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Mathematical Physics

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Captain: Lucas

Carneiro 2006: From de Sitter to de Sitter — a non-singular universe driven by vacuumResearch Paper

Motivation

The cosmological constant problem is the mismatch between the vacuum energy density predicted by quantum field theory in flat space–time and the small value of the cosmological term inferred from observations (Weinberg 1989). One line of work replaces the constant by a decaying vacuum: a time-dependent cosmological term Λ(t)\Lambda(t)Λ(t) that falls as the universe expands, while the energy it loses is transferred to matter so that total energy is conserved.

S. Carneiro's essay From de Sitter to de Sitter: a non-singular inflationary universe driven by vacuum (Int. J. Mod. Phys. D 15 (2006) 2241–2247, honorable mention in the 2006 Gravity Research Foundation essay competition) derives such a law from a semi-classical argument, Λ≈(m+H)4−m4\Lambda\approx(m+H)^4-m^4Λ≈(m+H)4−m4, and studies the cosmologies it produces. In the early-time regime Λ≈H4\Lambda\approx H^4Λ≈H4 it finds a universe with no initial singularity: an eternal quasi-de Sitter phase at the Planck scale, followed by a fast transition to a radiation era. In the late-time regime Λ≈m3H\Lambda\approx m^3HΛ≈m3H it finds a dust era that tends again to a de Sitter universe. The calculations in the paper are explicit closed-form computations, which makes them a good target for a complete machine-checked development.

Setting

All quantities are in Planck units, and space is flat. The expansion is described by the Hubble parameter H(t)=a˙(t)/a(t)H(t)=\dot a(t)/a(t)H(t)=a˙(t)/a(t) of a scale factor a(t)a(t)a(t). The cosmic fluid has total energy density ρT=ρm+Λ\rho_T=\rho_m+\LambdaρT​=ρm​+Λ and total pressure pT=pm−Λp_T=p_m-\LambdapT​=pm​−Λ, where ρm,pm\rho_m,p_mρm​,pm​ are the matter density and pressure and Λ\LambdaΛ is the vacuum term. The Friedmann equation is ρT=3H2\rho_T=3H^2ρT​=3H2 and the conservation equation is

ρ˙T+3H(ρT+pT)=0.\dot\rho_T+3H(\rho_T+p_T)=0 .ρ˙​T​+3H(ρT​+pT​)=0.

Radiation has pm=ρm/3p_m=\rho_m/3pm​=ρm​/3 and dust has pm=0p_m=0pm​=0. The relative energy densities are Ωm=ρm/ρT\Omega_m=\rho_m/\rho_TΩm​=ρm​/ρT​ and ΩΛ=Λ/ρT\Omega_\Lambda=\Lambda/\rho_TΩΛ​=Λ/ρT​, and the deceleration parameter is q=−1−H˙/H2q=-1-\dot H/H^2q=−1−H˙/H2.

The vacuum term comes from a massless scalar field ϕ\phiϕ obeying ϕ¨+3Hϕ˙−∇2ϕ=0\ddot\phi+3H\dot\phi-\nabla^2\phi=0ϕ¨​+3Hϕ˙​−∇2ϕ=0. For slowly varying HHH this has the damped radial plane-wave solution ϕ=ϕ0e−bre−i(ωt−kr)\phi=\phi_0e^{-br}e^{-i(\omega t-kr)}ϕ=ϕ0​e−bre−i(ωt−kr), with k(ω,H)k(\omega,H)k(ω,H) and b(ω,H)b(\omega,H)b(ω,H) given by explicit square-root formulas (Eqs. (7)–(8)), and energy density (ω2+b2)∣ϕ∣2(\omega^2+b^2)|\phi|^2(ω2+b2)∣ϕ∣2. Shifting the cutoff mmm of the thermally regularized vacuum integral ∫0∞ω3 dω/(eω/m−1)\int_0^\infty\omega^3\,d\omega/(e^{\omega/m}-1)∫0∞​ω3dω/(eω/m−1) by b≈Hb\approx Hb≈H and subtracting the flat-space value gives the vacuum term Λ(m,H)=(m+H)4−m4\Lambda(m,H)=(m+H)^4-m^4Λ(m,H)=(m+H)4−m4. In the mission's Lean development these objects are waveNumber, dampingRate, planeWave, vacuumTerm, dustScaleFactor and decelerationParameter, all in the namespace CarneiroDeSitter.

Formalization targets

Goal: the non-singular early universe

With radiation and Λ=3H4\Lambda=3H^4Λ=3H4, the evolution equation is H˙+2H2−2H4=0\dot H+2H^2-2H^4=0H˙+2H2−2H4=0 (Eq. (12)). The goal asserts that it has a solution defined for all times, given implicitly by Eq. (13):

∃ H:R→(0,1),2t=1H(t)−artanh⁡H(t),H˙=−2H2+2H4,H→t→−∞1,H→t→+∞0.\exists\,H:\mathbb R\to(0,1),\quad 2t=\frac1{H(t)}-\operatorname{artanh}H(t),\quad \dot H=-2H^2+2H^4,\quad H\xrightarrow[t\to-\infty]{}1,\quad H\xrightarrow[t\to+\infty]{}0 .∃H:R→(0,1),2t=H(t)1​−artanhH(t),H˙=−2H2+2H4,Ht→−∞​1,Ht→+∞​0.

Milestones (in the order of the paper)

  1. Eq. (2): ∫0∞ω3 dωeω/m−1=π415m4\int_0^\infty\frac{\omega^3\,d\omega}{e^{\omega/m}-1}=\frac{\pi^4}{15}m^4∫0∞​eω/m−1ω3dω​=15π4​m4.
  2. Eqs. (5)–(8): the damped plane wave solves ϕ¨+3Hϕ˙−∂r2ϕ=0\ddot\phi+3H\dot\phi-\partial_r^2\phi=0ϕ¨​+3Hϕ˙​−∂r2​ϕ=0 for constant HHH.
  3. Eqs. (9)–(10): its energy density is (ω2+b2)∣ϕ∣2(\omega^2+b^2)|\phi|^2(ω2+b2)∣ϕ∣2.
  4. Eq. (11): (m+H)4−m4∼H4(m+H)^4-m^4\sim H^4(m+H)4−m4∼H4 as H→∞H\to\inftyH→∞ and ∼4m3H\sim4m^3H∼4m3H as H→0+H\to0^+H→0+.
  5. Eq. (12): the conservation equation with ρT=3H2\rho_T=3H^2ρT​=3H2, Λ=3H4\Lambda=3H^4Λ=3H4, pm=ρm/3p_m=\rho_m/3pm​=ρm​/3 gives H˙+2H2−2H4=0\dot H+2H^2-2H^4=0H˙+2H2−2H4=0.
  6. Eq. (13): every solution on R\mathbb RR with 0<H<10<H<10<H<1 satisfies 2(t−t0)=1/H−artanh⁡H2(t-t_0)=1/H-\operatorname{artanh}H2(t−t0​)=1/H−artanhH.
  7. p. 2245: Ωm=1−H2\Omega_m=1-H^2Ωm​=1−H2, ΩΛ=H2\Omega_\Lambda=H^2ΩΛ​=H2, q=1−2H2q=1-2H^2q=1−2H2.
  8. Eq. (14): a=C(eσt/2−1)2/3a=C(e^{\sigma t/2}-1)^{2/3}a=C(eσt/2−1)2/3 solves the dust era with Λ=σH\Lambda=\sigma HΛ=σH.
  9. Limits of (14): a∼C(σ/2)2/3t2/3a\sim C(\sigma/2)^{2/3}t^{2/3}a∼C(σ/2)2/3t2/3 as t→0+t\to0^+t→0+ and H→σ/3H\to\sigma/3H→σ/3 as t→∞t\to\inftyt→∞.
  10. Eq. (15): ∫0∞ω2 dωeω/(m+H)−1=2ζ(3)(m+H)3\int_0^\infty\frac{\omega^2\,d\omega}{e^{\omega/(m+H)}-1}=2\zeta(3)(m+H)^3∫0∞​eω/(m+H)−1ω2dω​=2ζ(3)(m+H)3.

Significance

The goal is the paper's central claim: under the stated vacuum law the universe has existed for an infinite past, in a quasi-de Sitter phase with H≈1H\approx1H≈1, and leaves it through a transition in which HHH and Λ\LambdaΛ fall towards zero, producing radiation. The milestones cover the steps the paper uses to reach it (the vacuum law, the evolution equation and its integration) and the late-time picture (the dust solution and its de Sitter limit, which the paper links to the Eddington–Dirac large-number relation H≈m3H\approx m^3H≈m3).

The results are proved by hand calculation in the paper. The same evolution equation and implicit solution reappear in Carneiro's later paper Cosmological Concordance Model with Particle Creation (2012), whose statements are also on the platform (namespace CarneiroParticleCreation); this mission formalizes the 2006 paper, its vacuum law and its late-time dust solution. Formalizing them produces a verified account of which statements are exact identities and which are approximations. Where the paper writes "≈\approx≈", the milestones state the exact identity or asymptotic equivalence behind it.

Difficulty

The algebraic milestones (5, 7) are routine. The goal concerns a function known only implicitly: the solution is the inverse of H↦12(1/H−artanh⁡H)H\mapsto\frac12\big(1/H-\operatorname{artanh}H\big)H↦21​(1/H−artanhH) on (0,1)(0,1)(0,1), and its existence on the whole line, its differentiability and its end behaviour all have to be established for an inverse function, not read off a formula. Milestone 6 is a uniqueness statement on all of R\mathbb RR, so it cannot be checked by substitution. Milestones 1 and 10 are improper integrals whose values involve ζ(4)=π4/90\zeta(4)=\pi^4/90ζ(4)=π4/90 and ζ(3)\zeta(3)ζ(3), and they need integrability arguments near 000 and ∞\infty∞. Milestones 2, 3, 8 and 9 involve derivatives of complex exponentials, square roots and real powers, where Lean's conventions for ⋅\sqrt{\cdot}⋅​ and x2/3x^{2/3}x2/3 at non-positive arguments must be handled.

Formalization scope

  • Real numbers throughout; the scalar field is complex-valued, and derivatives are one-variable derivatives in ttt or rrr.
  • In milestones 2–3 the Hubble parameter is a constant and the Laplacian of the radial plane wave is ∂r2\partial_r^2∂r2​, which is the paper's approximation.
  • artanh⁡\operatorname{artanh}artanh is Mathlib's Real.artanh, the real power x2/3x^{2/3}x2/3 is Real.rpow, ∼\sim∼ is Asymptotics.IsEquivalent, and ζ(3)\zeta(3)ζ(3) is written as ∑n≥01/(n+1)3\sum_{n\ge0}1/(n+1)^3∑n≥0​1/(n+1)3.
  • Every statement that divides by ω\omegaω or HHH assumes ω>0\omega>0ω>0 or H(t)≠0H(t)\neq0H(t)=0. The goal requires the solution on the whole real line and states both limits, so a solution on a half-line or a constant function does not satisfy it.
  • Approximate steps of the paper that are not exact statements (the identification b≈Hb\approx Hb≈H, the radiation law a∝t1/2a\propto t^{1/2}a∝t1/2 quoted from earlier work, and the holographic entropy estimates) are not formalized.

Contributions are welcome on all milestones. The inverse-function and Bose-integral arguments can be reused outside this mission.

Selected references

  • S. Carneiro, From de Sitter to de Sitter: a non-singular inflationary universe driven by vacuum, Int. J. Mod. Phys. D 15 (2006) 2241–2247. https://doi.org/10.1142/S0218271806009510
  • S. Weinberg, The cosmological constant problem, Rev. Mod. Phys. 61 (1989) 1–23. https://doi.org/10.1103/RevModPhys.61.1
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Condensed Matter PhysicsLinear algebraQuantum Information+2·Captain: Alien60

Seiberg–Seifnashri–Shao 2024: Non-invertible Kramers–Wannier symmetry on the Ising chainResearch Paper

Motivation

Kramers–Wannier duality was found in 1941 as a map between the high- and low-temperature phases of the two-dimensional Ising model (Kramers–Wannier 1941). In its quantum form it exchanges the transverse field XjX_jXj​ and the nearest-neighbour coupling Zj−1ZjZ_{j-1}Z_jZj−1​Zj​ of the transverse-field Ising chain, and it fixes the critical point. In conformal field theory it is implemented by a topological defect line (Fröhlich–Fuchs–Runkel–Schweigert 2004), the prototypical non-invertible symmetry: its fusion with itself is a sum of operators, not a single invertible one (Shao, TASI lectures 2023).

On a finite periodic chain the duality cannot be a unitary operator, because it maps the Z2\mathbb Z_2Z2​-even sector to itself and annihilates the odd sector. Seiberg–Shao 2023 and Seiberg–Seifnashri–Shao 2024 wrote the exact lattice operator D\mathsf DD on the tensor-product Hilbert space (C2)⊗L(\mathbb C^2)^{\otimes L}(C2)⊗L. They showed that its algebra closes only after the lattice translation is included: D2=(1+η)T−1\mathsf D^2=(1+\eta)T^{-1}D2=(1+η)T−1. This is a lattice relation that a fusion category does not describe, since the continuum fusion rule N2=1+η\mathcal N^2=1+\etaN2=1+η appears only at low energy. The same identity drives the LSM-type constraint proved in that paper.

Timeline. 1941: Kramers and Wannier find the duality of the 2D Ising model. 2004: Fröhlich, Fuchs, Runkel and Schweigert realise it as a conformal defect. 2016: Aasen–Mong–Fendley construct the lattice defects. 2023–2024: Seiberg, Seifnashri and Shao find the exact operator algebra on the tensor-product Hilbert space, including the translation factor.

Setting

Fix L≥1L\ge1L≥1 qubits on a ring, with site indices in Z/L\mathbb Z/LZ/L (Fin L with modular arithmetic). A computational-basis state is labelled by a configuration s=(s0,…,sL−1)∈(Z/2)Ls=(s_0,\dots,s_{L-1})\in(\mathbb Z/2)^Ls=(s0​,…,sL−1​)∈(Z/2)L (Config L). Operators are complex 2L×2L2^L\times2^L2L×2L matrices indexed by configurations (Op L). Write sgn⁡(a)=(−1)a\operatorname{sgn}(a)=(-1)^asgn(a)=(−1)a.

  • Pauli operators. Xj∣s⟩=∣s+ej⟩X_j|s\rangle=|s+e_j\rangleXj​∣s⟩=∣s+ej​⟩ flips spin jjj (pauliX), and Zj∣s⟩=(−1)sj∣s⟩Z_j|s\rangle=(-1)^{s_j}|s\rangleZj​∣s⟩=(−1)sj​∣s⟩ (pauliZ).
  • Z2\mathbb Z_2Z2​ symmetry. η=∏jXj\eta=\prod_j X_jη=∏j​Xj​ flips every spin (eta).
  • Translation. T∣s⟩=∣s′⟩T|s\rangle=|s'\rangleT∣s⟩=∣s′⟩ with sk′=sk−1s'_k=s_{k-1}sk′​=sk−1​ (transl), so that TXjT−1=Xj+1TX_jT^{-1}=X_{j+1}TXj​T−1=Xj+1​.
  • Kramers–Wannier operator (kwD):
⟨t∣ D ∣s⟩  =  2−L/2 (−1)∑ktk (sk+sk+1).\langle t|\,\mathsf D\,|s\rangle \;=\; 2^{-L/2}\,(-1)^{\sum_{k} t_k\,(s_k+s_{k+1})}.⟨t∣D∣s⟩=2−L/2(−1)∑k​tk​(sk​+sk+1​).

This explicit formula is the definition used throughout. Relations (1.5) together with Dη=D\mathsf D\eta=\mathsf DDη=D determine D\mathsf DD up to a scalar, and (1.4) fixes the scalar up to a sign. Every statement below is invariant under D↦−D\mathsf D\mapsto-\mathsf DD↦−D, so this is the operator of Seiberg–Seifnashri–Shao in that paper's normalisation (footnote 1). Its equality with their matrix-product presentation (2.64) is not formalised here.

Formalization targets

Goal: the non-invertible fusion rule (eqs. (1.4), (2.65), (F.18))

D2=(1+η) T−1for every L≥1.\mathsf D^2=(1+\eta)\,T^{-1}\qquad\text{for every }L\ge1 .D2=(1+η)T−1for every L≥1.

Milestones

  1. Invertible algebra (eqs. (1.1)–(1.3), (2.10), (2.65)): η2=1\eta^2=1η2=1, Tη=ηTT\eta=\eta TTη=ηT, TL=1T^L=1TL=1, TXjT−1=Xj+1TX_jT^{-1}=X_{j+1}TXj​T−1=Xj+1​, TZjT−1=Zj+1TZ_jT^{-1}=Z_{j+1}TZj​T−1=Zj+1​, ηXj=Xjη\eta X_j=X_j\etaηXj​=Xj​η, ηZj=−Zjη\eta Z_j=-Z_j\etaηZj​=−Zj​η.
  2. Duality on XXX (eq. (1.5)): DXj=Zj−1Zj D\mathsf D X_j=Z_{j-1}Z_j\,\mathsf DDXj​=Zj−1​Zj​D.
  3. Duality on ZZZZZZ (eq. (1.5)): DZj−1Zj=Xj−1 D\mathsf D Z_{j-1}Z_j=X_{j-1}\,\mathsf DDZj−1​Zj​=Xj−1​D.
  4. Absorbing η\etaη (eqs. (1.4), (2.65)): Dη=ηD=D\mathsf D\eta=\eta\mathsf D=\mathsf DDη=ηD=D.
  5. Translation and adjoint (eq. (2.65), Table 1): TD=DTT\mathsf D=\mathsf DTTD=DT and D†=DT\mathsf D^\dagger=\mathsf DTD†=DT.
  6. Non-invertibility (§1.1): D\mathsf DD is not a unit, and ker⁡D≠0\ker\mathsf D\neq0kerD=0.

