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Functional AnalysisMathematical Physics·Captain: mikedeng1

Mathematical Methods in Quantum Mechanics IV: The Min-Max Principle and Temple's InequalityTextbook

Motivation

In quantum mechanics the energy levels of a system are the eigenvalues of a self-adjoint Hamiltonian AAA, and for almost every Hamiltonian of interest (atoms with more than one electron, molecules) they cannot be computed in closed form. What can be computed are expectation values ⟨ψ,Aψ⟩\langle \psi, A\psi\rangle⟨ψ,Aψ⟩ of explicit trial functions ψ\psiψ. The min-max principle turns such numbers into rigorous statements about the eigenvalues: every trial computation gives an upper bound, and the optimal choices reproduce the eigenvalues exactly. It goes back to Fischer (1905) for quadratic forms in finitely many variables and to Courant (1920) for differential operators; Temple (1928) added the matching lower bound. This mission formalizes the version for unbounded self-adjoint operators with essential spectrum, as stated in Chapter 4 of Teschl's Mathematical Methods in Quantum Mechanics (AMS GSM 99, 2009), where eigenvalues below the essential spectrum are characterized and estimated.

Setting

Let H\mathfrak HH be a complex Hilbert space, with inner product ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle⟨⋅,⋅⟩ conjugate linear in the first argument. An operator AAA is a linear map defined on a subspace D(A)⊆H\mathfrak D(A) \subseteq \mathfrak HD(A)⊆H, its domain; AAA is self-adjoint if D(A)\mathfrak D(A)D(A) is dense and AAA equals its adjoint. The resolvent set ρ(A)\rho(A)ρ(A) is the set of z∈Cz \in \mathbb Cz∈C for which A−z:D(A)→HA - z : \mathfrak D(A) \to \mathfrak HA−z:D(A)→H is a bijection with bounded inverse, and the spectrum is σ(A)=C∖ρ(A)\sigma(A) = \mathbb C \setminus \rho(A)σ(A)=C∖ρ(A). For self-adjoint AAA, σ(A)⊆R\sigma(A) \subseteq \mathbb Rσ(A)⊆R.

For z∈Cz \in \mathbb Cz∈C the eigenspace is Ker⁡(A−z)={ψ∈D(A)∣Aψ=zψ}\operatorname{Ker}(A - z) = \{\psi \in \mathfrak D(A) \mid A\psi = z\psi\}Ker(A−z)={ψ∈D(A)∣Aψ=zψ}; zzz is an eigenvalue when it is nonzero, and its dimension is the multiplicity. The discrete spectrum σd(A)\sigma_d(A)σd​(A) consists of the eigenvalues that are isolated points of σ(A)\sigma(A)σ(A) and have finite multiplicity, and the essential spectrum is σess(A)=σ(A)∖σd(A)\sigma_{ess}(A) = \sigma(A) \setminus \sigma_d(A)σess​(A)=σ(A)∖σd​(A).

Let Σ=inf⁡σess(A)∈[−∞,+∞]\Sigma = \inf \sigma_{ess}(A) \in [-\infty, +\infty]Σ=infσess​(A)∈[−∞,+∞] (+∞+\infty+∞ if σess(A)\sigma_{ess}(A)σess​(A) is empty). The numbers E1≤E2≤E3≤⋯E_1 \le E_2 \le E_3 \le \cdotsE1​≤E2​≤E3​≤⋯ are the eigenvalues of AAA below Σ\SigmaΣ, listed in increasing order and repeated according to multiplicity; if there are only NNN of them, En=ΣE_n = \SigmaEn​=Σ for n>Nn > Nn>N. For vectors ψ1,…,ψm∈H\psi_1, \dots, \psi_m \in \mathfrak Hψ1​,…,ψm​∈H let

U(ψ1,…,ψm)={ψ∈D(A)∣∥ψ∥=1, ψ⊥ψ1,…,ψm}.U(\psi_1, \dots, \psi_m) = \{\psi \in \mathfrak D(A) \mid \|\psi\| = 1,\ \psi \perp \psi_1, \dots, \psi_m\}.U(ψ1​,…,ψm​)={ψ∈D(A)∣∥ψ∥=1, ψ⊥ψ1​,…,ψm​}.

Some statements involve the spectral projections PA(Ω)P_A(\Omega)PA​(Ω) of AAA, for Borel sets Ω⊆R\Omega \subseteq \mathbb RΩ⊆R: the projection-valued measure with A=∫λ dPA(λ)A = \int \lambda\, dP_A(\lambda)A=∫λdPA​(λ). With the spectral measures μψ(Ω)=⟨ψ,PA(Ω)ψ⟩\mu_\psi(\Omega) = \langle \psi, P_A(\Omega)\psi\rangleμψ​(Ω)=⟨ψ,PA​(Ω)ψ⟩, the form domain is Q(A)={ψ∣∫∣λ∣ dμψ(λ)<∞}\mathfrak Q(A) = \{\psi \mid \int |\lambda|\, d\mu_\psi(\lambda) < \infty\}Q(A)={ψ∣∫∣λ∣dμψ​(λ)<∞}, and on it ⟨ψ,Aψ⟩\langle \psi, A\psi\rangle⟨ψ,Aψ⟩ means ∫λ dμψ(λ)\int \lambda\, d\mu_\psi(\lambda)∫λdμψ​(λ).

Formalization targets

Goal: the min-max principle (Theorem 4.10)

For self-adjoint AAA and every n≥1n \ge 1n≥1,

En=sup⁡ψ1,…,ψn−1∈H inf⁡ψ∈U(ψ1,…,ψn−1)⟨ψ,Aψ⟩.E_n = \sup_{\psi_1, \dots, \psi_{n-1} \in \mathfrak H} \ \inf_{\psi \in U(\psi_1, \dots, \psi_{n-1})} \langle \psi, A\psi\rangle .En​=ψ1​,…,ψn−1​∈Hsup​ ψ∈U(ψ1​,…,ψn−1​)inf​⟨ψ,Aψ⟩.

Both sides are extended real numbers; the infimum over an empty set is +∞+\infty+∞.

Milestones

  • Theorem 2.19 (the case n=1n = 1n=1 and its mirror image): inf⁡σ(A)=inf⁡ψ∈D(A),∥ψ∥=1⟨ψ,Aψ⟩\inf \sigma(A) = \inf_{\psi \in \mathfrak D(A), \|\psi\| = 1} \langle\psi, A\psi\rangleinfσ(A)=infψ∈D(A),∥ψ∥=1​⟨ψ,Aψ⟩ and sup⁡σ(A)=sup⁡ψ∈D(A),∥ψ∥=1⟨ψ,Aψ⟩\sup \sigma(A) = \sup_{\psi \in \mathfrak D(A), \|\psi\| = 1} \langle\psi, A\psi\ranglesupσ(A)=supψ∈D(A),∥ψ∥=1​⟨ψ,Aψ⟩.
  • Theorem 4.12 (i): if ψ1,…,ψk∈Q(A)\psi_1, \dots, \psi_k \in \mathfrak Q(A)ψ1​,…,ψk​∈Q(A) are linearly independent and ⟨ψ,Aψ⟩<λ∥ψ∥2\langle \psi, A\psi\rangle < \lambda\|\psi\|^2⟨ψ,Aψ⟩<λ∥ψ∥2 for every nonzero ψ∈span⁡{ψj}\psi \in \operatorname{span}\{\psi_j\}ψ∈span{ψj​}, then dim⁡Ran⁡PA((−∞,λ))≥k\dim \operatorname{Ran} P_A((-\infty,\lambda)) \ge kdimRanPA​((−∞,λ))≥k; with >>>, dim⁡Ran⁡PA((λ,∞))≥k\dim \operatorname{Ran} P_A((\lambda,\infty)) \ge kdimRanPA​((λ,∞))≥k.
  • Theorem 4.12 (ii): if ψ1,…,ψk∈D(A)\psi_1, \dots, \psi_k \in \mathfrak D(A)ψ1​,…,ψk​∈D(A) are linearly independent, λ1<λ2\lambda_1 < \lambda_2λ1​<λ2​, and ∥(A−λ2+λ12)ψ∥<λ2−λ12∥ψ∥\|(A - \tfrac{\lambda_2+\lambda_1}{2})\psi\| < \tfrac{\lambda_2-\lambda_1}{2}\|\psi\|∥(A−2λ2​+λ1​​)ψ∥<2λ2​−λ1​​∥ψ∥ for every nonzero ψ\psiψ in their span, then dim⁡Ran⁡PA((λ1,λ2))≥k\dim \operatorname{Ran} P_A((\lambda_1,\lambda_2)) \ge kdimRanPA​((λ1​,λ2​))≥k.
  • Corollary 4.11: if A,BA, BA,B are self-adjoint, D(A)⊆D(B)\mathfrak D(A) \subseteq \mathfrak D(B)D(A)⊆D(B) and ⟨ψ,(A−B)ψ⟩≥0\langle \psi, (A - B)\psi\rangle \ge 0⟨ψ,(A−B)ψ⟩≥0 on D(A)\mathfrak D(A)D(A), then En(A)≥En(B)E_n(A) \ge E_n(B)En​(A)≥En​(B) for all n≥1n \ge 1n≥1.
  • Theorem 4.13 (Temple's inequality): if λ1<λ2\lambda_1 < \lambda_2λ1​<λ2​, ψ∈D(A)\psi \in \mathfrak D(A)ψ∈D(A), ∥ψ∥=1\|\psi\| = 1∥ψ∥=1, λ=⟨ψ,Aψ⟩∈(λ1,λ2)\lambda = \langle \psi, A\psi\rangle \in (\lambda_1, \lambda_2)λ=⟨ψ,Aψ⟩∈(λ1​,λ2​) and σ(A)∩(λ1,λ2)={E}\sigma(A) \cap (\lambda_1, \lambda_2) = \{E\}σ(A)∩(λ1​,λ2​)={E}, then
λ−∥(A−λ)ψ∥2λ2−λ≤E≤λ+∥(A−λ)ψ∥2λ−λ1.\lambda - \frac{\|(A-\lambda)\psi\|^2}{\lambda_2 - \lambda} \le E \le \lambda + \frac{\|(A-\lambda)\psi\|^2}{\lambda - \lambda_1}.λ−λ2​−λ∥(A−λ)ψ∥2​≤E≤λ+λ−λ1​∥(A−λ)ψ∥2​.

Significance

The min-max principle is the standard tool for comparing eigenvalues of different operators: Corollary 4.11 (monotonicity under operator inequalities) follows from it, and with it the stability of eigenvalues under perturbations, Dirichlet–Neumann bracketing and the Rayleigh–Ritz method used in computational quantum chemistry. Theorem 4.12 converts a finite-dimensional computation into a lower bound for the number of eigenvalues in an interval, and Temple's inequality supplies lower bounds on an eigenvalue to complement the variational upper bounds, which is what makes numerical eigenvalue enclosures rigorous.

All of these results are classical and proved in the literature. What is not available is a machine-checked version for unbounded operators: Mathlib has the Courant–Fischer characterization only for finite-dimensional or compact self-adjoint operators, and existing formal developments of Temple's inequality and min-max levels treat bounded operators. This mission formalizes the unbounded case, with the essential spectrum and the counting of eigenvalues by multiplicity made explicit, and with the edge cases (operators unbounded below, empty essential spectrum) covered by extended-real values.

Difficulty

The central difficulty is that EnE_nEn​ is defined by spectral data (which points of the spectrum are isolated eigenvalues of finite multiplicity, and how many there are below a given level), while the right-hand side is defined by expectation values on the domain. Relating the two needs the spectral theorem for unbounded operators: for every level below Σ\SigmaΣ the spectral subspace must be shown to be finite dimensional and spanned by eigenvectors, and for the level Σ\SigmaΣ itself one needs infinite-dimensional spectral subspaces in every neighbourhood, which is where the essential spectrum enters. When En=ΣE_n = \SigmaEn​=Σ the supremum and infimum need not be attained, so the finite-dimensional argument with eigenvectors does not transfer. For Corollary 4.11 and Temple's inequality the hypotheses concern only the operator and one vector, while the conclusions concern the spectrum.

Formalization scope

The formalization uses Lean 4 with Mathlib. Operators are partially defined linear maps (LinearPMap, H →ₗ.[ℂ] H) on a complex Hilbert space; self-adjointness is Mathlib's IsSelfAdjoint, which includes a dense domain. The Hilbert space is not assumed separable. The spectrum is the resolvent spectrum defined above, not Mathlib's Banach-algebra spectrum, and for self-adjoint operators it enters through its real points. Eigenspace dimensions are cardinals (Module.rank). EnE_nEn​ is defined from the spectrum, the essential spectrum and these dimensions, as an element of EReal, indexed from n=1n = 1n=1; if AAA is unbounded below its value is −∞-\infty−∞, and if the essential spectrum is empty and the eigenvalues run out it is +∞+\infty+∞. The min-max identity is stated in EReal, with ⟨ψ,Aψ⟩\langle\psi, A\psi\rangle⟨ψ,Aψ⟩ entering through its real part.

A formalization that defines EnE_nEn​ as the min-max expression itself would make the goal true by definition. This is ruled out: EnE_nEn​ is defined only from the spectrum, the essential spectrum and the dimensions of eigenspaces.

The spectral theorem is not part of this mission. Theorem 4.12 takes a projection-valued measure PPP on the Borel sets of R\mathbb RR as data, together with the hypothesis that A=∫λ dP(λ)A = \int \lambda\, dP(\lambda)A=∫λdP(λ) (domain {ψ∣∫λ2dμψ<∞}\{\psi \mid \int \lambda^2 d\mu_\psi < \infty\}{ψ∣∫λ2dμψ​<∞} and ⟨ψ,Aψ⟩=∫λ dμψ\langle\psi, A\psi\rangle = \int \lambda\, d\mu_\psi⟨ψ,Aψ⟩=∫λdμψ​), which is the form the spectral theorem guarantees; PAP_APA​ is then PPP, and Q(A)\mathfrak Q(A)Q(A) and the quadratic form are defined from it. Nothing else the book derives is taken as a hypothesis. The goal, Theorem 2.19, Corollary 4.11 and Temple's inequality use no projection-valued measure. Corollary 4.11 states the domain inclusion D(A)⊆D(B)\mathfrak D(A) \subseteq \mathfrak D(B)D(A)⊆D(B) explicitly, as the meaning of A−B≥0A - B \ge 0A−B≥0.

A complete development needs the spectral theorem for unbounded self-adjoint operators (or an equivalent functional calculus), the identification of σess\sigma_{ess}σess​ with the points where spectral projections have infinite rank, and the orthogonality of eigenspaces. These are reusable across the rest of the book. Proofs of any milestone, and of lemmas connecting the resolvent spectrum with spectral projections, are welcome.

Selected references

  • G. Teschl, Mathematical Methods in Quantum Mechanics, With Applications to Schrödinger Operators, Graduate Studies in Mathematics 99, American Mathematical Society, 2009. doi:10.1090/gsm/099. Theorem 2.19 (p. 77), Section 4.3–4.4 (pp. 117–120), essential spectrum (p. 145).
  • E. Fischer, Über quadratische Formen mit reellen Koeffizienten, Monatshefte für Mathematik und Physik 16 (1905), 234–249. doi:10.1007/BF01693781.
  • R. Courant, Über die Eigenwerte bei den Differentialgleichungen der mathematischen Physik, Mathematische Zeitschrift 7 (1920), 1–57. doi:10.1007/BF01199396.
  • G. Temple, The theory of Rayleigh's principle as applied to continuous systems, Proceedings of the Royal Society of London A 119 (1928), 276–293. doi:10.1098/rspa.1928.0098.
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Functional AnalysisMathematical Physics·Captain: mikedeng1

Mathematical Methods in Quantum Mechanics XI: Weyl's Limit Circle / Limit Point AlternativeTextbook

Why the endpoint behaviour of Sturm–Liouville operators matters

A quantum particle on a line or half-line, and the radial part of a particle in a spherically symmetric potential, are described by a Sturm–Liouville expression

τf=1r(−(pf′)′+qf)\tau f = \frac{1}{r}\big(-(pf')' + qf\big)τf=r1​(−(pf′)′+qf)

on an interval I=(a,b)I = (a, b)I=(a,b). The expression alone does not define a Hamiltonian: a self-adjoint operator needs a domain, and on a general interval the choice of domain is a choice of boundary conditions at aaa and bbb. Whether a boundary condition is needed at all depends on the behaviour of τ\tauτ near the endpoint. H. Weyl settled this in 1910 (Math. Ann. 68, 220–269) with his limit circle / limit point dichotomy: at each endpoint either all solutions of τu=zu\tau u = z uτu=zu are square integrable near it and a boundary condition must be imposed, or they are not and no condition is possible. This mission formalizes Sections 9.1–9.2 of G. Teschl, Mathematical Methods in Quantum Mechanics (AMS GSM 99, 2009), which develop the theory for coefficients that are only locally integrable, and culminate in Theorem 9.9, the Weyl alternative.

Setting

Let −∞≤a<b≤∞-\infty \le a < b \le \infty−∞≤a<b≤∞ and I=(a,b)I = (a,b)I=(a,b). The coefficients satisfy: p−1∈Lloc1(I)p^{-1} \in L^1_{loc}(I)p−1∈Lloc1​(I) with p>0p > 0p>0; q∈Lloc1(I)q \in L^1_{loc}(I)q∈Lloc1​(I) real-valued; r∈Lloc1(I)r \in L^1_{loc}(I)r∈Lloc1​(I) with r>0r > 0r>0. The Hilbert space is L2(I,r dx)L^2(I, r\,dx)L2(I,rdx) with ⟨f,g⟩=∫abf∗g r dx\langle f, g\rangle = \int_a^b f^* g\, r\,dx⟨f,g⟩=∫ab​f∗grdx.

A function fff is locally absolutely continuous, f∈ACloc(I)f \in AC_{loc}(I)f∈ACloc​(I), if it is an indefinite integral of a locally integrable function on III. The equation τf=g\tau f = gτf=g means that fff and its quasi-derivative pf′pf'pf′ both lie in ACloc(I)AC_{loc}(I)ACloc​(I) and −(pf′)′+qf=rg-(pf')' + qf = rg−(pf′)′+qf=rg almost everywhere. A solution of (τ−z)u=0(\tau - z)u = 0(τ−z)u=0, z∈Cz \in \mathbb{C}z∈C, is a complex-valued uuu with τu=zu\tau u = z uτu=zu in this sense. The maximal domain is

D(τ)={f∈L2(I,r dx)∣f,pf′∈ACloc(I), τf∈L2(I,r dx)}.\mathfrak{D}(\tau) = \{ f \in L^2(I, r\,dx) \mid f, pf' \in AC_{loc}(I),\ \tau f \in L^2(I, r\,dx) \}.D(τ)={f∈L2(I,rdx)∣f,pf′∈ACloc​(I), τf∈L2(I,rdx)}.

The modified Wronskian is Wx(f1,f2)=f1(x)(pf2′)(x)−(pf1′)(x)f2(x)W_x(f_1, f_2) = f_1(x)(pf_2')(x) - (pf_1')(x) f_2(x)Wx​(f1​,f2​)=f1​(x)(pf2′​)(x)−(pf1′​)(x)f2​(x), with no complex conjugation, and Wa(f1,f2)=lim⁡x→aWx(f1,f2)W_a(f_1, f_2) = \lim_{x \to a} W_x(f_1, f_2)Wa​(f1​,f2​)=limx→a​Wx​(f1​,f2​), WbW_bWb​ likewise.

τ\tauτ is limit circle (l.c.) at aaa if there is a v∈D(τ)v \in \mathfrak{D}(\tau)v∈D(τ) with Wa(v∗,v)=0W_a(v^*, v) = 0Wa​(v∗,v)=0 and Wa(v,f)≠0W_a(v, f) \ne 0Wa​(v,f)=0 for some f∈D(τ)f \in \mathfrak{D}(\tau)f∈D(τ); otherwise it is limit point (l.p.) at aaa. The same holds at bbb. A function uuu is square integrable near aaa if ∫ac∣u∣2r dx<∞\int_a^c |u|^2 r\,dx < \infty∫ac​∣u∣2rdx<∞ for some c∈Ic \in Ic∈I.

Formalization targets

Goal: the Weyl alternative (Theorem 9.9)

For every Sturm–Liouville expression as above,

τ is l.c. at a  ⟺  for one z0∈C, all solutions of (τ−z0)u=0 are square integrable near a,\tau \text{ is l.c. at } a \iff \text{for one } z_0 \in \mathbb{C}, \text{ all solutions of } (\tau - z_0)u = 0 \text{ are square integrable near } a,τ is l.c. at a⟺for one z0​∈C, all solutions of (τ−z0​)u=0 are square integrable near a,

and if τ\tauτ is l.c. at aaa, then for every z∈Cz \in \mathbb{C}z∈C all solutions of (τ−z)u=0(\tau - z)u = 0(τ−z)u=0 are square integrable near aaa. The same two statements hold at bbb.

Milestones

  1. Theorem 9.1. For rg∈Lloc1(I)rg \in L^1_{loc}(I)rg∈Lloc1​(I), c∈Ic \in Ic∈I, α,β∈C\alpha, \beta \in \mathbb{C}α,β∈C, the problem (τ−z)f=g(\tau - z) f = g(τ−z)f=g, f(c)=αf(c) = \alphaf(c)=α, (pf′)(c)=β(pf')(c) = \beta(pf′)(c)=β has a unique solution, entire in zzz.
  2. Lemma 9.2. If u1,u2u_1, u_2u1​,u2​ solve (τ−z)u=0(\tau - z)u = 0(τ−z)u=0 with W(u1,u2)=1W(u_1, u_2) = 1W(u1​,u2​)=1, every solution of (τ−z)f=g(\tau - z)f = g(τ−z)f=g is given by the variation-of-constants formula (9.10).
  3. Eq. (9.7). For f,g∈D(τ)f, g \in \mathfrak{D}(\tau)f,g∈D(τ) the limits Wa(g∗,f)W_a(g^*, f)Wa​(g∗,f), Wb(g∗,f)W_b(g^*, f)Wb​(g∗,f) exist and ⟨g,τf⟩=Wa(g∗,f)−Wb(g∗,f)+⟨τg,f⟩\langle g, \tau f\rangle = W_a(g^*, f) - W_b(g^*, f) + \langle \tau g, f\rangle⟨g,τf⟩=Wa​(g∗,f)−Wb​(g∗,f)+⟨τg,f⟩ (the printed Wb−WaW_b - W_aWb​−Wa​ has the wrong sign for the Wronskian (9.5)).
  4. Lemma 9.5. If v∈D(τ)v \in \mathfrak{D}(\tau)v∈D(τ), Wa(v∗,v)=0W_a(v^*, v) = 0Wa​(v∗,v)=0 and Wa(v∗,f^)≠0W_a(v^*, \hat f) \ne 0Wa​(v∗,f^​)=0 for some f^∈D(τ)\hat f \in \mathfrak{D}(\tau)f^​∈D(τ), then Wa(v,f)=0⇔Wa(v,f∗)=0W_a(v, f) = 0 \Leftrightarrow W_a(v, f^*) = 0Wa​(v,f)=0⇔Wa​(v,f∗)=0, and Wa(v,f)=Wa(v,g)=0⇒Wa(g∗,f)=0W_a(v, f) = W_a(v, g) = 0 \Rightarrow W_a(g^*, f) = 0Wa​(v,f)=Wa​(v,g)=0⇒Wa​(g∗,f)=0.
  5. Theorem 9.6. The operator Af=τfAf = \tau fAf=τf on D(A)={f∈D(τ)∣Wa(v,f)=0 if l.c. at a, Wb(w,f)=0 if l.c. at b}\mathfrak{D}(A) = \{ f \in \mathfrak{D}(\tau) \mid W_a(v, f) = 0 \text{ if l.c. at } a,\ W_b(w, f) = 0 \text{ if l.c. at } b\}D(A)={f∈D(τ)∣Wa​(v,f)=0 if l.c. at a, Wb​(w,f)=0 if l.c. at b} is self-adjoint, and the set D1\mathfrak{D}_1D1​ of (9.21) is a core.
  6. Lemma 9.7. For z∈ρ(A)z \in \rho(A)z∈ρ(A) there are solutions uau_aua​, ubu_bub​ of (τ−z)u=0(\tau - z)u = 0(τ−z)u=0, square integrable near aaa resp. bbb and satisfying the boundary condition there, and (A−z)−1(A - z)^{-1}(A−z)−1 is the integral operator with the Green function (9.28).

Significance

The Weyl alternative turns a question about operators into a question about an ordinary differential equation. Whether a Schrödinger operator −d2/dx2+q-d^2/dx^2 + q−d2/dx2+q on a half-line needs a boundary condition at infinity, or whether −Δ+V-\Delta + V−Δ+V with a radial potential is essentially self-adjoint on smooth functions, reduces to checking square integrability of solutions for a single value of zzz. Combined with Theorem 9.6 it classifies the self-adjoint realizations with separated boundary conditions: none at an l.p. endpoint, a one-parameter family at an l.c. endpoint. The Green function of Lemma 9.7 is the starting point of the spectral theory of one-dimensional Schrödinger operators: Weyl–Titchmarsh mmm-functions, spectral transformations, and oscillation theory in the rest of Teschl's Chapter 9.

The results are classical and proved in many textbooks. The formal content is new: Mathlib has unbounded operators (LinearPMap) and their adjoints, but no Sturm–Liouville theory, no quasi-derivatives, no ODE existence theorem for measurable, locally integrable coefficients (its Picard–Lindelöf theorem needs Lipschitz right-hand sides), and no self-adjoint realizations of differential operators on general intervals.

Difficulty

The definition of limit circle refers only to D(τ)\mathfrak{D}(\tau)D(τ) and boundary limits of Wronskians, while the conclusion is about all solutions of an ODE for all z∈Cz \in \mathbb{C}z∈C. The two sides are linked only through self-adjoint operators: the passage from boundary Wronskians to square integrable solutions goes through the resolvent of a self-adjoint realization, which exists only for z∈ρ(A)z \in \rho(A)z∈ρ(A), and so only for nonreal zzz in general. Extending the conclusion to real zzz, where no resolvent is available, needs an argument of a different kind. On the ODE side, the coefficients are only locally integrable, so solutions are merely locally absolutely continuous, equations hold only almost everywhere, and every boundary quantity is a limit whose existence must itself be established.

Formalization scope

  • Interval and coefficients. The structure SLData bundles a,b∈a, b \ina,b∈ EReal with a<ba < ba<b (infinite endpoints allowed), p,q,r:R→Rp, q, r : \mathbb{R} \to \mathbb{R}p,q,r:R→R, and the standing hypotheses (i)–(iii) of p. 181; p,r>0p, r > 0p,r>0 pointwise on III. L2(I,r dx)L^2(I, r\,dx)L2(I,rdx) is Lp ℂ 2 for the measure r dxr\,dxrdx on III.
  • Regularity. ACloc(I)AC_{loc}(I)ACloc​(I) is encoded by its integral characterization. The quasi-derivative pf′pf'pf′ is the continuous function f[1]∈ACloc(I)f^{[1]} \in AC_{loc}(I)f[1]∈ACloc​(I) with f(y)−f(x)=∫xyf[1]/pf(y) - f(x) = \int_x^y f^{[1]}/pf(y)−f(x)=∫xy​f[1]/p, chosen by Classical.choose (it is unique on III). τf=g\tau f = gτf=g is (pf′)(y)−(pf′)(x)=∫xy(qf−rg)(pf')(y) - (pf')(x) = \int_x^y (qf - rg)(pf′)(y)−(pf′)(x)=∫xy​(qf−rg) with a local integrability clause. No smoothness of the coefficients and no C2C^2C2 solutions are assumed.
  • Boundary Wronskians WaW_aWa​, WbW_bWb​ are Filter.limUnder along x→ax \to ax→a, x→bx \to bx→b inside III. They are used only on D(τ)\mathfrak{D}(\tau)D(τ), where milestone (9.7) states that the limits exist. In Lemma 9.7, where uau_aua​ need not lie in D(τ)\mathfrak{D}(\tau)D(τ), the boundary condition is stated as a convergence.
  • Operators. Operators in L2(I,r dx)L^2(I, r\,dx)L2(I,rdx) are LinearPMaps; self-adjointness is Mathlib's IsSelfAdjoint. Theorem 9.6 asserts that an operator with graph {(f,τf)∣f∈D(A)}\{(f, \tau f) \mid f \in \mathfrak{D}(A)\}{(f,τf)∣f∈D(A)} exists (i.e. is well defined) and is self-adjoint. ρ(A)\rho(A)ρ(A) and (A−z)−1(A - z)^{-1}(A−z)−1 follow Teschl (2.66): a bounded two-sided inverse of A−zA - zA−z. No projection-valued measure or functional calculus is used.
  • Corrections to the printed text. Lemma 9.7 says "a solution uau_aua​ of (τ−z)u=g(\tau - z)u = g(τ−z)u=g"; the proof and (9.28) need (τ−z)u=0(\tau - z)u = 0(τ−z)u=0, which is what is stated. The condition at an endpoint in (9.21) is imposed only where τ\tauτ is l.c., as in (9.20). The second line of (9.10) is stated for quasi-derivatives. The boundary term of (9.7) is printed as Wb(g∗,f)−Wa(g∗,f)W_b(g^*, f) - W_a(g^*, f)Wb​(g∗,f)−Wa​(g∗,f); integration by parts with (9.5) gives Wa(g∗,f)−Wb(g∗,f)W_a(g^*, f) - W_b(g^*, f)Wa​(g∗,f)−Wb​(g∗,f) (check: p=r=1p = r = 1p=r=1, q=0q = 0q=0 on (0,1)(0,1)(0,1), f=x2f = x^2f=x2, g=1g = 1g=1), and the corrected identity is stated.
  • Ruling out trivialization. Limit circle is the Wronskian notion of p. 187, never "all solutions are square integrable", which would make the goal circular. The goal has no hypothesis beyond the standing assumptions on p,q,rp, q, rp,q,r.

