the remaining work is to formalize it against Mathlib's alternating-map API. Machine-checked versions exist elsewhere only in other representations: Mathlib proves degree 1 for 1-forms written as E → E →L F on convex sets, and this platform's Rudin chapter 10 mission has proved Poincaré's lemma (Rudin, Theorem 10.39) as Rudin.ch10_poincare_lemma and Rudin.ch10_primitive_of_closed, for its own coefficient-style KForm on convex open subsets of Rn\mathbb R^nRn. A bridge from those statements to Mathlib's extDeriv would be a welcome contribution.

Difficulty

The obstacle is the homotopy formula in general degree. Each side involves the alternatization alternatizeUncurryFin of a derivative, the insertion curryLeft of the position vector as the first argument, and Fin.removeNth reindexing. Matching the two sides requires the signs (−1)i(-1)^i(−1)i from moving an argument to the front to cancel exactly against those of ddd. The degree-1 shortcut through Mathlib's existing curve-integral Poincaré lemma does not generalize, because it uses a different representation of 1-forms and has no analogue in degree 2, which the essential-surjectivity clause needs. A second, routine obstacle is smoothness of KωK\omegaKω: EEE need not be finite-dimensional, so differentiating under the integral needs bounds that are uniform in t∈[0,1]t \in [0,1]t∈[0,1] near each point.

Formalization scope

  • Forms. Forms are Mathlib's E → E [⋀^Fin k]→L[ℝ] F and the exterior derivative is extDeriv. "Smooth" is ContDiff ℝ ∞, where ∞ means C∞C^\inftyC∞, not analytic. EEE is any real normed space, not necessarily finite-dimensional or complete, and FFF is a real Banach space (CompleteSpace F), so the integral defining KKK is the Bochner integral.
  • Domain. The domain is the whole space EEE, which is star-shaped about 000. Open subsets and manifolds are out of scope.
  • Categories. Fld P is a Mathlib Discrete category. Pot P has a hand-written Category instance whose arrows are the structure GaugeHom. Fullness, faithfulness and essential surjectivity are Mathlib's Functor.Full, Functor.Faithful and Functor.EssSurj.
  • Non-triviality. Statements that need an object assume [Nonempty (Pot P)], meaning the field equation has a solution. Without it Pot P is empty and faithfulness and fullness hold vacuously. The cohomology conditions are explicit statements about extDeriv and grad, not definitions that make a target hold by construction. The goal fixes nothing about PPP.
  • Symmetries. Spacetime symmetries are not included as arrows; as in the discrete mission, the categories compare potentials and fields over the fixed space EEE, and the only non-identity arrows are gauge transformations.
  • No metric. No Hodge star or metric appears. Duality and 1-form symmetries are out of scope.
  • Reusable infrastructure. The definitions file proves smoothness of extDeriv, d2=0d^2 = 0d2=0 in the form used here, and the gauge invariance d(A+dχ)=dAd(A + d\chi) = dAd(A+dχ)=dA. The homotopy operator, the homotopy formula and the Poincaré lemma are stated for arbitrary degree and are intended for reuse in de Rham and gauge-theory missions. Contributions toward a Mathlib-quality homotopy-operator API are welcome.

Selected references

  • J. O. Weatherall, "Understanding Gauge", Philosophy of Science 83 (2016) 1039–1049. arXiv:1505.02229, doi:10.1086/687936. §4: EM1/EM2, Proposition 1, footnotes 9 and 15; the erratum to Proposition 2 is on p. 15 of arXiv v2.
  • M. Spivak, Calculus on Manifolds, W. A. Benjamin, 1965. Theorem 4-11 (Poincaré lemma) and its proof via the operator III, which is KKK above.
  • R. A. Kycia, "The Poincaré lemma, antiexact forms, and fermionic quantum harmonic oscillator", Results in Mathematics 75 (2020) 122. arXiv:1908.02349, doi:10.1007/s00025-020-01247-8.
  • J. Nguyen, N. J. Teh, L. Wells, "Why surplus structure is not superfluous", British Journal for the Philosophy of Science 71 (2020). arXiv:1712.01228.
  • Y. Kudryashov, Mathlib, MeasureTheory/Integral/CurveIntegral/Poincare.lean (Poincaré lemma for 1-forms on convex sets), mathlib4 PR #24019.
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