Significance

The result. The goal identity is the defining relation of the lattice Kramers–Wannier symmetry. Together with milestones 4–5 it shows that D/2\mathsf D/\sqrt2D/2​ restricted to the η\etaη-even sector squares to a translation, so D\mathsf DD is a square root of T−1T^{-1}T−1 there. The paper uses this to derive its LSM-type constraint, and also to show that the lattice symmetry is not a fusion category, because the continuum rule N2=1+η\mathcal N^2=1+\etaN2=1+η only emerges at low energy. Milestones 2–3 are the lattice Kramers–Wannier map on Z2\mathbb Z_2Z2​-invariant operators, so D\mathsf DD commutes with the critical Ising Hamiltonian H=−∑j(Zj−1Zj+Xj)H=-\sum_j(Z_{j-1}Z_j+X_j)H=−∑j​(Zj−1​Zj​+Xj​).

Formalizing it. The identities are proved in the physics literature by tensor-network manipulations ((F.14)–(F.18)) and checked numerically, but none of this is machine-checked. This mission produces a reusable Lean setup for qubit chains: Pauli strings on (Z/2)L(\mathbb Z/2)^L(Z/2)L, Z2\mathbb Z_2Z2​ and translation symmetries, and an exact non-invertible operator with its full operator algebra for every chain length. No mission on the platform or file in Mathlib currently formalizes a non-invertible lattice symmetry.

Difficulty

Each identity is easy to check for a fixed small LLL by brute force. The content is that it holds for all LLL at once, on a 2L2^L2L-dimensional space. The difficulty is bookkeeping with periodic indices: sums over (Z/2)L(\mathbb Z/2)^L(Z/2)L of characters (−1)⟨t, ⋅⟩(-1)^{\langle t,\,\cdot\rangle}(−1)⟨t,⋅⟩, reindexing k↦k±1k\mapsto k\pm1k↦k±1 in Fin L (including L=1L=1L=1, where k+1=kk+1=kk+1=k, and L=2L=2L=2, where k+1=k−1k+1=k-1k+1=k−1), and the exact normalisation 2−L/22^{-L/2}2−L/2, so that the right-hand side carries no stray factor 2L2^L2L. The goal also involves the matrix inverse T−1T^{-1}T−1, so a proof must establish that TTT is invertible rather than rely on Lean's junk value.

Formalization scope

  • Representation. Operators are Matrix (Fin L → ZMod 2) (Fin L → ZMod 2) ℂ; products are matrix products; T−1T^{-1}T−1 is Mathlib's matrix inverse (transl L)⁻¹; †\dagger† is conjTranspose. Every theorem assumes [NeZero L], i.e. L≥1L\ge1L≥1.
  • Conventions committed to. Zj=(−1)sjZ_j=(-1)^{s_j}Zj​=(−1)sj​ on basis states, translation to the right (sk′=sk−1s'_k=s_{k-1}sk′​=sk−1​), and D\mathsf DD normalised by 2−L/22^{-L/2}2−L/2 as in eqs. (1.4)/(2.65). Other conventions (left translation, unnormalised D\mathsf DD) change the statements to TTT instead of T−1T^{-1}T−1 or add a factor 2L2^L2L; the conventions here reproduce the paper's equations verbatim.
  • No trivialisation. kwD is an explicit formula, not a hypothesis. The goal fixes both sides completely, and milestone 1 pins the translation convention against eq. (2.10).
  • Out of scope. The defect Hamiltonians, the MPO presentation (2.64) itself, the Z2\mathbb Z_2Z2​- and duality-twisted operators of §§2.3.3–2.3.4, and the LSM constraint of §4.
  • Reusable. Pauli operators, translation and η\etaη on qubit chains; character-sum lemmas over (Z/2)L(\mathbb Z/2)^L(Z/2)L. Contributions of general Mathlib lemmas on Walsh–Hadamard-type sums are welcome.

Selected references

  • H. A. Kramers, G. H. Wannier, Statistics of the Two-Dimensional Ferromagnet. Part I, Phys. Rev. 60, 252–262 (1941). doi:10.1103/PhysRev.60.252
  • J. Fröhlich, J. Fuchs, I. Runkel, C. Schweigert, Kramers–Wannier duality from conformal defects, Phys. Rev. Lett. 93, 070601 (2004). arXiv:cond-mat/0404051
  • D. Aasen, R. S. K. Mong, P. Fendley, Topological Defects on the Lattice I: The Ising model, J. Phys. A 49, 354001 (2016). arXiv:1601.07185
  • N. Seiberg, S.-H. Shao, Majorana chain and Ising model – (non-invertible) translations, anomalies, and emanant symmetries, SciPost Phys. 16, 064 (2024). arXiv:2307.02534
  • S.-H. Shao, What's Done Cannot Be Undone: TASI Lectures on Non-Invertible Symmetries (2023). arXiv:2308.00747
  • Source: N. Seiberg, S. Seifnashri, S.-H. Shao, Non-invertible symmetries and LSM-type constraints on a tensor product Hilbert space, SciPost Phys. 16, 154 (2024). arXiv:2401.12281
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Captain: Lucas

Onsager Reciprocal Relations: Symmetry of Kinetic CoefficientsTextbook

Motivation

Near thermodynamic equilibrium, flows of extensive quantities (heat, matter, charge) depend linearly on the thermodynamic forces (gradients of the conjugate intensive variables). Some of the coefficients in these linear laws describe cross effects: a temperature gradient driving an electric current (Seebeck effect), a voltage driving a heat flow (Peltier effect), a temperature gradient driving diffusion (Soret effect) and its converse (Dufour effect). In 1931 Lars Onsager showed that, as a consequence of the time-reversibility of microscopic dynamics, the matrix of these coefficients is symmetric (Onsager 1931). These reciprocal relations were confirmed experimentally across many classes of irreversible processes (Miller 1960), and Onsager received the 1968 Nobel Prize in Chemistry for them.

This mission formalizes the abstract, finite-dimensional version of Onsager's principle as presented by Landau and Lifshitz (Statistical Physics, Part 1, 1975) and reproduced in the Wikipedia article Onsager reciprocal relations, sections "Abstract formulation" and "Proof".

Setting

Let x=(x1,…,xn)∈Rnx=(x_1,\dots,x_n)\in\mathbb R^nx=(x1​,…,xn​)∈Rn be the fluctuations of nnn thermodynamic quantities from their equilibrium values. For small fluctuations the entropy is quadratic, and Boltzmann's formula gives the Gaussian fluctuation distribution

w(x)=A~ e−12βikxixk,w(x)=\tilde A\,e^{-\frac12\beta_{ik}x_ix_k},w(x)=A~e−21​βik​xi​xk​,

where β\betaβ is a positive definite symmetric real n×nn\times nn×n matrix and summation over repeated indices is understood. Write ⟨f⟩\langle f\rangle⟨f⟩ for the average of f(x)f(x)f(x) with respect to www.

The thermodynamic conjugate quantities are Xi=βikxkX_i=\beta_{ik}x_kXi​=βik​xk​. In the quasi-stationary regime the fluctuations relax according to x˙i=−λikxk\dot x_i=-\lambda_{ik}x_kx˙i​=−λik​xk​ for a real matrix λ\lambdaλ, so that x˙i=−γikXk\dot x_i=-\gamma_{ik}X_kx˙i​=−γik​Xk​ with the kinetic coefficients

γik=λil (β−1)lk.\gamma_{ik}=\lambda_{il}\,(\beta^{-1})_{lk}.γik​=λil​(β−1)lk​.

The mean value at time ttt of a fluctuation which takes the value xxx at t=0t=0t=0 is ξ(t)=e−tλx\xi(t)=e^{-t\lambda}xξ(t)=e−tλx, and Ξ(t)=βξ(t)\Xi(t)=\beta\xi(t)Ξ(t)=βξ(t). The time correlation is ⟨xi(t)xk(0)⟩=⟨ξi(t)xk⟩\langle x_i(t)x_k(0)\rangle=\langle\xi_i(t)x_k\rangle⟨xi​(t)xk​(0)⟩=⟨ξi​(t)xk​⟩.

Formalization targets

Goal: Onsager's principle

If fluctuations are symmetric under time reversal,

⟨ξi(t) xk⟩=⟨xi ξk(t)⟩(t≥0, 1≤i,k≤n),\langle \xi_i(t)\,x_k\rangle=\langle x_i\,\xi_k(t)\rangle\qquad(t\ge0,\ 1\le i,k\le n),⟨ξi​(t)xk​⟩=⟨xi​ξk​(t)⟩(t≥0, 1≤i,k≤n),

then the kinetic coefficients are symmetric:

γik=γki.\gamma_{ik}=\gamma_{ki}.γik​=γki​.

Milestones (in the order of the source's argument)

  1. x˙i=−λikxk=−γikXk\dot x_i=-\lambda_{ik}x_k=-\gamma_{ik}X_kx˙i​=−λik​xk​=−γik​Xk​ (definition of kinetic coefficients).
  2. ξ(0)=x\xi(0)=xξ(0)=x and ξ˙i(t)=−γikΞk(t)\dot\xi_i(t)=-\gamma_{ik}\Xi_k(t)ξ˙​i​(t)=−γik​Ξk​(t).
  3. ddt⟨ξi(t)xk⟩=−γil⟨Ξl(t)xk⟩\frac{d}{dt}\langle\xi_i(t)x_k\rangle=-\gamma_{il}\langle\Xi_l(t)x_k\rangledtd​⟨ξi​(t)xk​⟩=−γil​⟨Ξl​(t)xk​⟩.
  4. ⟨Xixk⟩=δik\langle X_ix_k\rangle=\delta_{ik}⟨Xi​xk​⟩=δik​.
  5. Under time-reversal symmetry, γil⟨Xlxk⟩=γkl⟨Xlxi⟩\gamma_{il}\langle X_lx_k\rangle=\gamma_{kl}\langle X_lx_i\rangleγil​⟨Xl​xk​⟩=γkl​⟨Xl​xi​⟩.

Significance

The symmetry γik=γki\gamma_{ik}=\gamma_{ki}γik​=γki​ is the mathematical content of the reciprocal relations: it reduces the number of independent transport coefficients from n2n^2n2 to n(n+1)/2n(n+1)/2n(n+1)/2 and yields the equality of measurable cross-coefficients such as the Peltier and Seebeck coefficients. Together with the positive semi-definiteness of the coefficient matrix (from non-negative entropy production), it is the basic structural input of linear irreversible thermodynamics.

The result is classical and its proof is standard in physics textbooks; this mission produces a machine-checked version of the finite-dimensional argument, including the Gaussian moment identity ⟨Xixk⟩=δik\langle X_ix_k\rangle=\delta_{ik}⟨Xi​xk​⟩=δik​ and the differentiation of the time-correlation function under the integral sign. No machine-checked formalization of this statement is known to the proposer.

Difficulty

The algebraic core is short, but the formal argument needs analytic input that the textbook treats as routine: Gaussian integrals over Rn\mathbb R^nRn for a general positive definite β\betaβ (integrability of polynomial moments against e−12xTβxe^{-\frac12x^{\mathsf T}\beta x}e−21​xTβx and the value of the second moments), differentiation of a parameter-dependent integral involving a matrix exponential, and the passage from an identity valid for t≥0t\ge0t≥0 to an identity between derivatives at the boundary point t=0t=0t=0, where only a one-sided derivative is available from the hypothesis.

Formalization scope

Vectors are functions Fin n → ℝ with Lebesgue measure; matrices are Matrix (Fin n) (Fin n) ℝ, and β.PosDef (which includes symmetry) is assumed in every theorem. The average ⟨f⟩\langle f\rangle⟨f⟩ is the ratio ∫f w dx/∫w dx\int f\,w\,dx/\int w\,dx∫fwdx/∫wdx of Bochner integrals, so the normalizing constant A~\tilde AA~ cancels. The mean relaxation is the matrix exponential ξ(t)=e−tλx\xi(t)=e^{-t\lambda}xξ(t)=e−tλx. The time-reversal hypothesis is assumed only for t≥0t\ge0t≥0. The entropy SSS and Boltzmann's constant are not modelled; β\betaβ is the primitive datum, as in the source's statement of the principle. The hypothesis is non-vacuous (e.g. λ=β\lambda=\betaλ=β satisfies it), and the conclusion concerns γ=λβ−1\gamma=\lambda\beta^{-1}γ=λβ−1, not λ\lambdaλ.

All definitions are collected in Definitions.Def_OnsagerReciprocal_basic (namespace OnsagerReciprocal). Reusable Gaussian-moment lemmas for positive definite quadratic forms are welcome contributions.

Selected references

  • L. Onsager, Reciprocal Relations in Irreversible Processes. I, Physical Review 37 (1931) 405–426. doi:10.1103/physrev.37.405
  • D. G. Miller, Thermodynamics of Irreversible Processes. The Experimental Verification of the Onsager Reciprocal Relations, Chemical Reviews 60 (1960) 15–37. doi:10.1021/cr60203a003
  • L. D. Landau, E. M. Lifshitz, Statistical Physics, Part 1, Butterworth-Heinemann (1975).
  • Wikipedia, Onsager reciprocal relations, oldid 1355014688.
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Differential Geometry·Captain: Lucas

Einstein–Grossmann 1913 (Entwurf): energy-momentum conservation for matter and gravitational fieldResearch Paper

Motivation

In 1913 Albert Einstein and the mathematician Marcel Grossmann published the Entwurf ("outline") of a generalized theory of relativity and a theory of gravitation. It is the first theory in which the gravitational field is described by the ten components gμνg_{\mu\nu}gμν​ of a space-time metric, ds2=∑μνgμν dxμdxνds^2=\sum_{\mu\nu}g_{\mu\nu}\,dx_\mu dx_\nuds2=∑μν​gμν​dxμ​dxν​, and in which Ricci and Levi-Civita's absolute differential calculus (Grossmann's mathematical part) is brought into physics. Its gravitational field equations were superseded by the generally covariant field equations of November 1915, but the framework of the Entwurf — metric as gravitational potential, the energy-momentum law of matter in a gravitational field, a stress-energy expression for the gravitational field itself — carried over to general relativity.

The physical part (Part I, by Einstein) derives the field equations from one requirement: the energy-momentum law must hold for matter and gravitational field together. The derivation runs through an explicit differential identity, eq. (12), whose rewritten form (12a) yields the field equations (18) and the total conservation law (19). This mission formalizes that chain of statements.

Timeline.

  • 1912: Einstein's theory of the static gravitational field, with a single scalar potential c(x)c(x)c(x) (Ann. d. Physik 38).
  • 1913: Einstein–Grossmann, Entwurf: metric tensor gμνg_{\mu\nu}gμν​, energy-momentum law (10), field equations (18), conservation law (19).
  • 1915: Einstein, Die Feldgleichungen der Gravitation (Sitzungsber. Preuss. Akad. Wiss.): generally covariant field equations replace (18).

Setting

All objects live in one coordinate chart, x=(x1,x2,x3,x4)∈R4x=(x_1,x_2,x_3,x_4)\in\mathbb R^4x=(x1​,x2​,x3​,x4​)∈R4, with x4x_4x4​ the time coordinate. The fundamental tensor gμν(x)g_{\mu\nu}(x)gμν​(x) is a symmetric 4×44\times44×4 matrix field with negative determinant g=det⁡(gμν)g=\det(g_{\mu\nu})g=det(gμν​); γμν\gamma_{\mu\nu}γμν​ is the reciprocal (contravariant) tensor, the inverse matrix, and −g\sqrt{-g}−g​ is the density factor. All sums run over 1,…,41,\dots,41,…,4.

A material process is described by its contravariant stress-energy tensor Θμν\Theta_{\mu\nu}Θμν​ (for incoherent dust, Θμν=ϱ0dxμdsdxνds\Theta_{\mu\nu}=\varrho_0\frac{dx_\mu}{ds}\frac{dx_\nu}{ds}Θμν​=ϱ0​dsdxμ​​dsdxν​​). Its energy-momentum law in the gravitational field is eq. (10):

∑μν∂∂xν(−g gσμΘμν)−12∑μν−g ∂gμν∂xσΘμν=0(σ=1,2,3,4).\sum_{\mu\nu}\frac{\partial}{\partial x_\nu}\big(\sqrt{-g}\,g_{\sigma\mu}\Theta_{\mu\nu}\big)-\tfrac12\sum_{\mu\nu}\sqrt{-g}\,\frac{\partial g_{\mu\nu}}{\partial x_\sigma}\Theta_{\mu\nu}=0\qquad(\sigma=1,2,3,4).μν∑​∂xν​∂​(−g​gσμ​Θμν​)−21​μν∑​−g​∂xσ​∂gμν​​Θμν​=0(σ=1,2,3,4).

The second sum is the momentum (for σ=4\sigma=4σ=4, the energy) transferred per unit volume from the gravitational field to matter.