A complete development needs a Carathéodory-type existence theorem for linear first-order systems with Lloc1L^1_{loc}Lloc1​ coefficients, the Lagrange identity with its boundary limits, Lemma 9.3 (a linear-algebra fact about functionals) and the computation of the closure and adjoint of the minimal operator (Lemma 9.4). The ODE layer and the L2(I,r dx)L^2(I, r\,dx)L2(I,rdx) operator layer can be reused for the Weyl–Titchmarsh theory, oscillation theory (Sec. 9.7) and one-particle Schrödinger operators (Ch. 10). Contributions that build them as general lemmas are welcome.

Selected references

  • G. Teschl, Mathematical Methods in Quantum Mechanics, With Applications to Schrödinger Operators, AMS Graduate Studies in Mathematics 99, 2009, Sections 9.1–9.2. https://doi.org/10.1090/gsm/099
  • H. Weyl, "Über gewöhnliche Differentialgleichungen mit Singularitäten und die zugehörigen Entwicklungen willkürlicher Funktionen", Math. Ann. 68 (1910), 220–269. https://doi.org/10.1007/BF01474161
  • J. Weidmann, Spectral Theory of Ordinary Differential Operators, Lecture Notes in Mathematics 1258, Springer, 1987. https://doi.org/10.1007/BFb0077960
  • A. Zettl, Sturm–Liouville Theory, Mathematical Surveys and Monographs 121, AMS, 2005. https://doi.org/10.1090/surv/121
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Functional AnalysisMathematical Physics·Captain: mikedeng1

Mathematical Methods in Quantum Mechanics II: The Spectral Theorem for Unbounded Self-Adjoint OperatorsTextbook

Motivation

In quantum mechanics an observable is a self-adjoint operator AAA on a complex Hilbert space H\mathfrak HH, and the dynamics is the Schrödinger equation i ddtψ(t)=Hψ(t)i\,\tfrac{d}{dt}\psi(t) = H\psi(t)idtd​ψ(t)=Hψ(t). In finite dimensions the solution is the matrix exponential e−itHψ(0)e^{-itH}\psi(0)e−itHψ(0), computed by diagonalizing HHH. The operators of physics (the Laplacian, Schrödinger operators with Coulomb potentials, position and momentum) are unbounded, defined only on a dense subspace, and have no eigenbasis in general. The spectral theorem is the substitute for diagonalization in this setting: it expresses every self-adjoint operator as an integral of the identity function against a family of orthogonal projections, and so gives meaning to f(A)f(A)f(A) for every Borel function fff, in particular to e−itAe^{-itA}e−itA and to the spectral projections χΩ(A)\chi_\Omega(A)χΩ​(A).

The theorem goes back to Hilbert (bounded symmetric forms, 1906) and was extended to unbounded self-adjoint operators by von Neumann (1929/30), Stone (1932) and Riesz. This mission follows the treatment in G. Teschl, Mathematical Methods in Quantum Mechanics (AMS Graduate Studies in Mathematics 99, 2009), Section 3.1: projection-valued measures, their functional calculus for bounded and unbounded functions, and the spectral theorem obtained from resolvents through the Herglotz representation of Borel transforms.

Setting

Let H\mathfrak HH be a complex Hilbert space, with inner product ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle⟨⋅,⋅⟩ conjugate linear in the first argument, and let L(H)\mathfrak L(\mathfrak H)L(H) be the bounded operators on it. An (unbounded) operator AAA is a linear map defined on a subspace D(A)⊆H\mathfrak D(A) \subseteq \mathfrak HD(A)⊆H; A⊆BA \subseteq BA⊆B means BBB extends AAA. AAA is self-adjoint if D(A)\mathfrak D(A)D(A) is dense and A∗=AA^* = AA∗=A, domains included.

The resolvent set of AAA is the set of z∈Cz \in \mathbb{C}z∈C for which A−z:D(A)→HA - z : \mathfrak D(A) \to \mathfrak HA−z:D(A)→H is a bijection with bounded inverse, and the spectrum is its complement, σ(A)=C∖ρ(A)\sigma(A) = \mathbb{C} \setminus \rho(A)σ(A)=C∖ρ(A).

A projection-valued measure assigns to every Borel set Ω⊆R\Omega \subseteq \mathbb{R}Ω⊆R an orthogonal projection P(Ω)=P(Ω)∗=P(Ω)2P(\Omega) = P(\Omega)^* = P(\Omega)^2P(Ω)=P(Ω)∗=P(Ω)2 such that P(R)=IP(\mathbb{R}) = \mathbb{I}P(R)=I and, for pairwise disjoint Borel sets Ωn\Omega_nΩn​, ∑nP(Ωn)ψ=P(⋃nΩn)ψ\sum_n P(\Omega_n)\psi = P(\bigcup_n \Omega_n)\psi∑n​P(Ωn​)ψ=P(⋃n​Ωn​)ψ for every vector ψ\psiψ (strong, not norm, σ\sigmaσ-additivity). Each ψ\psiψ gives the spectral measure μψ(Ω)=⟨ψ,P(Ω)ψ⟩=∥P(Ω)ψ∥2\mu_\psi(\Omega) = \langle\psi, P(\Omega)\psi\rangle = \|P(\Omega)\psi\|^2μψ​(Ω)=⟨ψ,P(Ω)ψ⟩=∥P(Ω)ψ∥2, a finite Borel measure of total mass ∥ψ∥2\|\psi\|^2∥ψ∥2, and by polarization the complex measures μφ,ψ(Ω)=⟨φ,P(Ω)ψ⟩\mu_{\varphi,\psi}(\Omega) = \langle\varphi, P(\Omega)\psi\rangleμφ,ψ​(Ω)=⟨φ,P(Ω)ψ⟩.

For a bounded Borel function fff the operator P(f)=∫f(λ) dP(λ)∈L(H)P(f) = \int f(\lambda)\,dP(\lambda) \in \mathfrak L(\mathfrak H)P(f)=∫f(λ)dP(λ)∈L(H) is the bounded operator with ⟨ψ,P(f)ψ⟩=∫f dμψ\langle\psi, P(f)\psi\rangle = \int f\,d\mu_\psi⟨ψ,P(f)ψ⟩=∫fdμψ​ for all ψ\psiψ. For an arbitrary Borel function fff it is the operator with domain

Df={ψ∈H  ∣  ∫R∣f(λ)∣2 dμψ(λ)<∞}\mathfrak D_f = \Big\{\psi \in \mathfrak H \;\Big|\; \int_{\mathbb{R}} |f(\lambda)|^2\, d\mu_\psi(\lambda) < \infty\Big\}Df​={ψ∈H​∫R​∣f(λ)∣2dμψ​(λ)<∞}

and ⟨ψ,P(f)ψ⟩=∫f dμψ\langle\psi, P(f)\psi\rangle = \int f\,d\mu_\psi⟨ψ,P(f)ψ⟩=∫fdμψ​ for ψ∈Df\psi \in \mathfrak D_fψ∈Df​. An operator TTT is normal if it is densely defined, D(T)=D(T∗)\mathfrak D(T) = \mathfrak D(T^*)D(T)=D(T∗) and ∥Tψ∥=∥T∗ψ∥\|T\psi\| = \|T^*\psi\|∥Tψ∥=∥T∗ψ∥ on D(T)\mathfrak D(T)D(T).

Formalization targets

Goal: the spectral theorem (Theorem 3.7)

For every self-adjoint operator AAA in H\mathfrak HH there is a unique projection-valued measure PAP_APA​ with

A=∫Rλ dPA(λ),A = \int_{\mathbb{R}} \lambda\, dP_A(\lambda),A=∫R​λdPA​(λ),

an equality of operators including their domains. Uniqueness is among projection-valued measures, compared on Borel sets.

Milestones

  • Theorem 3.1. For a projection-valued measure PPP, the map f↦P(f)f \mapsto P(f)f↦P(f) from bounded Borel functions (sup norm) to L(H)\mathfrak L(\mathfrak H)L(H) is a unital C∗C^*C∗-algebra homomorphism of norm one, ⟨P(g)φ,P(f)ψ⟩=∫g∗f dμφ,ψ\langle P(g)\varphi, P(f)\psi\rangle = \int g^* f\, d\mu_{\varphi,\psi}⟨P(g)φ,P(f)ψ⟩=∫g∗fdμφ,ψ​, and P(fn)→P(f)P(f_n) \to P(f)P(fn​)→P(f) strongly when fn→ff_n \to ffn​→f pointwise with sup⁡λ∣fn(λ)∣\sup_\lambda |f_n(\lambda)|supλ​∣fn​(λ)∣ bounded.
  • Theorem 3.2. For every Borel fff, the operator P(f)P(f)P(f) with D(P(f))=Df\mathfrak D(P(f)) = \mathfrak D_fD(P(f))=Df​ exists, is normal, and P(f)∗=P(f∗)P(f)^* = P(f^*)P(f)∗=P(f∗).
  • Lemma 3.5. αP(f)+βP(g)⊆P(αf+βg)\alpha P(f) + \beta P(g) \subseteq P(\alpha f + \beta g)αP(f)+βP(g)⊆P(αf+βg) with domain D∣f∣+∣g∣\mathfrak D_{|f|+|g|}D∣f∣+∣g∣​, and P(f)P(g)⊆P(fg)P(f)P(g) \subseteq P(fg)P(f)P(g)⊆P(fg) with domain Dg∩Dfg\mathfrak D_g \cap \mathfrak D_{fg}Dg​∩Dfg​.
  • Theorem 3.8. For self-adjoint AAA, σ(A)={λ∈R∣PA((λ−ε,λ+ε))≠0 for all ε>0}\sigma(A) = \{\lambda \in \mathbb{R} \mid P_A((\lambda-\varepsilon, \lambda+\varepsilon)) \ne 0 \text{ for all } \varepsilon > 0\}σ(A)={λ∈R∣PA​((λ−ε,λ+ε))=0 for all ε>0}.
  • Corollary 3.9. PA(σ(A))=IP_A(\sigma(A)) = \mathbb{I}PA​(σ(A))=I and PA(R∩ρ(A))=0P_A(\mathbb{R} \cap \rho(A)) = 0PA​(R∩ρ(A))=0.

A further supporting statement (not a milestone) records that μψ\mu_\psiμψ​ is a finite measure with μψ(Ω)=⟨ψ,P(Ω)ψ⟩=∥P(Ω)ψ∥2\mu_\psi(\Omega) = \langle\psi, P(\Omega)\psi\rangle = \|P(\Omega)\psi\|^2μψ​(Ω)=⟨ψ,P(Ω)ψ⟩=∥P(Ω)ψ∥2.

Significance

The result itself. The spectral theorem is the foundation of the rest of the book and of mathematical quantum mechanics generally. Stone's theorem and the time evolution e−itAe^{-itA}e−itA, the min-max principle, the RAGE theorem, the decomposition of the spectrum into absolutely continuous, singular continuous and pure point parts, Weyl's theorem on essential spectra and scattering theory are all statements about f(A)f(A)f(A) or PA(Ω)P_A(\Omega)PA​(Ω). Theorem 3.8 identifies the spectrum with the support of PAP_APA​, which is what makes spectral questions accessible to measure theory.

Formalizing it. The result is classical and fully proved in the literature. Mathlib has the continuous functional calculus for bounded normal elements of C∗C^*C∗-algebras and the finite-dimensional spectral theorem, but no projection-valued measures, no spectral integral of unbounded functions, and no spectral theorem for unbounded operators (LinearPMap). On Prove2Me the related published material is bounded or finite-dimensional (for example diagonalization of self-adjoint endomorphisms and the Fuglede–Putnam theorem). A formal proof here supplies the object f(A)f(A)f(A) that every later mission of this series currently has to take as data.

Difficulty

The obvious route through the bounded case fails. For bounded self-adjoint AAA one can build f(A)f(A)f(A) from polynomials by the sup norm on σ(A)\sigma(A)σ(A) and extend by monotone limits; for unbounded AAA there are no polynomials in AAA defined on a common useful domain and no sup-norm estimate. The standard reductions (the Cayley transform (A−i)(A+i)−1(A-i)(A+i)^{-1}(A−i)(A+i)−1, or the bounded resolvent (A−z)−1(A-z)^{-1}(A−z)−1) produce bounded normal operators whose spectral measures must then be transported back, and the domain D(A)\mathfrak D(A)D(A) must be recovered exactly as Dλ\mathfrak D_\lambdaDλ​; getting the domains right, not just the formulas on a core, is where unbounded arguments usually break. Beyond the domain issue, the projections PA(Ω)P_A(\Omega)PA​(Ω) are not given by any formula in AAA that Mathlib can evaluate: they have to be recovered from resolvent data, which in the book's development requires the Herglotz representation of Borel transforms and the Stieltjes inversion formula for finite measures, neither of which is in Mathlib. Uniqueness is also not automatic: it requires that a projection-valued measure is determined by the operator ∫λ dP(λ)\int \lambda\, dP(\lambda)∫λdP(λ) alone.

Formalization scope

H\mathfrak HH is {H : Type*} [NormedAddCommGroup H] [InnerProductSpace ℂ H] [CompleteSpace H]; separability is not assumed, since none of the stated results or their proofs in the book need it. Operators are LinearPMaps H →ₗ.[ℂ] H; self-adjointness is Mathlib's IsSelfAdjoint, which includes density. A projection-valued measure is a function Set ℝ → (H →L[ℂ] H) constrained on Borel sets only (IsProjValuedMeasure); uniqueness in the goal compares values on Borel sets. The spectral measure spectralMeasure P ψ is built with Measure.ofMeasurable from Ω↦∥P(Ω)ψ∥2\Omega \mapsto \|P(\Omega)\psi\|^2Ω↦∥P(Ω)ψ∥2. The spectral integral spectralIntegral P f is the operator with domain Df\mathfrak D_fDf​ and quadratic form ∫f dμψ\int f\,d\mu_\psi∫fdμψ​ (the predicate IsSpectralIntegral), selected by choice; its existence for Borel fff is part of the milestone for Theorem 3.2, not an assumption. The bounded calculus boundedSpectralIntegral is characterized the same way in L(H)\mathfrak L(\mathfrak H)L(H). The spectrum is the resolvent-based TeschlQM.Spectral.spectrum of Section 2.4, not Mathlib's spectrum ℂ of a Banach algebra element. In Theorems 3.8 and 3.9, PAP_APA​ enters as a projection-valued measure P with the hypothesis A = spectralIntegral P (fun x => x), which by the goal's uniqueness is exactly PAP_APA​.

Nothing is taken as data that the book derives. In particular the goal is not stated for "a projection-valued measure with A=∫λ dPA = \int\lambda\,dPA=∫λdP" given as a hypothesis, and PAP_APA​ is not defined by choosing such a measure: the goal quantifies existentially and uniquely over projection-valued measures, with self-adjointness of AAA as the only hypothesis.

Lemma 3.4 (spectral bases), Lemma 3.6 (the family PA(Ω)P_A(\Omega)PA​(Ω) built from the Herglotz representation) and the results of Sections 3.2–3.3 are not stated. A complete development needs finite Borel measures and L2L^2L2 spaces (in Mathlib), the Herglotz representation and Stieltjes inversion (the subject of the next mission of this series), and the adjoint theory of LinearPMap. The projection-valued measure and spectral-integral layer is reusable by every later mission of the series. Contributions of any milestone, of general lemmas about IsProjValuedMeasure (finite additivity, P(Ω1)P(Ω2)=P(Ω1∩Ω2)P(\Omega_1)P(\Omega_2) = P(\Omega_1 \cap \Omega_2)P(Ω1​)P(Ω2​)=P(Ω1​∩Ω2​), monotonicity), and of alternative proofs of the goal are welcome.

Selected references

  • G. Teschl, Mathematical Methods in Quantum Mechanics, With Applications to Schrödinger Operators, Graduate Studies in Mathematics 99, American Mathematical Society, 2009, Chapter 3. https://doi.org/10.1090/gsm/099
  • J. von Neumann, Allgemeine Eigenwerttheorie Hermitescher Funktionaloperatoren, Mathematische Annalen 102 (1930), 49–131. https://doi.org/10.1007/BF01782338
  • M. H. Stone, Linear Transformations in Hilbert Space and Their Applications to Analysis, AMS Colloquium Publications 15, 1932. https://doi.org/10.1090/coll/015
  • M. Reed and B. Simon, Methods of Modern Mathematical Physics I: Functional Analysis, Academic Press, 1980, Chapters VII–VIII. https://doi.org/10.1016/B978-0-12-585050-6.X5001-4
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Differential GeometryPartial Differential EquationsPure Mathematics·Captain: mikedeng1

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

Motivation

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

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

Setting

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

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

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

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

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

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

Formalization targets

Goal: Severi's theorem (Theorem 3.2.9)

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

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

Selected references

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

Tasty Bits of Several Complex Variables IV: Plurisubharmonic Functions and Hartogs PseudoconvexityTextbook

Motivation

In one complex variable every open set is the natural domain of some holomorphic function. In several variables this fails: by the Hartogs phenomenon, every function holomorphic on some domains extends to a strictly larger one. The domains that are "natural", the domains of holomorphy, are characterised by a convexity condition on the domain. Since the work of Levi (1910), Hartogs, Oka and Cartan–Thullen (1932), the way to state that condition intrinsically has been pseudoconvexity. The tool that makes it work is the plurisubharmonic function, the complex analogue of a convex function.

This mission formalizes the part of that theory that needs no partial differential equations: harmonic, subharmonic and plurisubharmonic functions; smoothing of plurisubharmonic functions; the characterizations of Hartogs pseudoconvexity; and the Cartan–Thullen theorem. The source is §2.4–2.6 of Jiří Lebl's open textbook Tasty Bits of Several Complex Variables (version 4.4, 2026), pp. 78–103.

Timeline, as the book presents it:

  • Hartogs (1906) found the extension phenomenon.
  • Levi (1910) found the boundary condition now called Levi pseudoconvexity.
  • Cartan and Thullen (1932) proved that domains of holomorphy are exactly the holomorphically convex domains.
  • Oka (1942–1953), Bremermann and Norguet (1954) solved the Levi problem: every pseudoconvex domain is a domain of holomorphy. The book states this result (its Theorem 2.6.2) but does not prove it.

Setting

Throughout, Cn\mathbb{C}^nCn carries the Euclidean norm ∥z∥=(∣z1∣2+⋯+∣zn∣2)1/2\|z\| = (|z_1|^2 + \dots + |z_n|^2)^{1/2}∥z∥=(∣z1​∣2+⋯+∣zn​∣2)1/2. A domain is a nonempty connected open set. For K,U⊂CnK, U \subset \mathbb{C}^nK,U⊂Cn, K⊂⊂UK \subset\subset UK⊂⊂U means that KKK is relatively compact in UUU: its closure is compact and contained in UUU.

Harmonic and subharmonic functions (one variable). A C2C^2C2 function fff on an open U⊂CU \subset \mathbb{C}U⊂C is harmonic if ∇2f=0\nabla^2 f = 0∇2f=0. A function f:U→R∪{−∞}f : U \to \mathbb{R} \cup \{-\infty\}f:U→R∪{−∞} is subharmonic if it is upper-semicontinuous and, for every disc Br(a)B_r(a)Br​(a) with Br(a)‾⊂U\overline{B_r(a)} \subset UBr​(a)​⊂U and every ggg continuous on Br(a)‾\overline{B_r(a)}Br​(a)​ and harmonic inside it, f≤gf \le gf≤g on ∂Br(a)\partial B_r(a)∂Br​(a) implies f≤gf \le gf≤g on Br(a)B_r(a)Br​(a).

Plurisubharmonic functions. For U⊂CnU \subset \mathbb{C}^nU⊂Cn open, f:U→R∪{−∞}f : U \to \mathbb{R} \cup \{-\infty\}f:U→R∪{−∞} is plurisubharmonic if it is upper-semicontinuous and ξ↦f(a+bξ)\xi \mapsto f(a + b\xi)ξ↦f(a+bξ) is subharmonic on {ξ:a+bξ∈U}\{\xi : a + b\xi \in U\}{ξ:a+bξ∈U} for all a,b∈Cna, b \in \mathbb{C}^na,b∈Cn.

Hulls and convexity. For a class F\mathcal{F}F of extended-real functions on UUU and K⊂UK \subset UK⊂U, the hull is

K^={x∈U:f(x)≤sup⁡y∈Kf(y) for all f∈F}.\widehat{K} = \{x \in U : f(x) \le \sup_{y \in K} f(y) \text{ for all } f \in \mathcal{F}\}.K={x∈U:f(x)≤y∈Ksup​f(y) for all f∈F}.

UUU is convex with respect to F\mathcal{F}F if K⊂⊂UK \subset\subset UK⊂⊂U implies K^⊂⊂U\widehat{K} \subset\subset UK⊂⊂U. For F={∣f∣:f∈O(U)}\mathcal{F} = \{|f| : f \in \mathcal{O}(U)\}F={∣f∣:f∈O(U)} this is holomorphic convexity, with hull K^U\widehat{K}_UKU​.

Hartogs pseudoconvexity. f:U→Rf : U \to \mathbb{R}f:U→R is an exhaustion function if {z∈U:f(z)<r}⊂⊂U\{z \in U : f(z) < r\} \subset\subset U{z∈U:f(z)<r}⊂⊂U for every rrr. A domain is Hartogs pseudoconvex if it admits a continuous plurisubharmonic exhaustion function.

Analytic discs. A closed analytic disc is a nonconstant holomorphic φ:D→Cn\varphi : \mathbb{D} \to \mathbb{C}^nφ:D→Cn that extends continuously to D‾\overline{\mathbb{D}}D. Its image is Δ=φ(D)\Delta = \varphi(\mathbb{D})Δ=φ(D) and its boundary is ∂Δ=φ(∂D)\partial\Delta = \varphi(\partial\mathbb{D})∂Δ=φ(∂D).

Formalization targets

Goal: Theorem 2.5.6

For a domain U⊊CnU \subsetneq \mathbb{C}^nU⊊Cn with ρ(z)=dist⁡(z,∂U)\rho(z) = \operatorname{dist}(z, \partial U)ρ(z)=dist(z,∂U), the following are equivalent:

(i) −log⁡ρ is plurisubharmonic;(ii) U is Hartogs pseudoconvex;\text{(i) } -\log\rho \text{ is plurisubharmonic};\quad \text{(ii) } U \text{ is Hartogs pseudoconvex};(i) −logρ is plurisubharmonic;(ii) U is Hartogs pseudoconvex; (iii) U is convex w.r.t. plurisubharmonic functions on U;(iv) ⋃α∂Δα⊂⊂U⇒⋃αΔα⊂⊂U\text{(iii) } U \text{ is convex w.r.t. plurisubharmonic functions on } U;\quad \text{(iv) } \textstyle\bigcup_\alpha \partial\Delta_\alpha \subset\subset U \Rightarrow \bigcup_\alpha \Delta_\alpha \subset\subset U(iii) U is convex w.r.t. plurisubharmonic functions on U;(iv) ⋃α​∂Δα​⊂⊂U⇒⋃α​Δα​⊂⊂U

for every collection of closed analytic discs Δα⊂U\Delta_\alpha \subset UΔα​⊂U.

Milestones

  • Proposition 2.4.3. A continuous fff is harmonic iff it has the mean-value property. An upper-semicontinuous fff is subharmonic iff f(a)≤12π∫02πf(a+reiθ) dθf(a) \le \frac{1}{2\pi}\int_0^{2\pi} f(a + re^{i\theta})\,d\thetaf(a)≤2π1​∫02π​f(a+reiθ)dθ whenever Δr(a)‾⊂U\overline{\Delta_r(a)} \subset UΔr​(a)​⊂U.
  • Proposition 2.4.7. Finite suprema of subharmonic functions are subharmonic, and so are arbitrary suprema that are finite and upper-semicontinuous.
  • Proposition 2.4.9. A C2C^2C2 function is plurisubharmonic iff its complex Hessian [∂2f/∂zˉk∂zℓ][\partial^2 f/\partial\bar z_k \partial z_\ell][∂2f/∂zˉk​∂zℓ​] is positive semidefinite.
  • Theorem 2.4.10. Every plurisubharmonic fff is the pointwise limit of smooth plurisubharmonic fϵ≥ff_\epsilon \ge ffϵ​≥f on Uϵ={z∈U:dist⁡(z,∂U)>ϵ}U_\epsilon = \{z \in U : \operatorname{dist}(z, \partial U) > \epsilon\}Uϵ​={z∈U:dist(z,∂U)>ϵ}.
  • Theorem 2.5.2 (Kontinuitätssatz, second version): (iii) implies (iv).
  • Lemma 2.5.7. Hartogs pseudoconvexity is a local property of the boundary.
  • Theorem 2.4.12 (Radó): a continuous function holomorphic off its zero set is holomorphic.
  • Theorem 2.6.3 (Cartan–Thullen): for a domain U⊊CnU \subsetneq \mathbb{C}^nU⊊Cn, being a domain of holomorphy, dist⁡(K,∂U)=dist⁡(K^U,∂U)\operatorname{dist}(K, \partial U) = \operatorname{dist}(\widehat{K}_U, \partial U)dist(K,∂U)=dist(KU​,∂U) for all K⊂⊂UK \subset\subset UK⊂⊂U, and holomorphic convexity are equivalent.

Significance

The result. Theorem 2.5.6 makes pseudoconvexity checkable. Condition (i) involves one explicitly given function of the domain's geometry. Condition (iv) involves only families of discs. Condition (ii) is the form the Levi problem and Hörmander's L2L^2L2 theory need. From these equivalences one gets, for example, that intersections and increasing unions of pseudoconvex domains are pseudoconvex, that pseudoconvexity is a biholomorphic invariant, and, with Lemma 2.5.7, that it is a local boundary property. In the smooth case that local property is Levi pseudoconvexity (Theorem 2.5.8, chapter III of this series). Cartan–Thullen supplies the other half of the picture for domains of holomorphy.

Formalizing it. All of these results are classical and proved in the book, apart from routine steps left as exercises. As far as is known, none of them is formalized in any proof assistant. Mathlib has harmonic functions (InnerProductSpace.HarmonicOnNhd) and the circle average, but no subharmonic or plurisubharmonic functions, no hulls and no pseudoconvexity. The Prove2Me corpus holds a one-variable subharmonic definition based on the sub-mean-value property and the one-directional mean-value property of harmonic functions; neither is the book's definition or statement. The mission would give Lean a first library of plurisubharmonic functions in Cn\mathbb{C}^nCn, with the definition matching the textbook.

Difficulty

The obvious route to (iv) ⇒ (i) of the goal would show −log⁡ρ-\log\rho−logρ is plurisubharmonic by computing a complex Hessian (Proposition 2.4.9). That fails: ρ\rhoρ is in general not even differentiable, so no Hessian is available. Several other steps also need measure theory with extended-real values. The sub-mean-value property requires Lebesgue integrals of upper-semicontinuous functions that may equal −∞-\infty−∞ on large sets. Smoothing requires convolution of such functions with a mollifier, and pointwise convergence in [−∞,∞)[-\infty, \infty)[−∞,∞). Suprema of families lose upper semicontinuity in general, which is why Proposition 2.4.7 carries that hypothesis. In Cartan–Thullen, holomorphic convexity alone must produce a holomorphic function on UUU that extends across no boundary point. Nothing in the hypothesis supplies such a function directly.