The gravitational field carries its own stress-energy tensor ϑμν\vartheta_{\mu\nu}ϑμν​, eq. (13):

−2κ ϑμν=∑αβτρ(γαμγβν∂gτρ∂xα∂γτρ∂xβ−12γμνγαβ∂gτρ∂xα∂γτρ∂xβ),-2\kappa\,\vartheta_{\mu\nu}=\sum_{\alpha\beta\tau\rho}\Big(\gamma_{\alpha\mu}\gamma_{\beta\nu}\frac{\partial g_{\tau\rho}}{\partial x_\alpha}\frac{\partial\gamma_{\tau\rho}}{\partial x_\beta}-\tfrac12\gamma_{\mu\nu}\gamma_{\alpha\beta}\frac{\partial g_{\tau\rho}}{\partial x_\alpha}\frac{\partial\gamma_{\tau\rho}}{\partial x_\beta}\Big),−2κϑμν​=αβτρ∑​(γαμ​γβν​∂xα​∂gτρ​​∂xβ​∂γτρ​​−21​γμν​γαβ​∂xα​∂gτρ​​∂xβ​∂γτρ​​),

and the field equations involve the second-order operator of eq. (15),

Δμν(γ)=∑αβ1−g∂∂xα(γαβ−g ∂γμν∂xβ)−∑αβτργαβgτρ∂γμτ∂xα∂γνρ∂xβ.\Delta_{\mu\nu}(\gamma)=\sum_{\alpha\beta}\frac{1}{\sqrt{-g}}\frac{\partial}{\partial x_\alpha}\Big(\gamma_{\alpha\beta}\sqrt{-g}\,\frac{\partial\gamma_{\mu\nu}}{\partial x_\beta}\Big)-\sum_{\alpha\beta\tau\rho}\gamma_{\alpha\beta}g_{\tau\rho}\frac{\partial\gamma_{\mu\tau}}{\partial x_\alpha}\frac{\partial\gamma_{\nu\rho}}{\partial x_\beta}.Δμν​(γ)=αβ∑​−g​1​∂xα​∂​(γαβ​−g​∂xβ​∂γμν​​)−αβτρ∑​γαβ​gτρ​∂xα​∂γμτ​​∂xβ​∂γνρ​​.

The Entwurf field equations (18) read Δμν(γ)=κ(Θμν+ϑμν)\Delta_{\mu\nu}(\gamma)=\kappa(\Theta_{\mu\nu}+\vartheta_{\mu\nu})Δμν​(γ)=κ(Θμν​+ϑμν​), with κ\kappaκ a constant. Lowering indices with ggg gives the covariant objects Tμν=∑gμαgνβΘαβT_{\mu\nu}=\sum g_{\mu\alpha}g_{\nu\beta}\Theta_{\alpha\beta}Tμν​=∑gμα​gνβ​Θαβ​, tμνt_{\mu\nu}tμν​ (eq. (14)) and the operator Dμν(g)D_{\mu\nu}(g)Dμν​(g) (eq. (16)).

Formalization targets

Goal: eq. (19)

If the energy-momentum law (10) and the field equations (18) hold, then for σ=1,2,3,4\sigma=1,2,3,4σ=1,2,3,4

∑μν∂∂xν{−g gσμ(Θμν+ϑμν)}=0.\sum_{\mu\nu}\frac{\partial}{\partial x_\nu}\Big\{\sqrt{-g}\,g_{\sigma\mu}(\Theta_{\mu\nu}+\vartheta_{\mu\nu})\Big\}=0.μν∑​∂xν​∂​{−g​gσμ​(Θμν​+ϑμν​)}=0.

Milestones

  1. The electrostatic model identity of p. 14, which illustrates the method.
  2. Identity (12a): ∑μν∂∂xν{−g gσμκϑμν}=12∑μν−g ∂gμν∂xσ{−Δμν(γ)+κϑμν}\sum_{\mu\nu}\frac{\partial}{\partial x_\nu}\{\sqrt{-g}\,g_{\sigma\mu}\kappa\vartheta_{\mu\nu}\}=\tfrac12\sum_{\mu\nu}\sqrt{-g}\,\frac{\partial g_{\mu\nu}}{\partial x_\sigma}\{-\Delta_{\mu\nu}(\gamma)+\kappa\vartheta_{\mu\nu}\}∑μν​∂xν​∂​{−g​gσμ​κϑμν​}=21​∑μν​−g​∂xσ​∂gμν​​{−Δμν​(γ)+κϑμν​}, for every metric.
  3. Identity (12b), the covariant counterpart, with tμνt_{\mu\nu}tμν​ and Dμν(g)D_{\mu\nu}(g)Dμν​(g).
  4. Eq. (10) ⇔\Leftrightarrow⇔ eq. (20), the covariant energy-momentum law.
  5. Eq. (18) ⇒\Rightarrow⇒ eq. (21), −Dμν(g)=κ(tμν+Tμν)-D_{\mu\nu}(g)=\kappa(t_{\mu\nu}+T_{\mu\nu})−Dμν​(g)=κ(tμν​+Tμν​).
  6. Eq. (22), the covariant conservation law for matter plus field.

Significance

The result itself. Eq. (19) is the property Einstein required of any relativistic theory of gravitation: the energy of the gravitational field acts as a source in the same way as every other form of energy, and matter together with field obeys conservation laws of divergence form. Identity (12a) is what makes this work for the Entwurf operator Δμν(γ)\Delta_{\mu\nu}(\gamma)Δμν​(γ); together with the matter law (10), the field equations (18) and the gravitational stress-energy ϑμν\vartheta_{\mu\nu}ϑμν​ are fixed by it.

Formalizing it. These statements are proved in the source by explicit computation, and the steps (12) → (12a) and the covariant forms (20)–(22) are given without the intermediate algebra. A machine-checked development provides the full index computations: derivatives of γμν\gamma_{\mu\nu}γμν​ and −g\sqrt{-g}−g​ in terms of those of gμνg_{\mu\nu}gμν​, the contractions in (12a) and (12b), and the lowering identities linking Δμν(γ)\Delta_{\mu\nu}(\gamma)Δμν​(γ) to Dμν(g)D_{\mu\nu}(g)Dμν​(g) and ϑμν\vartheta_{\mu\nu}ϑμν​ to tμνt_{\mu\nu}tμν​. A search of the platform library found no existing formalization of these statements.

Difficulty

There is no conceptual obstacle, but the identities are long. Identity (12a) involves second derivatives of γμν\gamma_{\mu\nu}γμν​, the derivative of −g\sqrt{-g}−g​, and contractions over up to six indices. The source gives only the final form of (12) and says the identity is obtained "nach dem angedeuteten Verfahren"; the intermediate algebra, and the analytic facts behind it (differentiability of matrix inversion and of −det⁡g\sqrt{-\det g}−detg​ under the standing assumptions), are not written out. A naive expansion of all sums produces thousands of terms.

Formalization scope

  • Space-time is R4\mathbb R^4R4 as one global chart, with points x:Fin 4→Rx:\mathrm{Fin}\,4\to\mathbb Rx:Fin4→R; two-index fields are matrix-valued functions. Partial derivatives are Fréchet derivatives along coordinate directions.
  • Standing assumptions on the metric: entries C2C^2C2, symmetric, det⁡g<0\det g<0detg<0 everywhere. No signature condition beyond the sign of the determinant; γ\gammaγ is the matrix inverse, −g\sqrt{-g}−g​ the real square root of −det⁡g-\det g−detg.
  • κ≠0\kappa\neq0κ=0 is assumed wherever ϑμν\vartheta_{\mu\nu}ϑμν​ or tμνt_{\mu\nu}tμν​ (defined with the factor 1/(2κ)1/(2\kappa)1/(2κ)) appears. Matter tensors are assumed C1C^1C1, and symmetric where the source's manipulation needs it (eq. (20)).
  • In eq. (14) the sum over α,β\alpha,\betaα,β is taken only in the term containing them, following the paper's convention. The printed eq. (22) has an inconsistent index placement; milestone 6 uses the placement of (20) and (12b).
  • The goal must not be trivialized: the field equations and the matter law are hypotheses about the same Θμν\Theta_{\mu\nu}Θμν​, and the hypotheses are satisfiable (e.g. constant metric, Θ=0\Theta=0Θ=0) but not degenerate in general.
  • Reusable infrastructure: derivative formulas for the inverse and determinant of a CkC^kCk matrix field, coordinate tensor calculus on R4\mathbb R^4R4. Contributions of these as separate lemmas are welcome.

Selected references

  • A. Einstein and M. Grossmann, Entwurf einer verallgemeinerten Relativitätstheorie und einer Theorie der Gravitation, B. G. Teubner, Leipzig und Berlin, 1913; reprinted in Zeitschrift für Mathematik und Physik 62 (1914). The source of all statements of this mission (Part I, §§4–5, pp. 10–17).
  • A. Einstein, Die Feldgleichungen der Gravitation, Sitzungsberichte der Preußischen Akademie der Wissenschaften, 1915, pp. 844–847.
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Captain: Lucas

First Law of Thermodynamics (Wikipedia) I: Internal Energy as a State Function from Adiabatic WorkTextbook

Motivation

The first law of thermodynamics is the form the law of conservation of energy takes for thermodynamic processes. For a closed system (no transfer of matter) it is usually written, in the sign convention of Clausius, as

ΔU=Q−W,\Delta U = Q - W,ΔU=Q−W,

where QQQ is the heat supplied to the system, WWW is the work done by the system on its surroundings, and UUU is the internal energy. Heat and work describe a process and depend on the path; the internal energy is a property of the state, and its change depends only on the initial and final states.

The Wikipedia article First law of thermodynamics (revision oldid=1366986255) describes two ways of reaching this statement. In the original "thermodynamic approach" (Clausius 1850, Rankine), heat, defined by calorimetry, and work are primitive notions. In the "mechanical approach" (Bryan 1907, Carathéodory 1909, Born 1921), only adiabatic work is primitive. The law then asserts that adiabatic work is independent of the path, and that this work defines a state function UUU, fixed up to an additive constant. Heat becomes a derived quantity, the residual Q=ΔU+WQ = \Delta U + WQ=ΔU+W. This mission formalizes the logical core of the mechanical approach.

Setting

A closed system has a set σ\sigmaσ of states. A process ppp has an initial state pstartp_{\mathrm{start}}pstart​, a final state pfinishp_{\mathrm{finish}}pfinish​, a net work W(p)∈RW(p)\in\mathbb RW(p)∈R done by the system on its surroundings, and a label recording whether it is adiabatic (carried out inside an adiabatic enclosure, so that energy is transferred only as work). A set P\mathcal PP of processes stands for the processes that can actually be carried out. It is assumed to satisfy:

  1. Composition: if p,q∈Pp,q\in\mathcal Pp,q∈P and pfinish=qstartp_{\mathrm{finish}}=q_{\mathrm{start}}pfinish​=qstart​, then the composite "first ppp, then qqq" lies in P\mathcal PP. Its work is W(p)+W(q)W(p)+W(q)W(p)+W(q), and it is adiabatic exactly when both stages are.
  2. Null processes: for every state AAA, leaving the system in state AAA (with no work and no exchange) is in P\mathcal PP.
  3. Path independence of adiabatic work: any two adiabatic processes in P\mathcal PP with the same initial and final states involve the same work.
  4. Adiabatic accessibility: there is a reference state OOO such that every state AAA is reached from OOO, or reaches OOO, by some adiabatic process in P\mathcal PP.

A function U:σ→RU:\sigma\to\mathbb RU:σ→R is an internal energy for P\mathcal PP if U(pfinish)−U(pstart)=−W(p)U(p_{\mathrm{finish}})-U(p_{\mathrm{start}})=-W(p)U(pfinish​)−U(pstart​)=−W(p) for every adiabatic p∈Pp\in\mathcal Pp∈P. For a given UUU, the heat supplied in a process is the residual

QU(p)=U(pfinish)−U(pstart)+W(p).Q_U(p)=U(p_{\mathrm{finish}})-U(p_{\mathrm{start}})+W(p).QU​(p)=U(pfinish​)−U(pstart​)+W(p).

Formalization targets

Goal: existence and uniqueness of internal energy

Under assumptions 1 to 4,

∃ U internal energy for P,andU,U′ internal energies  ⟹  ∃c∈R ∀A, U′(A)=U(A)+c.\exists\,U \text{ internal energy for } \mathcal P,\qquad\text{and}\qquad U,U' \text{ internal energies} \implies \exists c\in\mathbb R\ \forall A,\ U'(A)=U(A)+c.∃U internal energy for P,andU,U′ internal energies⟹∃c∈R ∀A, U′(A)=U(A)+c.

This is the article's statement: "For all adiabatic processes between two specified states of a closed system of any nature, the net work done is the same regardless the details of the process, and determines a state function called internal energy, UUU", together with its remark that the internal energy "is defined only up to an arbitrary additive constant of integration".

Milestones

  1. Formula (1) and the chain through the reference state. If quasi-static adiabatic work WA→BW_{A\to B}WA→B​ satisfies WA→O=−WO→AW_{A\to O}=-W_{O\to A}WA→O​=−WO→A​ and WA→B=WA→O+WO→BW_{A\to B}=W_{A\to O}+W_{O\to B}WA→B​=WA→O​+WO→B​, and U(A)=U(O)−WO→AU(A)=U(O)-W_{O\to A}U(A)=U(O)−WO→A​, then −WA→B=U(B)−U(A)-W_{A\to B}=U(B)-U(A)−WA→B​=U(B)−U(A).
  2. Shifting an internal energy by a constant gives an internal energy.
  3. Under adiabatic accessibility, two internal energies differ by a constant.
  4. Under assumptions 1 to 4, an internal energy exists (normalized by U(O)=0U(O)=0U(O)=0).
  5. The Clausius form ΔU=Q−W\Delta U=Q-WΔU=Q−W holds for the residual heat.
  6. Adiabatic processes involve no heat.
  7. In an adynamic process (no work), Q=ΔUQ=\Delta UQ=ΔU.
  8. Heat does not depend on the additive constant in UUU.
  9. In a cyclic process, the net work done equals the net heat taken in.
  10. No adiabatic cyclic process produces net work (no perpetual motion machine of the first kind).

Significance

The goal makes precise the step in the mechanical approach where internal energy is defined from adiabatic work instead of being postulated. It shows which properties of the set of realizable processes are needed for the definition to make sense. Once UUU exists, the familiar consequences follow at once: the Clausius equation for every process, the heat-free character of adiabatic processes, Q=ΔUQ=\Delta UQ=ΔU for adynamic processes, the equality of work and heat over a cycle, and the impossibility of perpetual motion of the first kind. Milestones 5 to 10 record these.

The mathematics is elementary and the results are classical. The value of the formalization is that it states exactly the hypotheses under which "path-independent adiabatic work defines a state function" holds. The article itself notes the gaps: experimental evidence for independence from the order of stages is thin (Bailyn), and Münster observes that one cannot always go adiabatically in both directions between two states. Assumption 4 therefore asks only for one direction.

Difficulty

The only non-routine step is existence when accessibility holds in just one direction per state. One defines U(A)=−W(O→A)U(A)=-W(O\to A)U(A)=−W(O→A) or U(A)=W(A→O)U(A)=W(A\to O)U(A)=W(A→O), depending on which link exists. Showing that this choice is consistent, and that it gives ΔU=−W\Delta U=-WΔU=−W for an arbitrary adiabatic process A→BA\to BA→B, requires splitting into four cases according to how AAA and BBB are linked to OOO. In some of these cases the composite process is an adiabatic cycle, which must be compared with a null process. Without null processes, or without closure under composition, the naive definition is not well-defined.

Formalization scope

  • States form an arbitrary type σ\sigmaσ. Work is real-valued and is work done by the system (Clausius convention), so that ΔU=−W\Delta U=-WΔU=−W for adiabatic processes and ΔU=Q−W\Delta U=Q-WΔU=Q−W in general.
  • "Adiabatic" is a primitive label on processes, as adiabatic walls are primitive in the mechanical approach. Heat is not primitive: it is defined as the residual QU(p)=ΔU+WQ_U(p)=\Delta U+WQU​(p)=ΔU+W.
  • The physically realizable processes form a set P\mathcal PP. All hypotheses are stated about P\mathcal PP, never about every conceivable process.
  • The goal is not vacuous: assumptions 1 to 4 can all hold at once (for example, states R\mathbb RR, with adiabatic work from aaa to bbb equal to a−ba-ba−b).
  • Open systems, matter transfer, the extensivity statement U0=U1+U2U_0=U_1+U_2U0​=U1​+U2​, and the differential form dU=δQ−δWdU=\delta Q-\delta WdU=δQ−δW are out of scope for this first mission.

Selected references

  • Wikipedia, First law of thermodynamics, revision oldid=1366986255. https://en.wikipedia.org/w/index.php?title=First_law_of_thermodynamics&oldid=1366986255
  • C. Carathéodory, Untersuchungen über die Grundlagen der Thermodynamik, Mathematische Annalen 67 (1909), 355–386. https://ui.adsabs.harvard.edu/abs/1909MatAn..67..355C
  • M. Born, Kritische Betrachtungen zur traditionellen Darstellung der Thermodynamik, Physikalische Zeitschrift 22 (1921), 218–224.
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Quantum Gravity·Captain: Lucas

Non-renormalizability of gravity from black-hole entropy (Shomer 2007)Research Paper

Motivation

Why is general relativity not a renormalizable quantum field theory? The textbook answer is perturbative: Newton's constant has negative mass dimension, so the gravitational coupling is irrelevant and loop divergences cannot be absorbed into finitely many counterterms. That argument can in principle be evaded (Weinberg's asymptotic safety). Shomer's note (arXiv:0709.3555), following Banks and Aharony–Banks, gives a non-perturbative, thermodynamic argument instead: the very-high-energy spectrum of any renormalizable ddd-dimensional QFT is that of a ddd-dimensional conformal field theory (CFT), whereas the high-energy spectrum of gravity is dominated by black holes, whose Bekenstein–Hawking entropy grows with energy in a way no CFT can match.