Formalization scope

  • Cn\mathbb{C}^nCn is EuclideanSpace ℂ (Fin n), so balls, ρ(z)\rho(z)ρ(z) = Metric.infDist z (frontier U), UϵU_\epsilonUϵ​ and dist⁡(K,∂U)\operatorname{dist}(K, \partial U)dist(K,∂U) are all Euclidean, as in the book. They are not sup-norm polydisc quantities.
  • Functions with values in R∪{−∞}\mathbb{R} \cup \{-\infty\}R∪{−∞} are EReal-valued with +∞+\infty+∞ excluded on UUU. Upper semicontinuity is UpperSemicontinuousOn for the order of EReal.
  • Hulls take suprema in EReal, and holomorphic hulls in [0,∞][0, \infty][0,∞], so no supremum takes a junk value. Set distances are infima in [0,∞][0, \infty][0,∞] (Metric.infEDist).
  • The circle mean in Proposition 2.4.3 (ii) is the Lebesgue integral of the positive part minus that of the negative part.
  • Holomorphic on an open set is DifferentiableOn ℂ, which is equivalent to the book's Definition 1.1.2 there.
  • A domain is IsOpen U ∧ IsConnected U. Relative compactness is compact closure contained in UUU.
  • Harmonic and subharmonic functions are defined only on open subsets of C=R2\mathbb{C} = \mathbb{R}^2C=R2. The book defines them on Rn\mathbb{R}^nRn, but only uses n=2n = 2n=2. This is the one restriction of scope.
  • A collection of analytic discs is a set of parametrizing maps, and Δα=φα(D)\Delta_\alpha = \varphi_\alpha(\mathbb{D})Δα​=φα​(D) as in Definition 1.4.5.
  • Definitions 1.4.5 and 2.1.1 are restated locally in the namespace LeblSCV.Pseudoconvex.

Several trivializing formalizations are ruled out. Plurisubharmonicity is not defined through the Hessian condition, so the mission does not reduce to C2C^2C2 functions. Nor is it defined by the sub-mean-value property, which would make Proposition 2.4.3 (ii) a tautology. ρ\rhoρ is not the sup-norm distance. Suprema, infima and integrals are nowhere allowed to default to 000 on empty, unbounded or non-integrable input.

A complete development needs:

  • mean values of upper-semicontinuous functions and the Poisson integral on discs (Theorem 2.4.2, not a milestone);
  • convolution with a radial mollifier on Cn\mathbb{C}^nCn;
  • Cauchy estimates on polydiscs.

The subharmonic and plurisubharmonic layer is reusable beyond this mission. Chapters on the Levi problem, the ∂ˉ\bar\partial∂ˉ-problem and Bergman kernels would all build on it. Proofs of the smaller milestones, and alternative arguments for the goal, are welcome.

Selected references

  • J. Lebl, Tasty Bits of Several Complex Variables: A Whirlwind Tour of the Subject, version 4.4, 2026. https://www.jirka.org/scv/scv.pdf
  • L. Hörmander, An Introduction to Complex Analysis in Several Variables, 3rd ed., North-Holland Mathematical Library 7, 1990 (the book's reference [H] for the Levi problem).
  • H. Cartan and P. Thullen, "Zur Theorie der Singularitäten der Funktionen mehrerer komplexen Veränderlichen: Regularitäts- und Konvergenzbereiche", Mathematische Annalen 106 (1932), 617–647.
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Harmonic AnalysisPartial Differential Equations·Captain: mikedeng1

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

Motivation

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

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

Setting

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

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

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

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

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

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

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

Formalization targets

Goal: smoothing by the heat kernel (Theorem 5.5)

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

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

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

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

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

Milestones

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

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

Significance

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

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

Difficulty

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

Formalization scope

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

Selected references

  • J. K. Hunter, Notes on Partial Differential Equations, UC Davis lecture notes, revised 6/18/2014, Chapter 5. https://www.math.ucdavis.edu/~hunter/pdes/pde_notes.pdf
  • M. E. Taylor, Partial Differential Equations I: Basic Theory, 2nd ed., Springer, 2011. https://doi.org/10.1007/978-1-4419-7055-8
  • L. C. Evans, Partial Differential Equations, 2nd ed., AMS Graduate Studies in Mathematics 19, 2010, §2.3 and §4.3. https://doi.org/10.1090/gsm/019
  • T. Cazenave, Semilinear Schrödinger Equations, Courant Lecture Notes 10, AMS, 2003, Ch. 2. https://doi.org/10.1090/cln/010
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Operations ResearchStochastic Systems·Captain: mikedeng1

Diffusion approximations for open queueing networks with service interruptions 1: explicit Lipschitz bounds for the oblique reflection mapResearch Paper

Motivation

Heavy-traffic and fluid approximations for open queueing networks are obtained by writing the queue-content process as a deterministic function of a simpler netput process (arrivals minus potential service, corrected for routing) and then transferring a functional limit theorem for the netput through that function. The function is the multidimensional reflection map of Harrison and Reiman (Harrison and Reiman 1981), extended from continuous paths to paths with jumps by Reiman (Reiman 1984). The transfer works only if the map is continuous, and quantitative bounds on the approximation error require it to be Lipschitz with a known modulus.

Chen and Whitt (Chen and Whitt 1993) use this map to derive diffusion approximations for networks whose servers are subject to interruptions. Before doing so, Section 2 of the paper supplies "explicit Lipschitz bounds" for the map in the uniform topology: a bound in the Harrison–Reiman scaling (Proposition 2.1) and a new bound that depends on the routing matrix only through its powers (Proposition 2.3).

Timeline. Harrison and Reiman (1981) proved existence, uniqueness and continuity of the map on continuous paths for a routing matrix of spectral radius less than one. Reiman (1984) extended it to paths with jumps. Chen and Mandelbaum (Leontief systems, RBV's and RBM's, 1991, cited in the paper as [4]) noted that a minor extension of the argument makes the map Lipschitz on D([0,T],Rn)D([0,T],\mathbb R^n)D([0,T],Rn) with the uniform topology. Chen and Whitt (1993, Section 2) made the Lipschitz constants explicit.

Setting

Fix a dimension nnn and an n×nn\times nn×n matrix QQQ whose transpose QtQ^{\mathsf t}Qt is substochastic: all entries of QQQ are nonnegative and every column sum of QQQ is at most 111. Assume also Qk→0Q^k \to 0Qk→0 as k→∞k\to\inftyk→∞. With Markovian routing, QtQ^{\mathsf t}Qt is the routing matrix of an open network of nnn queues.

Vectors c∈Rnc\in\mathbb R^nc∈Rn carry the norm ∥c∥=∑j∣cj∣\|c\| = \sum_j |c_j|∥c∥=∑j​∣cj​∣, and matrices carry the maximum absolute column sum ∥P∥=max⁡j∑i∣Pij∣\|P\| = \max_j \sum_i |P_{ij}|∥P∥=maxj​∑i​∣Pij​∣ (Eq. (2.5)). D([0,T],Rn)D([0,T],\mathbb R^n)D([0,T],Rn) is the space of paths that are right-continuous with left limits on [0,T][0,T][0,T]. For a path xxx, ∣x∣∈Rn|x|\in\mathbb R^n∣x∣∈Rn is the vector of coordinatewise sup norms, ∣x∣j=sup⁡0≤t≤T∣xj(t)∣|x|_j = \sup_{0\le t\le T}|x_j(t)|∣x∣j​=sup0≤t≤T​∣xj​(t)∣, and ∥x∥=∥∣x∣∥=∑jsup⁡t∣xj(t)∣\|x\| = \big\||x|\big\| = \sum_j \sup_{t}|x_j(t)|∥x∥=​∣x∣​=∑j​supt​∣xj​(t)∣.

The reflection of x∈Dx \in Dx∈D is the pair (y,z)=(ψ(x),ϕ(x))(y,z) = (\psi(x),\phi(x))(y,z)=(ψ(x),ϕ(x)) with y∈Dy \in Dy∈D and

z=x+(I−Q) y≥0,yj nondecreasing, yj(0)=0,∫0Tzj(t) dyj(t)=0(1≤j≤n).z = x + (I-Q)\,y \ge 0, \qquad y_j \text{ nondecreasing},\ y_j(0) = 0, \qquad \int_0^T z_j(t)\,dy_j(t) = 0 \quad (1\le j\le n).z=x+(I−Q)y≥0,yj​ nondecreasing, yj​(0)=0,∫0T​zj​(t)dyj​(t)=0(1≤j≤n).

The last condition says that yjy_jyj​ increases only when zj=0z_j = 0zj​=0. In queueing terms, zzz is the vector of queue contents and yyy the cumulative idleness. The operator πx(y)=(Qy−x)↑∨0\pi_x(y) = (Qy - x)^{\uparrow}\vee 0πx​(y)=(Qy−x)↑∨0, where f↑(t)=sup⁡0≤s≤tf(s)f^{\uparrow}(t) = \sup_{0\le s\le t} f(s)f↑(t)=sup0≤s≤t​f(s) coordinatewise, has the reflection as its fixed point (Eq. (2.4)). Write γ=∥Qn∥\gamma = \|Q^n\|γ=∥Qn∥.

Formalization targets

Goal: Proposition 2.3

For all x1,x2∈Dx_1,x_2\in Dx1​,x2​∈D with reflections (ψ(xi),ϕ(xi))(\psi(x_i),\phi(x_i))(ψ(xi​),ϕ(xi​)),

∣ψ(x1)−ψ(x2)∣≤(I−Q)−1∣x1−x2∣componentwise,(2.9)|\psi(x_1)-\psi(x_2)| \le (I-Q)^{-1}|x_1-x_2| \quad\text{componentwise},\tag{2.9}∣ψ(x1​)−ψ(x2​)∣≤(I−Q)−1∣x1​−x2​∣componentwise,(2.9) ∥ψ(x1)−ψ(x2)∥≤∥(I−Q)−1∥ ∥x1−x2∥≤∑k=0∞∥Qk∥ ∥x1−x2∥≤n1−γ∥x1−x2∥,(2.10)\|\psi(x_1)-\psi(x_2)\| \le \|(I-Q)^{-1}\|\,\|x_1-x_2\| \le \sum_{k=0}^\infty \|Q^k\|\,\|x_1-x_2\| \le \frac{n}{1-\gamma}\|x_1-x_2\|,\tag{2.10}∥ψ(x1​)−ψ(x2​)∥≤∥(I−Q)−1∥∥x1​−x2​∥≤k=0∑∞​∥Qk∥∥x1​−x2​∥≤1−γn​∥x1​−x2​∥,(2.10) ∥ϕ(x1)−ϕ(x2)∥≤(1+∥I−Q∥ ∥(I−Q)−1∥)∥x1−x2∥≤(1+2n1−γ)∥x1−x2∥.(2.11)\|\phi(x_1)-\phi(x_2)\| \le \big(1+\|I-Q\|\,\|(I-Q)^{-1}\|\big)\|x_1-x_2\| \le \Big(1+\frac{2n}{1-\gamma}\Big)\|x_1-x_2\|.\tag{2.11}∥ϕ(x1​)−ϕ(x2​)∥≤(1+∥I−Q∥∥(I−Q)−1∥)∥x1​−x2​∥≤(1+1−γ2n​)∥x1​−x2​∥.(2.11)

The constants are those of the paper. The goal fixes nothing beyond the standing assumptions on QQQ.

Milestones

  1. Existence and uniqueness of the reflection for x∈Dx\in Dx∈D with x(0)≥0x(0)\ge0x(0)≥0 (Section 2, p. 337).
  2. Eq. (2.4): given (2.1)–(2.2), the complementarity condition (2.3) is equivalent to y=πx(y)y = \pi_x(y)y=πx​(y).
  3. γ=∥Qn∥<1\gamma = \|Q^n\| < 1γ=∥Qn∥<1 (p. 338).
  4. Proposition 2.2: ∥πxk(y1)−πxk(y2)∥≤∥Qk∣y1−y2∣∥≤∥y1−y2∥\|\pi_x^k(y_1)-\pi_x^k(y_2)\| \le \|Q^k|y_1-y_2|\| \le \|y_1-y_2\|∥πxk​(y1​)−πxk​(y2​)∥≤∥Qk∣y1​−y2​∣∥≤∥y1​−y2​∥ for k≥1k\ge1k≥1, the factor γ\gammaγ for k≥nk\ge nk≥n, and πxk(y1)→ψ(x)\pi_x^k(y_1)\to\psi(x)πxk​(y1​)→ψ(x).
  5. Proposition 2.1: for Q∗=Λ−1QΛQ^* = \Lambda^{-1}Q\LambdaQ∗=Λ−1QΛ with Λ\LambdaΛ diagonal and ∥Q∗∥=α<1\|Q^*\| = \alpha<1∥Q∗∥=α<1, the moduli ∥Λ∥∥Λ−1∥/(1−α)\|\Lambda\|\|\Lambda^{-1}\|/(1-\alpha)∥Λ∥∥Λ−1∥/(1−α) for ψ\psiψ and 1+∥I−Q∥∥Λ∥∥Λ−1∥/(1−α)1 + \|I-Q\|\|\Lambda\|\|\Lambda^{-1}\|/(1-\alpha)1+∥I−Q∥∥Λ∥∥Λ−1∥/(1−α) for ϕ\phiϕ.
  6. Remark (2.1): for n=1n=1n=1, Q=0Q=0Q=0 the bounds are attained.
  7. Remark (2.2): for two queues in series, (2.10) gives modulus 222, while (2.7) gives at best 444 (every modulus ≥4\ge 4≥4 is attained, 444 at z=1/2z = 1/2z=1/2).

Significance

Proposition 2.3 makes the queue-content and idleness processes of an open network Lipschitz functions of the netput, in the uniform norm, with a modulus computed from the routing matrix alone. Combined with the fact that Lipschitz continuity in the uniform topology passes to the Skorohod J1J_1J1​ and M1M_1M1​ topologies (Section 2 of the paper), it is what turns a functional central limit theorem for arrival and service processes into a heavy-traffic limit for the network. The paper uses it in exactly this way in Sections 3–4. Explicit moduli also yield rates: an error of order ε\varepsilonε in the netput produces an error of at most nε/(1−γ)n\varepsilon/(1-\gamma)nε/(1−γ) in the idleness process.

On the formal side, the results are proved in the paper, but neither the reflection map nor D([0,T],Rn)D([0,T],\mathbb R^n)D([0,T],Rn) has a machine-checked development in Mathlib or on this platform. The mission would provide a reusable definition of the oblique reflection map with a Lebesgue–Stieltjes complementarity condition, its fixed-point characterization, and certified Lipschitz constants, as a foundation for any later formal heavy-traffic limit.

Difficulty

The componentwise bound (2.9) is short once the fixed-point form of the map is available. The difficulty lies in the infrastructure beneath it. The fixed-point characterization (2.4) is a one-dimensional Skorokhod-problem argument carried out coordinatewise for paths with jumps, where the complementarity condition must be handled through Lebesgue–Stieltjes measures. A jump of yjy_jyj​ is allowed at a time where zj=0z_j = 0zj​=0 even if zjz_jzj​ was positive just before. Existence needs the iterates πxk(0)\pi_x^k(0)πxk​(0) to converge in DDD and the limit to satisfy (2.1)–(2.3). The explicit constants involve (I−Q)−1(I-Q)^{-1}(I−Q)−1, ∑k∥Qk∥\sum_k\|Q^k\|∑k​∥Qk∥ and γ=∥Qn∥<1\gamma = \|Q^n\|<1γ=∥Qn∥<1. The last inequality is a combinatorial fact about transient substochastic matrices. It does not follow from ∥Q∥≤1\|Q\|\le1∥Q∥≤1.

Formalization scope

Vectors are Fin n → ℝ, matrices Matrix (Fin n) (Fin n) ℝ, and ∥P∥\|P\|∥P∥ is the maximum absolute column sum. Paths are functions ℝ → Fin n → ℝ, of which only the restriction to [0,T][0,T][0,T] matters. Membership in D([0,T],Rn)D([0,T],\mathbb R^n)D([0,T],Rn) is the predicate IsCadlagOn T x: right-continuous on [0,T)[0,T)[0,T), left limits on (0,T](0,T](0,T], and (redundantly) bounded on [0,T][0,T][0,T]. The reflection is the predicate IsReflection Q T x y z. Every theorem is stated for all pairs satisfying it, so no choice function and no junk value are involved. Condition (2.3) is encoded as "the Lebesgue–Stieltjes measure dyjdy_jdyj​ of {t∈[0,T]:zj(t)>0}\{t\in[0,T]: z_j(t)>0\}{t∈[0,T]:zj​(t)>0} is zero". For z≥0z\ge0z≥0 this is equivalent to ∫0Tzj dyj=0\int_0^T z_j\,dy_j=0∫0T​zj​dyj​=0. πxk\pi_x^kπxk​ is Nat.iterate, (I−Q)−1(I-Q)^{-1}(I−Q)−1 is Mathlib's matrix inverse (invertible under the standing assumptions), and ∑k∥Qk∥\sum_k\|Q^k\|∑k​∥Qk∥ is a tsum stated together with its summability.

Corrections and conventions, each disclosed in the item concerned:

  • The norm (2.6). The page prints ∥x∥=sup⁡t∑j∣xj(t)∣\|x\| = \sup_t\sum_j|x_j(t)|∥x∥=supt​∑j​∣xj​(t)∣. Under that norm Propositions 2.1 and 2.3 are false for n≥2n\ge2n≥2. With Q=0Q=0Q=0, n=2n=2n=2, T=1T=1T=1, x1≡0x_1\equiv0x1​≡0 and x2=(−1[0.1,0.2),−1[0.3,0.4))x_2 = (-\mathbf 1_{[0.1,0.2)}, -\mathbf 1_{[0.3,0.4)})x2​=(−1[0.1,0.2)​,−1[0.3,0.4)​), one gets ∥x1−x2∥=1\|x_1-x_2\|=1∥x1​−x2​∥=1 but ψ(x2)=(1[0.1,1],1[0.3,1])\psi(x_2) = (\mathbf 1_{[0.1,1]},\mathbf 1_{[0.3,1]})ψ(x2​)=(1[0.1,1]​,1[0.3,1]​) has norm 222. The paper's proofs are valid for ∥x∥=∑jsup⁡t∣xj(t)∣\|x\| = \sum_j\sup_t|x_j(t)|∥x∥=∑j​supt​∣xj​(t)∣, which is used throughout. In dimension one the two norms coincide.
  • (2.8) prints ϕ(x1)−ϕ(x1)\phi(x_1)-\phi(x_1)ϕ(x1​)−ϕ(x1​). The formalization states ϕ(x1)−ϕ(x2)\phi(x_1)-\phi(x_2)ϕ(x1​)−ϕ(x2​).
  • (2.2)–(2.3) print the index range 1≤j≤J1\le j\le J1≤j≤J. The dimension is nnn.
  • x(0)≥0x(0)\ge0x(0)≥0 is added to the existence item. Conditions (2.1)–(2.2) force z(0)=x(0)z(0)=x(0)z(0)=x(0), so no reflection exists otherwise. The Lipschitz bounds are stated for all solution pairs and are vacuous exactly when some xi(0)x_i(0)xi​(0) has a negative coordinate.
  • Proposition 2.1 assumes only that Λ\LambdaΛ is diagonal with nonzero entries. All quantities depend on ∣Λ∣|\Lambda|∣Λ∣, so this covers the positive scaling of Harrison and Reiman.
  • Eq. (2.4) keeps the standing assumptions on QQQ as on the page, although the equivalence does not use them.

A trivializing formalization would read (2.3) through a Bochner integral, which is 000 for non-integrable integrands, or take suprema over unbounded families. The measure-zero encoding and the boundedness built into IsCadlagOn rule both out. A sorry-free check shows that Remark (2.1)'s jump example satisfies IsReflection.

Welcome contributions: a general API for càdlàg paths on [0,T][0,T][0,T] (boundedness, measurability, running suprema), the one-dimensional Skorokhod lemma for càdlàg paths, and the Neumann series for transient substochastic matrices. All of these are reusable beyond this mission.

Selected references

  • H. Chen and W. Whitt, Diffusion approximations for open queueing networks with service interruptions, Queueing Systems 13 (1993) 335–359. https://doi.org/10.1007/BF01149260
  • J. M. Harrison and M. I. Reiman, Reflected Brownian motion on an orthant, Annals of Probability 9 (1981) 302–308. https://doi.org/10.1214/aop/1176994428
  • M. I. Reiman, Open queueing networks in heavy traffic, Mathematics of Operations Research 9 (1984) 441–458. https://doi.org/10.1287/moor.9.3.441
  • H. Chen and A. Mandelbaum, Discrete flow networks: diffusion approximations and bottlenecks, Annals of Probability 19 (1991) 1463–1519. https://doi.org/10.1214/aop/1176990220
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Machine LearningProbabilityTheoretical Computer Science·Captain: MiltMont

Flow Matching Theorem 1: Marginal Continuity EquationResearch Paper

From conditional motion to a marginal probability path

Flow matching models a changing probability distribution using a time-dependent velocity field. A conditional model specifies a density and a velocity separately for each conditioning point. The mathematical question is whether those conditional descriptions determine a velocity for the mixture distribution. This mission concerns the continuity-equation formulation of Theorem 1 of Lipman, Chen, Ben-Hamu, Nickel, and Le, Flow Matching for Generative Modeling (ICLR 2023). The source is arXiv:2210.02747v2, Section 3.1 and Appendix A.

Densities, velocities, and probability flux

Fix a natural number ddd and let E=RdE=\mathbb R^dE=Rd. The conditioning distribution QQQ is a Borel probability measure on EEE. At time ttt, position xxx, and conditioning point zzz, write ρ(t,x,z)\rho(t,x,z)ρ(t,x,z) for the conditional density and v(t,x,z)∈Ev(t,x,z)\in Ev(t,x,z)∈E for the conditional velocity. The variable xxx is integrated against Lebesgue measure; zzz is integrated against QQQ. These roles remain distinct even though both variables take values in the same space.

The conditional flux is F(t,x,z)=ρ(t,x,z)v(t,x,z)F(t,x,z)=\rho(t,x,z)v(t,x,z)F(t,x,z)=ρ(t,x,z)v(t,x,z). The marginal density, marginal flux, and marginal velocity are defined by

p(t,x)=∫Eρ(t,x,z) dQ(z),J(t,x)=∫EF(t,x,z) dQ(z),u(t,x)=p(t,x)−1J(t,x).p(t,x)=\int_E\rho(t,x,z)\,dQ(z),\qquad J(t,x)=\int_E F(t,x,z)\,dQ(z),\qquad u(t,x)=p(t,x)^{-1}J(t,x).p(t,x)=∫E​ρ(t,x,z)dQ(z),J(t,x)=∫E​F(t,x,z)dQ(z),u(t,x)=p(t,x)−1J(t,x).

These definitions express equations (6) and (8) using a probability measure rather than a data-density function. This representation also allows discrete conditioning distributions. Every conditional density is strictly positive and normalized on 0≤t≤10\leq t\leq10≤t≤1, jointly measurable in (x,z)(x,z)(x,z), and integrable in zzz at each fixed (t,x)(t,x)(t,x).

The divergence of a differentiable vector field is the sum of the diagonal entries of its derivative. A density and velocity satisfy the classical continuity equation when their flux is spatially differentiable and the density has time derivative equal to minus that divergence.

Formalization targets

The goal asserts that p(t,⋅)p(t,\cdot)p(t,⋅) is a positive probability density for every t∈[0,1]t\in[0,1]t∈[0,1] and that

∂tp(t,x)+div⁡x(p(t,x)u(t,x))=0(0<t<1, x∈E).\partial_t p(t,x)+\operatorname{div}_x\bigl(p(t,x)u(t,x)\bigr)=0\qquad(0<t<1,\ x\in E).∂t​p(t,x)+divx​(p(t,x)u(t,x))=0(0<t<1, x∈E).

The hypotheses require the conditional continuity equation for QQQ-almost every conditioning point, at each interior time and spatial point. They also specify a sufficient local domination package for differentiation under the integral. This is an explicit classical interpretation of the regularity qualification in the proof of Theorem 1.

Four supporting targets isolate the mathematical assertions used by this formulation: the probability-density property of equation (6); time differentiation under the conditioning integral; spatial divergence under the conditioning integral; and the velocity/flux identity corresponding to equation (8). The source contains these equations and operations rather than separately numbered supporting lemmas, so the milestone titles identify the relevant equation or proof passage.

What completing the formalization provides

The deliverable is a checked interface for passing from a measurable family of conditional continuity equations to the continuity equation of its mixture. It records which variables are differentiated, which measure is used for averaging, where positivity is needed, and which assumptions justify each analytic operation. The time and spatial differentiation lemmas are stated for general measures and integrands, making them reusable outside this particular probability model.

The mathematical result is already proved in the cited paper. The uploaded theorem items are open formalization targets, with explicit proof placeholders. Successful local compilation checks their types and imports; it does not establish their conclusions. The definition module contains no proof placeholders.

Analytic obligations

Pointwise differentiability of every conditional function does not by itself justify differentiating an integral over the conditioning variable. The regularity predicates therefore require a neighborhood independent of that variable, an integrable bound for the derivative norm throughout that neighborhood, and almost-everywhere measurability of the integrand and derivative. Time and space receive separate predicates because their derivatives take values in different spaces.

There is also a distinction between density normalization in xxx and integrability in zzz at a fixed position. The formal assumptions record both. A probability measure on the conditioning space does not make every measurable function integrable. These conditions prevent the totalized Bochner integral from silently supplying a default value where an intended integral fails to exist.

Formalization scope

Space is represented by Fin d → ℝ, with its standard finite-product Borel structure and Lebesgue measure. Its norm is the standard product norm used by mathlib. All finite dimensions, including dimension zero, are included. Time-dependent functions are defined on all real times, while density assumptions apply on the closed unit interval and derivative conclusions apply on its interior. No endpoint time derivative is asserted.

The regularity package is one sufficient realization of the source's Leibniz-rule assumption, not a claim to the weakest possible hypotheses. Conditional continuity equations may hold almost everywhere in the conditioning variable; their exceptional sets may depend on the fixed time and position. Spatial differentiability of the marginal flux is part of the conclusion, so the equation cannot be satisfied merely through the default value of an undefined derivative.

The target is the PDE formulation. It does not assert existence of a global ODE flow, uniqueness of transported measures, or equality with a flow pushforward. Those require a separate transport development. It also asserts no endpoint approximation to a data distribution and no theorem about optimization, neural networks, or Gaussian paths. No marginal continuity equation or differentiation–integration interchange is assumed as an input.

Required infrastructure consists of Bochner integration, finite-dimensional differentiation, finite sums of derivative coordinates, and product-measure integration. Contributions may prove the supporting targets or the goal directly while preserving their statements and the distinction between classical PDE and flow-transport claims.

Selected references

  • Yaron Lipman, Ricky T. Q. Chen, Heli Ben-Hamu, Maximilian Nickel, and Matt Le. Flow Matching for Generative Modeling. ICLR 2023. arXiv:2210.02747v2, Section 2, Section 3.1, Theorem 1, equations (6), (8), and (26), and Appendix A's proof of Theorem 1.
  • mathlib contributors. ParametricIntegral.lean, revision 0df444a360eaa60ab8c11dca51a86af692955474. Differentiation under the integral.
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Mathematical Physics·Captain: Lucas

Luminous efficacy of radiation: the 683.002 lm/W ceilingTextbook

Motivation

Two different numbers describe the output of a lamp. Radiant flux Φe\Phi_eΦe​ is the power it radiates, in watts. Luminous flux Φv\Phi_vΦv​ is how much of that radiation the standard human eye registers, in lumens — a weighted integral of the radiated power in which each wavelength is counted according to the sensitivity of the eye at that wavelength. Their ratio

K  =  ΦvΦeK \;=\; \frac{\Phi_v}{\Phi_e}K=Φe​Φv​​

is the luminous efficacy of radiation, measured in lumens per watt: it says what fraction of the radiated power is usable for illumination. Photometry is built on this pair of quantities. The lumen and the candela are defined from the watt through exactly such a weighting, with the SI defining constant Kcd=683K_{\mathrm{cd}} = 683Kcd​=683 lm/W fixing the scale at the frequency 540×1012540 \times 10^{12}540×1012 Hz, and every efficiency figure quoted for a lamp — a tungsten filament at 151515 lm/W, a white LED above 100100100 lm/W — is a statement about this ratio or its wall-plug variant.

The basic structural fact of the subject is that this ratio is bounded. Since the eye's sensitivity curve is normalized to a maximum of 111, no source, however designed, can exceed the maximum spectral luminous efficacy: 683.002683.002683.002 lm/W under photopic (daylight, cone) vision, and about 170017001700 lm/W under scotopic (dark-adapted, rod) vision. Those two numbers are the ceilings against which every lighting technology is measured, and they are what this mission formalizes.

Setting

Wavelengths are real numbers (nanometres). A spectral radiant flux distribution of a source is modelled as a finite Borel measure μ\muμ on the wavelength axis: μ(A)\mu(A)μ(A) is the power, in watts, that the source radiates at wavelengths in AAA. Its radiant flux is the total mass

Φe  =  μ(R).\Phi_e \;=\; \mu(\mathbb{R}).Φe​=μ(R).

A luminosity function (luminous efficiency function) with peak at λ0\lambda_0λ0​ is a measurable V:R→RV : \mathbb{R} \to \mathbb{R}V:R→R with

0≤V(λ)≤1for all λ,V(λ0)=1.0 \le V(\lambda) \le 1 \quad \text{for all } \lambda, \qquad V(\lambda_0) = 1 .0≤V(λ)≤1for all λ,V(λ0​)=1.

For photopic vision the CIE 1924 curve VVV peaks at λ0=555\lambda_0 = 555λ0​=555 nm; the scotopic curve V′V'V′ peaks at λ0=507\lambda_0 = 507λ0​=507 nm. The development assumes only the normalization above, never a specific tabulated curve, so every statement holds for the photopic curve, the scotopic curve, and any other normalized weighting.

Given a maximum spectral luminous efficacy Kmax⁡K_{\max}Kmax​ — the value Km=683.002K_m = 683.002Km​=683.002 lm/W for photopic vision, 170017001700 lm/W for scotopic vision — the spectral luminous efficacy is K(λ)=Kmax⁡V(λ)K(\lambda) = K_{\max} V(\lambda)K(λ)=Kmax​V(λ) and the luminous flux is

Φv  =  ∫RK(λ) dμ(λ)  =  Kmax⁡∫RV dμ.\Phi_v \;=\; \int_{\mathbb{R}} K(\lambda) \, \mathrm{d}\mu(\lambda) \;=\; K_{\max} \int_{\mathbb{R}} V \,\mathrm{d}\mu .Φv​=∫R​K(λ)dμ(λ)=Kmax​∫R​Vdμ.

The luminous efficacy of radiation is K=Φv/ΦeK = \Phi_v / \Phi_eK=Φv​/Φe​, the dimensionless luminous efficiency is K/Kmax⁡K / K_{\max}K/Kmax​, and the luminous efficacy of a source (overall, or wall-plug, efficacy) is Φv/P\Phi_v / PΦv​/P, where PPP is the total input power the source consumes — electrical, chemical or other — of which the radiated part is Φe≤P\Phi_e \le PΦe​≤P.

Modelling the spectrum as a measure rather than as a density is what makes the two halves of the target statement expressible at once. A spectrum with a spectral radiant flux density Φe,λ\Phi_{e,\lambda}Φe,λ​ is the measure dμ=Φe,λ dλ\mathrm{d}\mu = \Phi_{e,\lambda} \, \mathrm{d}\lambdadμ=Φe,λ​dλ, for which the formulas above reduce to the usual integrals

Φv=Kmax⁡∫V(λ) Φe,λ dλ,Φe=∫Φe,λ dλ;\Phi_v = K_{\max}\int V(\lambda)\, \Phi_{e,\lambda} \,\mathrm{d}\lambda, \qquad \Phi_e = \int \Phi_{e,\lambda} \,\mathrm{d}\lambda ;Φv​=Kmax​∫V(λ)Φe,λ​dλ,Φe​=∫Φe,λ​dλ;

an ideal monochromatic source at λ0\lambda_0λ0​, which has no density with respect to wavelength, is the point mass δλ0\delta_{\lambda_0}δλ0​​.

Formalization targets

Goal — the photopic ceiling is attained at 683.002683.002683.002 lm/W

683.002  =  max⁡{ Km∫V dμμ(R)  :  μ finite, μ(R)>0 },Km=683.002 lm/W.683.002 \;=\; \max\left\{\, \frac{K_m \int V \,\mathrm{d}\mu}{\mu(\mathbb{R})} \;:\; \mu \text{ finite}, \ \mu(\mathbb{R}) > 0 \,\right\}, \qquad K_m = 683.002 \text{ lm/W}.683.002=max{μ(R)Km​∫Vdμ​:μ finite, μ(R)>0},Km​=683.002 lm/W.

This is a maximum, not a supremum: the assertion is both that no spectral radiant flux distribution exceeds 683.002683.002683.002 lm/W and that some distribution — the monochromatic source at 555555555 nm — attains it exactly.

Scotopic counterpart

1700  =  max⁡{ 1700∫V′ dμμ(R)  :  μ finite, μ(R)>0 }1700 \;=\; \max\left\{\, \frac{1700 \int V' \,\mathrm{d}\mu}{\mu(\mathbb{R})} \;:\; \mu \text{ finite}, \ \mu(\mathbb{R}) > 0 \,\right\}1700=max{μ(R)1700∫V′dμ​:μ finite, μ(R)>0}

for a scotopic luminosity function V′V'V′ with V′(507)=1V'(507) = 1V′(507)=1.

Supporting statements

Φv≥0\Phi_v \ge 0Φv​≥0; Φv≤Kmax⁡Φe\Phi_v \le K_{\max}\Phi_eΦv​≤Kmax​Φe​; 0≤K≤Kmax⁡0 \le K \le K_{\max}0≤K≤Kmax​; luminous efficiency in [0,1][0,1][0,1]; the point mass at the peak realizes K=Kmax⁡K = K_{\max}K=Kmax​; the reduction of KKK to the integral formula for a spectrum with a density; invariance of KKK under rescaling the spectrum; Φv/P≤K\Phi_v / P \le KΦv​/P≤K when Φe≤P\Phi_e \le PΦe​≤P; and K=0K = 0K=0 for a source radiating only where VVV vanishes.

Significance

The ceiling is the reference point for the whole of lighting efficiency: quoted luminous efficiencies are efficacies divided by 683.002683.002683.002 lm/W, so "37%37\%37%" for a truncated 580058005800 K black body and "2%2\%2%" for a tungsten filament are statements about the distance to this bound. The supporting statements are the facts that make such comparisons well posed — that the efficacy depends only on the shape of the spectrum and not on the wattage, that the wall-plug efficacy of a device is never better than the efficacy of its radiation, and that power radiated outside the response band is pure loss.

Formalizing the material produces a small, reusable measure-theoretic layer for photometric and, more generally, for weighted-average quantities: a bounded weight integrated against a finite measure, normalized by the total mass, with the extreme value attained at a point mass. Nothing here is open mathematics; the value of the mission is a machine-checked model in which the definitions of the International Electrotechnical Vocabulary are stated once and the standard consequences are derived from them, rather than each being asserted in prose.

Difficulty

The mathematical content is elementary — the ceiling is the inequality ∫V dμ≤μ(R)\int V \,\mathrm{d}\mu \le \mu(\mathbb{R})∫Vdμ≤μ(R) for 0≤V≤10 \le V \le 10≤V≤1 — and the work is in the modelling. Three points need care.

First, attainment. On the space of L1L^1L1 densities the value 683.002683.002683.002 lm/W is a supremum that is never attained: for the actual CIE curve the set {V=1}\{V = 1\}{V=1} is a single point, hence Lebesgue-null, so a density supported there is zero almost everywhere and has no radiant flux at all. A formalization restricted to densities would either have to weaken the goal to a supremum or state an attainment claim that is vacuously true. Measures avoid this: the monochromatic source is the point mass δ555\delta_{555}δ555​.

Second, division. Efficacy is a quotient, and the quotient of a real by zero is a junk value; every statement about KKK therefore carries the hypothesis Φe>0\Phi_e > 0Φe​>0, which is also the physically meaningful one.

Third, integrability. The luminous flux is a Bochner integral, which returns 000 for a non-integrable integrand; the mission's hypotheses (VVV measurable and bounded, μ\muμ finite) are what rule this degeneracy out.

Formalization scope

The wavelength axis is all of R\mathbb{R}R, with Lebesgue measure where a density is used; no restriction to positive wavelengths or to a visible band is imposed, since the luminosity function already performs the restriction. A spectral radiant flux distribution is a finite Borel measure; the finiteness hypothesis is carried as a typeclass assumption and the positivity of the radiant flux as an explicit one. The luminosity function is assumed measurable with values in [0,1][0,1][0,1] and equal to 111 at its peak, and nothing more: no continuity, no unimodality, no tabulated values. The maximum spectral luminous efficacy appears as an explicit parameter Kmax⁡K_{\max}Kmax​, so that the photopic constant 683.002683.002683.002 and the scotopic constant 170017001700 are instances of the same statements rather than separate developments. Units are not represented in the types: all quantities are plain real numbers, and lumens per watt appears only in the prose.

The goal is stated as "683.002683.002683.002 is the greatest element of the set of achievable efficacies", which rules out the two trivializing readings: a bare upper bound (true of any number above the ceiling) and an attainment claim over a class of spectra that is empty or null.

A complete development needs Mathlib's measure theory and Bochner integration only: finite measures, withDensity, Dirac measures, and monotonicity of the integral. The resulting definitions are reusable for any normalized weighted average of a finite measure, and contributions extending the model — mesopic weighting, black-body spectra and the efficacy figures computed from them, or the CIE curve as tabulated data — are welcome.

Selected references

  • International Electrotechnical Commission, International Electrotechnical Vocabulary, entries 845-21-089 (luminous efficacy of a source) and 845-21-090 (luminous efficacy of radiation), electropedia.org.
  • Bureau International des Poids et Mesures, Principles Governing Photometry, 2nd edition, 2019, p. 10, bipm.org — the value 683.002683.002683.002 lm/W.
  • ISO/CIE, ISO 23539:2005 Photometry — The CIE system of physical photometry, iso.org.
  • T. W. Murphy, "Maximum spectral luminous efficacy of white light", Journal of Applied Physics 111 (2012) 104909, arXiv:1309.7039.
  • Wikipedia, Luminous efficacy, en.wikipedia.org/wiki/Luminous_efficacy — the source material for this mission.
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Mathematical Physics·Captain: Lucas

Planck's Law: Classical Limits and the Ultraviolet CatastropheTextbook

Motivation

A black body is an idealized body that absorbs all radiation falling on it and, when held at a fixed absolute temperature TTT, re-emits radiation whose spectrum depends on TTT alone. At the end of the nineteenth century two incompatible descriptions of that spectrum were on the table. Wien's distribution law (1896) fitted the measurements at short wavelengths and high temperatures but failed at long wavelengths. The formula Rayleigh obtained from classical equipartition, later the Rayleigh-Jeans law, reproduced the long-wavelength data and grew without bound at short wavelengths - the failure Ehrenfest named the ultraviolet catastrophe in 1911.

Planck's 1900 formula fits at every frequency. He reached it by refusing to treat the vibrational energy of the oscillators as a continuous quantity, writing it instead as an integer multiple of an energy element ε=hν\varepsilon = h\nuε=hν; the constant hhh entered physics as the proportionality factor in that hypothesis. Fitting black-body data, Planck obtained h≈6.55×10−34 J sh \approx 6.55\times10^{-34}\ \mathrm{J\,s}h≈6.55×10−34 Js, within about 1.2%1.2\%1.2% of the value h=6.626 070 15×10−34 J sh = 6.626\,070\,15\times10^{-34}\ \mathrm{J\,s}h=6.62607015×10−34 Js that today defines the SI.

What makes Planck's formula the successful one is not only that it fits the data. It contains both classical laws: it degenerates to Rayleigh-Jeans at low frequency and to Wien's law at high frequency, and unlike Rayleigh-Jeans it has a finite total emission. This mission formalizes those four statements - two limits and two integrability claims - about the spectral radiance function itself.

Setting

Fix three positive real parameters: the Planck constant hhh, the speed of light ccc, and the Boltzmann constant kBk_BkB​. They are kept as variables rather than numerical constants, so every statement is a theorem about the functional form, valid in any system of units. Let T>0T > 0T>0 be an absolute temperature.

Per unit frequency ν\nuν, Planck's law gives the spectral radiance

Bν(ν,T)  =  2hν3/c2exp⁡ ⁣(hνkBT)−1,B_\nu(\nu, T) \;=\; \frac{2h\nu^3/c^2}{\exp\!\left(\dfrac{h\nu}{k_B T}\right) - 1},Bν​(ν,T)=exp(kB​Thν​)−12hν3/c2​,

which is the function planckFreq of the already-published definition bundle BlackbodyRadiation_planck. That bundle also provides the dimensionless shape function

gn(x)  =  xnex−1,n∈N,g_n(x) \;=\; \frac{x^n}{e^x - 1}, \qquad n \in \mathbb{N},gn​(x)=ex−1xn​,n∈N,

in terms of which Bν(ν,T)=2kB3T3h2c2 g3 ⁣(hνkBT)B_\nu(\nu,T) = \dfrac{2k_B^3T^3}{h^2c^2}\, g_3\!\left(\dfrac{h\nu}{k_BT}\right)Bν​(ν,T)=h2c22kB3​T3​g3​(kB​Thν​).

Two further functions are introduced by this mission. The Rayleigh-Jeans spectral radiance, the classical equipartition prediction,

BνRJ(ν,T)  =  2ν2kBTc2,B^{\mathrm{RJ}}_\nu(\nu, T) \;=\; \frac{2\nu^2 k_B T}{c^2},BνRJ​(ν,T)=c22ν2kB​T​,

and Wien's distribution law, the short-wavelength approximation,

BνW(ν,T)  =  2hν3c2 exp⁡ ⁣(−hνkBT).B^{\mathrm{W}}_\nu(\nu, T) \;=\; \frac{2h\nu^3}{c^2}\,\exp\!\left(-\frac{h\nu}{k_B T}\right).BνW​(ν,T)=c22hν3​exp(−kB​Thν​).

Write x=hν/(kBT)x = h\nu/(k_B T)x=hν/(kB​T) for the dimensionless frequency. All three radiances are positive on ν>0\nu > 0ν>0; the two comparisons below are stated as ratios, which is the precise form of "agrees with, in this regime".

Formalization targets

Goal

For all h,c,kB,T>0h, c, k_B, T > 0h,c,kB​,T>0, all four of the following hold simultaneously:

lim⁡ν→0+Bν(ν,T)BνRJ(ν,T)=1,lim⁡ν→∞Bν(ν,T)BνW(ν,T)=1,\lim_{\nu \to 0^+} \frac{B_\nu(\nu,T)}{B^{\mathrm{RJ}}_\nu(\nu,T)} = 1, \qquad \lim_{\nu \to \infty} \frac{B_\nu(\nu,T)}{B^{\mathrm{W}}_\nu(\nu,T)} = 1,ν→0+lim​BνRJ​(ν,T)Bν​(ν,T)​=1,ν→∞lim​BνW​(ν,T)Bν​(ν,T)​=1, Bν(⋅,T)∈L1((0,∞)),BνRJ(⋅,T)∉L1((0,∞)).B_\nu(\cdot,T) \in L^1\big((0,\infty)\big), \qquad B^{\mathrm{RJ}}_\nu(\cdot,T) \notin L^1\big((0,\infty)\big).Bν​(⋅,T)∈L1((0,∞)),BνRJ​(⋅,T)∈/L1((0,∞)).

The goal asserts only the shape of the truth - ratios tending to 111 and membership or non-membership in L1L^1L1 - and fixes no constant, so it is not invalidated by any sharper rate or by the exact value of the total emission.

Milestones

The four conjuncts are milestones in their own right, together with the two shape-function limits that drive them:

lim⁡x→0+xex−1=1,lim⁡x→∞exex−1=1.\lim_{x \to 0^+} \frac{x}{e^x - 1} = 1, \qquad \lim_{x \to \infty} \frac{e^x}{e^x - 1} = 1 .x→0+lim​ex−1x​=1,x→∞lim​ex−1ex​=1.

Significance

The result itself. The two limits are the sense in which Planck's law reproduces Wien's law for short wavelengths and the empirical long-wavelength formula, which is the criterion Planck was working to when he introduced hhh; the non-integrability of BνRJB^{\mathrm{RJ}}_\nuBνRJ​ is the ultraviolet catastrophe, stated exactly rather than as an asymptotic remark; and the integrability of BνB_\nuBν​ is what makes the total emitted power

  • the Stefan-Boltzmann law - a well-defined finite number in the first place. In Lean this last point is not cosmetic: the Bochner integral of a non-integrable function is defined and equal to 000, so an integral identity such as ∫0∞πBν dν=σT4\int_0^\infty \pi B_\nu \, d\nu = \sigma T^4∫0∞​πBν​dν=σT4 carries no information until integrability is known separately. This mission supplies that missing side condition for the Stefan-Boltzmann statements already on the platform (CODATA2022.blackbody_exitance_eq_stefanBoltzmann, CODATA2022.bose_einstein_integral_cube), both of which are Open.

Formalizing it. The physics has been settled for over a century; none of it is open mathematics. What is missing is machine-checked statements: the platform's existing black-body development (BlackbodyRadiation_planck, and the mission Planck's Law and Wien's Displacement Law) covers the peak of the spectrum and the exact radiation constants, but not the two classical regimes, and not integrability. The limit and integrability lemmas about xn/(ex−1)x^n/(e^x-1)xn/(ex−1) produced here are reusable for any later work on Bose-Einstein integrals, the Debye model, or the Stefan-Boltzmann constant.

Difficulty

The obvious argument for each limit is a one-line asymptotic expansion, and the obvious argument for integrability is "the integrand decays exponentially". Neither survives contact with a formal proof as stated. The ratio Bν/BνRJB_\nu/B^{\mathrm{RJ}}_\nuBν​/BνRJ​ equals x/(ex−1)x/(e^x-1)x/(ex−1) only after cancelling ν2\nu^2ν2, c2c^2c2 and 222, which requires those factors to be nonzero - so the algebraic reduction is valid on a punctured neighbourhood, and must be transported to the limit through a congruence-along-a-filter step rather than by rewriting the function globally. At ν=0\nu = 0ν=0 the ratio is a 0/00/00/0 junk value, which is exactly why the limit is taken within (0,∞)(0,\infty)(0,∞).

For integrability the difficulty is at the two ends at once: near 000 the integrand is O(ν2)O(\nu^2)O(ν2) but the defining expression is a quotient whose denominator vanishes, and near ∞\infty∞ the exponential decay has to be turned into a dominating integrable function rather than a limit statement. Non-integrability of BνRJB^{\mathrm{RJ}}_\nuBνRJ​ must be derived from unboundedness of ∫0Rν2dν\int_0^R \nu^2 d\nu∫0R​ν2dν, not asserted from the divergence of the integral, since an unproved-integrability integral in Lean silently evaluates to 000.

Formalization scope

Everything is over R\mathbb{R}R with the Lebesgue (volume) measure; L1L^1L1 membership is MeasureTheory.IntegrableOn ... (Set.Ioi 0) volume, which includes measurability. One-sided limits are filters: ν→0+\nu \to 0^+ν→0+ is the neighbourhood filter of 000 restricted to (0,∞)(0,\infty)(0,∞), and ν→∞\nu\to\inftyν→∞ is Filter.atTop. The three physical parameters and the temperature are explicit real arguments, each carrying its own strict positivity hypothesis; no statement is quantified over a possibly empty set of parameters, and every hypothesis h,c,kB,T>0h,c,k_B,T>0h,c,kB​,T>0 is satisfiable, so nothing here is vacuous.

The radiance functions are total: division by zero yields 000 in Lean, so Bν(0,T)=0B_\nu(0,T) = 0Bν​(0,T)=0 and the comparison ratios are 0/0=00/0 = 00/0=0 at ν=0\nu = 0ν=0. That is harmless for the limits, which are taken strictly inside (0,∞)(0,\infty)(0,∞), and it is why the integrability statements are on (0,∞)(0,\infty)(0,∞) rather than on [0,∞)[0,\infty)[0,∞). The comparisons are deliberately stated as ratios tending to 111 rather than as differences tending to 000: the latter would be a weaker claim, and near ν=0\nu=0ν=0 it would be satisfied by functions that are not asymptotically equal.

Contributions welcome beyond the milestones: the corresponding statements in the wavelength parameterization, quantitative error bounds on the two approximations, and the integrability of gng_ngn​ on (0,∞)(0,\infty)(0,∞) for general nnn, which would close the remaining gap in the Stefan-Boltzmann chain.

Selected references

  • Max Planck, Ueber das Gesetz der Energieverteilung im Normalspectrum, Annalen der Physik 4 (1901) 553-563. https://doi.org/10.1002/andp.19013090310
  • Planck constant, Wikipedia. https://en.wikipedia.org/wiki/Planck_constant
  • Planck's law, Wikipedia. https://en.wikipedia.org/wiki/Planck%27s_law
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Mathematical Physics·Captain: Lucas

Speed of Light: c as an Invariant and Unattainable LimitTextbook

Motivation

The encyclopedic account of the speed of light makes two claims that look physical but whose content is mathematical. First, invariance: "the speed of light in vacuum is the same for all observers, no matter their relative velocity", so that light travels at ccc "regardless of the motion of the source or the inertial reference frame of the observer". Second, unattainability: ccc "is the upper limit for the speed at which information, matter, or energy can travel through space", and "particles with nonzero rest mass can be accelerated to approach ccc but can never reach it". The supporting apparatus quoted in the same source is likewise mathematical: the Lorentz factor γ\gammaγ, which "diverges to infinity as vvv approaches ccc"; the Lorentz interval, in which spatial and temporal differences "are combined with a negative sign"; and the kinetic energy (γ−1)mc2(\gamma-1)mc^2(γ−1)mc2, from which the source concludes that "it would take an infinite amount of energy to accelerate an object with mass to the speed of light".

This mission isolates that mathematical core, in one spatial dimension, over the real numbers, and asks for machine-checked proofs of it. Nothing here depends on the numerical value c=299 792 458 m s−1c = 299\,792\,458\ \mathrm{m\,s^{-1}}c=299792458 ms−1: every statement is proved for an arbitrary parameter c>0c > 0c>0, which is the sense in which the source's claims are structural rather than metrological.

Setting

Fix a real constant c>0c > 0c>0, the invariant speed. Work in one spatial dimension, with a spatial coordinate x∈Rx \in \mathbb{R}x∈R and a time coordinate t∈Rt \in \mathbb{R}t∈R; speeds are real numbers, and a speed vvv is called subluminal when ∣v∣<c|v| < c∣v∣<c.

Four objects are used throughout, written in the prose exactly as in the mission's Lean development.

Relativistic velocity addition. For speeds u,vu, vu,v,

u⊕cv  =  u+v1+uvc2.u \oplus_c v \;=\; \frac{u+v}{1 + \dfrac{uv}{c^{2}}}.u⊕c​v=1+c2uv​u+v​.

Lorentz factor. For a speed vvv,

γc(v)  =  11−v2c2.\gamma_c(v) \;=\; \frac{1}{\sqrt{1 - \dfrac{v^{2}}{c^{2}}}}.γc​(v)=1−c2v2​​1​.

Lorentz interval and Lorentz boost. The interval of an event (x,t)(x,t)(x,t) is

Ic(x,t)  =  c2t2−x2,I_c(x,t) \;=\; c^{2}t^{2} - x^{2},Ic​(x,t)=c2t2−x2,

and the boost of velocity vvv sends the event (x,t)(x,t)(x,t) to

Bc v(x,t)  =  (γc(v) (x−vt), γc(v) (t−vxc2)).B_c^{\,v}(x,t) \;=\; \Bigl(\gamma_c(v)\,(x - vt),\ \gamma_c(v)\,\bigl(t - \tfrac{vx}{c^{2}}\bigr)\Bigr).Bcv​(x,t)=(γc​(v)(x−vt), γc​(v)(t−c2vx​)).

Relativistic kinetic energy. For rest mass mmm and speed vvv,

Kc(m,v)  =  (γc(v)−1) m c2.K_c(m,v) \;=\; \bigl(\gamma_c(v) - 1\bigr)\,m\,c^{2}.Kc​(m,v)=(γc​(v)−1)mc2.

Formalization targets

Goal

For every c>0c > 0c>0 and every rest mass m>0m > 0m>0, all three of the following hold:

∀v, ∣v∣<c ⟹ c⊕cv=c;\forall v,\ |v| < c \ \Longrightarrow\ c \oplus_c v = c;∀v, ∣v∣<c ⟹ c⊕c​v=c; ∀u,v, ∣u∣<c and ∣v∣<c ⟹ ∣u⊕cv∣<c;\forall u, v,\ |u| < c \ \text{and}\ |v| < c \ \Longrightarrow\ |u \oplus_c v| < c;∀u,v, ∣u∣<c and ∣v∣<c ⟹ ∣u⊕c​v∣<c; ∀E∈R, ∃v, 0<v<c and E<Kc(m,v).\forall E \in \mathbb{R},\ \exists v,\ 0 < v < c \ \text{and}\ E < K_c(m,v).∀E∈R, ∃v, 0<v<c and E<Kc​(m,v).

The three conjuncts are, in order, the invariance of light speed under a change of inertial frame, the fact that composing subluminal speeds never reaches ccc, and the unboundedness of the energy required to approach ccc. The goal deliberately asserts only the shape of the claims — no rate of divergence, no numerical constant — so it is not invalidated by any sharper quantitative statement a solver may prove separately.

Milestones

The milestone list decomposes the goal along the four notions above: interval preservation under a boost, invariance of ccc under composition, closure of the subluminal range under composition, divergence of γc\gamma_cγc​ at ccc, and unboundedness of kinetic energy below ccc.

Significance

The three conjuncts of the goal are what make ccc a limit rather than merely a large speed. Closure of {∣v∣<c}\{|v| < c\}{∣v∣<c} under ⊕c\oplus_c⊕c​ says that no finite chain of subluminal boosts produces a luminal speed; invariance says that the boundary of that range is fixed by every boost; the energy statement says that the boundary is not approached at finite cost. Interval preservation is the geometric statement behind them: a boost is an isometry of the quadratic form c2t2−x2c^2t^2 - x^2c2t2−x2, so the light cone c2t2=x2c^2t^2 = x^2c2t2=x2 is frame-independent.

These results are classical and have been standard since the 1905 formulation of special relativity; nothing in this mission is mathematically open. What the mission produces is the machine-checked version and a small reusable layer of one-dimensional relativistic kinematics: a search for declarations mentioning "Lorentz" in the Mathlib revision used for the drafting check returned none, so the definitions here are contributed rather than reused. The statements are stated for an arbitrary c>0c > 0c>0, so they can be reused at c=1c = 1c=1 (natural units) without restatement.

Difficulty

The algebraic milestones are short once the right nonvanishing facts are in hand, and the obvious first attempt — clear denominators and call a ring normalizer — fails on all of them for the same reason: the denominators 1+uv/c21 + uv/c^21+uv/c2, ccc, and 1−v2/c21 - v^2/c^21−v2/c2 must first be shown nonzero, and each of those facts needs the hypothesis ∣v∣<c|v| < c∣v∣<c, not merely c≠0c \neq 0c=0. For velocity addition the usable identities are

c(1+uvc2)±(u+v)=(c±u)(c±v)c,c\Bigl(1 + \tfrac{uv}{c^{2}}\Bigr) \pm (u+v) = \frac{(c \pm u)(c \pm v)}{c},c(1+c2uv​)±(u+v)=c(c±u)(c±v)​,

whose positivity is where the strict inequality comes from.

The analytic milestone is the one that is not formal manipulation: γc\gamma_cγc​ must be shown to tend to +∞+\infty+∞ along the punctured left neighbourhood of ccc, which requires the inner expression to be shown positive, not merely convergent to 000, on a neighbourhood — the one-sided filter is essential, since γc\gamma_cγc​ takes a junk value beyond ccc (see below).

Formalization scope

All quantities are real; there is no vector or manifold structure, and spacetime is R2\mathbb{R}^2R2 presented as a pair of coordinates (x,t)(x,t)(x,t). The invariant speed ccc is a parameter with hypothesis c>0c > 0c>0; the numerical SI value is never used. The definitions are total functions, so two junk-value conventions are fixed and must be respected when reading the statements:

  • γc(v)\gamma_c(v)γc​(v) uses the real square root, which is 000 on negative arguments; hence γc(v)=0\gamma_c(v) = 0γc​(v)=0 whenever ∣v∣≥c|v| \ge c∣v∣≥c, rather than being undefined or infinite. Every statement about γc\gamma_cγc​ therefore carries an explicit subluminality or one-sided-limit hypothesis.
  • u⊕cvu \oplus_c vu⊕c​v is a quotient, and division by zero yields 000; the hypotheses ∣u∣<c|u| < c∣u∣<c, ∣v∣<c|v| < c∣v∣<c are what exclude the vanishing denominator.