Setting

  • CFT side (Sec. IV, Eqs. 29–30). For a ddd-dimensional CFT on Rtime×Sd−1\mathbb R_{\text{time}}\times S^{d-1}Rtime​×Sd−1 (sphere radius RRR) at temperature TTT, dimensional analysis and extensivity give S=a (RT)d−1S=a\,(RT)^{d-1}S=a(RT)d−1 and E=b Rd−1TdE=b\,R^{d-1}T^{d}E=bRd−1Td with constants a,b>0a,b>0a,b>0. Eliminating TTT gives the entropy as a function of energy, SCFT(E)=a (R (E/(bRd−1))1/d)d−1∼E(d−1)/dS_{\rm CFT}(E)=a\,\bigl(R\,(E/(bR^{d-1}))^{1/d}\bigr)^{d-1}\sim E^{(d-1)/d}SCFT​(E)=a(R(E/(bRd−1))1/d)d−1∼E(d−1)/d.
  • Flat gravity (Sec. V.1, Eqs. 31–32). The ddd-dimensional Schwarzschild metric has f(r)=1−ωd−2GNM/rd−3f(r)=1-\omega_{d-2}G_N M/r^{d-3}f(r)=1−ωd−2​GN​M/rd−3 with ωn=16π/(n Vol(Sn))\omega_n=16\pi/(n\,\mathrm{Vol}(S^n))ωn​=16π/(nVol(Sn)). The horizon rHr_HrH​ is the zero of fff, and the Bekenstein–Hawking entropy is S=A/(4GN)S=A/(4G_N)S=A/(4GN​) with A=Vol(Sd−2) rHd−2A=\mathrm{Vol}(S^{d-2})\,r_H^{d-2}A=Vol(Sd−2)rHd−2​, giving S∼M(d−2)/(d−3)S\sim M^{(d-2)/(d-3)}S∼M(d−2)/(d−3).
  • AdS gravity (Sec. V.2, Eqs. 33–34). With f(r)=1−ωd−2GNM/rd−3+r2/RAdS2f(r)=1-\omega_{d-2}G_NM/r^{d-3}+r^2/R_{\rm AdS}^2f(r)=1−ωd−2​GN​M/rd−3+r2/RAdS2​ the horizon is the largest zero of fff and S∼M(d−2)/(d−1)S\sim M^{(d-2)/(d-1)}S∼M(d−2)/(d−1) — the CFT law of one dimension lower (a shadow of AdS/CFT).

Formalization targets

Goal — black-hole entropy is not CFT entropy (flat space, Sec. V.1)

For every spacetime dimension d≥4d\ge 4d≥4, every GN>0G_N>0GN​>0 and every CFT datum a,b,R>0a,b,R>0a,b,R>0,

SBH(E) is not Θ(SCFT(E))as E→∞.S_{\rm BH}(E)\ \text{is not}\ \Theta\bigl(S_{\rm CFT}(E)\bigr)\quad\text{as }E\to\infty .SBH​(E) is not Θ(SCFT​(E))as E→∞.

Here Θ\ThetaΘ means bounded above and below by positive multiples of each other for all large EEE; this is how the paper's "∼\sim∼" is read.

Milestones

Eq. (29) (the elimination of TTT), Eq. (30), Eq. (32) exactly, footnote 26 (exponent comparison), Eq. (34) asymptotically, the AdS mismatch with a ddd-dimensional CFT, and the AdS match with a (d−1)(d-1)(d−1)-dimensional CFT.

Significance

The goal is the precise mathematical content of the paper's one-line argument: once the black-hole entropy formula and the CFT scaling law are fixed, their large-energy growth exponents (d−2)/(d−3)>1>(d−1)/d(d-2)/(d-3)>1>(d-1)/d(d−2)/(d−3)>1>(d−1)/d are incompatible. The physics inputs (that a renormalizable QFT flows to a CFT in the UV, that black holes dominate the gravitational density of states, the Bekenstein–Hawking formula) are modelling assumptions, encoded as definitions; the mission formalizes the asymptotic analysis that turns them into a contradiction, not the physics itself.

Difficulty

Mathematically elementary but fiddly: the horizon radius is defined implicitly as the largest positive zero of fff, so one must solve f(rH)=0f(r_H)=0f(rH​)=0 (exactly in flat space, asymptotically in AdS, where rHd−3(1+rH2/RAdS2)=ωd−2GNMr_H^{d-3}(1+r_H^2/R_{\rm AdS}^2)=\omega_{d-2}G_NMrHd−3​(1+rH2​/RAdS2​)=ωd−2​GN​M), handle real powers, and compare asymptotic classes with distinct exponents.

Formalization scope

All statements live in namespace GravityNonRenorm and import one definition file. The unit-sphere volume is the closed form Vol(Sn)=2π(n+1)/2/Γ((n+1)/2)\mathrm{Vol}(S^n)=2\pi^{(n+1)/2}/\Gamma((n+1)/2)Vol(Sn)=2π(n+1)/2/Γ((n+1)/2). Horizon radii are sSup of the set of positive zeros of fff (junk value 000 when that set is empty, e.g. for M≤0M\le 0M≤0); all claims are asymptotic as E→∞E\to\inftyE→∞ or assume M>0M>0M>0, so the junk value is never used. Dimensions are natural numbers; d≥4d\ge 4d≥4 for flat-space statements, d≥3d\ge3d≥3 for AdS, d≥2d\ge2d≥2 for CFT statements.

Selected references

  • A. Shomer, A pedagogical explanation for the non-renormalizability of gravity, arXiv:0709.3555 (2007). https://arxiv.org/abs/0709.3555
  • O. Aharony and T. Banks, Note on the quantum mechanics of M theory, JHEP 9903:016 (1999), arXiv:hep-th/9812237.
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Partial Differential Equations·Captain: Lucas

Fick's Laws of Diffusion: Fundamental Solution and Classical SolutionsTextbook

Motivation

Fick's laws of diffusion, posited by Adolf Fick in 1855, are the basic constitutive and evolution laws for the transport of mass by diffusion. The first law states that the diffusive flux is proportional to minus the concentration gradient, J=−D ∂xφJ=-D\,\partial_x\varphiJ=−D∂x​φ; the second law is the resulting evolution equation for the concentration,

∂φ∂t=D ∂2φ∂x2.\frac{\partial\varphi}{\partial t}=D\,\frac{\partial^2\varphi}{\partial x^2}.∂t∂φ​=D∂x2∂2φ​.

They are the standard model for diffusion in solids, liquids and gases (in the absence of bulk flow), and are used to model transport in foods, neurons, biopolymers, pharmaceuticals, porous soils, nuclear materials and semiconductor doping. Mathematically, the second law is the heat equation with the thermal diffusivity replaced by the diffusion coefficient D>0D>0D>0.

This mission formalizes the mathematical content of the Wikipedia article Fick's laws of diffusion: the derivation of the second law from the first, the steady state, the fundamental solution, the error-function solutions for a constant source, and the mean-squared-displacement law.

Setting

A concentration is a real function φ(x,t)\varphi(x,t)φ(x,t) of position xxx and time ttt; a flux is a real function J(x,t)J(x,t)J(x,t). The diffusion coefficient is a constant D>0D>0D>0. For t>0t>0t>0 the diffusion kernel is

φD(x,t)=14πDtexp⁡(−x24Dt),\varphi_D(x,t)=\frac{1}{\sqrt{4\pi Dt}}\exp\Big(-\frac{x^2}{4Dt}\Big),φD​(x,t)=4πDt​1​exp(−4Dtx2​),

and in nnn space dimensions

φD(n)(x,t)=(4πDt)−n/2exp⁡(−∥x∥24Dt),x∈Rn.\varphi^{(n)}_D(x,t)=(4\pi Dt)^{-n/2}\exp\Big(-\frac{\|x\|^2}{4Dt}\Big),\qquad x\in\mathbb R^n.φD(n)​(x,t)=(4πDt)−n/2exp(−4Dt∥x∥2​),x∈Rn.

The complementary error function is erfc⁡(u)=2π∫u∞e−s2 ds\operatorname{erfc}(u)=\frac{2}{\sqrt\pi}\int_u^\infty e^{-s^2}\,dserfc(u)=π​2​∫u∞​e−s2ds.

Formalization targets

Goal: the fundamental solution

For D>0D>0D>0, φD\varphi_DφD​ solves ∂tφ=D∂x2φ\partial_t\varphi=D\partial_x^2\varphi∂t​φ=D∂x2​φ for t>0t>0t>0, has ∫RφD(x,t) dx=1\int_{\mathbb R}\varphi_D(x,t)\,dx=1∫R​φD​(x,t)dx=1 for every t>0t>0t>0, and satisfies

lim⁡t→0+∫RφD(x−y,t)f(y) dy=f(x)\lim_{t\to0^+}\int_{\mathbb R}\varphi_D(x-y,t)f(y)\,dy=f(x)t→0+lim​∫R​φD​(x−y,t)f(y)dy=f(x)

for every bounded continuous fff and every xxx.

Milestones

  1. Fick's second law follows from Fick's first law and mass conservation ∂tφ+∂xJ=0\partial_t\varphi+\partial_xJ=0∂t​φ+∂x​J=0 (constant DDD).
  2. A C2C^2C2 steady state in one dimension is linear: c(x)=ax+bc(x)=ax+bc(x)=ax+b.
  3. The three components of the goal, separately (PDE, unit mass, initial point source).
  4. n(x,t)=n0erfc⁡(x/(2Dt))n(x,t)=n_0\operatorname{erfc}\big(x/(2\sqrt{Dt})\big)n(x,t)=n0​erfc(x/(2Dt​)) solves the second law with n(0,t)=n0n(0,t)=n_0n(0,t)=n0​ and n(x,0+)=0n(x,0^+)=0n(x,0+)=0 for x>0x>0x>0.
  5. n(x,t)=n02erfc⁡(x/(2Dt))n(x,t)=\frac{n_0}{2}\operatorname{erfc}\big(x/(2\sqrt{Dt})\big)n(x,t)=2n0​​erfc(x/(2Dt​)) solves the second law with initial profile n0n_0n0​ on x<0x<0x<0 and 000 on x>0x>0x>0.
  6. Mean squared displacement in Rn\mathbb R^nRn: ∫∥x∥2φD(n)(x,t) dx=2nDt\int\|x\|^2\varphi^{(n)}_D(x,t)\,dx=2nDt∫∥x∥2φD(n)​(x,t)dx=2nDt.

Significance

The fundamental solution is what makes the second law usable: the solution of the one-dimensional diffusion problem with bounded continuous initial data is the convolution of the data with φD\varphi_DφD​, and the erfc profiles and diffusion length 2Dt2\sqrt{Dt}2Dt​ quoted throughout applications are derived from it. The mean-squared-displacement law 2nDt2nDt2nDt connects the macroscopic diffusion coefficient to the microscopic Brownian motion of particles.

All statements are classical and proved in the literature; the task here is to formalize them. Mathlib provides the Gaussian integral but has no error function and no development of the one-dimensional diffusion equation, so the mission also produces reusable infrastructure (erfc and its derivative and limits, Gaussian moments in Rn\mathbb R^nRn, the approximate-identity property).

Difficulty

The individual computations are routine on paper; the formal difficulty lies in rigor that the article leaves implicit: differentiating the kernel in both variables only on t>0t>0t>0, justifying limits of parameter-dependent integrals as t→0+t\to0^+t→0+ (dominated convergence for the point-source property), computing the second moment of an nnn-dimensional Gaussian on Euclidean space, and building erfc from scratch, including its derivative −2πe−u2-\frac{2}{\sqrt\pi}e^{-u^2}−π​2​e−u2 and its limits at ±∞\pm\infty±∞.

Formalization scope

All objects are real-valued; derivatives are Mathlib's deriv (which is 000 at non-differentiable points), integrals are Lebesgue integrals, and limits as t→0+t\to0^+t→0+ use the right-neighbourhood filter. Every statement about the kernel or erfc profiles assumes D>0D>0D>0 and evaluates the PDE only at t>0t>0t>0, so junk values of square root and division never matter. The steady-state milestone assumes C2C^2C2 regularity, without which deriv would admit non-smooth "solutions" such as ∣x∣|x|∣x∣. Rn\mathbb R^nRn is EuclideanSpace ℝ (Fin n). Physical parts of the article (Stokes–Einstein relation, Maxwell–Stefan, sorption kinetics, approximations) are out of scope.

Selected references

  • Wikipedia contributors, Fick's laws of diffusion. https://en.wikipedia.org/wiki/Fick%27s_laws_of_diffusion
  • A. Fick, Ueber Diffusion, Annalen der Physik 170 (1855) 59–86. https://doi.org/10.1002/andp.18551700105
  • J. Crank, The Mathematics of Diffusion, 2nd ed., Oxford University Press, 1975.
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Analysis·Captain: Lucas

BCS Theory: the universal gap ratio Δ(0) = (π/e^γ) k_B T_cTextbook

Motivation

The BCS theory of Bardeen, Cooper and Schrieffer (1957) is the microscopic theory of conventional superconductivity in metals; its authors received the 1972 Nobel Prize in Physics. Its most quoted quantitative predictions are universal numbers: in the weak-coupling limit the zero-temperature energy gap and the transition temperature are related by Δ(0)=(π/eγ) kBTc≈1.764 kBTc\Delta(0) = (\pi/e^{\gamma})\,k_BT_c \approx 1.764\,k_BT_cΔ(0)=(π/eγ)kB​Tc​≈1.764kB​Tc​, the gap closes as Δ(T)/Δ(0)≈1.741−T/Tc\Delta(T)/\Delta(0)\approx 1.74\sqrt{1-T/T_c}Δ(T)/Δ(0)≈1.741−T/Tc​​, and the specific heat jumps by (Ces−Cen)/Cen≈1.43(C_{es}-C_{en})/C_{en}\approx 1.43(Ces​−Cen​)/Cen​≈1.43 at TcT_cTc​. These numbers are what experiments compare against, and they follow from a single scalar integral equation, the BCS gap equation. This mission formalizes that mathematical core, following the section Erfolge der BCS-Theorie of the German Wikipedia article BCS-Theorie.

Timeline (as summarized in the source):

  • 1950 — isotope effect observed (Lock et al.; Maxwell; Serin et al.): TcT_cTc​ depends on the ionic mass MMM.
  • 1956 — Cooper shows that an arbitrarily weak attraction binds two electrons above a filled Fermi sea.
  • 1957 — Bardeen, Cooper and Schrieffer publish Theory of Superconductivity, including the gap equation and its consequences.

Setting

Fix the Boltzmann constant kB>0k_B>0kB​>0, the Debye energy ℏωD>0\hbar\omega_D>0ℏωD​>0 (called hbarOmegaD in Lean) and the dimensionless coupling λ=V0 Z(EF)>0\lambda = V_0\,Z(E_F)>0λ=V0​Z(EF​)>0 (called coupling), where V0V_0V0​ is the attractive pairing potential and Z(EF)Z(E_F)Z(EF​) is half the electronic density of states at the Fermi energy. With the quasiparticle energy E(η,Δ)=η2+Δ2E(\eta,\Delta)=\sqrt{\eta^2+\Delta^2}E(η,Δ)=η2+Δ2​ define

I0(ℏωD,Δ)=∫0ℏωDdηη2+Δ2,I(kB,ℏωD,Δ,T)=∫0ℏωDdηη2+Δ2tanh⁡η2+Δ22kBT.I_0(\hbar\omega_D,\Delta)=\int_0^{\hbar\omega_D}\frac{d\eta}{\sqrt{\eta^2+\Delta^2}},\qquad I(k_B,\hbar\omega_D,\Delta,T)=\int_0^{\hbar\omega_D}\frac{d\eta}{\sqrt{\eta^2+\Delta^2}}\tanh\frac{\sqrt{\eta^2+\Delta^2}}{2k_BT}.I0​(ℏωD​,Δ)=∫0ℏωD​​η2+Δ2​dη​,I(kB​,ℏωD​,Δ,T)=∫0ℏωD​​η2+Δ2​dη​tanh2kB​Tη2+Δ2​​.

The zero-temperature gap Δ(0)\Delta(0)Δ(0) is the positive solution of 1/λ=I0(ℏωD,Δ)1/\lambda = I_0(\hbar\omega_D,\Delta)1/λ=I0​(ℏωD​,Δ); the critical temperature TcT_cTc​ is the positive solution of 1/λ=I(kB,ℏωD,0,T)1/\lambda = I(k_B,\hbar\omega_D,0,T)1/λ=I(kB​,ℏωD​,0,T); and for 0<T<Tc0<T<T_c0<T<Tc​ the gap Δ(T)\Delta(T)Δ(T) is the positive solution of 1/λ=I(kB,ℏωD,Δ,T)1/\lambda = I(k_B,\hbar\omega_D,\Delta,T)1/λ=I(kB​,ℏωD​,Δ,T). The Fermi–Dirac function is f(E,T)=1/(eE/kBT+1)f(E,T) = 1/(e^{E/k_BT}+1)f(E,T)=1/(eE/kB​T+1), and 1−2f(E,T)=tanh⁡(E/2kBT)1-2f(E,T) = \tanh(E/2k_BT)1−2f(E,T)=tanh(E/2kB​T).