No statement in the mission is vacuous: each hypothesis set is satisfiable, e.g. by c=1c = 1c=1, u=v=1/2u = v = 1/2u=v=1/2, m=1m = 1m=1, and the goal quantifies over all c>0c > 0c>0 and all m>0m > 0m>0.

A complete development needs only Mathlib's real analysis: Real.sqrt, field-simplification and positivity reasoning, and one-sided neighbourhood filters for the divergence milestone. The definition layer (velocity addition, Lorentz factor, interval, boost, kinetic energy) is reusable beyond this mission — natural follow-ups, welcome as contributions, are the associativity and group structure of ⊕c\oplus_c⊕c​, the rapidity parametrization v=ctanh⁡θv = c\tanh\thetav=ctanhθ, time dilation and length contraction, and the composition law for boosts.

Note on the read-backs attached to this proposal

The read-backs attached to the draft items of this proposal are not blind and not independent: they were written by the same agent that drafted the Lean statements, at the explicit instruction of the proposal owner, with full sight of the source material and of the intended meaning. They should be read as an author's restatement, not as independent testimony, and they do not provide the error-catching value of an independent audit.

Selected references

  • Speed of light, Wikipedia (source material supplied for this mission), sections "Invariance of ccc and the Lorentz factor", "Synthesis of space and time", and "Mass and massless particles". https://en.wikipedia.org/wiki/Speed_of_light
  • A. Einstein, Zur Elektrodynamik bewegter Körper, Annalen der Physik 17 (1905), 891–921. https://doi.org/10.1002/andp.19053221004
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Harmonic Analysis·Captain: Lucas

Analise de Fourier I: Parseval's Theorem for Fourier SeriesTextbook

Motivation

Periodic signals are the basic objects of audio processing, electrical engineering and the analytic study of partial differential equations, and the standard first-course tool for handling them is the Fourier series: a decomposition of a TTT-periodic signal into sinusoids of frequencies ωn=2πn/T\omega_n = 2\pi n / Tωn​=2πn/T. The identity that makes the decomposition quantitatively useful is Parseval's theorem: the average power of the signal equals the sum of the squared moduli of its Fourier coefficients, so energy can be accounted for frequency by frequency.

This mission formalizes the chain of results leading to that identity exactly as it is presented in the open-access undergraduate textbook Análise de Fourier — Um Livro Colaborativo (Esequia Sauter and Fabio Souto de Azevedo, orgs., UFRGS/REAMAT, 2022): the orthogonality relations of the trigonometric system (Teorema 3.2.1), the coefficient formulas (Teorema 3.2.2), the passage to the exponential form (§4.2), and the Parseval identity itself (Teorema 5.1.1).

Setting

Fix a period T>0T > 0T>0 and write

ωn  =  2πnT,n∈Z.\omega_n \;=\; \frac{2\pi n}{T}, \qquad n \in \mathbb{Z}.ωn​=T2πn​,n∈Z.

For a real-valued fff integrable on [0,T][0,T][0,T] the book defines the trigonometric Fourier coefficients (eq. 3.23)

an  =  2T∫0Tf(t)cos⁡(ωnt) dt,bn  =  2T∫0Tf(t)sin⁡(ωnt) dt,a_n \;=\; \frac{2}{T}\int_0^T f(t)\cos(\omega_n t)\,dt, \qquad b_n \;=\; \frac{2}{T}\int_0^T f(t)\sin(\omega_n t)\,dt,an​=T2​∫0T​f(t)cos(ωn​t)dt,bn​=T2​∫0T​f(t)sin(ωn​t)dt,

and for a complex-valued fff the exponential coefficients (§4.2, eq. 4.8)

Cn  =  1T∫0Tf(t) e−iωnt dt,n∈Z,C_n \;=\; \frac{1}{T}\int_0^T f(t)\,e^{-i\omega_n t}\,dt, \qquad n \in \mathbb{Z},Cn​=T1​∫0T​f(t)e−iωn​tdt,n∈Z,

which for real fff satisfy Cn=(an−ibn)/2C_n = (a_n - i b_n)/2Cn​=(an​−ibn​)/2. The average power of a TTT-periodic signal is (Definição 5.1.1)

Pf  =  1T∫0T∣f(t)∣2 dt.P_f \;=\; \frac{1}{T}\int_0^T |f(t)|^2\,dt .Pf​=T1​∫0T​∣f(t)∣2dt.

A trigonometric polynomial of degree NNN (Definição 3.2.1) is

a02+∑n=1N[ancos⁡(ωnt)+bnsin⁡(ωnt)].\frac{a_0}{2} + \sum_{n=1}^{N}\bigl[a_n\cos(\omega_n t) + b_n\sin(\omega_n t)\bigr].2a0​​+n=1∑N​[an​cos(ωn​t)+bn​sin(ωn​t)].

Formalization targets

Goal — Teorema 5.1.1 (Teorema de Parseval)

For T>0T > 0T>0 and f:R→Cf : \mathbb{R} \to \mathbb{C}f:R→C continuous and TTT-periodic,

1T∫0T∣f(t)∣2 dt  =  ∑n=−∞∞∣Cn∣2.\frac{1}{T}\int_0^T |f(t)|^2\,dt \;=\; \sum_{n=-\infty}^{\infty} |C_n|^2 .T1​∫0T​∣f(t)∣2dt=n=−∞∑∞​∣Cn​∣2.

The book states the identity for a periodic function "representable by a Fourier series"; the mission fixes continuity as the concrete sufficient regularity hypothesis, which keeps the statement non-vacuous and true, and leaves the sum as an unordered sum over Z\mathbb{Z}Z so that no summation order is smuggled in.

Supporting targets

  1. Teorema 3.2.1 — the three orthogonality relations of {cos⁡(ωnt),sin⁡(ωnt)}\{\cos(\omega_n t), \sin(\omega_n t)\}{cos(ωn​t),sin(ωn​t)} on [0,T][0,T][0,T], including the degenerate index n=m=0n = m = 0n=m=0.
  2. §4.2 — the orthogonality relation in exponential form, ∫0Teiωnte−iωmt dt=T\int_0^T e^{i\omega_n t}e^{-i\omega_m t}\,dt = T∫0T​eiωn​te−iωm​tdt=T for n=mn = mn=m and 000 otherwise, n,m∈Zn, m \in \mathbb{Z}n,m∈Z.
  3. Teorema 3.2.2 — recovery of the coefficients of a trigonometric polynomial by the integral formulas (3.23).
  4. Eq. (4.8) — Cn=(an−ibn)/2C_n = (a_n - i b_n)/2Cn​=(an​−ibn​)/2 for a real integrable fff.
  5. Bessel's inequality and summability — every finite partial sum of ∣Cn∣2|C_n|^2∣Cn​∣2 is at most PfP_fPf​, and the family (∣Cn∣2)n∈Z(|C_n|^2)_{n \in \mathbb{Z}}(∣Cn​∣2)n∈Z​ is summable. Summability is what gives the goal's infinite sum a meaning independent of any ordering.

Significance

Parseval's identity converts an integral estimate into a coefficientwise one: it is the bridge between the time domain and the frequency domain, underlies the RMS computations of the book's own electrical-engineering examples (Exemplo 5.1.2), and yields closed-form evaluations of numerical series (the book's Exemplo 5.1.3 computes a series of reciprocal odd squares this way).

Mathlib already contains the abstract Hilbert-space form of the identity for the Fourier basis on the circle AddCircle T. What this mission adds is the concrete, classroom-level layer that an engineering or physics reader recognizes: coefficients written as interval integrals of a function on R\mathbb{R}R with an explicit period TTT, the real (an,bn)(a_n, b_n)(an​,bn​) form, the exponential CnC_nCn​ form and the dictionary between them, and the orthogonality relations as free-standing computations. That layer is reusable by any later mission in this series (transformada de Fourier, equação do calor, equação da onda).

Difficulty

The obvious route — expand ∣f∣2=ffˉ|f|^2 = f\bar f∣f∣2=ffˉ​, substitute the Fourier series, and integrate term by term — is exactly the book's proof, and it is the step that a formal development cannot take for granted: interchanging the integral with an infinite sum requires a convergence theorem that the book explicitly places outside its scope (the remark after Definição 3.2.3), and pointwise convergence of the Fourier series of a merely continuous function is false in general. A complete proof must run through L2L^2L2 convergence rather than pointwise convergence, so the central task is to connect the interval-integral coefficients on [0,T][0,T][0,T] with the Hilbert-space machinery for the circle, including the change of variables and the normalization of Haar measure.

Formalization scope

The development commits to the following conventions, all fixed in the definition bundle so that every statement shares them:

  • The period is an explicit real parameter TTT with the hypothesis 0<T0 < T0<T written into each statement; at T=0T = 0T=0 the definitions would divide by zero and nothing is claimed.
  • Integrals are interval integrals over [0,T][0,T][0,T] of functions defined on all of R\mathbb{R}R; the book's alternative window [−T/2,T/2][-T/2, T/2][−T/2,T/2] is not used.
  • Coefficient indices range over Z\mathbb{Z}Z; ana_nan​ and bnb_nbn​ are defined for negative nnn as well, matching eq. (4.7) of the book.
  • an,bna_n, b_nan​,bn​ act on real-valued functions, CnC_nCn​ and the average power on complex-valued ones; a real signal enters the complex statements through the coercion of its values.
  • Sums over Z\mathbb{Z}Z are unordered sums, so the goal asserts convergence of the family, not of a symmetric partial-sum limit.
  • The sign convention is e−iωnte^{-i\omega_n t}e−iωn​t in the coefficient and e+iωnte^{+i\omega_n t}e+iωn​t in the synthesis, as in §4.2.

The goal is not trivializable: the hypotheses (a positive period, a continuous periodic function) are satisfiable, and both sides of the identity are non-degenerate already for f(t)=cos⁡(2πt/T)f(t) = \cos(2\pi t/T)f(t)=cos(2πt/T).

Useful infrastructure beyond the mission: the dictionary between the interval-integral coefficients on [0,T][0,T][0,T] and Mathlib's fourierCoeff on AddCircle T, and the orthogonality relations as standalone integral computations.

Selected references

  • Esequia Sauter, Fabio Souto de Azevedo (orgs.), Análise de Fourier — Um Livro Colaborativo, UFRGS/REAMAT, 26 July 2022. https://www.ufrgs.br/reamat/TransformadasIntegrais/livro-af/main.html
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Numerical Analysis·Captain: Lucas

Padé Approximants: Existence and Uniqueness of the [m/n] ApproximantTextbook

Motivation

A Padé approximant is the "best" approximation of a function near a point by a rational function of prescribed numerator and denominator degrees. The idea goes back to Georg Frobenius (1881), who studied relations among the convergents of a power series, and was developed systematically by Henri Padé in his 1892 thesis. Unlike a truncated Taylor polynomial, a rational approximant can reproduce poles, and it often converges where the Taylor series does not; this is why Padé approximants are standard tools in numerical computation, in the resummation of divergent perturbation series in physics, and — through the "ad hoc methods inspired by Padé theory" — in Diophantine approximation and transcendence proofs.

The theory rests on one structural fact, stated in the source as a single sentence: when it exists, the Padé approximant is unique as a formal power series for the given mmm and nnn. That sentence hides the two theorems this mission asks for — that a suitable pair of polynomials always exists, and that any two such pairs define the same rational function.

Setting

Fix a field FFF and a formal power series

f(x)  =  c0+c1x+c2x2+⋯∈F[[x]].f(x) \;=\; c_0 + c_1 x + c_2 x^2 + \cdots \in F[[x]] .f(x)=c0​+c1​x+c2​x2+⋯∈F[[x]].

Given integers m≥0m \ge 0m≥0 and n≥0n \ge 0n≥0, one looks for a rational function

R(x)  =  ∑j=0majxj1+∑k=1nbkxk  =  P(x)Q(x)R(x) \;=\; \frac{\sum_{j=0}^{m} a_j x^j}{1 + \sum_{k=1}^{n} b_k x^k} \;=\; \frac{P(x)}{Q(x)}R(x)=1+∑k=1n​bk​xk∑j=0m​aj​xj​=Q(x)P(x)​

whose Maclaurin expansion agrees with that of fff through order m+nm+nm+n, i.e.

f(x)−R(x)  =  cm+n+1′xm+n+1+cm+n+2′xm+n+2+⋯ .f(x) - R(x) \;=\; c_{m+n+1}' x^{m+n+1} + c_{m+n+2}' x^{m+n+2} + \cdots .f(x)−R(x)=cm+n+1′​xm+n+1+cm+n+2′​xm+n+2+⋯.

This is denoted [m/n]f(x)[m/n]_f(x)[m/n]f​(x).

Written this way the condition is nonlinear in the unknowns and presupposes Q(0)≠0Q(0) \neq 0Q(0)=0. The classical device, due to Frobenius, is to linearize: instead of asking that f−P/Qf - P/Qf−P/Q vanish to order m+n+1m+n+1m+n+1, one asks that

Q(x)f(x)−P(x)  ≡  0(modxm+n+1),deg⁡P≤m,deg⁡Q≤n,Q≠0.Q(x) f(x) - P(x) \;\equiv\; 0 \pmod{x^{m+n+1}}, \qquad \deg P \le m,\quad \deg Q \le n,\quad Q \neq 0 .Q(x)f(x)−P(x)≡0(modxm+n+1),degP≤m,degQ≤n,Q=0.

A pair (P,Q)(P, Q)(P,Q) satisfying these three conditions is what this mission calls a Padé pair of type [m/n][m/n][m/n] for fff; it is the predicate every statement below is phrased with. The linearized problem is a homogeneous linear system, so it is always solvable, whereas the original ratio problem is not: the linearized solution may have Q(0)=0Q(0) = 0Q(0)=0, in which case no normalized RRR of the displayed shape exists (the "[m/n][m/n][m/n] entry of the Padé table is defect"). The two formulations coincide exactly when Q(0)≠0Q(0) \neq 0Q(0)=0.

Target

The goal theorem is the conjunction of existence and uniqueness for the linearized problem, over an arbitrary field FFF, for all m,n≥0m, n \ge 0m,n≥0:

(E)∃ P,Q∈F[x]: Q≠0, deg⁡P≤m, deg⁡Q≤n, Qf−P≡0 (mod xm+n+1),\textbf{(E)} \quad \exists\, P, Q \in F[x] : \ Q \neq 0,\ \deg P \le m,\ \deg Q \le n,\ Q f - P \equiv 0 \ (\mathrm{mod}\ x^{m+n+1}),(E)∃P,Q∈F[x]: Q=0, degP≤m, degQ≤n, Qf−P≡0 (mod xm+n+1), (U)(P1,Q1),(P2,Q2) Padeˊ pairs of type [m/n] ⟹ P1Q2=P2Q1.\textbf{(U)} \quad (P_1,Q_1), (P_2,Q_2) \ \text{Padé pairs of type } [m/n] \ \Longrightarrow\ P_1 Q_2 = P_2 Q_1 .(U)(P1​,Q1​),(P2​,Q2​) Padeˊ pairs of type [m/n] ⟹ P1​Q2​=P2​Q1​.

Statement (U) is the precise content of "the Padé approximant is unique": the two pairs need not be equal — they may differ by a common polynomial factor — but they determine the same element of F(x)F(x)F(x), and hence the same formal power series wherever the quotient is defined.

The milestones are: existence (E); uniqueness (U); the equivalence between the linearized condition and agreement of Maclaurin expansions when Q(0)≠0Q(0) \neq 0Q(0)=0; the Bézout form P=Q Tm+n+Kxm+n+1P = Q\,T_{m+n} + K x^{m+n+1}P=QTm+n​+Kxm+n+1 used by the extended-Euclidean computation of the approximant; the normalization of the denominator to constant term 111; and the two worked examples given in the source, namely [2/2][2/2][2/2] for ln⁡(1+x)\ln(1+x)ln(1+x) and [5/5][5/5][5/5] for exp⁡(x)\exp(x)exp(x).

Significance

The result itself. Existence and uniqueness are what make the Padé table — the doubly indexed array ([m/n]f)m,n≥0([m/n]_f)_{m,n \ge 0}([m/n]f​)m,n≥0​ — a well-defined object, and therefore what make every identity among its entries (the block structure of the table, the Frobenius identities, Wynn's ε\varepsilonε-algorithm and the cross rules) meaningful. Every computational route to the approximant, including the extended-Euclidean route recorded in the source, computes the [m/n][m/n][m/n] approximant only because of (U).

Formalizing it. Mathlib has formal power series, polynomials, truncation, and the inverse of a power series with invertible constant term, but no Padé theory: there is no predicate for the [m/n][m/n][m/n] condition and no existence or uniqueness statement. This mission adds the linearized predicate and the two structural theorems, which is the minimum foundation on which the Padé table, the block theorem, and convergence results such as Nuttall–Pommerenke could later be built. The results are classical and have textbook proofs; the contribution here is the machine-checked development, not new mathematics.

Difficulty

Neither theorem is deep, but both have a specific step where the obvious approach fails.

For existence, the naive route — solve for QQQ, then read off PPP — requires knowing that the homogeneous system for the n+1n+1n+1 coefficients of QQQ given by the nnn equations "coefficients of xm+1,…,xm+nx^{m+1}, \dots, x^{m+n}xm+1,…,xm+n of QfQfQf vanish" has a nonzero solution. That is a rank argument about a rectangular Toeplitz-like matrix, and the work in Lean is in packaging it as a linear-algebra statement rather than in the mathematics.

For uniqueness, the one-line argument is to divide: from Q1f≡P1Q_1 f \equiv P_1Q1​f≡P1​ and Q2f≡P2Q_2 f \equiv P_2Q2​f≡P2​ conclude P1/Q1=P2/Q2P_1/Q_1 = P_2/Q_2P1​/Q1​=P2​/Q2​. This is invalid, because QiQ_iQi​ need not be invertible modulo xm+n+1x^{m+n+1}xm+n+1 (its constant term may vanish) and F[x]/(xm+n+1)F[x]/(x^{m+n+1})F[x]/(xm+n+1) is not a domain. The correct argument compares Q2(Q1f−P1)−Q1(Q2f−P2)=Q1P2−Q2P1Q_2(Q_1 f - P_1) - Q_1(Q_2 f - P_2) = Q_1 P_2 - Q_2 P_1Q2​(Q1​f−P1​)−Q1​(Q2​f−P2​)=Q1​P2​−Q2​P1​, whose left side is divisible by xm+n+1x^{m+n+1}xm+n+1 while its right side has degree at most m+nm+nm+n; the difficulty is the degree bookkeeping, not the algebra.

A solver should also note that (U) is not the claim P1=P2∧Q1=Q2P_1 = P_2 \wedge Q_1 = Q_2P1​=P2​∧Q1​=Q2​, which is false — rescaling, or a common factor, gives distinct pairs.

Formalization scope

The development is over an arbitrary field F (the definition itself only needs a commutative ring), with f : PowerSeries F, and P Q : Polynomial F. Conventions fixed in Lean, and worth reading before starting:

  • Degree bounds use Polynomial.degree ≤ (m : WithBot ℕ), so the zero polynomial satisfies every bound; in particular P=0P = 0P=0 is allowed and Q=0Q = 0Q=0 is excluded by an explicit hypothesis.
  • The congruence modulo xm+n+1x^{m+n+1}xm+n+1 is expressed coefficientwise: all coefficients of index k≤m+nk \le m+nk≤m+n of Qf−PQ f - PQf−P vanish. Polynomials are viewed inside PowerSeries F through the canonical coercion.
  • The degenerate cases m=0m = 0m=0, n=0n = 0n=0 and f=0f = 0f=0 are included; nothing in the statements excludes them.
  • The inverse Q−1Q^{-1}Q−1 in the Maclaurin-agreement milestone is Mathlib's power series inverse, which is a genuine inverse precisely under the stated hypothesis Q(0)≠0Q(0) \neq 0Q(0)=0.
  • Nothing is normalized silently: the hypothesis Q(0)≠0Q(0)\ne 0Q(0)=0 appears only where the source's normalized form 1+b1x+⋯1 + b_1x + \cdots1+b1​x+⋯ is used, and the normalization itself is a separate milestone.
  • The two examples are over Q\mathbb{Q}Q, with exp⁡\expexp taken to be Mathlib's PowerSeries.exp ℚ and ln⁡(1+x)\ln(1+x)ln(1+x) supplied as an explicit series ∑k≥1(−1)k+1xk/k\sum_{k \ge 1} (-1)^{k+1} x^k / k∑k≥1​(−1)k+1xk/k.

Contributions of further Padé material — the Padé table, defect entries, the block structure, or the ε\varepsilonε-algorithm — are welcome as follow-up missions built on this predicate.

Selected references

  • Frobenius, G., "Ueber Relationen zwischen den Näherungsbrüchen von Potenzreihen", Journal für die reine und angewandte Mathematik 90 (1881), 1–17. https://gdz.sub.uni-goettingen.de/id/PPN243919689_0090
  • Padé, H., "Sur la représentation approchée d'une fonction par des fractions rationnelles" (thesis), Ann. Sci. École Norm. Sup. (3) 9 (1892), 3–93 (supplement). https://www.numdam.org/item/?id=ASENS_1892_3_9__S3_0
  • Baker, G. A., Jr., and Graves-Morris, P., Padé Approximants, 2nd ed., Cambridge University Press, 1996.
  • Gragg, W. B., "The Padé Table and Its Relation to Certain Algorithms of Numerical Analysis", SIAM Review 14 (1972), 1–62. https://doi.org/10.1137/1014001
  • Bini, D., and Pan, V., Polynomial and Matrix Computations, Vol. 1, Birkhäuser, 1994 (Problem 5.2b and Algorithm 5.2, p. 46).
  • "Padé approximant", Wikipedia, revision 1374746248. https://en.wikipedia.org/w/index.php?title=Pad%C3%A9_approximant&oldid=1374746248
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Mathematical Physics·Captain: Lucas

Flat ΛCDM Cosmology: The Closed-Form Expansion LawTextbook

Motivation

The ΛCDM model — "Lambda cold dark matter" — is the standard cosmological model: a spatially homogeneous and isotropic universe governed by general relativity, whose energy content is dominated today by cold dark matter and by a cosmological constant Λ\LambdaΛ acting as dark energy. It is the framework in which the cosmic microwave background, the large-scale distribution of galaxies, the primordial light-element abundances, and the observed accelerating expansion are fitted simultaneously with a handful of parameters.

Inside this model, almost everything quantitative requires numerical integration of the Friedmann equations. There is one striking exception: for a spatially flat universe containing only pressureless matter and a positive cosmological constant, and with radiation neglected, the expansion history has a closed form in elementary functions. That closed form is where the textbook statements "the universe is about 13.813.813.8 billion years old" and "the expansion switched from decelerating to accelerating at redshift z≈0.6z \approx 0.6z≈0.6" actually come from. This mission formalizes that closed form and the two consequences just named.

Setting

Write a(t)a(t)a(t) for the dimensionless scale factor of a homogeneous isotropic universe, normalized so that a=1a = 1a=1 at the present epoch, and H(t)=a˙(t)/a(t)H(t) = \dot a(t)/a(t)H(t)=a˙(t)/a(t) for the Hubble parameter; H0>0H_0 > 0H0​>0 denotes its present-day value. The energy content is described by present-day density parameters Ωi\Omega_iΩi​, the ratios of each species' density to the critical density ρc=3H02/(8πG)\rho_c = 3H_0^2/(8\pi G)ρc​=3H02​/(8πG). This mission works with the minimal, radiation-free, spatially flat case: a matter parameter Ωm>0\Omega_m > 0Ωm​>0 and a dark-energy parameter ΩΛ>0\Omega_\Lambda > 0ΩΛ​>0 with

Ωm+ΩΛ=1.\Omega_m + \Omega_\Lambda = 1 .Ωm​+ΩΛ​=1.

Matter dilutes as a−3a^{-3}a−3 and the cosmological constant does not dilute at all, so the first Friedmann equation for this content reads

(a˙a)2  =  H02(Ωma3+ΩΛ).\left(\frac{\dot a}{a}\right)^{2} \;=\; H_0^{2}\left(\frac{\Omega_m}{a^{3}} + \Omega_\Lambda\right).(aa˙​)2=H02​(a3Ωm​​+ΩΛ​).

The candidate closed-form solution, with the big bang placed at t=0t = 0t=0, is

a(t)  =  (ΩmΩΛ)1/3 sinh⁡2/3 ⁣(32ΩΛ H0 t),t>0,a(t) \;=\; \left(\frac{\Omega_m}{\Omega_\Lambda}\right)^{1/3}\, \sinh^{2/3}\!\left(\tfrac{3}{2}\sqrt{\Omega_\Lambda}\,H_0\,t\right), \qquad t > 0,a(t)=(ΩΛ​Ωm​​)1/3sinh2/3(23​ΩΛ​​H0​t),t>0,

and the time at which it reaches a=1a = 1a=1 — the predicted age of the universe — is

t0  =  23H0ΩΛ  arsinh⁡ΩΛΩm.t_0 \;=\; \frac{2}{3H_0\sqrt{\Omega_\Lambda}}\;\operatorname{arsinh}\sqrt{\frac{\Omega_\Lambda}{\Omega_m}}.t0​=3H0​ΩΛ​​2​arsinhΩm​ΩΛ​​​.

All quantities are real; sinh⁡2/3\sinh^{2/3}sinh2/3 is the real power x↦x2/3x \mapsto x^{2/3}x↦x2/3 applied to sinh⁡\sinhsinh, which is positive for t>0t > 0t>0.

Target

The goal theorem asserts that the displayed a(t)a(t)a(t) is a positive solution of the flat matter-plus-Λ\LambdaΛ Friedmann equation on t>0t > 0t>0, normalized by a(t0)=1a(t_0) = 1a(t0​)=1 at the age t0>0t_0 > 0t0​>0 given above:

0<a(t),(a˙(t)a(t))2=H02(Ωma(t)3+ΩΛ)(t>0),0<t0,a(t0)=1.0 < a(t), \qquad \left(\frac{\dot a(t)}{a(t)}\right)^{2} = H_0^{2}\left(\frac{\Omega_m}{a(t)^{3}} + \Omega_\Lambda\right) \quad (t > 0), \qquad 0 < t_0, \qquad a(t_0) = 1 .0<a(t),(a(t)a˙(t)​)2=H02​(a(t)3Ωm​​+ΩΛ​)(t>0),0<t0​,a(t0​)=1.

The milestones build to this and then go beyond it, in increasing strength: the derivative a˙=aH0ΩΛcoth⁡θ\dot a = a H_0\sqrt{\Omega_\Lambda}\coth\thetaa˙=aH0​ΩΛ​​cothθ with θ=32ΩΛH0t\theta = \tfrac32\sqrt{\Omega_\Lambda}H_0 tθ=23​ΩΛ​​H0​t; the Friedmann equation itself; the normalization a(t0)=1a(t_0) = 1a(t0​)=1; the equivalent logarithmic age formula

t0=23H0ΩΛ log⁡1+ΩΛΩm;t_0 = \frac{2}{3H_0\sqrt{\Omega_\Lambda}}\,\log\frac{1+\sqrt{\Omega_\Lambda}}{\sqrt{\Omega_m}};t0​=3H0​ΩΛ​​2​logΩm​​1+ΩΛ​​​;

the deceleration-to-acceleration transition, a¨(t)=0\ddot a(t) = 0a¨(t)=0 exactly when a(t)3=Ωm/(2ΩΛ)a(t)^3 = \Omega_m/(2\Omega_\Lambda)a(t)3=Ωm​/(2ΩΛ​), together with the sign criterion a¨(t)>0  ⟺  Ωm<2ΩΛa(t)3\ddot a(t) > 0 \iff \Omega_m < 2\Omega_\Lambda a(t)^3a¨(t)>0⟺Ωm​<2ΩΛ​a(t)3; the qualitative picture that aaa is strictly increasing on (0,∞)(0,\infty)(0,∞) and tends to 000 as t↓0t \downarrow 0t↓0; and finally the statement that the closed form, together with the density ρ=ρc(Ωma−3+ΩΛ)\rho = \rho_c(\Omega_m a^{-3} + \Omega_\Lambda)ρ=ρc​(Ωm​a−3+ΩΛ​) and the pressure p=−ρcΩΛp = -\rho_c\Omega_\Lambdap=−ρc​ΩΛ​, satisfies both Friedmann equations, i.e. assembles into an FRW universe in the sense of the platform's existing FRWUniverse definition.

Significance

The result. The closed form turns cosmological parameter statements into arithmetic. With Ωm≈0.315\Omega_m \approx 0.315Ωm​≈0.315, ΩΛ≈0.685\Omega_\Lambda \approx 0.685ΩΛ​≈0.685 and H0≈67.4 km s−1Mpc−1H_0 \approx 67.4\ \mathrm{km\,s^{-1}Mpc^{-1}}H0​≈67.4 kms−1Mpc−1 it yields the standard age of roughly 13.813.813.8 billion years, and the transition condition a3=Ωm/(2ΩΛ)a^3 = \Omega_m/(2\Omega_\Lambda)a3=Ωm​/(2ΩΛ​) gives 1+z=(2ΩΛ/Ωm)1/3≈1.61+z = (2\Omega_\Lambda/\Omega_m)^{1/3} \approx 1.61+z=(2ΩΛ​/Ωm​)1/3≈1.6, i.e. z≈0.6z \approx 0.6z≈0.6. Both numbers are quoted constantly; here they are consequences of a theorem rather than of a numerical integration. The transition result is also the precise sense in which a positive Λ\LambdaΛ is what makes the late-time expansion accelerate.

Formalizing it. The mathematics is classical and the derivation is standard in cosmology texts; nothing here is an open question. What the mission produces is a machine-checked account: a reusable parameter bundle for the flat ΛCDM model, a verified closed-form solution of a nonlinear ODE, verified transcendental identities for the age, and a bridge to the platform's existing FRW-cosmology development, so that later work on distances, horizons, or the radiation-inclusive model can build on published statements instead of restating them.

Difficulty

The obstruction is not conceptual but analytic. The scale factor is a real power x2/3x^{2/3}x2/3 of sinh⁡\sinhsinh, so it is not differentiable by the polynomial-power rules: every derivative step goes through the real rpow API, needs positivity of sinh⁡θ\sinh\thetasinhθ on t>0t > 0t>0, and produces exponents that must be recombined by hand (a3a^3a3 collapses to (Ωm/ΩΛ)sinh⁡2θ(\Omega_m/\Omega_\Lambda)\sinh^2\theta(Ωm​/ΩΛ​)sinh2θ only after such a step). The Friedmann identity itself then rests on coth⁡2=1+csch⁡2\coth^2 = 1 + \operatorname{csch}^2coth2=1+csch2, which must be applied where sinh⁡θ≠0\sinh\theta \neq 0sinhθ=0. The age milestones require the explicit value of arsinh⁡\operatorname{arsinh}arsinh as a logarithm together with the flatness relation Ωm=1−ΩΛ\Omega_m = 1 - \Omega_\LambdaΩm​=1−ΩΛ​. The second-derivative milestones require differentiating the first-derivative formula again and tracking the sign of sinh⁡2θ−13cosh⁡2θ\sinh^2\theta - \tfrac13\cosh^2\thetasinh2θ−31​cosh2θ; the naive route of computing deriv (deriv ·) symbolically without first establishing a HasDerivAt statement on a neighbourhood is the main trap.

Formalization scope

Parameters are bundled in a structure carrying H0>0H_0 > 0H0​>0, Ωm>0\Omega_m > 0Ωm​>0, ΩΛ>0\Omega_\Lambda > 0ΩΛ​>0 and Ωm+ΩΛ=1\Omega_m + \Omega_\Lambda = 1Ωm​+ΩΛ​=1; radiation and curvature are absent by construction, and dark energy is a true cosmological constant (w=−1w = -1w=−1), not a general equation of state. Time is a real variable with the big bang at t=0t = 0t=0, and every statement about the solution is restricted to t>0t > 0t>0, where sinh⁡θ>0\sinh\theta > 0sinhθ>0; outside that range the real power of a non-positive base is a junk value and nothing is claimed. Powers x1/3x^{1/3}x1/3, x2/3x^{2/3}x2/3 are real powers, while a3a^3a3 is a natural-number power. Derivatives are Mathlib's deriv/HasDerivAt; the Friedmann equation is stated in the source's ratio form (a˙/a)2=H02(Ωma−3+ΩΛ)(\dot a/a)^2 = H_0^2(\Omega_m a^{-3} + \Omega_\Lambda)(a˙/a)2=H02​(Ωm​a−3+ΩΛ​) rather than a cleared-denominator variant, and a(t)>0a(t) > 0a(t)>0 is part of the goal, so the statement cannot be satisfied by a degenerate a≡0a \equiv 0a≡0. The hypotheses Ωm,ΩΛ>0\Omega_m, \Omega_\Lambda > 0Ωm​,ΩΛ​>0 with Ωm+ΩΛ=1\Omega_m + \Omega_\Lambda = 1Ωm​+ΩΛ​=1 are jointly satisfiable, so no statement is vacuous.

The final milestone reuses the published FRWUniverse structure (an FRW universe with Newton's constant GGG, curvature KKK, time domain III, scale factor and its two derivatives, density, its derivative, and pressure, subject to both Friedmann equations pointwise) rather than introducing a competing model; contributions that connect these statements to distance–redshift relations, or that relax flatness or restore radiation, are welcome.

Selected references

  • Wikipedia, Lambda-CDM model, https://en.wikipedia.org/wiki/Lambda-CDM_model — section "Cosmic expansion history" (the Friedmann equation in density parameters, the closed-form solution, the age, and the acceleration transition).
  • Planck Collaboration, Planck 2018 results. VI. Cosmological parameters, Astronomy & Astrophysics 641 (2020) A6, https://doi.org/10.1051/0004-6361/201833910.
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Mathematical Physics·Captain: Lucas

Lorentz Factor: Kinematics of the Gamma FactorTextbook

Motivation

Every quantitative statement of special relativity — how much a moving clock slows, how much a moving rod shortens, how the momentum and energy of a fast particle grow — is controlled by a single dimensionless number, the Lorentz factor γ\gammaγ. It is the factor by which the time, length, and inertia of a body in uniform motion differ from their rest values, and it is the quantity that makes relativistic kinematics quantitative rather than qualitative. Its consequences are measured routinely: cosmic-ray muons with a mean lifetime of 2.2 μs2.2\,\mu\mathrm{s}2.2μs reach the ground from an altitude of about 10 km10\ \mathrm{km}10 km in numbers explained by their large γ\gammaγ, and the standard model of long gamma-ray bursts requires ejecta with initial γ≳100\gamma \gtrsim 100γ≳100 to resolve the compactness problem.

The material formalized here is textbook kinematics rather than open research: the definition of γ\gammaγ, the identities relating it to its reciprocal, to momentum, and to rapidity, its numerical and asymptotic behaviour, and the composition law of the boosts it parametrizes. The value of the mission is a reusable, machine-checked treatment of that material in Lean 4 — a small, self-contained piece of relativistic kinematics that later formalizations of Minkowski geometry or relativistic dynamics can build on.

Setting

Fix an inertial frame and a relative velocity vvv along a single spatial axis, and let ccc be the speed of light in vacuum. Write β=v/c\beta = v/cβ=v/c for the dimensionless velocity ratio. All statements in this mission are in units where c=1c = 1c=1, so β\betaβ is the only kinematic parameter and takes values in the interval (−1,1)(-1, 1)(−1,1) for a massive body.

The Lorentz factor is

γ(β)=11−β2,\gamma(\beta) = \frac{1}{\sqrt{1 - \beta^{2}}},γ(β)=1−β2​1​,

and its reciprocal is α(β)=1−β2=1/γ(β)\alpha(\beta) = \sqrt{1 - \beta^{2}} = 1/\gamma(\beta)α(β)=1−β2​=1/γ(β), the quantity tabulated alongside γ\gammaγ in the source article.

Two derived objects appear throughout. Relativistic velocity addition is

β1⊕β2=β1+β21+β1β2,\beta_1 \oplus \beta_2 = \frac{\beta_1 + \beta_2}{1 + \beta_1 \beta_2},β1​⊕β2​=1+β1​β2​β1​+β2​​,

and the Lorentz boost of velocity β\betaβ, acting on the coordinate pair (t,x)(t, x)(t,x) by t′=γ(t−βx)t' = \gamma(t - \beta x)t′=γ(t−βx) and x′=γ(x−βt)x' = \gamma(x - \beta t)x′=γ(x−βt), is the symmetric matrix

B(β)=(γ(β)−γ(β)β−γ(β)βγ(β)).B(\beta) = \begin{pmatrix} \gamma(\beta) & -\gamma(\beta)\beta \\ -\gamma(\beta)\beta & \gamma(\beta) \end{pmatrix}.B(β)=(γ(β)−γ(β)β​−γ(β)βγ(β)​).

Finally, the rapidity www of a motion is the hyperbolic angle with β=tanh⁡w\beta = \tanh wβ=tanhw.

Formalization targets

Goal — boosts compose by relativistic velocity addition

B(β1) B(β2)=B(β1⊕β2),γ(β1⊕β2)=γ(β1)γ(β2)(1+β1β2),∣β1⊕β2∣<1,B(\beta_1)\,B(\beta_2) = B(\beta_1 \oplus \beta_2), \qquad \gamma(\beta_1 \oplus \beta_2) = \gamma(\beta_1)\gamma(\beta_2)(1 + \beta_1\beta_2), \qquad |\beta_1 \oplus \beta_2| < 1,B(β1​)B(β2​)=B(β1​⊕β2​),γ(β1​⊕β2​)=γ(β1​)γ(β2​)(1+β1​β2​),∣β1​⊕β2​∣<1,

for all subluminal β1,β2\beta_1, \beta_2β1​,β2​. The goal asserts only the shape of the composition law — that the boosts are closed under composition and that the composed velocity is the relativistic sum — and fixes no numerical constants, so it is stable under any later refinement of the surrounding development.

Supporting targets

The milestones cover, in the order of the source article: the bound γ≥1\gamma \ge 1γ≥1 with equality exactly at rest; the reciprocal identity α=1/γ\alpha = 1/\gammaα=1/γ; strict monotonicity of γ\gammaγ on [0,1)[0,1)[0,1) and its divergence as β→1−\beta \to 1^{-}β→1−; the rapidity identities γ(tanh⁡w)=cosh⁡w\gamma(\tanh w) = \cosh wγ(tanhw)=coshw and γ(tanh⁡w)tanh⁡w=sinh⁡w\gamma(\tanh w)\tanh w = \sinh wγ(tanhw)tanhw=sinhw; additivity of rapidity, tanh⁡w1⊕tanh⁡w2=tanh⁡(w1+w2)\tanh w_1 \oplus \tanh w_2 = \tanh(w_1 + w_2)tanhw1​⊕tanhw2​=tanh(w1​+w2​); the momentum form γ=1+(p/m)2\gamma = \sqrt{1 + (p/m)^2}γ=1+(p/m)2​; the Newtonian limit (γ−1)/β2→12(\gamma - 1)/\beta^{2} \to \tfrac12(γ−1)/β2→21​ as β→0\beta \to 0β→0; the exact table entries γ(3/5)=5/4\gamma(3/5) = 5/4γ(3/5)=5/4, γ(4/5)=5/3\gamma(4/5) = 5/3γ(4/5)=5/3, γ(3/2)=2\gamma(\sqrt3/2) = 2γ(3​/2)=2; and the inversion 1−1/γ2=β\sqrt{1 - 1/\gamma^{2}} = \beta1−1/γ2​=β on [0,1)[0,1)[0,1).

Significance

The composition law is what turns the Lorentz factor from a formula into a group structure: closure of the boosts under composition, with velocities combining by ⊕\oplus⊕, is the reason rapidity is additive and the reason the velocity of light is the same in every inertial frame, since β1⊕β2\beta_1 \oplus \beta_2β1​⊕β2​ stays inside (−1,1)(-1,1)(−1,1). The supporting milestones are the facts a downstream development actually consumes — positivity and monotonicity of γ\gammaγ, the reciprocal identity, the momentum and rapidity representations, and the low-speed limit that recovers Newtonian kinetic energy.

None of these statements is mathematically open; all are standard. What the mission produces is their machine-checked form in Lean 4, stated against one fixed set of definitions so that the results compose with each other, together with a boost model usable by later work on Minkowski space. Mathlib supplies the analytic infrastructure (real square roots, hyperbolic functions, filters and limits, 2×22 \times 22×2 matrices) but carries no development of relativistic kinematics built on it.

Difficulty

The individual statements are elementary; the friction is in the analysis, not the physics. Three specific places are where a naive attempt stalls.

First, the real square root is a total function returning 000 on negative inputs, so γ\gammaγ is defined — and useless — outside ∣β∣<1|\beta| < 1∣β∣<1. Every algebraic step needs the positivity of 1−β2\sqrt{1-\beta^{2}}1−β2​ in hand before dividing, and the hypothesis ∣β∣<1|\beta| < 1∣β∣<1 must be propagated to each intermediate expression, including to the composed velocity β1⊕β2\beta_1 \oplus \beta_2β1​⊕β2​ in the goal.

Second, the goal's matrix identity does not follow from entrywise algebra alone: the entries of B(β1⊕β2)B(\beta_1 \oplus \beta_2)B(β1​⊕β2​) contain γ(β1⊕β2)\gamma(\beta_1 \oplus \beta_2)γ(β1​⊕β2​), a nested square root, and the composition law only becomes polynomial after the identity γ(β1⊕β2)=γ(β1)γ(β2)(1+β1β2)\gamma(\beta_1 \oplus \beta_2) = \gamma(\beta_1)\gamma(\beta_2)(1 + \beta_1\beta_2)γ(β1​⊕β2​)=γ(β1​)γ(β2​)(1+β1​β2​) has been proved. Attempting field_simp on the raw matrix equation, before establishing that identity, produces a goal with three independent radicals.

Third, the two asymptotic milestones are statements about filters, not pointwise bounds. The divergence at β→1−\beta \to 1^{-}β→1− is a one-sided limit that must be routed through the positivity of 1−β2\sqrt{1 - \beta^{2}}1−β2​ on a left neighbourhood of 111, and the Newtonian limit is stated on the punctured neighbourhood of 000, where the quotient (γ−1)/β2(\gamma - 1)/\beta^{2}(γ−1)/β2 has to be rewritten as a function continuous at 000 before any limit theorem applies.

Formalization scope

Everything is over the real numbers in units c=1c = 1c=1; the definitions bundle fixes γ\gammaγ, α\alphaα, ⊕\oplus⊕, and BBB as total functions, and the boost is the 2×22 \times 22×2 matrix acting on (t,x)(t, x)(t,x) with the sign convention t′=γ(t−βx)t' = \gamma(t - \beta x)t′=γ(t−βx). Subluminality is never built into the types: it appears as an explicit hypothesis ∣β∣<1|\beta| < 1∣β∣<1 on each statement that needs it, so the statements are about the physical regime and not about the junk values the definitions take elsewhere. Those junk values are the one trivialization risk worth naming: for ∣β∣≥1|\beta| \ge 1∣β∣≥1 the square root is 000 and γ(β)=0\gamma(\beta) = 0γ(β)=0, so a statement that omitted the hypothesis would be false rather than vacuous, and a statement that replaced it by an unsatisfiable condition would be vacuous — every milestone here carries hypotheses that are satisfiable and that exclude only the unphysical range.

A complete development needs Mathlib's real square root, hyperbolic functions, filter and limit API, and matrix notation; nothing beyond Mathlib is assumed. The boost model and the velocity-addition operation are the reusable parts: extensions to boosts in 3+13{+}13+1 dimensions, to the invariance of the Minkowski quadratic form, to time dilation and length contraction as corollaries of the goal, and to the energy–momentum relation are all welcome as follow-up contributions.

Selected references

  • Lorentz factor, Wikipedia (revision oldid=1355686906). https://en.wikipedia.org/w/index.php?title=Lorentz_factor&oldid=1355686906
  • J. Forshaw and G. Smith, Dynamics and Relativity, John Wiley & Sons, 2014, p. 118.
  • J. D. Jackson, Kinematics, Particle Data Group review, 2005 (rapidity, p. 7). https://pdg.lbl.gov/2005/reviews/kinemarpp.pdf
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Mathematical Physics·Captain: Lucas

The Lenz Coincidence: 6π56\pi^56π5 and the Proton-to-Electron Mass RatioTextbook

Motivation

The proton-to-electron mass ratio μ=mp/me\mu = m_p/m_eμ=mp​/me​ is a dimensionless constant of nature; the CODATA 2022 recommended value is

μ=1836.152673426(32),\mu = 1836.152673426(32),μ=1836.152673426(32),

the parenthesised digits being the standard uncertainty on the last two places, i.e. a relative standard uncertainty of 1.7×10−111.7\times10^{-11}1.7×10−11 (NIST CODATA).

In a two-sentence note in Physical Review in 1951, Friedrich Lenz observed that the then best experimental value, 1836.12±0.051836.12 \pm 0.051836.12±0.05, is matched almost exactly by the closed-form expression 6π56\pi^56π5. The observation is regarded as a numerical coincidence rather than a physical relation: measurement precision has improved by roughly nine orders of magnitude since 1951, and at today's precision the two numbers are close but demonstrably different. This mission fixes that statement as a machine-checked one — it asks for rational enclosures of 6π56\pi^56π5 sharp enough to decide the comparison in both directions: agreement with the 1951 datum, disagreement with the modern one.

The mathematics is elementary. The content is entirely in the rigour of the numerics: certified rational enclosures of a transcendental quantity rather than floating-point evaluations.

Setting

Throughout, all quantities are real numbers.

  • L:=6π5L := 6\pi^5L:=6π5 is Lenz's expression (lenzExpression in the formal development), with π\piπ the usual circle constant.
  • μ2022:=1836.152673426\mu_{2022} := 1836.152673426μ2022​:=1836.152673426 is the CODATA 2022 value of the mass ratio (codataValue), and u2022:=3.2×10−8u_{2022} := 3.2\times10^{-8}u2022​:=3.2×10−8 its standard uncertainty (codataUncertainty), the "(32)" attached to the last two digits.
  • μ1951:=1836.12\mu_{1951} := 1836.12μ1951​:=1836.12 is the experimental value available to Lenz (lenz1951Measurement) and u1951:=0.05u_{1951} := 0.05u1951​:=0.05 its quoted uncertainty (lenz1951Uncertainty).

These five constants are exactly the numbers appearing in the source; no physical model, no unit system and no dimensional analysis enters the mission. A "mass ratio" is modelled simply as a quotient mp/mem_p/m_emp​/me​ of two reals.

Formalization targets

Goal

For all reals mp,mem_p, m_emp​,me​ with mp/me=μ2022m_p/m_e = \mu_{2022}mp​/me​=μ2022​:

mp/me≠L,∣mp/me−L∣>106 u2022,1.88×10−5<mp/me−Lmp/me<1.89×10−5,m_p/m_e \neq L,\qquad |m_p/m_e - L| > 10^6\,u_{2022},\qquad 1.88\times10^{-5} < \frac{m_p/m_e - L}{m_p/m_e} < 1.89\times10^{-5},mp​/me​=L,∣mp​/me​−L∣>106u2022​,1.88×10−5<mp​/me​mp​/me​−L​<1.89×10−5,

while at the same time

∣L−μ1951∣<u1951.|L - \mu_{1951}| < u_{1951}.∣L−μ1951​∣<u1951​.

The goal deliberately packages both halves of the historical statement: Lenz's expression is inside the 1951 error bar and outside the 2022 one by more than a million standard uncertainties. The constants 10610^6106, 1.88×10−51.88\times10^{-5}1.88×10−5 and 1.89×10−51.89\times10^{-5}1.89×10−5 are stated with slack — the true values are about 1.08×1061.08\times10^61.08×106 and 1.8825×10−51.8825\times10^{-5}1.8825×10−5 — so the goal does not depend on the last digits quoted by any one source.

Supporting levels

306.019684<π5<306.019685,1836.1181<6π5<1836.11811.306.019684 < \pi^5 < 306.019685, \qquad 1836.1181 < 6\pi^5 < 1836.11811.306.019684<π5<306.019685,1836.1181<6π5<1836.11811.

Note that the second window must be narrower than 10−410^{-4}10−4: an enclosure of 6π56\pi^56π5 of width 10−410^{-4}10−4 is not sharp enough to imply the relative-deviation bounds of the goal, whose window has absolute width about 1.8×10−31.8\times10^{-3}1.8×10−3 but is centred 0.03460.03460.0346 away from μ2022\mu_{2022}μ2022​.

Significance

The result itself. The claim "6π5≠μ6\pi^5 \ne \mu6π5=μ" is quoted in reference works but is normally supported only by decimal expansions computed in floating point. What this mission produces is a certified version: enclosures of π5\pi^5π5 and 6π56\pi^56π5 with rational endpoints, verified by the kernel, separating Lenz's expression from the measured constant by more than a million standard uncertainties, together with the complementary fact that the same number is consistent with the 1951 datum — which is why the coincidence was reported in the first place.

Formalizing it. Status honesty: none of this is open mathematics, and the numerical facts are standard. Mathlib already provides 20-digit bounds for π\piπ (Real.pi_gt_d20, Real.pi_lt_d20) as well as the Real.pi_gt_sqrtTwoAddSeries / Real.pi_lt_sqrtTwoAddSeries machinery behind them, so the enclosures are reachable by monotonicity of x↦x5x \mapsto x^5x↦x5 on the nonnegative reals plus rational arithmetic. The mission's value is a clean, reusable formal record of a frequently quoted numerical comparison, not a new theorem. Contributions that go beyond a first proof — sharper enclosures, a general lemma bounding πn\pi^nπn, or comparisons against other quoted values of the ratio — are welcome.

Difficulty

This is an easy mission by design; the one place a first attempt goes wrong is precision bookkeeping.

  • The commonly used six-digit bounds 3.141592<π<3.1415933.141592 < \pi < 3.1415933.141592<π<3.141593 propagate to an uncertainty of about ±1.5×10−3\pm 1.5\times10^{-3}±1.5×10−3 in 6π56\pi^56π5, which decides the comparison with μ1951\mu_{1951}μ1951​ but is two orders of magnitude too coarse for the goal's relative-deviation window. The 20-digit bounds are needed.
  • The relative-deviation bounds are the binding constraint: they require an enclosure of 6π56\pi^56π5 of width about 10−510^{-5}10−5, not the 10−410^{-4}10−4 that a first draft naturally writes down.
  • Raising an enclosure of π\piπ to the fifth power multiplies the relative error by about 555; the input enclosure must be tighter than the target by that factor.

Formalization scope

All statements are over ℝ. The constants are published as a single definition file; lenzExpression is noncomputable since it mentions Real.pi. Decimal literals such as 1836.152673426 denote exact real numbers (the corresponding rationals), not floating-point approximations. Inequalities are strict throughout, and comparisons are stated with absolute values so that no sign convention is hidden.

The goal quantifies over two reals mp,mem_p, m_emp​,me​ subject only to mp/me=μ2022m_p/m_e = \mu_{2022}mp​/me​=μ2022​; no positivity is assumed, since the hypothesis already pins the quotient, and the hypothesis is satisfiable (e.g. me=1m_e = 1me​=1), so the statement is not vacuous. No measurement-theoretic notion of "uncertainty" is formalized: u2022u_{2022}u2022​ and u1951u_{1951}u1951​ are plain real constants appearing in the stated inequalities.

A complete development needs only Mathlib's Real.pi bound API and norm_num/linarith. The enclosure of π5\pi^5π5 is the one piece reusable beyond this mission.

Selected references

  • F. Lenz, The Ratio of Proton and Electron Masses, Physical Review 82 (1951) 554. doi:10.1103/PhysRev.82.554.2
  • CODATA 2022, proton-electron mass ratio, NIST Reference on Constants, Units, and Uncertainty. physics.nist.gov
  • Wikipedia, Proton-to-electron mass ratio, revision 1371273020. link
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Numerical Analysis·Captain: Lucas

Métodos Numéricos (Freitas) IV: Ajuste de Curvas e o Sistema Normal dos Mínimos QuadradosTextbook

Motivation

Experimental data are not exact, and forcing a curve through every measured point reproduces the noise rather than the law behind it. Curve fitting replaces interpolation by approximation: choose a family of shapes — a straight line, a polynomial of low degree, a combination of prescribed base functions — and pick the member of the family that is closest to the data in the least-squares sense. The resulting minimization is the numerical method most often used outside numerical analysis itself, from calibration curves to regression in statistics.

This mission is the fourth in a series formalizing the lecture notes Métodos Numéricos by Sergio Roberto de Freitas (UFMS, 2000). It covers Chapter 6, Ajuste de Curvas.

Setting

Data are m+1m+1m+1 pairs (xi,fi)(x_i, f_i)(xi​,fi​), i=0,dots,mi = 0, \\dots, mi=0,dots,m. Fix n+1n+1n+1 base functions varphi0,dots,varphin\\varphi_0, \\dots, \\varphi_nvarphi0​,dots,varphin​ and look for coefficients c0,dots,cnc_0, \\dots, c_nc0​,dots,cn​ making

g(x)=c0varphi0(x)+dots+cnvarphin(x)g(x) = c_0\\varphi_0(x) + \\dots + c_n\\varphi_n(x)g(x)=c0​varphi0​(x)+dots+cn​varphin​(x)

close to the data. The least-squares functional is

S(c0,dots,cn)=sumi=0mbigl(c0varphi0(xi)+dots+cnvarphin(xi)−fibigr)2.S(c_0,\\dots,c_n) = \\sum_{i=0}^{m}\\bigl(c_0\\varphi_0(x_i) + \\dots + c_n\\varphi_n(x_i) - f_i\\bigr)^2 .S(c0​,dots,cn​)=sumi=0m​bigl(c0​varphi0​(xi​)+dots+cn​varphin​(xi​)−fi​bigr)2.

Setting the partial derivatives to zero gives the normal system

sumi=0mvarphik(xi)bigl(c0varphi0(xi)+dots+cnvarphin(xi)bigr);=;sumi=0mvarphik(xi)fi,qquadk=0,dots,n,\\sum_{i=0}^{m}\\varphi_k(x_i)\\bigl(c_0\\varphi_0(x_i)+\\dots+c_n\\varphi_n(x_i)\\bigr) \\;=\\; \\sum_{i=0}^{m}\\varphi_k(x_i)f_i, \\qquad k = 0,\\dots,n,sumi=0m​varphik​(xi​)bigl(c0​varphi0​(xi​)+dots+cn​varphin​(xi​)bigr);=;sumi=0m​varphik​(xi​)fi​,qquadk=0,dots,n,

whose matrix is the Gram matrix akj=sumivarphik(xi)varphij(xi)a_{kj} = \\sum_i \\varphi_k(x_i)\\varphi_j(x_i)akj​=sumi​varphik​(xi​)varphij​(xi​).

Target

The goal theorem is the necessity direction of §6.3: a coefficient vector that minimizes SSS satisfies the normal system.

The milestones complete the picture the source leaves informal. First, the converse: any solution of the normal system is a global minimizer, so the normal system characterizes the least-squares fit rather than merely constraining it. Second, existence and uniqueness of the minimizer when the Gram matrix is invertible — the source assumes a minimum exists on geometric grounds, and this milestone supplies the hypothesis under which the assumption is a theorem. Third, the classical linear case varphi0=1\\varphi_0 = 1varphi0​=1, varphi1=x\\varphi_1 = xvarphi1​=x, where the normal system is the familiar pair of equations in the sums sumxi\\sum x_isumxi​, sumxi2\\sum x_i^2sumxi2​, sumfi\\sum f_isumfi​, sumxifi\\sum x_i f_isumxi​fi​.

Significance

The normal equations are the computational content of least squares: they turn an optimization over mathbbRn+1\\mathbb{R}^{n+1}mathbbRn+1 into one linear system, which the previous mission's methods can solve. The converse direction matters in practice because it is what licenses stopping at a stationary point, and the invertibility criterion is what tells a practitioner when the fit is determined by the data rather than under-determined by a badly chosen family of base functions.

Difficulty

The source differentiates SSS formally and reads off the necessary condition; a formal proof must either differentiate rigorously or argue directly with the quadratic expansion

S(c+tv)=S(c)+2tlangletextresidual,Phivrangle+t2lVertPhivrVert2,S(c+tv) = S(c) + 2t\\langle \\text{residual}, \\Phi v\\rangle + t^2\\lVert \\Phi v\\rVert^2,S(c+tv)=S(c)+2tlangletextresidual,Phivrangle+t2lVertPhivrVert2,

which also gives the converse at once. The existence-and-uniqueness milestone is where the real work is: invertibility of the Gram matrix has to be converted into positive definiteness of the quadratic form, and that into the existence of a unique global minimum.