Formalization targets

Goal: the universal gap ratio

lim⁡λ→0+Δ(0)kBTc=πeγ=1.764…\lim_{\lambda\to0^+}\frac{\Delta(0)}{k_BT_c}=\frac{\pi}{e^{\gamma}}=1.764\ldotsλ→0+lim​kB​Tc​Δ(0)​=eγπ​=1.764…

with γ\gammaγ the Euler–Mascheroni constant. The source writes Δ(T=0)=2ℏωDe−1/V0Z(EF)=πeγkBTc\Delta(T=0)=2\hbar\omega_D e^{-1/V_0Z(E_F)}=\frac{\pi}{e^\gamma}k_BT_cΔ(T=0)=2ℏωD​e−1/V0​Z(EF​)=eγπ​kB​Tc​; both equalities are weak-coupling asymptotics, so the goal is stated as a limit λ→0+\lambda\to0^+λ→0+ at fixed kBk_BkB​, ℏωD\hbar\omega_DℏωD​.

Milestones

  1. I0(ℏωD,Δ)=arsinh⁡(ℏωD/Δ)I_0(\hbar\omega_D,\Delta) = \operatorname{arsinh}(\hbar\omega_D/\Delta)I0​(ℏωD​,Δ)=arsinh(ℏωD​/Δ).
  2. Δ(0)=ℏωD/sinh⁡(1/λ)\Delta(0)=\hbar\omega_D/\sinh(1/\lambda)Δ(0)=ℏωD​/sinh(1/λ), the unique positive solution of the T=0T=0T=0 gap equation.
  3. Δ(0)∼2ℏωDe−1/λ\Delta(0)\sim 2\hbar\omega_D e^{-1/\lambda}Δ(0)∼2ℏωD​e−1/λ as λ→0+\lambda\to0^+λ→0+.
  4. The Fermi–Dirac and tanh⁡\tanhtanh forms of the finite-temperature gap equation agree.
  5. The TcT_cTc​ equation has exactly one positive solution.
  6. kBTc∼2eγπℏωDe−1/λk_BT_c\sim\frac{2e^\gamma}{\pi}\hbar\omega_D e^{-1/\lambda}kB​Tc​∼π2eγ​ℏωD​e−1/λ (the source's 1,141{,}141,14).
  7. Isotope effect: with ℏωD=C/M\hbar\omega_D = C/\sqrt MℏωD​=C/M​, Tc∝M−1/2T_c\propto M^{-1/2}Tc​∝M−1/2.
  8. Δ(T)\Delta(T)Δ(T) exists uniquely for 0<T<Tc0<T<T_c0<T<Tc​, and the gap equation has no positive solution for T≥TcT\ge T_cT≥Tc​.
  9. Near TcT_cTc​: Δ(T)2/(1−T/Tc)\Delta(T)^2/(1-T/T_c)Δ(T)2/(1−T/Tc​) has a limit L(λ)L(\lambda)L(λ) as T→Tc−T\to T_c^-T→Tc−​, and L(λ)/Δ(0)2→8e2γ/(7ζ(3))=1.73672L(\lambda)/\Delta(0)^2\to 8e^{2\gamma}/(7\zeta(3)) = 1.7367^2L(λ)/Δ(0)2→8e2γ/(7ζ(3))=1.73672 as λ→0+\lambda\to0^+λ→0+.
  10. Specific-heat jump: the left derivative D(λ)D(\lambda)D(λ) of Δ(T)2\Delta(T)^2Δ(T)2 at TcT_cTc​ exists, and −D(λ)/(2π23kB2Tc)→12/(7ζ(3))=1.426…-D(\lambda)/(\tfrac{2\pi^2}{3}k_B^2T_c)\to 12/(7\zeta(3)) = 1.426\ldots−D(λ)/(32π2​kB2​Tc​)→12/(7ζ(3))=1.426….

Significance

The universal ratios are the standard quantitative test that separates weak-coupling (BCS-like) superconductors from strong-coupling ones; deviations from 1.7641.7641.764 and 1.431.431.43 are used to diagnose strong electron–phonon coupling. Mathematically, each statement is an assertion about a parameter-dependent integral equation and its asymptotics as λ→0+\lambda\to0^+λ→0+, with the Euler–Mascheroni constant and ζ(3)\zeta(3)ζ(3) arising from the asymptotics of ∫0Xtanh⁡(x)/x dx\int_0^X\tanh(x)/x\,dx∫0X​tanh(x)/xdx and from a Sommerfeld-type expansion near TcT_cTc​. These results are classical in the physics literature; the mission aims at a machine-checked derivation of the textbook constants from the gap equation, together with reusable lemmas on monotone parameter-dependent integrals.

Difficulty

The T=0T=0T=0 statements reduce to an explicit antiderivative. The finite-temperature statements do not: TcT_cTc​ and Δ(T)\Delta(T)Δ(T) are defined only implicitly, so the asymptotics require a uniform expansion ∫0Xtanh⁡(x)/x dx=log⁡X+log⁡(4eγ/π)+o(1)\int_0^X\tanh(x)/x\,dx=\log X+\log(4e^\gamma/\pi)+o(1)∫0X​tanh(x)/xdx=logX+log(4eγ/π)+o(1). The near-TcT_cTc​ and specific-heat statements additionally concern the behaviour of Δ(T)2\Delta(T)^2Δ(T)2 at the boundary point TcT_cTc​, where Δ\DeltaΔ itself is not differentiable, and the evaluation of the resulting coefficient in the limit ℏωD/kBTc→∞\hbar\omega_D/k_BT_c\to\inftyℏωD​/kB​Tc​→∞.

Formalization scope

  • All quantities are real numbers. Δ(0)\Delta(0)Δ(0), TcT_cTc​ and Δ(T)\Delta(T)Δ(T) are defined as real suprema (sSup) of the corresponding positive solution sets, so they equal 000 when no positive solution exists; existence and uniqueness are separate milestones. In particular Δ(T)=0\Delta(T)=0Δ(T)=0 for T≥TcT\ge T_cT≥Tc​.
  • The zero-temperature gap is a separate definition: at T=0T=0T=0 the finite-temperature integrand is not used.
  • The coupling enters only through λ=V0Z(EF)\lambda = V_0Z(E_F)λ=V0​Z(EF​); asymptotic claims are limits λ→0+\lambda\to0^+λ→0+ at fixed kB,ℏωD>0k_B,\hbar\omega_D>0kB​,ℏωD​>0, with the exact constants 2eγ/π2e^\gamma/\pi2eγ/π, 8e2γ/(7ζ(3))8e^{2\gamma}/(7\zeta(3))8e2γ/(7ζ(3)) and 12/(7ζ(3))12/(7\zeta(3))12/(7ζ(3)) in place of the rounded 1,141{,}141,14, 1,7421{,}74^21,742 and 1,431{,}431,43. ζ(3)\zeta(3)ζ(3) is written as the real part of riemannZeta 3.
  • The specific heat is not modeled thermodynamically; the jump milestone formalizes the source's closed-form expression in terms of −dΔ2/dT-d\Delta^2/dT−dΔ2/dT at TcT_cTc​.
  • Needed infrastructure: monotonicity and continuity of parameter-dependent interval integrals, the integral identity for arsinh⁡\operatorname{arsinh}arsinh, asymptotics of ∫0Xtanh⁡x/x dx\int_0^X\tanh x/x\,dx∫0X​tanhx/xdx, and Mathlib's Euler–Mascheroni constant and ζ(3)\zeta(3)ζ(3).

Selected references

  • J. Bardeen, L. N. Cooper, J. R. Schrieffer, Theory of Superconductivity, Phys. Rev. 108, 1175 (1957). https://doi.org/10.1103/PhysRev.108.1175
  • L. N. Cooper, Bound Electron Pairs in a Degenerate Fermi Gas, Phys. Rev. 104, 1189 (1956). https://doi.org/10.1103/PhysRev.104.1189
  • Wikipedia (de), BCS-Theorie, section Erfolge der BCS-Theorie (source used for all statements). https://de.wikipedia.org/wiki/BCS-Theorie
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Analysis·Captain: Lucas

Titius–Bode Law I: The −25%/+50% Coverage Band of Doubling Distance RulesTextbook

Motivation

The Titius–Bode law is an empirical rule, published in the eighteenth century by J. D. Titius and J. E. Bode, for the semi-major axes of the planets: in units in which the Earth's semi-major axis is 101010, the planets lie near 4+x4+x4+x with x=0,3,6,12,24,48,96,…x = 0, 3, 6, 12, 24, 48, 96, \dotsx=0,3,6,12,24,48,96,…. It anticipated the positions of Uranus (1781) and Ceres (1801), failed for Neptune (1846), and has since become a standard example of how a numerical pattern can fit data without a physical mechanism. Dermott's law (S. F. Dermott, 1968) is the analogous power law T(n)=T(0) CnT(n) = T(0)\,C^nT(n)=T(0)Cn for the orbital periods of the major satellites of Jupiter, Saturn and Uranus.

Much of the debate about such rules is quantitative rather than physical. The Wikipedia article on the law records, in a footnote to its data table, the observation that because consecutive predicted distances roughly double, an arbitrary planet may be found within −25%-25\%−25% to +50%+50\%+50% of one of the predicted positions. In other words, the agreement of any single body with the rule at that level carries no information. This mission formalizes that observation and the elementary arithmetic of the law as stated in the source.

Timeline (as recorded in the source). Gregory (1702, 1715) and Wolff (1723–24) give the sequence 4,7,10,16,52,1004, 7, 10, 16, 52, 1004,7,10,16,52,100; Titius (1766) and Bode (1772) publish the rule; Uranus (1781) and Ceres (1801) fit it; Neptune (1846) does not; Blagg (1913) and Richardson (1945) replace the ratio 222 by about 1.731.731.73; Dermott (1968) proposes the period law for satellite systems; Nieto (1970, 1972) reviews the subject.

Setting

For a formal exponent n∈{−∞,0,1,2,… }n \in \{-\infty, 0, 1, 2, \dots\}n∈{−∞,0,1,2,…} put 2−∞=02^{-\infty} = 02−∞=0. The Titius–Bode distance in astronomical units is

a(n)=0.4+0.3⋅2n,n=−∞,0,1,2,…,a(n) = 0.4 + 0.3 \cdot 2^{n}, \qquad n = -\infty, 0, 1, 2, \dots,a(n)=0.4+0.3⋅2n,n=−∞,0,1,2,…,

so a(−∞)=0.4a(-\infty) = 0.4a(−∞)=0.4, a(0)=0.7a(0) = 0.7a(0)=0.7, a(1)=1.0a(1) = 1.0a(1)=1.0, a(2)=1.6,…a(2) = 1.6, \dotsa(2)=1.6,…. The same numbers appear in three other guises in the source: the original form 4+x4 + x4+x (Earth =10=10=10), the form 4+3⋅2n4 + 3 \cdot 2^n4+3⋅2n (Earth =10=10=10), and the canonical form an=0.4+0.3⋅2na_n = 0.4 + 0.3 \cdot 2^nan​=0.4+0.3⋅2n for n=0,1,2,…n = 0, 1, 2, \dotsn=0,1,2,…. The relative deviation of an observed value ddd from a predicted value ppp is (d−p)/p(d - p)/p(d−p)/p, which the source reports as a percentage.

Dermott's law models the period of the nnn-th satellite as T(n)=T(0) CnT(n) = T(0)\,C^nT(n)=T(0)Cn. Kepler's third law makes the semi-major axis proportional to the 2/32/32/3 power of the period, a=K T2/3a = K\,T^{2/3}a=KT2/3.

Formalization targets

Goal: the coverage band

∀d≥0.3:∃ n∈{−∞,0,1,2,… },−14  ≤  d−a(n)a(n)  ≤  12.\forall d \ge 0.3:\quad \exists\, n \in \{-\infty,0,1,2,\dots\},\qquad -\tfrac14 \;\le\; \frac{d - a(n)}{a(n)} \;\le\; \tfrac12 .∀d≥0.3:∃n∈{−∞,0,1,2,…},−41​≤a(n)d−a(n)​≤21​.

Every distance of at least 0.30.30.3 au lies within −25%-25\%−25% to +50%+50\%+50% of some Titius–Bode position. The lower limit 0.3=34⋅0.40.3 = \tfrac34 \cdot 0.40.3=43​⋅0.4 is exactly where the statement begins to hold: below it no predicted position is close enough. The source says "an arbitrary planet"; the formal statement makes the range explicit.

Supporting milestones

  1. The four representations of the rule (original, Earth =10=10=10, au, canonical) agree.
  2. The recursion an+1=2an−0.4a_{n+1} = 2a_n - 0.4an+1​=2an​−0.4 holds for the canonical form; started from a0=0.55a_0 = 0.55a0​=0.55, as printed in the source, it produces the canonical sequence shifted by one index.
  3. The predicted distances in the data table: 0.4,0.7,1.0,1.6,2.8,5.2,10.0,19.6,38.80.4, 0.7, 1.0, 1.6, 2.8, 5.2, 10.0, 19.6, 38.80.4,0.7,1.0,1.6,2.8,5.2,10.0,19.6,38.8 au, and 77.277.277.2 au for the next term.
  4. Consecutive predicted distances less than double, with ratio tending to 222.
  5. The abstract principle behind the goal: for any unbounded sequence with pk+1≤2pkp_{k+1} \le 2p_kpk+1​≤2pk​, every d≥34p0d \ge \tfrac34 p_0d≥43​p0​ lies within −25%-25\%−25% to +50%+50\%+50% of some pkp_kpk​.
  6. The 2:32{:}32:3 resonance figures: semi-major axes of bodies with periods in ratio 2:32{:}32:3 differ by −23.69%-23.69\%−23.69% and +31.04%+31.04\%+31.04% relative to one another.
  7. Dermott's law gives geometric spacing of periods (ratio CCC) and, through Kepler's third law, of semi-major axes (ratio C2/3C^{2/3}C2/3).

Significance

The goal makes precise why a fit of a single body to the Titius–Bode rule within tens of percent is weak evidence: the predicted positions are spaced so that the whole half-line [0.3,∞)[0.3, \infty)[0.3,∞) is covered by such bands. The resonance milestone gives the corresponding figures for a 2:32{:}32:3 period commensurability, and the Dermott milestone connects period power laws to Titius–Bode-type distance laws, as the source asserts.

All results are elementary and none is open. The value of the mission is a checked, unambiguous record of the arithmetic claims in the source, including one place where the source's formulas disagree: the "recursive form" with a0=0.55a_0 = 0.55a0​=0.55 does not reproduce the canonical form index-for-index but is shifted by one (milestone 2). No machine-checked version of these statements is known to exist on the platform.

Difficulty

There is no deep obstacle. The covering argument needs care in two places: the first step of the rule (0.4→0.70.4 \to 0.70.4→0.7) is not a doubling, and the generic doubling lemma must locate the first term that exceeds ddd without assuming monotonicity. The resonance milestone requires certified numerical bounds on the irrational numbers (2/3)2/3(2/3)^{2/3}(2/3)2/3 and (3/2)2/3(3/2)^{2/3}(3/2)2/3 that are tight enough to fix the second decimal place of a percentage.

Formalization scope

Distances, periods and deviations are real numbers. The exponent set {−∞,0,1,2,… }\{-\infty, 0, 1, 2, \dots\}{−∞,0,1,2,…} is encoded as the natural numbers with a bottom element adjoined, and 2−∞2^{-\infty}2−∞ is defined to be 000. The relative deviation is the plain quotient (d−p)/p(d-p)/p(d−p)/p; every statement only evaluates it at positive ppp. Percent figures from the source (−23.69%-23.69\%−23.69%, +31.04%+31.04\%+31.04%) are stated as "within 0.0050.0050.005 percentage points", i.e. correct to the two decimals printed. Kepler's law enters only as the hypothesis a=K T2/3a = K\,T^{2/3}a=KT2/3 with K>0K > 0K>0; no orbital mechanics is formalized. The doubling lemma is stated for an arbitrary real sequence and is reusable for any Titius–Bode-type rule.

Trivializing encodings are ruled out: the goal is not stated for an empty or bounded range of ddd, the predicted set is the full image of the rule, and the deviation band is the one printed in the source.

Selected references

  • Wikipedia, Titius–Bode law, revision 1372822920. https://en.wikipedia.org/w/index.php?title=Titius%E2%80%93Bode_law&oldid=1372822920
  • Wikipedia, Dermott's law, revision 1315813288. https://en.wikipedia.org/w/index.php?title=Dermott%27s_law&oldid=1315813288
  • M. M. Nieto, Conclusions about the Titius–Bode Law of Planetary Distances, Astronomy and Astrophysics 8 (1970), 105–111.
  • S. F. Dermott, On the origin of commensurabilities in the solar system – II: The orbital period relation, MNRAS 141 (1968), 363–376. https://doi.org/10.1093/mnras/141.3.363
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Quantum Mechanics·Captain: Lucas

Koch, Mean-Field Theory: Hartree-Fock and BCS I: The Brillouin TheoremTextbook

Motivation

The Hartree-Fock method approximates the ground state of an interacting many-electron system by the best single Slater determinant. It is the starting point of essentially all of quantum chemistry and of mean-field theories in condensed-matter physics: post-Hartree-Fock methods (configuration interaction, coupled cluster, perturbation theory) expand around it, and its orbital energies are the standard first estimate of ionization and excitation energies. E. Koch's lecture notes Mean-Field Theory: Hartree-Fock and BCS (Jülich Autumn School on Correlated Electrons, 2016) derive the method entirely within second quantization: Slater determinants are products of creation operators acting on a vacuum, variations are generated by one-body unitaries eiλM^e^{i\lambda\hat M}eiλM^, and the stationarity condition becomes an algebraic statement about matrix elements. The central result of the Hartree-Fock section is the Brillouin theorem: a Slater determinant is stationary exactly when the Hamiltonian does not couple it to its single excitations.

Timeline of the ideas involved: Hartree introduces the self-consistent field (1928); Fock and Slater add exchange through antisymmetrized wave functions (1930); Koopmans relates orbital energies to ionization energies (1934); Brillouin formulates the single-excitation condition (1934); Thouless gives the representation of Slater determinants by exponentials of one-body operators (1960).

Setting

Fix KKK orthonormal reference orbitals ϕ0,…,ϕK−1\phi_0,\dots,\phi_{K-1}ϕ0​,…,ϕK−1​; an orbital is a coefficient vector φ∈CK\varphi\in\mathbb C^Kφ∈CK with ⟨φ∣χ⟩=∑μφμ‾χμ\langle\varphi|\chi\rangle=\sum_\mu\overline{\varphi_\mu}\chi_\mu⟨φ∣χ⟩=∑μ​φμ​​χμ​. The Fock space has orthonormal basis ∣S⟩|S\rangle∣S⟩, S⊆{0,…,K−1}S\subseteq\{0,\dots,K-1\}S⊆{0,…,K−1} (the set of occupied orbitals). The creation operator ci†c^\dagger_ici†​ maps ∣S⟩|S\rangle∣S⟩ to (−1)#{j∈S: j>i}∣S∪{i}⟩(-1)^{\#\{j\in S:\,j>i\}}|S\cup\{i\}\rangle(−1)#{j∈S:j>i}∣S∪{i}⟩ if i∉Si\notin Si∈/S and to 000 otherwise; the annihilation operator cic_ici​ is its adjoint, and for a general orbital cφ†=∑μφμcμ†c^\dagger_\varphi=\sum_\mu\varphi_\mu c^\dagger_\mucφ†​=∑μ​φμ​cμ†​. The vacuum is ∣0⟩=∣∅⟩|0\rangle=|\emptyset\rangle∣0⟩=∣∅⟩.

The Slater determinant of orbitals α1,…,αN\alpha_1,\dots,\alpha_Nα1​,…,αN​ is ∣Φ⟩=cαN†⋯cα1†∣0⟩|\Phi\rangle=c^\dagger_{\alpha_N}\cdots c^\dagger_{\alpha_1}|0\rangle∣Φ⟩=cαN​†​⋯cα1​†​∣0⟩. A one-body operator with matrix MMM is M^=∑αβMαβcα†cβ\hat M=\sum_{\alpha\beta}M_{\alpha\beta}c^\dagger_\alpha c_\betaM^=∑αβ​Mαβ​cα†​cβ​. For a hermitian MMM the operators eiλM^e^{i\lambda\hat M}eiλM^ map Slater determinants to Slater determinants, and the energy functional along such a variation is

EM(λ)=⟨Φ∣eiλM^ H^ e−iλM^∣Φ⟩.E_M(\lambda)=\langle\Phi|e^{i\lambda\hat M}\,\hat H\,e^{-i\lambda\hat M}|\Phi\rangle .EM​(λ)=⟨Φ∣eiλM^H^e−iλM^∣Φ⟩.

For the concrete Hamiltonian of Sec. 3.2,

H^=∑n,mcn†Tnmcm+∑n>n′, m>m′cn†cn′†(Unn′,mm′−Unn′,m′m)cm′cm,\hat H=\sum_{n,m}c^\dagger_nT_{nm}c_m+\sum_{n>n',\,m>m'}c^\dagger_nc^\dagger_{n'}\bigl(U_{nn',mm'}-U_{nn',m'm}\bigr)c_{m'}c_m,H^=n,m∑​cn†​Tnm​cm​+n>n′,m>m′∑​cn†​cn′†​(Unn′,mm′​−Unn′,m′m​)cm′​cm​,

the Fock matrix of the determinant with occupied reference orbitals SSS is Fnm=Tnm+∑m′∈S(Unm′,mm′−Unm′,m′m)F_{nm}=T_{nm}+\sum_{m'\in S}(U_{nm',mm'}-U_{nm',m'm})Fnm​=Tnm​+∑m′∈S​(Unm′,mm′​−Unm′,m′m​), with diagonal entries the orbital energies εm\varepsilon_mεm​.

Formalization targets

Goal: the Brillouin theorem (Eqs. (62)–(63))

For a hermitian H^\hat HH^ and orthonormal α1,…,αN\alpha_1,\dots,\alpha_Nα1​,…,αN​,

(∀M=M†: EM′(0)=0)  ⟺  (∀ φo∈span⁡{αn}, φv⊥{αn}: ⟨Φ∣cφo†cφvH^∣Φ⟩=0).\Bigl(\forall M=M^\dagger:\ E_M'(0)=0\Bigr)\iff\Bigl(\forall\,\varphi_o\in\operatorname{span}\{\alpha_n\},\ \varphi_v\perp\{\alpha_n\}:\ \langle\Phi|c^\dagger_{\varphi_o}c_{\varphi_v}\hat H|\Phi\rangle=0\Bigr).(∀M=M†: EM′​(0)=0)⟺(∀φo​∈span{αn​}, φv​⊥{αn​}: ⟨Φ∣cφo​†​cφv​​H^∣Φ⟩=0).

It asserts no specific Hamiltonian, no particle number and no basis choice; it is the basis-independent form of the source's condition (63).

Milestones

The milestone list follows the source's own steps: the anticommutation relations (15); the overlap formula (7)/(46); the action of cφc_\varphicφ​, cφ†c^\dagger_\varphicφ†​ on a determinant (42); the one-body density matrix (43) and Wick's theorem (45); the transformation of vacuum and creators under eiλM^e^{i\lambda\hat M}eiλM^ (57), (59); the first-order variation (61)–(62). For the two-body Hamiltonian it adds the Fock-matrix form of the Brillouin condition (64), the Hartree-Fock energy, Koopmans' theorem (66) and the electron-hole excitation energy (67).

Significance

The Brillouin theorem turns the nonlinear variational problem over all Slater determinants into a condition on finitely many matrix elements; for a two-body Hamiltonian it says that the occupied–virtual block of the Fock matrix vanishes, which is the self-consistency condition solved by every Hartree-Fock code. Koopmans' theorem and the particle-hole formula give the physical interpretation of the orbital energies.

All results are classical and proved in the source and in standard textbooks. What this mission adds is a machine-checked account of second quantization on a finite orbital basis: the anticommutation relations, determinant overlaps and Wick's theorem for Slater determinants are reusable for any later formalization of configuration interaction, coupled cluster or BCS theory.

Difficulty

The source's arguments are short manipulations of operator identities, but each hides bookkeeping that is easy to get wrong: fermionic signs when operators are reordered, the identification of Slater determinants with ordered products of creators, and the Laplace expansion behind Wick's theorem. The variational step requires differentiating a matrix exponential on Fock space and identifying the derivative with a commutator. The direction from the Brillouin condition back to stationarity needs the hermiticity of H^\hat HH^ and a decomposition of an arbitrary hermitian MMM into occupied–occupied, virtual–virtual and occupied–virtual blocks; the first two blocks act on ∣Φ⟩|\Phi\rangle∣Φ⟩ only by a scalar. The Fock-matrix milestones additionally need the exchange symmetry Unn′,mm′=Un′n,m′mU_{nn',mm'}=U_{n'n,m'm}Unn′,mm′​=Un′n,m′m​ of two-body matrix elements stated in Sec. 2.3.2; without it the stated formulas fail.

Formalization scope

Fock space over KKK orbitals is represented concretely: vectors are functions on Finset (Fin K) and operators are complex matrices indexed by Finset (Fin K). Creators carry the sign (−1)#{j∈S: j>i}(-1)^{\#\{j\in S:\,j>i\}}(−1)#{j∈S:j>i}, so ordered products of creators of increasing orbitals give +∣S⟩+|S\rangle+∣S⟩. All quantities are complex; the exponential is NormedSpace.exp; stationarity is HasDerivAt … 0 0 for a function R→C\mathbb R\to\mathbb CR→C. Orthonormality of the occupied orbitals is an explicit hypothesis wherever the source assumes it. The source works with a possibly infinite orbital basis; here the basis is finite, as in the variational setting of its Sec. 3.

The equivalence in the goal cannot be satisfied vacuously: hermiticity of H^\hat HH^ and orthonormality of the orbitals are both satisfiable, and both sides quantify over all admissible MMM, respectively all occupied and virtual orbitals.

Two printed formulas are not taken verbatim: Eq. (60) lacks the minus sign in the exponent and is omitted, and Eq. (61) prints the first-order commutator in the opposite order; the milestone records the correct derivative i⟨Φ∣[M^,H^]∣Φ⟩i\langle\Phi|[\hat M,\hat H]|\Phi\ranglei⟨Φ∣[M^,H^]∣Φ⟩, which leaves (62) unchanged.

Contributions welcome: a general API for products of creation and annihilation operators in this model (sign lemmas, normal ordering), which all milestones share.

Selected references

  • E. Koch, Mean-Field Theory: Hartree-Fock and BCS, in E. Pavarini, E. Koch, J. van den Brink, G. Sawatzky (eds.), Quantum Materials: Experiments and Theory, Modeling and Simulation Vol. 6, Forschungszentrum Jülich, 2016. http://www.cond-mat.de/events/correl16
  • A. Szabo and N. S. Ostlund, Modern Quantum Chemistry: Introduction to Advanced Electronic Structure Theory, Dover, 1996.
  • T. Koopmans, Über die Zuordnung von Wellenfunktionen und Eigenwerten zu den einzelnen Elektronen eines Atoms, Physica 1 (1934) 104–113.
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Zeroth Law of Thermodynamics: Thermal Equilibrium and the Existence of TemperatureTextbook

Motivation

The zeroth law of thermodynamics is the principle that makes temperature a meaningful notion. In the formulation of Fowler and Guggenheim, and in the standard textbooks of Guggenheim, Buchdahl and Bailyn, it states: if two systems are both in thermal equilibrium with a third system, then they are in thermal equilibrium with each other. It was named by R. H. Fowler in the 1930s, after the first, second and third laws were already established, because it is logically prior to them: it is what justifies the use of thermometers and the assignment of a single "temperature" to each equilibrated system.

Mathematically, the content of the law is a statement about a binary relation. Together with the convention that each system is in equilibrium with itself, it turns thermal equilibrium into an equivalence relation, and an equivalence relation is exactly what is needed to "tag" every system with a label (an empirical temperature) so that two systems are in equilibrium precisely when their labels agree. This mission formalizes that chain of reasoning as presented in the Wikipedia article Zeroth law of thermodynamics.

Setting

Let SSS be a set (a type) whose elements are thermodynamic systems, each in its own state of internal equilibrium, and let TE\mathrm{TE}TE be a binary relation on SSS; TE(A,B)\mathrm{TE}(A,B)TE(A,B) reads "AAA is in thermal equilibrium with BBB". No further structure is assumed.

  • The zeroth law (right-Euclidean form) is the property
∀A,B,C∈S,TE(A,C) ∧ TE(B,C) ⟹ TE(A,B).\forall A,B,C\in S,\quad \mathrm{TE}(A,C)\ \wedge\ \mathrm{TE}(B,C)\ \Longrightarrow\ \mathrm{TE}(A,B).∀A,B,C∈S,TE(A,C) ∧ TE(B,C) ⟹ TE(A,B).
  • Planck's form (left-Euclidean form) is the property
∀A,B,C∈S,TE(C,A) ∧ TE(C,B) ⟹ TE(A,B).\forall A,B,C\in S,\quad \mathrm{TE}(C,A)\ \wedge\ \mathrm{TE}(C,B)\ \Longrightarrow\ \mathrm{TE}(A,B).∀A,B,C∈S,TE(C,A) ∧ TE(C,B) ⟹ TE(A,B).
  • Reflexivity is the convention TE(A,A)\mathrm{TE}(A,A)TE(A,A) for all AAA.
  • A map t:S→Tt : S\to Tt:S→T into any set TTT is an empirical temperature for TE\mathrm{TE}TE if
∀A,B∈S,TE(A,B)  ⟺  t(A)=t(B).\forall A,B\in S,\quad \mathrm{TE}(A,B)\iff t(A)=t(B).∀A,B∈S,TE(A,B)⟺t(A)=t(B).

Formalization targets

Goal: existence of temperature

(∀A, TE(A,A)) ∧ zeroth law ⟹ ∃ T, ∃ t:S→T, t is an empirical temperature for TE.\Big(\forall A,\ \mathrm{TE}(A,A)\Big)\ \wedge\ \text{zeroth law} \ \Longrightarrow\ \exists\,T,\ \exists\, t:S\to T,\ t \text{ is an empirical temperature for } \mathrm{TE}.(∀A, TE(A,A)) ∧ zeroth law ⟹ ∃T, ∃t:S→T, t is an empirical temperature for TE.

This is the "existence of temperature" postulate of Fowler and Guggenheim: the condition for thermal equilibrium is equality of a single-valued function of the state. The labelling set TTT is left arbitrary, as in the source ("the labeling may be quite arbitrary").

Milestones

  1. Reflexivity + zeroth law ⇒\Rightarrow⇒ TE\mathrm{TE}TE is an equivalence relation.
  2. Reflexivity + Planck's form ⇒\Rightarrow⇒ TE\mathrm{TE}TE is an equivalence relation.
  3. Under reflexivity, the zeroth law and Planck's form are equivalent.
  4. Consequence: symmetry of thermal equilibrium.
  5. Consequence: transitivity of thermal equilibrium.
  6. A reflexive, transitive relation need not be an equivalence relation.
  7. An equivalence relation partitions the systems into classes of mutual equilibrium.
  8. An equivalence relation admits an empirical-temperature tagging.

Significance

The result is the logical foundation of thermometry: it is what allows any one system to serve as a thermometer for all others, and it underlies every empirical temperature scale and, via the second law, the absolute scale. The statements here are elementary and are known; the value of the mission is a clean, reusable formal vocabulary for thermal equilibrium (the two Euclidean forms of the law and the notion of an empirical temperature) on which formalizations of later parts of axiomatic thermodynamics can build.

Difficulty

None of the steps is deep. The point that needs care is that the zeroth law alone does not give an equivalence relation: reflexivity is an additional convention, and the source stresses that a reflexive and transitive relation is not automatically symmetric. Each milestone therefore states its reflexivity hypothesis explicitly.

Formalization scope

Systems form an arbitrary type S (possibly empty), and thermal equilibrium is an arbitrary relation TE : S → S → Prop. Equivalence relations are Lean's Equivalence; partitions use Mathlib's Setoid.IsPartition. The labelling type of an empirical temperature lives in the same universe as S. The richer structure of real-valued temperature (ordering into "hotter" and "colder", continuity) is explicitly not part of the zeroth law according to the source and is out of scope. Definitions ZerothLaw, ZerothLawPlanck, IsEmpiricalTemperature are shared by all statements, in the namespace ZerothLawThermo.

Selected references

  • Wikipedia contributors, Zeroth law of thermodynamics, revision 1328026962. https://en.wikipedia.org/w/index.php?title=Zeroth_law_of_thermodynamics&oldid=1328026962
  • R. Fowler, E. A. Guggenheim, Statistical Thermodynamics, Cambridge University Press, 1939 (corrected 1965), p. 56.
  • E. H. Lieb, J. Yngvason, The physics and mathematics of the second law of thermodynamics, Physics Reports 310 (1999) 1–96. https://arxiv.org/abs/cond-mat/9708200
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Classical Conservation Laws: Momentum, Energy and MassTextbook

Motivation

The conservation of momentum, of mechanical energy and of mass are the three bookkeeping laws on which elementary Newtonian mechanics and continuum mechanics rest. In Newtonian mechanics each of them is not an extra postulate but a theorem: momentum conservation follows from Newton's second and third laws, conservation of mechanical energy follows from Newton's second law when the forces are derived from a potential, and conservation of total mass in a fluid follows from the continuity equation. This mission asks for machine-checked proofs of these classical derivations, in the form in which they appear in the encyclopedia articles Momentum, Conservation of energy and Conservation of mass.

Historically, Huygens (1669) listed both the total momentum and the total vis viva ∑imivi2\sum_i m_i v_i^2∑i​mi​vi2​ as invariants of collisions; Leibniz (1676–1689) promoted the vis viva; the distinction between elastic and inelastic collisions and the general principle of energy conservation were clarified only in the 19th century. Lomonosov (1756) and Lavoisier (1773) established conservation of mass in chemical reactions; its continuum form is the continuity equation of fluid dynamics.

Setting

All motion takes place in Euclidean space Rd\mathbb{R}^dRd (any dimension ddd; d=3d = 3d=3 is the physical case), with the standard inner product ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle⟨⋅,⋅⟩ and norm ∥⋅∥\|\cdot\|∥⋅∥.