Formalization scope

The data are indexed by a finite type with m+1m+1m+1 elements and the coefficients by one with n+1n+1n+1 elements, so both families are nonempty; the number of data points is not assumed to exceed the number of base functions, and the degenerate cases (repeated nodes, linearly dependent base functions) are allowed except where the Gram hypothesis excludes them. The base functions are arbitrary real functions given as a family varphi\\varphivarphi, evaluated only at the nodes xix_ixi​. Minimality is stated globally — the coefficient vector is compared with every other coefficient vector — not as a local or stationary condition, which avoids any appeal to differentiability in the statement. The Gram matrix hypothesis is that its determinant is a unit of mathbbR\\mathbb{R}mathbbR, i.e. nonzero. In the linear case the base functions are supplied together with the equations identifying them as the constant function 111 and the identity, so that the statement's two displayed equations are exactly the classical normal system.

Selected references

  • S. R. Freitas, Métodos Numéricos, Departamento de Computação e Estatística, Universidade Federal de Mato Grosso do Sul, 2000. Chapter 6, Ajuste de Curvas, pp. 119–131. (Course notes supplied with this mission.)
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Numerical Analysis·Captain: Lucas

Métodos Numéricos (Freitas) VI: Integração Numérica e o Erro da Fórmula de SimpsonTextbook

Motivation

Many definite integrals cannot be evaluated in closed form — the normal distribution function is the standard example in the source — and many others are integrals of functions known only through a table of values. Numerical quadrature replaces the integrand by an interpolating polynomial on each subinterval and integrates that instead. The two classical rules obtained this way, the trapezoidal rule (linear interpolation) and Simpson's rule (quadratic interpolation), come with error terms proportional to h2h^2h2 and h4h^4h4 respectively, and it is those error terms that tell the user how fine the subdivision has to be.

This mission is the sixth in a series formalizing the lecture notes Métodos Numéricos by Sergio Roberto de Freitas (UFMS, 2000). It covers Chapter 8, Integração Numérica.

Setting

Let fff be defined on [a,b][a,b][a,b] and subdivide the interval into nnn equal parts of length h=(b−a)/nh = (b-a)/nh=(b−a)/n, with nodes xi=a+ihx_i = a + ihxi​=a+ih.

The composite trapezoidal rule is

Tn=hleft(fracf(x0)+f(xn)2+sumi=1n−1f(xi)right),T_n = h\\left(\\frac{f(x_0) + f(x_n)}{2} + \\sum_{i=1}^{n-1} f(x_i)\\right),Tn​=hleft(fracf(x0​)+f(xn​)2+sumi=1n−1​f(xi​)right),

and the composite Simpson rule, defined when the number of subintervals is even, n=2kn = 2kn=2k, is

Sn=frach3Bigl(f(x0)+4f(x1)+2f(x2)+dots+4f(x2k−1)+f(x2k)Bigr).S_n = \\frac{h}{3}\\Bigl(f(x_0) + 4f(x_1) + 2f(x_2) + \\dots + 4f(x_{2k-1}) + f(x_{2k})\\Bigr).Sn​=frach3Bigl(f(x0​)+4f(x1​)+2f(x2​)+dots+4f(x2k−1​)+f(x2k​)Bigr).

The chapter derives, for each rule, an exact error term containing a derivative of fff at an unspecified intermediate point.

Target

The goal theorem is the composite Simpson error formula, equation (8.3): if fff is four times continuously differentiable on [a,b][a,b][a,b] and n=2kn = 2kn=2k with kge1k \\ge 1kge1, then there is muin(a,b)\\mu \\in (a,b)muin(a,b) with

intabf(x),dx;=;Sn;−;frac(b−a)5180,n4f(4)(mu).\\int_a^b f(x)\\,dx \\;=\\; S_n \\;-\\; \\frac{(b-a)^5}{180\\,n^4} f^{(4)}(\\mu).intab​f(x),dx;=;Sn​;−;frac(b−a)5180,n4f(4)(mu).

The milestones are the three error formulas the derivation passes through: the simple trapezoidal error −frach312f′′(mu)-\\frac{h^3}{12}f''(\\mu)−frach312f′′(mu) on one subinterval, its composite version −frac(b−a)h212f′′(mu)-\\frac{(b-a)h^2}{12}f''(\\mu)−frac(b−a)h212f′′(mu), and the simple Simpson error −frach590f(4)(mu)-\\frac{h^5}{90}f^{(4)}(\\mu)−frach590f(4)(mu) on a pair of subintervals.

Significance

The two composite error formulas are what turn a quadrature rule into a method with an accuracy guarantee: bounding ∣f′′∣|f''|∣f′′∣ or ∣f(4)∣|f^{(4)}|∣f(4)∣ by a constant on [a,b][a,b][a,b] converts them into the bounds fracM2(b−a)312n2\\frac{M_2(b-a)^3}{12n^2}fracM2​(b−a)312n2 and fracM4(b−a)5180n4\\frac{M_4(b-a)^5}{180n^4}fracM4​(b−a)5180n4, from which the number of subintervals needed for a prescribed tolerance is read off directly. The n−4n^{-4}n−4 rate is also the standard illustration of why a higher-order rule is worth its extra function evaluations, and why Simpson's rule is exact for cubics despite being built from quadratic interpolation.

Difficulty

Both composite formulas are obtained from the per-subinterval error by summing and then invoking the intermediate value theorem to replace a sum of derivative values at unknown points by nnn times the derivative at a single unknown point. That step needs continuity of the relevant derivative on the whole interval and a genuine intermediate-value argument, which is the part that a formal proof cannot wave through. The simple Simpson error itself is not a one-line Taylor estimate: the source integrates a remainder three times, and the standard alternative is a Peano-kernel argument.

Formalization scope

Integrals are the interval integral of a real-valued function with respect to Lebesgue measure. Smoothness is stated as continuous differentiability of order 222 (trapezoid) or 444 (Simpson) on the relevant closed interval, and the derivative in the error term is the iterated derivative computed within that closed interval; on the interior this coincides with the ordinary derivative. The quadrature rules are defined for arbitrary aaa, bbb and subdivision count, with h=(b−a)/nh = (b-a)/nh=(b−a)/n computed by total division, so the definitions also make sense for n=0n = 0n=0; the theorems assume a<ba < ba<b and a positive number of subintervals. Simpson's rule is parameterised by the half-count kkk, so the number of subintervals is 2k2k2k and is even by construction. The intermediate point mu\\mumu is asserted to exist in the open interval, with no uniqueness and no relation to the subdivision.

Selected references

  • S. R. Freitas, Métodos Numéricos, Departamento de Computação e Estatística, Universidade Federal de Mato Grosso do Sul, 2000. Chapter 8, Integração Numérica, pp. 163–182. (Course notes supplied with this mission.)
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Numerical Analysis·Captain: Lucas

Métodos Numéricos (Freitas) VIII: Erros de Arredondamento e PropagaçãoTextbook

Motivation

Every numerical computation is performed in a finite arithmetic: a real number is stored with a fixed number of decimal digits, and each stored value carries an error. Before any method is analysed, a course in numerical methods has to say how large that error can be and how it grows when approximate values are combined. The answers are the two rounding bounds — 101−t10^{1-t}101−t for truncation and tfrac12101−t\\tfrac12 10^{1-t}tfrac12101−t for symmetric rounding with ttt digits — and the propagation formulas for sums, products and quotients.

This mission is the eighth in a series formalizing the lecture notes Métodos Numéricos by Sergio Roberto de Freitas (UFMS, 2000). It covers Chapter 2, Erros.

Setting

Every nonzero real xxx can be written in normalized decimal form with ttt retained digits,

x=ftimes10e+gtimes10e−t,qquad0.1le∣f∣<1,quad0leg<1,x = f \\times 10^{e} + g \\times 10^{e-t}, \\qquad 0.1 \\le |f| < 1, \\quad 0 \\le g < 1,x=ftimes10e+gtimes10e−t,qquad0.1le∣f∣<1,quad0leg<1,

where eee is the decimal exponent of xxx and fff its normalized mantissa.

Truncated rounding keeps tildex=ftimes10e\\tilde{x} = f\\times 10^{e}tildex=ftimes10e, discarding the tail; the error is ex=x−tildex=gtimes10e−te_x = x - \\tilde{x} = g\\times 10^{e-t}ex​=x−tildex=gtimes10e−t.

Symmetric rounding keeps tildex=ftimes10e\\tilde{x} = f\\times 10^{e}tildex=ftimes10e when g<0.5g < 0.5g<0.5 and tildex=ftimes10e+10e−t\\tilde{x} = f\\times10^{e} + 10^{e-t}tildex=ftimes10e+10e−t when gge0.5g \\ge 0.5gge0.5; this is the familiar school rule of rounding the (t+1)(t+1)(t+1)-st digit up when it is at least 555.

If tildex\\tilde{x}tildex approximates xxx and tildey\\tilde{y}tildey approximates yyy, the absolute errors are ex=x−tildexe_x = x - \\tilde{x}ex​=x−tildex and ey=y−tildeye_y = y - \\tilde{y}ey​=y−tildey, and the chapter computes the error of the four arithmetic operations in terms of them.

Target

The goal theorem is Proposição 2.4.3: with symmetric rounding to tge1t \\ge 1tge1 digits, the relative error of a stored positive number satisfies

frac∣x−tildex∣∣tildex∣;le;frac12,101−t.\\frac{|x - \\tilde{x}|}{|\\tilde{x}|} \\;\\le\\; \\frac{1}{2}\\,10^{1-t}.frac∣x−tildex∣∣tildex∣;le;frac12,101−t.

The milestones are the companion bound for truncated rounding, 101−t10^{1-t}101−t (Proposição 2.4.2), and the propagation identities of §2.5.1 for the sum and difference, for the product and for the quotient.

Significance

These bounds are the unit of account for every later error analysis: the machine epsilon of a ttt-digit decimal arithmetic is exactly the constant appearing in the goal, and the factor two between truncation and symmetric rounding is the reason the latter is the default. The propagation identities explain the two classical failure modes of floating-point computation — cancellation in a difference of nearly equal numbers, where the absolute errors survive while the result shrinks, and the amplification of a relative error by division by a small number.

Difficulty

The difficulty is entirely in the normalization. The bounds follow from two facts about the decimal decomposition — that the discarded part is at most one unit in the last retained place, and that the retained part is at least 10e−110^{e-1}10e−1 — and both have to be derived from the definition of the decimal exponent through the floor function and the logarithm, including the boundary case where xxx is an exact power of ten and the case where symmetric rounding carries into a new leading digit. The propagation statements, by contrast, are algebraic identities.

Formalization scope

The decimal exponent is defined as lfloorlog10∣x∣rfloor+1\\lfloor \\log_{10}|x| \\rfloor + 1lfloorlog10​∣x∣rfloor+1, and the two roundings are defined by scaling by 10t−e10^{t-e}10t−e, applying the floor function (with an added tfrac12\\tfrac12tfrac12 in the symmetric case, so that halves round up) and scaling back. This is a total definition for every real number; the theorems are stated for x>0x > 0x>0 and tge1t \\ge 1tge1, which is the situation the source describes, and no claim is made about negative arguments or about x=0x = 0x=0.

Two points of deviation should be checked by the auditor. First, the source states both bounds with a strict inequality; for symmetric rounding equality is attained when the discarded tail is exactly one half unit in the last place, so the formal statement uses a non-strict inequality, while the truncation bound remains strict. Second, the propagation formulas for the product and the quotient are stated here as exact identities: the source's versions drop the second-order term exeye_xe_yex​ey​ and the higher terms of a geometric series, which is a legitimate approximation but not an equality.

Selected references

  • S. R. Freitas, Métodos Numéricos, Departamento de Computação e Estatística, Universidade Federal de Mato Grosso do Sul, 2000. Chapter 2, Erros, pp. 17–31. (Course notes supplied with this mission.)
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Mathematical Physics·Captain: Lucas

Particle in a Ring: Quantized Energies on the CircleTextbook

Motivation

The particle in a ring is the simplest quantum system in which a boundary condition of purely topological origin — single-valuedness of the wave function on a circle — forces the energy spectrum to be discrete. A free particle of mass mmm confined to a circle of radius RRR has no potential well and no classical turning points; nothing about the differential equation alone selects a discrete set of energies. Quantization arises solely from the requirement that the solution close up after one revolution. For that reason the model is the standard first illustration of angular-momentum quantization in quantum mechanics courses, and the azimuthal factor of the hydrogen-atom eigenfunctions is exactly the eigenfunction family derived here.

The model is also used quantitatively. In organic chemistry the free-electron model treats the π\piπ electrons of an aromatic ring, such as benzene, as particles on a circular waveguide; filling all levels up to index nnn takes 2×(2n+1)=4n+22\times(2n+1) = 4n+22×(2n+1)=4n+2 electrons once electron spin is counted, which is the counting behind Hückel's rule for aromatic stability. In rotational spectroscopy the same spectrum approximates the rotational levels of a rigid rotor.

This mission formalizes the model as presented in the Wikipedia article Particle in a ring (revision 1318339663): the eigenfunctions, the eigenenergies, the normalization and orthogonality relations, the two-fold degeneracy of every level with n≠0n \neq 0n=0, the count of 2n+12n+12n+1 states up to level nnn, and — as the goal — the statement that the admissible energies are exactly the quantized values.

Setting

Write θ\thetaθ for the angular coordinate on the ring of radius RRR. A state is a function ψ:R→C\psi : \mathbb{R} \to \mathbb{C}ψ:R→C of θ\thetaθ alone. Since the Laplacian on the ring is ∇2=R−2 ∂2/∂θ2\nabla^2 = R^{-2}\,\partial^2/\partial\theta^2∇2=R−2∂2/∂θ2, the time-independent Schrödinger equation −ℏ22m∇2ψ=Eψ-\frac{\hbar^2}{2m}\nabla^2\psi = E\psi−2mℏ2​∇2ψ=Eψ becomes

−ℏ22mR2 ψ′′(θ)  =  E ψ(θ),θ∈R,-\frac{\hbar^{2}}{2mR^{2}}\,\psi''(\theta) \;=\; E\,\psi(\theta), \qquad \theta \in \mathbb{R},−2mR2ℏ2​ψ′′(θ)=Eψ(θ),θ∈R,

and single-valuedness on the circle is imposed as the periodic boundary condition

ψ(θ+2π)=ψ(θ),θ∈R.\psi(\theta + 2\pi) = \psi(\theta), \qquad \theta \in \mathbb{R}.ψ(θ+2π)=ψ(θ),θ∈R.

A stationary state of energy EEE is a function ψ\psiψ that is twice continuously differentiable on R\mathbb{R}R, satisfies the periodic boundary condition, and solves the displayed equation. Normalization is over one period,

∫02π∣ψ(θ)∣2 dθ=1.\int_0^{2\pi} |\psi(\theta)|^{2}\, d\theta = 1 .∫02π​∣ψ(θ)∣2dθ=1.

For each integer nnn put

ψn(θ)  =  12π einθ,En  =  n2ℏ22mR2.\psi_n(\theta) \;=\; \frac{1}{\sqrt{2\pi}}\, e^{i n \theta}, \qquad E_n \;=\; \frac{n^{2}\hbar^{2}}{2mR^{2}} .ψn​(θ)=2π​1​einθ,En​=2mR2n2ℏ2​.

Here ℏ,m,R\hbar, m, Rℏ,m,R are real parameters, taken positive where positivity matters.

Formalization targets

Goal — the spectrum is exactly the quantized set

For ℏ,m,R>0\hbar, m, R > 0ℏ,m,R>0 and E∈RE \in \mathbb{R}E∈R:

(∃ ψ≢0 of class C2, 2π-periodic, −ℏ22mR2ψ′′=Eψ)  ⟺  ∃ n∈Z, E=n2ℏ22mR2.\Bigl(\exists\, \psi \not\equiv 0 \ \text{of class } C^{2},\ 2\pi\text{-periodic},\ -\tfrac{\hbar^{2}}{2mR^{2}}\psi'' = E\psi \Bigr) \iff \exists\, n \in \mathbb{Z},\ E = \frac{n^{2}\hbar^{2}}{2mR^{2}} .(∃ψ≡0 of class C2, 2π-periodic, −2mR2ℏ2​ψ′′=Eψ)⟺∃n∈Z, E=2mR2n2ℏ2​.

The right-to-left direction is the construction of ψn\psi_nψn​; the left-to-right direction is the quantization statement proper, and it must rule out every EEE that is not of this form, including all E<0E < 0E<0 and every positive EEE whose associated wave number is not an integer.

Supporting targets

The milestones cover, in order: the periodicity of ψn\psi_nψn​; its normalization; the identity ψn′′=−n2ψn\psi_n'' = -n^{2}\psi_nψn′′​=−n2ψn​; the resulting fact that ψn\psi_nψn​ is a stationary state of energy EnE_nEn​; the orthonormality relation ∫02πψj‾ ψn dθ=δjn\int_0^{2\pi}\overline{\psi_j}\,\psi_n\,d\theta = \delta_{jn}∫02π​ψj​​ψn​dθ=δjn​; the two-fold degeneracy E−n=EnE_{-n} = E_nE−n​=En​ with ψn,ψ−n\psi_n, \psi_{-n}ψn​,ψ−n​ linearly independent for n≠0n \neq 0n=0; and the level count, that exactly 2N+12N+12N+1 integers nnn satisfy En≤ENE_n \le E_NEn​≤EN​.

Significance

The result itself fixes the spectrum of the free Hamiltonian on the circle, with the degeneracy pattern 1,2,2,2,…1, 2, 2, 2, \dots1,2,2,2,… and the 2N+12N+12N+1 level count that underlies the 4N+24N+24N+2 electron count of Hückel's rule. The orthonormality relation is the statement that the eigenfunctions form the classical Fourier system on [0,2π][0, 2\pi][0,2π]; the assertion that every ring wave function is a superposition of the ψn\psi_nψn​ is precisely the Fourier expansion theorem for periodic functions.

Formalizing it produces a small, reusable Lean development: a periodic-boundary-condition predicate, a second-order eigenvalue problem stated through iteratedDeriv, and a complete spectral determination for that problem. Mathlib supplies the Fourier exponentials on AddCircle and their orthonormality in L2L^2L2, but the pointwise, C2C^2C2, real-eigenvalue formulation used here is not present as such, and no formalization of this spectral statement currently exists on the platform. The supporting milestones are routine analysis; the goal theorem is where the content sits.

The physics is standard textbook material and is not in question; what this mission adds is the machine-checked proof.

Difficulty

The naive argument — "write the general solution as Aeikθ+Be−ikθA e^{ik\theta} + B e^{-ik\theta}Aeikθ+Be−ikθ with k=R2mE/ℏk = R\sqrt{2mE}/\hbark=R2mE​/ℏ, then impose periodicity" — assumes the classification of solutions of ψ′′=−k2ψ\psi'' = -k^{2}\psiψ′′=−k2ψ, which must itself be established over C\mathbb{C}C for a C2C^{2}C2, not a priori analytic, function. Three regimes must be treated separately and none may be skipped: E>0E > 0E>0, where periodicity forces k∈Zk \in \mathbb{Z}k∈Z and hence E=EkE = E_kE=Ek​; E=0E = 0E=0, where the solutions are affine in θ\thetaθ and periodicity kills the linear term, leaving n=0n = 0n=0; and E<0E < 0E<0, where the solutions are real exponentials and periodicity forces ψ≡0\psi \equiv 0ψ≡0, contradicting nontriviality. The third case is where a careless proof quietly assumes what it should prove.

Formalization scope

Wave functions are total functions R→C\mathbb{R} \to \mathbb{C}R→C of the angular variable, not functions on a quotient or on AddCircle; periodicity is an explicit hypothesis. Smoothness is ContDiff ℝ 2, and the second derivative is iteratedDeriv 2, so the Schrödinger equation is a pointwise identity in C\mathbb{C}C, holding at every real θ\thetaθ. The energy EEE ranges over R\mathbb{R}R, not C\mathbb{C}C: the mission does not address non-self-adjoint or complex-eigenvalue variants. The parameters ℏ,m,R\hbar, m, Rℏ,m,R are explicit real arguments rather than fixed constants, and positivity is assumed exactly where it is needed; note that under Lean's convention for division by zero, degenerate parameter values make both sides of the equation vanish, which is why the goal theorem carries ℏ,m,R>0\hbar, m, R > 0ℏ,m,R>0. Integrals are interval integrals over [0,2π][0, 2\pi][0,2π] with respect to Lebesgue measure.

The goal cannot be satisfied vacuously: the right-hand side of the equivalence is satisfiable (take n=0n = 0n=0), and the left-hand side explicitly requires a ψ\psiψ with ψ(θ)≠0\psi(\theta) \neq 0ψ(θ)=0 at some point, so the trivial solution is excluded. Contributions that build reusable infrastructure — a classification of C2C^{2}C2 solutions of ψ′′=c ψ\psi'' = c\,\psiψ′′=cψ over C\mathbb{C}C, or a bridge between this pointwise formulation and Mathlib's AddCircle Fourier basis — are welcome, and would serve any later mission on one-dimensional periodic Schrödinger operators.

Selected references

  • Wikipedia, Particle in a ring, revision 1318339663, https://en.wikipedia.org/wiki/Particle_in_a_ring — the source text for this mission's statements.
  • H. Cox, Problems and Solutions to accompany Physical Chemistry: a Molecular Approach, University Science Books, p. 141, ISBN 978-0935702439 — the reference cited by the source for the angular reduction of the Laplacian.
  • Wikipedia, Hückel's rule, https://en.wikipedia.org/wiki/H%C3%BCckel%27s_rule — the 4n+24n+24n+2 electron count obtained from the level count formalized here.
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Mathematical PhysicsPartial Differential Equations·Captain: Lucas

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

Motivation

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

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

Setting

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

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

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

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

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

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

and the Boltzmann equation with this operator is

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

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

Formalization targets

Goal — the BGK HHH-theorem with its equality case

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

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

Milestones

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

Significance

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

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

Difficulty

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

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

Formalization scope

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

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

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

Selected references

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

Planck's Law and Wien's Displacement LawTextbook

Motivation

A black body is an idealized object that absorbs all radiation falling on it and, when held at a fixed absolute temperature TTT, re-emits radiation whose spectrum depends on TTT alone — not on the material, shape, or history of the body. Measuring that spectrum, and explaining it, was the central problem of late nineteenth-century thermal physics: the classical prediction of Rayleigh and Jeans grows without bound at short wavelengths, which is not what cavity radiation does.

Max Planck's 1900 formula fits the measured spectrum at every temperature and every wavelength, and it does so by quantizing the energy exchanged between matter and the radiation field. Two features of that formula are used constantly outside physics proper — in astronomy, remote sensing, radiometry, and illumination engineering. The first is the shape of the curve. The second is where its maximum sits: the peak wavelength is inversely proportional to the temperature, which is Wien's displacement law, discovered by Wilhelm Wien several years before Planck's formula and recovered from it as a corollary. This is why a heated piece of metal runs red, then orange, then white; why the Sun's per-wavelength emission peaks near 500 nm500\ \mathrm{nm}500 nm; and why infrared cameras aimed at mammals at 300 K300\ \mathrm{K}300 K are built for about 10 μm10\ \mu\mathrm{m}10 μm.

This mission formalizes Planck's law as a definition and derives Wien's displacement law from it, in both the wavelength and the frequency parameterization, including the transcendental maximization equation and the numerical value of its root.

Setting

Fix three positive real parameters: the Planck constant hhh, the speed of light ccc, and the Boltzmann constant kBk_BkB​. They are left as variables rather than numerical constants, so that every statement is a theorem about the functional form, valid in any unit system.

For an absolute temperature T>0T > 0T>0, Planck's law is given in two parameterizations. Per unit frequency ν>0\nu > 0ν>0, the spectral radiance is

Bν(ν,T)  =  2hν3/c2exp⁡ ⁣(hνkBT)−1,B_\nu(\nu, T) \;=\; \frac{2h\nu^3/c^2}{\exp\!\left(\dfrac{h\nu}{k_B T}\right) - 1},Bν​(ν,T)=exp(kB​Thν​)−12hν3/c2​,

and per unit wavelength λ>0\lambda > 0λ>0 it is

Bλ(λ,T)  =  2hc2/λ5exp⁡ ⁣(hcλkBT)−1.B_\lambda(\lambda, T) \;=\; \frac{2hc^2/\lambda^5}{\exp\!\left(\dfrac{hc}{\lambda k_B T}\right) - 1}.Bλ​(λ,T)=exp(λkB​Thc​)−12hc2/λ5​.

These are different functions, not the same function in different letters: radiance is defined per increment of the independent variable, so passing between them carries the Jacobian factor ∣dν/dλ∣=c/λ2|d\nu/d\lambda| = c/\lambda^2∣dν/dλ∣=c/λ2. Consequently the two curves peak at different physical locations, and the mission keeps both.

The third object is the dimensionless shape function

gn(x)  =  xnex−1,x>0,g_n(x) \;=\; \frac{x^n}{e^x - 1}, \qquad x > 0,gn​(x)=ex−1xn​,x>0,

with n=5n = 5n=5 for the wavelength form and n=3n = 3n=3 for the frequency form.

Target

The goal is Wien's displacement law in the wavelength parameterization. Writing x5x_5x5​ for the positive solution of the maximization equation x=5 (1−e−x)x = 5\,(1 - e^{-x})x=5(1−e−x), the goal asserts the existence of a constant

b  =  hcx5kB  >  0b \;=\; \frac{hc}{x_5 k_B} \;>\; 0b=x5​kB​hc​>0

such that for every temperature T>0T > 0T>0 the function λ↦Bλ(λ,T)\lambda \mapsto B_\lambda(\lambda, T)λ↦Bλ​(λ,T) on (0,∞)(0, \infty)(0,∞) has a strict global maximum, attained at

λpeak  =  bT,\lambda_{\mathrm{peak}} \;=\; \frac{b}{T},λpeak​=Tb​,

and nowhere else. With SI values of hhh, ccc, kBk_BkB​ this is b=2.897 771 955…×10−3 m⋅Kb = 2.897\,771\,955\ldots \times 10^{-3}\ \mathrm{m\cdot K}b=2.897771955…×10−3 m⋅K.

The milestones build to this: the Jacobian relation between the two parameterizations; the strong (temperature-independent shape) form of the law; existence and uniqueness of the root of the maximization equation; the strict maximum of gng_ngn​ at that root; the frequency-parameterized displacement law, with νpeak=x3kBT/h\nu_{\mathrm{peak}} = x_3 k_B T / hνpeak​=x3​kB​T/h and x3=2.821 439 372…x_3 = 2.821\,439\,372\ldotsx3​=2.821439372…; and a rigorous numerical enclosure of x5x_5x5​.

Significance

The result itself. Wien's displacement law is the quantitative content of "hotter means bluer". It converts an observed color into a temperature, which is how stellar surface temperatures, incandescent filament temperatures, and remote-sensed surface temperatures are read off in practice. Its strong form — that the spectrum has one fixed shape, rescaled by TTT — is what licenses tabulating the Planck spectrum once and reusing it at all temperatures, including the percentile table of the radiation distribution.

Formalizing it. Both results are classical and completely settled mathematically; the work here is machine-checked derivation, not discovery. Mathlib has the exponential function, derivatives, and the tools for strict-monotonicity and interval arguments, but carries no formalization of the Planck spectrum. This mission contributes a definition bundle for the Planck spectral radiance that later work (Stefan–Boltzmann, the Rayleigh–Jeans and Wien-approximation limits, the percentile table) can import directly, plus reusable analytic lemmas about x↦xn/(ex−1)x \mapsto x^n/(e^x - 1)x↦xn/(ex−1) and about the equation x=n(1−e−x)x = n(1 - e^{-x})x=n(1−e−x) that are independent of the physics.

Difficulty

The obvious argument — differentiate, set the derivative to zero, solve — fails at the last step: x=5(1−e−x)x = 5(1 - e^{-x})x=5(1−e−x) has no closed-form solution in elementary functions, and the informal source resolves it with the Lambert WWW function. A formal proof therefore cannot produce the maximizer explicitly; it must establish existence and uniqueness of the critical point and separately prove the critical point is a strict global maximum, which needs the behavior of xn/(ex−1)x^n/(e^x - 1)xn/(ex−1) at both ends of (0,∞)(0, \infty)(0,∞) rather than a local second-derivative test. The numerical milestone adds a different difficulty: certified bounds on a transcendental root require explicit rigorous estimates on exp⁡\expexp at a specific rational point, not floating-point evaluation.