  • A system of NNN particles has masses mi>0m_i > 0mi​>0, positions xi(t)x_i(t)xi​(t), velocities vi(t)=x˙i(t)v_i(t) = \dot x_i(t)vi​(t)=x˙i​(t) and accelerations ai(t)=v˙i(t)a_i(t) = \dot v_i(t)ai​(t)=v˙i​(t), for i=1,…,Ni = 1,\dots,Ni=1,…,N and all times t∈Rt \in \mathbb{R}t∈R.
  • Newton's second law: miai(t)m_i a_i(t)mi​ai​(t) equals the net force on particle iii.
  • Newton's third law for internal forces: the force FijF_{ij}Fij​ exerted on iii by jjj satisfies Fij=−FjiF_{ij} = -F_{ji}Fij​=−Fji​.
  • The total momentum is P(t)=∑imivi(t)P(t) = \sum_i m_i v_i(t)P(t)=∑i​mi​vi​(t), the centre of mass is R(t)=M−1∑imixi(t)R(t) = M^{-1}\sum_i m_i x_i(t)R(t)=M−1∑i​mi​xi​(t) with M=∑imiM = \sum_i m_iM=∑i​mi​, the kinetic energy is ∑i12mi∥vi∥2\sum_i \tfrac12 m_i \|v_i\|^2∑i​21​mi​∥vi​∥2.
  • A pair potential is a function φij=φji\varphi_{ij} = \varphi_{ji}φij​=φji​ of the distance rij=∥xi−xj∥r_{ij} = \|x_i - x_j\|rij​=∥xi​−xj​∥; the force it produces on iii is −φij′(rij) (xi−xj)/rij-\varphi_{ij}'(r_{ij})\,(x_i - x_j)/r_{ij}−φij′​(rij​)(xi​−xj​)/rij​ (e.g. gravity, φij(r)=−Gmimj/r\varphi_{ij}(r) = -G m_i m_j / rφij​(r)=−Gmi​mj​/r).
  • A fluid has density ρ(t,x)\rho(t,x)ρ(t,x) and velocity field u(t,x)u(t,x)u(t,x); the continuity equation is ∂tρ+∇⋅(ρu)=0\partial_t \rho + \nabla\cdot(\rho u) = 0∂t​ρ+∇⋅(ρu)=0, and the total mass is ∫Rnρ(t,x) dx\int_{\mathbb{R}^n} \rho(t,x)\,dx∫Rn​ρ(t,x)dx.

Target

The goal theorem is the conservation of both total momentum and total mechanical energy for an isolated NNN-body system interacting through symmetric pair potentials, along any collision-free trajectory:

P(t)=P(s),∑i12mi∥vi(t)∥2+∑i<jφij(∥xi(t)−xj(t)∥)=the same expression at s.P(t) = P(s), \qquad \sum_i \tfrac12 m_i\|v_i(t)\|^2 + \sum_{i<j}\varphi_{ij}\big(\|x_i(t)-x_j(t)\|\big) = \text{the same expression at } s.P(t)=P(s),i∑​21​mi​∥vi​(t)∥2+i<j∑​φij​(∥xi​(t)−xj​(t)∥)=the same expression at s.

Milestones:

  1. Conservation of momentum under Newton's third law (any internal forces).
  2. Uniform rectilinear motion of the centre of mass, with velocity P/MP/MP/M.
  3. Conservation of mechanical energy for a particle in a conservative force field F=−∇VF = -\nabla VF=−∇V.
  4. The work–energy theorem: change in kinetic energy equals the work ∫⟨F,v⟩ dt\int \langle F, v\rangle\,dt∫⟨F,v⟩dt.
  5. Head-on elastic collision of two bodies: the final velocities are either the initial ones or the classical formulas.
  6. Perfectly inelastic collision: common final velocity and the kinetic energy lost, 12mAmBmA+mB(uA−uB)2\tfrac12\frac{m_A m_B}{m_A+m_B}(u_A-u_B)^221​mA​+mB​mA​mB​​(uA​−uB​)2.
  7. Conservation of total mass for a compactly supported C1C^1C1 solution of the continuity equation.

Significance

These are the textbook consequences of Newton's laws used throughout mechanics, astronomy and engineering: momentum conservation determines the outcome of collisions and explosions, energy conservation gives first integrals that reduce equations of motion, and mass conservation is the first of the Euler equations of fluid dynamics. The results themselves are classical and fully known; the work in this mission is formalization. The platform already contains specialised instances (for example a two-body centre-of-mass statement and energy conservation in the Kepler problem); this mission states the general NNN-body, arbitrary-dimension versions and the continuum mass law, which can be reused by later mechanics missions.

Difficulty

The algebraic milestones (collisions) are elementary. The analytic ones require care: energy conservation needs the chain rule for V∘xV \circ xV∘x and for the norm ∥xi−xj∥\|x_i - x_j\|∥xi​−xj​∥, which is differentiable only away from collisions; the work–energy theorem needs the fundamental theorem of calculus for a continuous integrand; mass conservation needs differentiation under the integral sign and the vanishing of the integral of the divergence of a compactly supported C1C^1C1 vector field, a form of the divergence theorem that must be assembled from one-dimensional integration by parts.

Formalization scope

  • Space is EuclideanSpace ℝ (Fin d); time is ℝ; trajectories are defined for all times, and derivatives are given explicitly through HasDerivAt hypotheses (x˙i=vi\dot x_i = v_ix˙i​=vi​, v˙i=ai\dot v_i = a_iv˙i​=ai​) rather than through deriv.
  • Masses are strictly positive. The NNN-body goal assumes that no two particles ever coincide (collision-free trajectory), so that the pair forces are defined; pair potentials are only required to be differentiable on (0,∞)(0,\infty)(0,∞).
  • No definitions are introduced; every quantity is written out explicitly in each statement.
  • In milestone 5 the trivial outcome (velocities unchanged) is kept as an explicit alternative instead of being excluded by a hypothesis, so the statement is never vacuous.
  • In milestone 7 the continuity equation is written with partial derivatives deriv / fderiv, the density and the velocity field are jointly C1C^1C1 in (t,x)(t,x)(t,x), and the density vanishes outside a fixed ball for all times. The integral is the Lebesgue integral on Rn\mathbb{R}^nRn.

Selected references

  • Wikipedia, Momentum, sections "Many particles", "Conservation", "Application to collisions" — https://en.wikipedia.org/wiki/Momentum
  • Wikipedia, Conservation of energy — https://en.wikipedia.org/wiki/Conservation_of_energy
  • Wikipedia, Conservation of mass, section "Formulation and examples" — https://en.wikipedia.org/wiki/Conservation_of_mass
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One Hundred Years of the Cosmological Constant: the EquationsResearch Paper

Motivation

The cosmological constant Λ\LambdaΛ was added by Einstein in 1917 to the field equations of general relativity so that a static, matter-filled, spatially closed universe would be a solution. It was sidelined after the discovery of cosmic expansion, invoked repeatedly for specific puzzles, and returned to the centre of cosmology after the supernova observations of 1998 showed that the expansion of the universe is accelerating. The centennial review of O'Raifeartaigh, O'Keeffe, Nahm and Mitton (EPJ H 43 (2018) 73) traces this history. Along the way it states, in numbered equations, the small body of mathematics on which the whole story rests: Seeliger's modified Poisson equation, Einstein's static universe, de Sitter's empty universe, Friedman's evolution equations, the Einstein–de Sitter model and critical density, and the deceleration parameter that links Λ\LambdaΛ to an accelerating universe.

Timeline of the results formalized here, as presented in the review:

  • 1895–1896 (Seeliger). For an infinite space uniformly filled with matter the Newtonian potential is indeterminate; Seeliger replaces the Poisson equation (3) by ∇2Φ−λΦ=4πGρ\nabla^2\Phi-\lambda\Phi=4\pi G\rho∇2Φ−λΦ=4πGρ (4).
  • 1917 (Einstein). The modified field equations (9) admit a static closed universe with λ=κρ/2=1/R2\lambda=\kappa\rho/2=1/R^2λ=κρ/2=1/R2 (10). The Newtonian limit of (9) is ∇2ϕ+c2λ=4πGρ\nabla^2\phi+c^2\lambda=4\pi G\rho∇2ϕ+c2λ=4πGρ (11), not Seeliger's (4).
  • 1917 (de Sitter). An empty solution with ρ=0\rho=0ρ=0, λ=3/R2\lambda=3/R^2λ=3/R2 (13); later written by Lemaître with an exponential line element (14).
  • 1922 (Friedman). Non-static solutions governed by (15)–(16), with the first integral (17).
  • 1930 (Eddington). The Einstein world is unstable against perturbations.
  • 1932 (Einstein–de Sitter). With λ=0\lambda=0λ=0 and flat space, (R′/R)2=κρc2/3(R'/R)^2=\kappa\rho c^2/3(R′/R)2=κρc2/3 (18); the critical density ρc=3H2/8πG\rho_c=3H^2/8\pi Gρc​=3H2/8πG classifies the spatial geometry; the expansion age is t=2/(3H0)t=2/(3H_0)t=2/(3H0​).
  • 1950s (Robertson; Hoyle–Sandage). The deceleration parameter q0q_0q0​, with q0=ΩM/2q_0=\Omega_M/2q0​=ΩM​/2 (28) without λ\lambdaλ and q0=ΩM/2−Ωλq_0=\Omega_M/2-\Omega_\lambdaq0​=ΩM​/2−Ωλ​ (29) in general.

Setting

Time is a real variable ttt. A homogeneous universe is described by a positive scale factor (radius) R(t)R(t)R(t) and a mean matter density ρ(t)\rho(t)ρ(t). The constants are Newton's constant GGG, the speed of light ccc, Einstein's constant κ=8πG/c2\kappa=8\pi G/c^2κ=8πG/c2, the cosmological constant Λ\LambdaΛ (the review's λ\lambdaλ) and a curvature index kkk (k=1k=1k=1 closed, k=0k=0k=0 flat, k=−1k=-1k=−1 open). The pair (R,ρ)(R,\rho)(R,ρ) is a Friedmann–Lemaître dust solution on a set of times III if R>0R>0R>0 is C2C^2C2 near each t∈It\in It∈I and

3R′2R2+3kc2R2−Λ=κc2ρ,R′2R2+2R′′R+kc2R2−Λ=0.\frac{3R'^2}{R^2}+\frac{3kc^2}{R^2}-\Lambda=\kappa c^2\rho,\qquad \frac{R'^2}{R^2}+\frac{2R''}{R}+\frac{kc^2}{R^2}-\Lambda=0 .R23R′2​+R23kc2​−Λ=κc2ρ,R2R′2​+R2R′′​+R2kc2​−Λ=0.

For k=1k=1k=1 these are exactly the review's equations (15)–(16). The Hubble parameter is H=R′/RH=R'/RH=R′/R, the deceleration parameter is q=−(1/H2)(R′′/R)q=-(1/H^2)(R''/R)q=−(1/H2)(R′′/R) (eq. 26), the critical density is ρc=3H2/(8πG)\rho_c=3H^2/(8\pi G)ρc​=3H2/(8πG), and the density parameters are ΩM=ρ/ρc\Omega_M=\rho/\rho_cΩM​=ρ/ρc​ and ΩΛ=Λ/(3H2)\Omega_\Lambda=\Lambda/(3H^2)ΩΛ​=Λ/(3H2) (Section 5.1). For the Newtonian part, ∇2\nabla^2∇2 is the Laplacian on R3\mathbb R^3R3.

Formalization targets

Goal: the deceleration parameter and cosmic acceleration (eqs. 25–29)

For every Friedmann–Lemaître dust solution, at every time with R′≠0R'\neq0R′=0,

q=12 ΩM−ΩΛ,q=\tfrac12\,\Omega_M-\Omega_\Lambda ,q=21​ΩM​−ΩΛ​,

and if the expansion is accelerating (R′′>0R''>0R′′>0) while the density is non-negative, then Λ>0\Lambda>0Λ>0. This is the statement through which accelerated expansion forces a positive cosmological constant, which the review's title points to.

Milestones (in the review's order)

Seeliger's no-bounded-potential paradox for (3) and the unique bounded solution of (4); Einstein's static universe (10); the bounded-potential criterion for the Newtonian limit (11); Eddington's instability of the Einstein world; de Sitter's solution B (13); Lemaître's exponential form (14); Friedman's first integral (17); the critical-density classification of curvature; recollapse of supercritical universes without Λ\LambdaΛ; the Einstein–de Sitter age t=2/(3H)t=2/(3H)t=2/(3H); and the matter-only deceleration law (25)–(28).

Significance

The goal is the formula used to read the sign of Λ\LambdaΛ off measurements of q0q_0q0​; it underlies the review's account of how the supernova data of 1998–1999 were interpreted as evidence for a positive cosmological constant. The milestones are the classical facts about Λ\LambdaΛ that the review uses to explain each episode of its history: why Seeliger and Einstein needed a decay or cosmological term, why the static universe was abandoned, and how matter density, curvature and expansion rate are related. All of them are established results; the work in this mission is to formalize them faithfully in the review's own notation. Several related Friedmann-equation statements exist on the platform in other conventions; this mission keeps the review's equations verbatim, in particular with explicit ccc and κ\kappaκ.

Difficulty

The algebraic statements (goal, static universe, de Sitter, classification) reduce to manipulations of the two equations, but they need care with derivatives and with the conventions κc2=8πG\kappa c^2=8\pi Gκc2=8πG. The analytic milestones are harder. Seeliger's statements require a Liouville-type theorem for bounded solutions of ∇2Φ=const\nabla^2\Phi=\text{const}∇2Φ=const and of ∇2Φ−λΦ=const\nabla^2\Phi-\lambda\Phi=\text{const}∇2Φ−λΦ=const on all of R3\mathbb R^3R3; such results are not readily available. Eddington's instability requires producing genuine nearby solutions of a nonlinear ODE system that leave a neighbourhood of the static state, not only a linearized computation. The recollapse and age statements need global arguments over an unbounded time interval.

Formalization scope

All quantities are real numbers. The Friedmann–Lemaître predicate quantifies over a time set III; theorems specify III (all of R\mathbb RR, a closed interval [0,T][0,T][0,T], a half-line, or a preconnected set). Derivatives are Lean's deriv; differentiability is enforced by requiring RRR to be C2C^2C2 near each time of III, so no junk derivative values enter. Division by zero is excluded explicitly where it matters (for instance R′≠0R'\neq0R′=0 in the goal, so that H≠0H\neq0H=0). The Laplacian is defined from scratch as the sum of the three second partial derivatives on Euclidean three-space. Pressure is zero throughout (dust), as in the review's equations (15)–(16). The review often sets c=1c=1c=1 (eqs. 10, 13); the formal statements keep ccc explicit, which reduces to the review's formulas at c=1c=1c=1. Contributions of general-purpose lemmas (Liouville theorems, ODE instability criteria) are welcome.

Selected references

  • C. O'Raifeartaigh, M. O'Keeffe, W. Nahm, S. Mitton, One hundred years of the cosmological constant: from "superfluous stunt" to dark energy, Eur. Phys. J. H 43, 73–117, 2018. https://doi.org/10.1140/epjh/e2017-80061-7
  • A. Einstein, Kosmologische Betrachtungen zur allgemeinen Relativitätstheorie, Sitzungsber. Preuss. Akad. Wiss., 142–152, 1917.
  • A. Friedman, Über die Krümmung des Raumes, Z. Phys. 10, 377–386, 1922. https://doi.org/10.1007/BF01332580
  • A. S. Eddington, On the instability of Einstein's spherical world, MNRAS 90, 668–678, 1930. https://doi.org/10.1093/mnras/90.7.668
  • A. Einstein, W. de Sitter, On the relation between the expansion and the mean density of the universe, PNAS 18, 213–214, 1932. https://doi.org/10.1073/pnas.18.3.213
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Weinberg 1967: A Model of Leptons — tree-level electroweak boson spectrumResearch Paper

Motivation

In A Model of Leptons (Weinberg, Phys. Rev. Lett. 19, 1264 (1967)) Steven Weinberg proposed that the photon and the intermediate bosons of the weak interaction are gauge fields of a single symmetry group, SU(2)×U(1)SU(2)\times U(1)SU(2)×U(1), and that the visible differences between them — the photon is massless, the weak bosons are heavy, and their couplings differ — come from a spontaneously broken symmetry of the vacuum rather than of the Lagrangian. The Goldstone bosons that such a breaking would normally produce are removed by the gauge fields (the Higgs–Englert–Brout–Guralnik–Hagen–Kibble mechanism). This model became the leptonic sector of the Standard Model of particle physics.

The paper is three pages long and its quantitative content is a short chain of finite-dimensional algebra: after the scalar field is replaced by its vacuum value, the gauge-boson mass terms form a quadratic form whose diagonalization gives the charged boson WWW, the neutral boson ZZZ and the massless photon, together with formulas for their masses, for the electric charge and for the weak coupling constant. This mission formalizes that chain.

Setting

The model has two gauge couplings ggg (for the isospin fields A⃗μ=(Aμ1,Aμ2,Aμ3)\vec A_\mu=(A^1_\mu,A^2_\mu,A^3_\mu)Aμ​=(Aμ1​,Aμ2​,Aμ3​)) and g′g'g′ (for the hypercharge field BμB_\muBμ​), and a complex scalar doublet φ\varphiφ whose vacuum expectation value is ⟨φ⟩=λ(10)\langle\varphi\rangle=\lambda\binom10⟨φ⟩=λ(01​) with λ\lambdaλ real. Replacing φ\varphiφ by ⟨φ⟩\langle\varphi\rangle⟨φ⟩ in the Lagrangian (eq. (4) of the paper) leaves the spin-one mass terms (eq. (7))

−18λ2g2[(Aμ1)2+(Aμ2)2]−18λ2(gAμ3+g′Bμ)2.-\tfrac18\lambda^2g^2\big[(A^1_\mu)^2+(A^2_\mu)^2\big]-\tfrac18\lambda^2\big(gA^3_\mu+g'B_\mu\big)^2 .−81​λ2g2[(Aμ1​)2+(Aμ2​)2]−81​λ2(gAμ3​+g′Bμ​)2.