A second trap is the parameterization. Substituting ν=c/λ\nu = c/\lambdaν=c/λ into BνB_\nuBν​ does not give BλB_\lambdaBλ​, and the two peaks genuinely differ (for T=6000 KT = 6000\ \mathrm{K}T=6000 K, 482.96 nm482.96\ \mathrm{nm}482.96 nm against 849.91 nm849.91\ \mathrm{nm}849.91 nm). The Jacobian milestone is stated precisely so that this cannot be blurred.

Formalization scope

Everything is over the real numbers. hhh, ccc, kBk_BkB​, TTT, λ\lambdaλ, ν\nuν are real variables carrying explicit positivity hypotheses wherever the statement needs them; no numerical values of the physical constants are hard-coded, and the physical dimensions are not modeled. The spectral radiance is defined by a total function, so it returns a junk value outside the intended domain (in particular where the denominator vanishes, at x=0x = 0x=0); every theorem restricts to the physical range by hypothesis, so no claim rests on junk values.

The peak statements are formulated as strict inequalities against all other admissible arguments — for the goal, every λ>0\lambda > 0λ>0 with λ≠b/T\lambda \neq b/Tλ=b/T — rather than as a local maximum or a vanishing-derivative condition. This rules out the trivializing formalizations: a first-order condition alone would not exclude a minimum or an inflection, and a local statement would not exclude a second, higher peak elsewhere.

The maximization constants are pinned down, not merely asserted to exist: the goal requires the constant bbb to equal hc/(xkB)hc/(x k_B)hc/(xkB​) for a positive xxx satisfying x=5(1−e−x)x = 5(1 - e^{-x})x=5(1−e−x), and a separate milestone gives the enclosure 4.9651142317<x<4.96511423184.9651142317 < x < 4.96511423184.9651142317<x<4.9651142318. Uniqueness of that root is itself a milestone, so the pair determines bbb completely.

A complete development needs Mathlib's Real.exp API, differentiability and the mean value theorem or a strict-monotonicity argument, and interval arithmetic or explicit Taylor bounds for the numerical enclosure. The lemmas about the shape function and about x=n(1−e−x)x = n(1 - e^{-x})x=n(1−e−x) are stated for a general exponent nnn and are reusable beyond this mission. Contributions of the Stefan–Boltzmann integral, the Rayleigh–Jeans and Wien approximation limits, and the logarithmic ("per proportional bandwidth") parameterization would be natural follow-ups but are out of scope here.

Selected references

  • M. Planck, Über das Gesetz der Energieverteilung im Normalspectrum, Annalen der Physik 4 (1901), 553–563. DOI: https://doi.org/10.1002/andp.19013090310
  • W. Wien, Über die Energievertheilung im Emissionsspectrum eines schwarzen Körpers, Annalen der Physik 294 (1896), 662–669. DOI: https://doi.org/10.1002/andp.18962940803
  • Planck's law, Wikipedia. https://en.wikipedia.org/wiki/Planck%27s_law
  • Wien's displacement law, Wikipedia. https://en.wikipedia.org/wiki/Wien%27s_displacement_law
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ProbabilityStochastic Systems·Captain: naimengye

Probability Theory and Examples V: Blumenthal's 0-1 Law and the Local Behaviour of Brownian PathsTextbook

Motivation

A Brownian path is continuous, and that is essentially all it is. It has no derivative anywhere, it crosses zero infinitely often in every interval (0,ϵ)(0,\epsilon)(0,ϵ), and it becomes positive and negative immediately after time zero. None of this is visible from the finite-dimensional distributions; it is a statement about the germ of the path at a point, and the tool that unlocks it is a zero-one law.

Chapter 7 of Rick Durrett's Probability: Theory and Examples (Version 5, 2019) develops that tool. The natural filtration Fs0=σ(Br:r≤s)\mathcal F^{0}_{s}=\sigma(B_r:r\le s)Fs0​=σ(Br​:r≤s) is enlarged to Fs+=⋂t>sFt0\mathcal F^{+}_{s}=\bigcap_{t>s}\mathcal F^{0}_{t}Fs+​=⋂t>s​Ft0​, which allows "an infinitesimal peek at the future" — a quantity like lim sup⁡t↓s(Bt−Bs)/f(t−s)\limsup_{t\downarrow s}(B_t-B_s)/f(t-s)limsupt↓s​(Bt​−Bs​)/f(t−s) is Fs+\mathcal F^{+}_{s}Fs+​-measurable but not Fs0\mathcal F^{0}_{s}Fs0​-measurable. Blumenthal's 0-1 law (Theorem 7.2.3) says that at s=0s=0s=0 this enlargement buys nothing probabilistically: the germ σ\sigmaσ-field F0+\mathcal F^{+}_{0}F0+​ is trivial.

Everything local follows. If the path had any chance of staying non-positive on some interval (0,ϵ)(0,\epsilon)(0,ϵ), that would be a germ event of probability at least 1/21/21/2 by symmetry, so it has probability one — and the path enters (0,∞)(0,\infty)(0,∞) immediately. Continuity then forces it to return to zero immediately as well. Combined with the time inversion Xt=tB(1/t)X_t=tB(1/t)Xt​=tB(1/t), which turns the germ at 000 into the tail at ∞\infty∞, the same law gives lim sup⁡t→∞Bt/t=∞\limsup_{t\to\infty}B_t/\sqrt t=\inftylimsupt→∞​Bt​/t​=∞ and the recurrence of one-dimensional Brownian motion.

Setting

Let (Ω,F,P)(\Omega,\mathcal F,\mathbb P)(Ω,F,P) be a probability space and B:R≥0→Ω→RB:\mathbb R_{\ge0}\to\Omega\to\mathbb RB:R≥0​→Ω→R a Brownian motion: its finite-dimensional laws are centred Gaussian with covariance cov⁡(Bs,Bt)=s∧t\operatorname{cov}(B_s,B_t)=s\wedge tcov(Bs​,Bt​)=s∧t, and almost every path is continuous. In particular B0=0B_0=0B0​=0 almost surely, so this is Durrett's P0\mathbb P_0P0​.

Three σ\sigmaσ-fields organize the chapter:

Ft0=σ(Bs:s≤t),F0+=⋂t>0Ft0,T=⋂t≥0σ(Bs:s≥t).\mathcal F^{0}_{t}=\sigma(B_s:s\le t),\qquad \mathcal F^{+}_{0}=\bigcap_{t>0}\mathcal F^{0}_{t},\qquad \mathcal T=\bigcap_{t\ge0}\sigma(B_s:s\ge t).Ft0​=σ(Bs​:s≤t),F0+​=t>0⋂​Ft0​,T=t≥0⋂​σ(Bs​:s≥t).

The first is the past, the second the germ at time zero, the third the tail at infinity.

A path fff is Lipschitz at the point sss with constant CCC when ∣f(t)−f(s)∣≤C∣t−s∣|f(t)-f(s)|\le C|t-s|∣f(t)−f(s)∣≤C∣t−s∣ for all ttt within some positive distance of sss. A path differentiable at sss is Lipschitz at sss, so failing this at every point and for every constant is a strong form of nowhere differentiability.

Formalization targets

Goal — Theorem 7.2.3, Blumenthal's 0-1 law

A∈F0+⟹P(A)∈{0,1}.A\in\mathcal F^{+}_{0}\quad\Longrightarrow\quad \mathbb P(A)\in\{0,1\}.A∈F0+​⟹P(A)∈{0,1}.

In words: the germ σ\sigmaσ-field is trivial. Nothing about the path in an arbitrarily short initial interval is genuinely random.

Supporting levels

Theorem 7.1.5, that Brownian paths are Hölder continuous of every exponent γ<1/2\gamma<1/2γ<1/2 on every bounded interval; Theorem 7.1.6, that with probability one they are not Lipschitz at any point, hence nowhere differentiable — the Paley–Wiener–Zygmund theorem in the proof of Dvoretsky, Erdős and Kakutani; Theorem 7.2.4, that the path enters (0,∞)(0,\infty)(0,∞) immediately; Theorem 7.2.5, that its zero set accumulates at 000; and Theorem 7.2.8, that lim sup⁡t→∞Bt/t=+∞\limsup_{t\to\infty}B_t/\sqrt t=+\inftylimsupt→∞​Bt​/t​=+∞ and lim inf⁡t→∞Bt/t=−∞\liminf_{t\to\infty}B_t/\sqrt t=-\inftyliminft→∞​Bt​/t​=−∞.

Significance

The results themselves. Blumenthal's law is the gateway to every local path property of Brownian motion, and Durrett uses it immediately for exactly that. Theorems 7.2.4 and 7.2.5 together say the path oscillates across zero infinitely often in every initial interval — the reason the zero set is an uncountable closed set of Lebesgue measure zero, and the reason the "first return to zero" is not a useful notion at time 000. Theorem 7.2.8 is the same law pushed to t→∞t\to\inftyt→∞ by time inversion, and it is what makes one-dimensional Brownian motion recurrent (Theorem 7.2.9).

The Hölder pair is the sharp description of path regularity. Exponent γ<1/2\gamma<1/2γ<1/2 always works, γ>1/2\gamma>1/2γ>1/2 never does, and the borderline 1/21/21/2 is subtle: P(t∈H1/2)=0\mathbb P(t\in H_{1/2})=0P(t∈H1/2​)=0 for each fixed ttt, but Davis (1983) showed P(H1/2≠∅)=1\mathbb P(H_{1/2}\ne\emptyset)=1P(H1/2​=∅)=1. Nowhere differentiability is the historical headline — Paley, Wiener and Zygmund (1933) — and the proof given here is a short covering argument rather than a series construction.

Formalizing them. Mathlib has the object but almost none of the theory. It defines IsPreBrownianReal and IsBrownianReal, proves that a centred Gaussian process with covariance s∧ts\wedge ts∧t is pre-Brownian, and supplies the invariances — negation, scaling t↦c−1/2B(ct)t\mapsto c^{-1/2}B(ct)t↦c−1/2B(ct), the shift t↦B(t0+t)−B(t0)t\mapsto B(t_0+t)-B(t_0)t↦B(t0​+t)−B(t0​), and the time inversion t↦tB(1/t)t\mapsto tB(1/t)t↦tB(1/t) — together with the weak Markov property IsPreBrownianReal.indepFun_shift. It does not have the germ or tail σ\sigmaσ-fields, Blumenthal's law, the strong Markov property, any path-regularity result, or the Kolmogorov–Chentsov continuity theorem: Probability/Process/Kolmogorov.lean defines IsKolmogorovProcess, the hypothesis, and stops there. So this mission supplies the σ\sigmaσ-fields and then everything Durrett proves with them.

Difficulty

The goal reduces to Durrett's Theorem 7.2.2, that E(Z∣Fs+)=E(Z∣Fs0)\mathbb E(Z\mid\mathcal F^{+}_{s})=\mathbb E(Z\mid\mathcal F^{0}_{s})E(Z∣Fs+​)=E(Z∣Fs0​) for bounded path-measurable ZZZ; at s=0s=0s=0, F00=σ(B0)\mathcal F^{0}_{0}=\sigma(B_0)F00​=σ(B0​) is trivial because B0=0B_0=0B0​=0 almost surely, so 1A=E(1A∣F0+)=P(A)\mathbf 1_A=\mathbb E(\mathbf 1_A\mid\mathcal F^{+}_{0})=\mathbb P(A)1A​=E(1A​∣F0+​)=P(A) almost surely, and an indicator almost surely equal to a constant forces that constant to be 000 or 111. Theorem 7.2.2 itself is a monotone class argument on top of the Markov property, and the Markov property in this setting is Mathlib's indepFun_shift plus the observation that the conditional expectation of a product ∏mfm(Btm)\prod_m f_m(B_{t_m})∏m​fm​(Btm​​) over Fs+\mathcal F^{+}_{s}Fs+​ lands in Fs0\mathcal F^{0}_{s}Fs0​. Assembling that is the work.

Theorem 7.2.4 is then three lines — P0(τ≤t)≥P0(Bt>0)=1/2\mathbb P_0(\tau\le t)\ge\mathbb P_0(B_t>0)=1/2P0​(τ≤t)≥P0​(Bt​>0)=1/2 by symmetry of the Gaussian, let t↓0t\downarrow0t↓0, apply the goal — provided the event has been shown to lie in the germ field, which is where continuity of paths enters. Theorem 7.2.5 follows from 7.2.4 applied to BBB and −B-B−B together with the intermediate value theorem.

Theorem 7.1.5 needs the Kolmogorov–Chentsov continuity theorem, which has to be built: from E∣Bt−Bs∣2m=Cm∣t−s∣m\mathbb E|B_t-B_s|^{2m}=C_m|t-s|^mE∣Bt​−Bs​∣2m=Cm​∣t−s∣m one gets Hölder-γ\gammaγ control for γ<(m−1)/2m\gamma<(m-1)/2mγ<(m−1)/2m, and m→∞m\to\inftym→∞ gives every γ<1/2\gamma<1/2γ<1/2. The dyadic chaining and Borel–Cantelli step is the substance, and it is worth building as a general theorem about IsKolmogorovProcess rather than only for Brownian motion.

Theorem 7.1.6 is self-contained and short: fix CCC, let AnA_nAn​ be the event that some s∈[0,1]s\in[0,1]s∈[0,1] has ∣Bt−Bs∣≤C∣t−s∣|B_t-B_s|\le C|t-s|∣Bt​−Bs​∣≤C∣t−s∣ whenever ∣t−s∣≤3/n|t-s|\le3/n∣t−s∣≤3/n, and bound P(An)≤n P(∣B1∣≤5Cn−1/2)3≤n{10Cn−1/2(2π)−1/2}3→0\mathbb P(A_n)\le n\,\mathbb P(|B_1|\le5Cn^{-1/2})^3\le n\{10Cn^{-1/2}(2\pi)^{-1/2}\}^3\to0P(An​)≤nP(∣B1​∣≤5Cn−1/2)3≤n{10Cn−1/2(2π)−1/2}3→0; since AnA_nAn​ increases, every P(An)=0\mathbb P(A_n)=0P(An​)=0.

Theorem 7.2.8 needs the tail 0-1 law, Theorem 7.2.7, which is the goal transported through the time inversion Xt=tB(1/t)X_t=tB(1/t)Xt​=tB(1/t) — Mathlib's IsPreBrownianReal.inv — because the tail field of BBB is the germ field of XXX. With that, P0(Bn/n≥K i.o.)≥P0(B1≥K)>0\mathbb P_0(B_n/\sqrt n\ge K\ \text{i.o.})\ge\mathbb P_0(B_1\ge K)>0P0​(Bn​/n​≥K i.o.)≥P0​(B1​≥K)>0 by scaling, so the probability is one, and KKK is arbitrary.

Formalization scope

The process is Mathlib's IsBrownianReal, indexed by ℝ≥0, on an abstract probability space — not the canonical path space C[0,∞)C[0,\infty)C[0,∞) that Durrett uses. This is why the shift operators θs\theta_sθs​ and the family {Px}\{\mathbb P_x\}{Px​} do not appear: there is one measure, the process starts at 000 almost surely, and each statement is about that process. Theorem 7.2.7 as Durrett states it quantifies over all starting points and has no direct analogue here; the tail 0-1 law for the process started at 000 does, and is listed under contributions as the route to Theorem 7.2.8.

The three σ\sigmaσ-fields are built as suprema and infima in the lattice of σ\sigmaσ-algebras on Ω\OmegaΩ: pastSigma B t is the supremum of the pullbacks of the Borel field along BsB_sBs​ for s≤ts\le ts≤t, and germSigma B, tailSigma B are the corresponding infima. The goal carries the hypothesis that each BtB_tBt​ is measurable, not merely almost-everywhere measurable, which is what IsPreBrownianReal gives and what puts these σ\sigmaσ-fields below the ambient one; the canonical construction satisfies it, and without it "P(A)\mathbb P(A)P(A)" for a germ event would be an outer measure.

Hölder continuity is stated locally — for almost every path, every TTT admits a constant — since global Hölder continuity on [0,∞)[0,\infty)[0,∞) is false. The order of quantifiers puts the null set first, so a single path works for every TTT at once.

The hitting statements avoid an infimum over a possibly empty set. "τ=0\tau=0τ=0 almost surely" is written as: almost surely, for every ϵ>0\epsilon>0ϵ>0 there is t∈(0,ϵ)t\in(0,\epsilon)t∈(0,ϵ) with Bt>0B_t>0Bt​>0; and "T0=0T_0=0T0​=0 almost surely" as the same with Bt=0B_t=0Bt​=0. These are equivalent to Durrett's statements and say what the infimum is there to say. Similarly Theorem 7.2.8 is written with ∃ᶠ … in atTop rather than as an extended-real lim sup⁡\limsuplimsup, which is what "lim sup⁡=+∞\limsup=+\inftylimsup=+∞" means and avoids a coercion.

LipschitzAtPoint f s C is "there is a scale δ>0\delta>0δ>0 on which ∣f(t)−f(s)∣≤C∣t−s∣|f(t)-f(s)|\le C|t-s|∣f(t)−f(s)∣≤C∣t−s∣". Its negation for every sss and every CCC is Theorem 7.1.6, and it has content in both directions: the identity path is Lipschitz at every point with C=1C=1C=1, while t↦tt\mapsto\sqrt tt↦t​ is not Lipschitz at 000 with C=1C=1C=1 — both checked in Lean before publishing.

Existence is not part of this mission. Mathlib proves nothing of the form "a Brownian motion exists", and nothing here needs it: every item takes a Brownian motion as a hypothesis. That the hypothesis is satisfiable is a theorem — Durrett's 7.1.1, via Kolmogorov extension and the continuity theorem — and it is listed under contributions, where it belongs, since building it is a project of its own.

Contributions welcome beyond the listed items: Kolmogorov–Chentsov as a general statement about IsKolmogorovProcess; Theorem 7.1.1, the existence of Brownian motion; Theorem 7.2.2 in full, for every sss; the tail 0-1 law and Theorem 7.2.9, recurrence; the strong Markov property and the reflection principle of section 7.3; and Exercise 7.1.5, that no path is Hölder of any exponent γ>1/2\gamma>1/2γ>1/2.

Selected references

  • Rick Durrett, Probability: Theory and Examples, Version 5 (11 January 2019), chapter 7, sections 7.1 and 7.2 (pp. 353–365); Theorems 7.1.5, 7.1.6, 7.2.3, 7.2.4, 7.2.5, 7.2.8. Published as the 5th edition, Cambridge University Press, 2019, DOI 10.1017/9781108591034
  • R. M. Blumenthal, An extended Markov property, Transactions of the American Mathematical Society 85 (1957), 52–72. DOI 10.1090/S0002-9947-1957-0088102-2
  • R. E. A. C. Paley, N. Wiener and A. Zygmund, Notes on random functions, Mathematische Zeitschrift 37 (1933), 647–668. DOI 10.1007/BF01474606
  • A. Dvoretzky, P. Erdős and S. Kakutani, Nonincrease everywhere of the Brownian motion process, Proceedings of the Fourth Berkeley Symposium II (1961), 103–116.
  • N. Wiener, Differential space, Journal of Mathematics and Physics 2 (1923), 131–174. DOI 10.1002/sapm192321131
  • I. Karatzas and S. E. Shreve, Brownian Motion and Stochastic Calculus, 2nd ed., Springer, 1991, chapter 2. DOI 10.1007/978-1-4612-0949-2
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Captain: abcdefg

Weighted Root Integral Identity for Ordered Positive RealsTextbook

Selected references

https://math.stackexchange.com/questions/4244874/can-we-prove-am-gm-inequality-using-these-integrals

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Topology·Captain: Lucas

Rudin PMA IV: ContinuityTextbook

Motivation

Continuity is the hypothesis under which limits may be moved inside a function, and Chapter 4 of Walter Rudin's Principles of Mathematical Analysis (3rd edition, McGraw-Hill, 1976) is about what continuity gives once the domain is compact or connected. Three of its theorems are used in nearly every later argument of the book: a continuous function on a compact set has compact image (Theorem 4.14), hence attains its bounds (4.16); a continuous function on a connected set has connected image (4.22), hence takes intermediate values (4.23); and a continuous function on a compact metric space is uniformly continuous (Theorem 4.19) — the δ\deltaδ can be chosen independently of the point.

The last of these is the chapter's capstone. Uniform continuity is exactly what is needed to prove that continuous functions are Riemann-integrable (Chapter 6), and it is the first place where compactness upgrades a pointwise hypothesis into a global one with a quantitative conclusion.

This mission is the fourth in a series formalizing Rudin Chapters 1–11; it uses the metric topology of Mission II and is a prerequisite for Missions V–VII.

Setting

Let X,YX, YX,Y be metric spaces, E⊆XE \subseteq XE⊆X, f:E→Yf : E \to Yf:E→Y, and let ppp be a limit point of EEE. Rudin writes lim⁡x→pf(x)=q\lim_{x \to p} f(x) = qlimx→p​f(x)=q when for every ε>0\varepsilon > 0ε>0 there is δ>0\delta > 0δ>0 with dY(f(x),q)<εd_Y(f(x), q) < \varepsilondY​(f(x),q)<ε for all x∈Ex \in Ex∈E satisfying 0<dX(x,p)<δ0 < d_X(x,p) < \delta0<dX​(x,p)<δ; the exclusion of x=px = px=p is deliberate, and it is what makes the notion agree with continuity only when f(p)=qf(p) = qf(p)=q (Theorem 4.6). fff is continuous at ppp if the same holds with the condition 0<dX(x,p)0 < d_X(x,p)0<dX​(x,p) dropped, and continuous if it is continuous at every point.

fff is uniformly continuous on XXX if for every ε>0\varepsilon > 0ε>0 there is a single δ>0\delta > 0δ>0 such that dY(f(p),f(q))<εd_Y(f(p), f(q)) < \varepsilondY​(f(p),f(q))<ε for all p,q∈Xp, q \in Xp,q∈X with dX(p,q)<δd_X(p,q) < \deltadX​(p,q)<δ. A real function on (a,b)(a,b)(a,b) is monotonically increasing if x<yx < yx<y implies f(x)≤f(y)f(x) \le f(y)f(x)≤f(y); its one-sided limits are written f(x−)f(x-)f(x−) and f(x+)f(x+)f(x+), and it has a discontinuity of the first kind at xxx when both exist but do not agree with f(x)f(x)f(x).

Formalization targets

Goal — uniform continuity on compacta (Theorem 4.19)

X compact metric space, f:X→Y continuous  ⟹  ∀ε>0 ∃δ>0 ∀p,q∈X, d(p,q)<δ⇒d(f(p),f(q))<ε.X \text{ compact metric space},\ f : X \to Y \text{ continuous} \;\Longrightarrow\; \forall \varepsilon > 0\ \exists \delta > 0\ \forall p, q \in X,\ d(p,q) < \delta \Rightarrow d(f(p), f(q)) < \varepsilon .X compact metric space, f:X→Y continuous⟹∀ε>0 ∃δ>0 ∀p,q∈X, d(p,q)<δ⇒d(f(p),f(q))<ε.

Milestones

f continuous at p  ⟺  lim⁡x→pf(x)=f(p)(4.6)f \text{ continuous at } p \iff \lim_{x \to p} f(x) = f(p) \qquad (4.6)f continuous at p⟺x→plim​f(x)=f(p)(4.6) f continuous  ⟺  f−1(V) open for every open V(4.8)f \text{ continuous} \iff f^{-1}(V) \text{ open for every open } V \qquad (4.8)f continuous⟺f−1(V) open for every open V(4.8) K compact⇒f(K) compact(4.14)K \text{ compact} \Rightarrow f(K) \text{ compact} \qquad (4.14)K compact⇒f(K) compact(4.14) a continuous real f on a compact X attains sup⁡f and inf⁡f(4.16)\text{a continuous real } f \text{ on a compact } X \text{ attains } \sup f \text{ and } \inf f \qquad (4.16)a continuous real f on a compact X attains supf and inff(4.16) f:X→Y continuous bijection, X compact⇒f−1 continuous(4.17)f : X \to Y \text{ continuous bijection, } X \text{ compact} \Rightarrow f^{-1} \text{ continuous} \qquad (4.17)f:X→Y continuous bijection, X compact⇒f−1 continuous(4.17) E connected⇒f(E) connected(4.22)E \text{ connected} \Rightarrow f(E) \text{ connected} \qquad (4.22)E connected⇒f(E) connected(4.22) f(a)<c<f(b)⇒f(x)=c for some x∈(a,b)(4.23)f(a) < c < f(b) \Rightarrow f(x) = c \text{ for some } x \in (a,b) \qquad (4.23)f(a)<c<f(b)⇒f(x)=c for some x∈(a,b)(4.23) f monotone⇒f(x−), f(x+) exist and f(x−)≤f(x)≤f(x+)(4.29)f \text{ monotone} \Rightarrow f(x-),\, f(x+) \text{ exist and } f(x-) \le f(x) \le f(x+) \qquad (4.29)f monotone⇒f(x−),f(x+) exist and f(x−)≤f(x)≤f(x+)(4.29) the discontinuity set of a monotone function is at most countable(4.30)\text{the discontinuity set of a monotone function is at most countable} \qquad (4.30)the discontinuity set of a monotone function is at most countable(4.30)

Significance

Uniform continuity is the hypothesis that converts local approximation into global approximation with a uniform error bound. In Chapter 6 it is what makes the upper and lower Riemann–Stieltjes sums of a continuous function come together; in Chapter 7 it underlies the equicontinuity of Arzelà–Ascoli; in Chapter 9 it appears again in the estimate of a C′C'C′ mapping on a compact ball. The extreme value theorem and the intermediate value theorem are the two existence theorems of elementary analysis, and both come from this chapter by combining Chapter 2's compactness and connectedness with continuity.

Theorem 4.30 — a monotone function has at most countably many discontinuities — is the result that makes monotone integrators well behaved in Chapter 6, and it is the first place in the book where a countability argument (Chapter 2) pays off analytically.

Mathlib has continuity, compactness and connectedness in general topological spaces, and most of the milestones can be matched to library results after the statements are put in Rudin's metric form. The formalization value is again in the dictionary: Rudin's punctured-limit definition versus ContinuousWithinAt, and his ε\varepsilonε–δ\deltaδ uniform continuity versus the library's uniformity-filter definition.

Difficulty

There is no single hard step; the difficulty is in the hypotheses being weaker than they look. In Theorem 4.6 the limit is taken through E∖{p}E \setminus \{p\}E∖{p}, so the equivalence with continuity genuinely needs p∈Ep \in Ep∈E and ppp a limit point; dropping the second hypothesis makes the statement false at isolated points. In Theorem 4.19 the naive proof — pick δp\delta_pδp​ at each point by continuity and take the infimum — fails because the infimum over infinitely many points can be 000; compactness is used to reduce to finitely many, and the factor of two in the radii of the covering balls is essential. Theorem 4.30 requires an injection from the discontinuity set into Q\mathbb{Q}Q, built from the gap between f(x−)f(x-)f(x−) and f(x+)f(x+)f(x+).

Formalization scope

Conventions fixed by this mission:

  • Continuity is Mathlib's Continuous, ContinuousOn, ContinuousWithinAt; Rudin's lim⁡x→pf(x)=q\lim_{x\to p} f(x) = qlimx→p​f(x)=q along EEE is Filter.Tendsto f (𝓝[E \ {p}] p) (𝓝 q).
  • Uniform continuity is Rudin.UniformlyContinuous, stated with explicit ε\varepsilonε and δ\deltaδ as in Definition 4.18, rather than through the uniformity filter.
  • Limit points are Rudin.IsLimitPoint from the Chapter 2 mission, so the two missions share one notion.
  • Compactness of the domain in 4.16, 4.17 and 4.19 is the typeclass [CompactSpace X], matching Rudin's phrase "compact metric space"; 4.14 is stated for a compact subset instead, which is the form later missions use.
  • Monotone functions are MonotoneOn f (Set.Ioo a b); one-sided limits are 𝓝[<] x and 𝓝[>] x filters, and 4.29 also identifies them with the supremum and infimum of the corresponding one-sided images, as Rudin does.

The goal is not vacuous and does not follow by unfolding: uniform continuity fails for continuous functions on non-compact domains (e.g. x↦x2x \mapsto x^2x↦x2 on R\mathbb{R}R, or x↦1/xx \mapsto 1/xx↦1/x on (0,1)(0,1)(0,1)), so compactness is doing the work.

Selected references

  • Walter Rudin, Principles of Mathematical Analysis, 3rd edition, McGraw-Hill, 1976, Chapter 4 (pp. 83–101).
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