At a fixed spacetime point we write the gauge fields as a vector V=(A1,A2,A3,B)∈R4V=(A^1,A^2,A^3,B)\in\mathbb R^4V=(A1,A2,A3,B)∈R4. The mass terms are then −12VTMV-\tfrac12V^{\mathsf T}\mathcal MV−21​VTMV for the symmetric mass-squared matrix

M=λ24(g20000g20000g2gg′00gg′g′2).\mathcal M=\frac{\lambda^2}{4}\begin{pmatrix}g^2&0&0&0\\0&g^2&0&0\\0&0&g^2&gg'\\0&0&gg'&g'^2\end{pmatrix}.M=4λ2​​g2000​0g200​00g2gg′​00gg′g′2​​.

A field of definite mass mmm is a linear combination c⋅Vc\cdot Vc⋅V whose coefficient vector ccc satisfies Mc=m2c\mathcal Mc=m^2cMc=m2c. The paper's candidates are

W=2−1/2(A1+iA2),Z=gA3+g′B(g2+g′2)1/2,A=−g′A3+gB(g2+g′2)1/2,W=2^{-1/2}(A^1+iA^2),\quad Z=\frac{gA^3+g'B}{(g^2+g'^2)^{1/2}},\quad A=\frac{-g'A^3+gB}{(g^2+g'^2)^{1/2}},W=2−1/2(A1+iA2),Z=(g2+g′2)1/2gA3+g′B​,A=(g2+g′2)1/2−g′A3+gB​,

with masses MW=12λgM_W=\tfrac12\lambda gMW​=21​λg, MZ=12λ(g2+g′2)1/2M_Z=\tfrac12\lambda(g^2+g'^2)^{1/2}MZ​=21​λ(g2+g′2)1/2, MA=0M_A=0MA​=0. The rationalized electric charge is e=gg′/(g2+g′2)1/2e=gg'/(g^2+g'^2)^{1/2}e=gg′/(g2+g′2)1/2, and the weak coupling constant GWG_WGW​ is defined by GW/2=g2/8MW2G_W/\sqrt2=g^2/8M_W^2GW​/2​=g2/8MW2​. The electron gets the mass Me=λGeM_e=\lambda G_eMe​=λGe​ from its Yukawa coupling GeG_eGe​. The electric charge in the paper's conventions is Q=T3−YQ=T_3-YQ=T3​−Y, where T3T_3T3​ is the third isospin component and Y=NR+12NLY=N_R+\tfrac12N_LY=NR​+21​NL​ the hypercharge.

Target

The goal theorem states, for g2+g′2>0g^2+g'^2>0g2+g′2>0:

Mw=MW2w,Mz=MZ2z,Ma=0,z⋅z=a⋅a=1, z⋅a=0,\mathcal Mw=M_W^2w,\qquad \mathcal Mz=M_Z^2z,\qquad \mathcal Ma=0,\qquad z\cdot z=a\cdot a=1,\ z\cdot a=0,Mw=MW2​w,Mz=MZ2​z,Ma=0,z⋅z=a⋅a=1, z⋅a=0,

where w,z,aw,z,aw,z,a are the coefficient vectors of W,Z,AW,Z,AW,Z,A, and, for all T3,YT_3,YT3​,Y and all field values,

gT3A3+g′YB=−e (T3−Y) A+g2T3+g′2Y(g2+g′2)1/2 Z,gT_3A^3+g'YB=-e\,(T_3-Y)\,A+\frac{g^2T_3+g'^2Y}{(g^2+g'^2)^{1/2}}\,Z,gT3​A3+g′YB=−e(T3​−Y)A+(g2+g′2)1/2g2T3​+g′2Y​Z,

so the massless field is the photon and it couples to Q=T3−YQ=T_3-YQ=T3​−Y with strength eee.

The milestones follow the paper's numbered equations: eq. (7) as a quadratic form; eqs. (8)–(9) (WWW and MWM_WMW​); eqs. (10), (12) (ZZZ and MZM_ZMZ​); eqs. (11), (13) (photon massless); the orthonormality of (10)–(11); eq. (15) (the charge); eq. (16) (GW/2=g2/8MW2=1/2λ2G_W/\sqrt2=g^2/8M_W^2=1/2\lambda^2GW​/2​=g2/8MW2​=1/2λ2); Ge=Me/λ=21/4MeGW1/2G_e=M_e/\lambda=2^{1/4}M_eG_W^{1/2}Ge​=Me​/λ=21/4Me​GW1/2​; g,g′>eg,g'>eg,g′>e; the parameter-free forms of the bounds MW>40M_W>40MW​>40 BeV, MZ>MWM_Z>M_WMZ​>MW​, MZ>80M_Z>80MZ​>80 BeV; and the tree-level vacuum condition λ2=M12/2h\lambda^2=M_1^2/2hλ2=M12​/2h.

Significance

The result itself. These formulas are the tree-level predictions that made the model testable: a massless photon, a charged WWW and a neutral ZZZ with MZ>MWM_Z>M_WMZ​>MW​, and the relations tying eee, GWG_WGW​, MWM_WMW​ and MZM_ZMZ​ to g,g′,λg,g',\lambdag,g′,λ. The existence of the neutral boson ZZZ (and its neutral currents) was the model's new prediction, later confirmed experimentally.

Formalizing it. The results are classical and fully proved on paper. The mission produces a machine-checked record of the paper's algebra, with every hypothesis stated (for example, that ggg and g′g'g′ are not both zero), and a reusable encoding of the electroweak boson mass matrix.

Difficulty

The mathematics is elementary; the difficulty lies in faithfulness. The paper's sign conventions are not fully consistent (substituting the vacuum value into eq. (4) as printed gives gA3−g′BgA^3-g'BgA3−g′B in the second mass term, while eq. (7) prints gA3+g′BgA^3+g'BgA3+g′B, which is the combination consistent with eq. (10)). The numerical claims (40 BeV, 80 BeV, 2.07×10−62.07\times10^{-6}2.07×10−6) depend on experimental inputs and on rounding. The formalization therefore takes eq. (7) as printed as its starting point and states the bounds in parameter-free form.

Formalization scope

  • Gauge-field configurations are vectors in R4\mathbb R^4R4 in the order (A1,A2,A3,B)(A^1,A^2,A^3,B)(A1,A2,A3,B); WWW uses C4\mathbb C^4C4. The mass matrix is given entrywise, and milestone eq. (7) connects it to the printed mass term.
  • The hypothesis g2+g′2>0g^2+g'^2>0g2+g′2>0 is imposed wherever ZZZ, AAA or eee must be nondegenerate: in Lean, division by zero returns 000, so for g=g′=0g=g'=0g=g′=0 these objects would silently be 000. Similarly GW=0G_W=0GW​=0 when λg=0\lambda g=0λg=0, so eq. (16) assumes g,λ≠0g,\lambda\neq0g,λ=0.
  • MWM_WMW​ and MZM_ZMZ​ are signed (12λg\tfrac12\lambda g21​λg without absolute value); mass statements are about squares.
  • Only stationarity is formalized for the vacuum condition, not the scalar masses. The Fierz-transformed eee–ν\nuν interaction and the fermion couplings of eq. (14) beyond the charge are not formalized.
  • All objects live in a single definition file, WeinbergLeptons_Model, in namespace WeinbergLeptons.

Selected references

  • S. Weinberg, A Model of Leptons, Phys. Rev. Lett. 19, 1264–1266 (1967). doi:10.1103/PhysRevLett.19.1264
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Celestial w_{1+∞} wedge algebra and gluon S-algebra (Zhu review, §7.1)Research Paper

Motivation

In celestial holography, scattering amplitudes of massless particles in four-dimensional flat spacetime are rewritten, by a Mellin transform in the particle energies, as correlation functions of operators on the two-dimensional celestial sphere. Soft theorems then become Ward identities of two-dimensional currents. Guevara, Himwich, Pate and Strominger (arXiv:2103.03961) found that the conformally soft graviton modes obtained this way close under the collinear OPE into an infinite-dimensional algebra, and Strominger (arXiv:2105.14346) identified it, after a rescaling, with the wedge subalgebra of w1+∞w_{1+\infty}w1+∞​, the Lie algebra of polynomial area-preserving (Hamiltonian) vector fields on a two-plane. The review of B. Zhu (arXiv:2606.24285, Section 7.1) summarises this derivation, together with its gauge-theory counterpart, the gluon SSS-algebra, and the action of w1+∞w_{1+\infty}w1+∞​ on it. The review describes the celestial www-algebra as a consistency test for any proposed flat-space hologram.

Setting

The wedge range is the set of labels (p,m)(p,m)(p,m) with

p∈{1,32,2,52,… },1−p≤m≤p−1,p−1−m∈Z,p\in\{1,\tfrac32,2,\tfrac52,\dots\},\qquad 1-p\le m\le p-1,\qquad p-1-m\in\mathbb Z,p∈{1,23​,2,25​,…},1−p≤m≤p−1,p−1−m∈Z,

equivalently: p+m−1p+m-1p+m−1 and p−m−1p-m-1p−m−1 are both natural numbers. Let WWW be the complex vector space with basis {wmp}\{w^p_m\}{wmp​} indexed by the wedge range, and define a bilinear bracket on WWW by Eq. (7.8),

[wmp,wnq]=(m(q−1)−n(p−1)) wm+np+q−2,[w^p_m,w^q_n]=\bigl(m(q-1)-n(p-1)\bigr)\,w^{p+q-2}_{m+n},[wmp​,wnq​]=(m(q−1)−n(p−1))wm+np+q−2​,

where the right-hand side is 000 whenever (p+q−2,m+n)(p+q-2,m+n)(p+q−2,m+n) falls outside the wedge.

Eq. (7.9) realises wmpw^p_mwmp​ as the monomial up+m−1vp−m−1u^{p+m-1}v^{p-m-1}up+m−1vp−m−1 in the polynomial ring C[u,v]\mathbb C[u,v]C[u,v], equipped with the Poisson bracket {f,g}=∂uf ∂vg−∂vf ∂ug\{f,g\}=\partial_uf\,\partial_vg-\partial_vf\,\partial_ug{f,g}=∂u​f∂v​g−∂v​f∂u​g.

The conformally soft graviton modes HmkH^k_mHmk​ (k=2,1,0,−1,…k=2,1,0,-1,\dotsk=2,1,0,−1,…, k−22≤m≤2−k2\tfrac{k-2}{2}\le m\le\tfrac{2-k}{2}2k−2​≤m≤22−k​) obey the commutator (7.5) with factorial coefficients and the gravitational coupling κ\kappaκ. The rescaling (7.6), wmp=1κ(p−m−1)!(p+m−1)! Hm−2p+4w^p_m=\tfrac1\kappa(p-m-1)!(p+m-1)!\,H^{-2p+4}_mwmp​=κ1​(p−m−1)!(p+m−1)!Hm−2p+4​, turns (7.5) into (7.8).

On the gauge-theory side, with colour index aaa and Lie-algebra structure constants fabcf^{ab}{}_cfabc​, the conformally soft gluon modes Rnk,aR^{k,a}_nRnk,a​ obey (7.14). The rescaling (7.15), Smq,a=(q−m−1)!(q+m−1)! Rm3−2q,aS^{q,a}_m=(q-m-1)!(q+m-1)!\,R^{3-2q,a}_mSmq,a​=(q−m−1)!(q+m−1)!Rm3−2q,a​, gives the SSS-algebra (7.16), [Smp,a,Snq,b]=−ifabcSm+np+q−1,c[S^{p,a}_m,S^{q,b}_n]=-if^{ab}{}_cS^{p+q-1,c}_{m+n}[Smp,a​,Snq,b​]=−ifabc​Sm+np+q−1,c​. The wedge algebra acts on it by (7.17), [wmp,Snq,a]=(m(q−1)−n(p−1))Sm+np+q−2,a[w^p_m,S^{q,a}_n]=\bigl(m(q-1)-n(p-1)\bigr)S^{p+q-2,a}_{m+n}[wmp​,Snq,a​]=(m(q−1)−n(p−1))Sm+np+q−2,a​.

Formalization targets

Goal: (7.8) is a Lie bracket

[X,X]=0,[X,[Y,Z]]=[[X,Y],Z]+[Y,[X,Z]]for all X,Y,Z∈W.[X,X]=0,\qquad [X,[Y,Z]]=[[X,Y],Z]+[Y,[X,Z]]\qquad\text{for all }X,Y,Z\in W.[X,X]=0,[X,[Y,Z]]=[[X,Y],Z]+[Y,[X,Z]]for all X,Y,Z∈W.

Milestones

  1. Closure of the wedge (7.7)–(7.8): if (p,m)(p,m)(p,m) and (q,n)(q,n)(q,n) are in the wedge and m(q−1)−n(p−1)≠0m(q-1)-n(p-1)\ne0m(q−1)−n(p−1)=0, then (p+q−2,m+n)(p+q-2,m+n)(p+q−2,m+n) is in the wedge.
  2. Rescaling (7.5) ⇒\Rightarrow⇒ (7.8): any family HmkH^k_mHmk​ satisfying (7.5) in a complex vector space with a bilinear bracket, rescaled by (7.6), satisfies (7.8) (for κ≠0\kappa\neq 0κ=0).
  3. Poisson realisation on generators (7.9): {up+m−1vp−m−1,uq+n−1vq−n−1}=2(m(q−1)−n(p−1))up+q+m+n−3vp+q−m−n−3\{u^{p+m-1}v^{p-m-1},u^{q+n-1}v^{q-n-1}\}=2\bigl(m(q-1)-n(p-1)\bigr)u^{p+q+m+n-3}v^{p+q-m-n-3}{up+m−1vp−m−1,uq+n−1vq−n−1}=2(m(q−1)−n(p−1))up+q+m+n−3vp+q−m−n−3. The review's "convention-dependent overall factor" is pinned to 222.
  4. Poisson realisation, linear form (7.9): the linear map wmp↦up+m−1vp−m−1w^p_m\mapsto u^{p+m-1}v^{p-m-1}wmp​↦up+m−1vp−m−1 intertwines (7.8) with 12{⋅,⋅}\tfrac12\{\cdot,\cdot\}21​{⋅,⋅}.
  5. Gluon rescaling (7.14) ⇒\Rightarrow⇒ (7.16).
  6. The SSS-algebra is a Lie algebra (7.16), given that fabcf^{ab}{}_cfabc​ are Lie structure constants.
  7. SSS is a w1+∞w_{1+\infty}w1+∞​-module (7.17): [[X,Y],s]=[X,[Y,s]]−[Y,[X,s]][[X,Y],s]=[X,[Y,s]]-[Y,[X,s]][[X,Y],s]=[X,[Y,s]]−[Y,[X,s]].

Significance

The statements fix, in a machine-checked form, the precise normalisations used in the celestial literature: the wedge range, the rescalings (7.6) and (7.15), and the overall factor in the Poisson realisation, which the review leaves convention-dependent. They form the algebraic base layer for later formalisations of deformations of w1+∞w_{1+\infty}w1+∞​, its loop algebra Lw1+∞Lw_{1+\infty}Lw1+∞​, and the gluon–graviton soft algebras. The results themselves are established in the physics literature. The formal work that remains is the combinatorics of the factorial coefficients, the closure of the finite wedge range, and the Jacobi identities.

Difficulty

None of the statements is deep, but each carries bookkeeping that is easy to get wrong. The factorial coefficients of (7.5) and (7.14) must cancel exactly against the rescalings. At the corners of the wedge (m=p−1m=p-1m=p−1, n=q−1n=q-1n=q−1, or p+q−2<1p+q-2<1p+q−2<1) the target label leaves the wedge, and the structure constant must be shown to vanish there. The Jacobi identity for (7.8) does not follow term by term from the formula; the natural route is through the Poisson realisation, which must first be shown to be faithful.

Formalization scope

All objects are over C\mathbb CC. Labels p,m,q,n,k,lp,m,q,n,k,lp,m,q,n,k,l are rationals, and every label set is carved out by the predicate "p+m−1p+m-1p+m−1 and p−m−1p-m-1p−m−1 are natural numbers". Vector spaces with a given basis are finitely supported functions on the index set, and brackets are the bilinear extensions of the basis formulas. When the target label of a bracket falls outside the wedge, the bracket is defined to be 000 (milestone 1 shows this only happens when the structure constant already vanishes). Factorials of rational arguments are taken of the truncation ⌊⋅⌋+\lfloor\cdot\rfloor_+⌊⋅⌋+​ to a natural number; on the relevant ranges the arguments are natural numbers, and at the single corner where (7.5) has argument −1-1−1 its prefactor vanishes. The operator-level identities (milestones 2 and 5) are stated for an arbitrary complex vector space with an arbitrary bilinear bracket, taking (7.5) resp. (7.14) as hypotheses on the given modes. The colour algebra is given by structure constants f:ι3→Cf:\iota^3\to\mathbb Cf:ι3→C on a finite index set ι\iotaι, with antisymmetry and the Jacobi identity as the definition of Lie structure constants. The factor κ−1\kappa^{-1}κ−1 uses the convention 0−1=00^{-1}=00−1=0, and milestone 2 assumes κ≠0\kappa\ne0κ=0.

Selected references

  • B. Zhu, Topics in Celestial holography: A bottom-up perspective, invited review for Physics Reports, arXiv:2606.24285v3, 2026. https://arxiv.org/abs/2606.24285 (Section 7.1, Eqs. (7.1)–(7.17)).
  • A. Guevara, E. Himwich, M. Pate, A. Strominger, Holographic symmetry algebras for gauge theory and gravity, JHEP 2021. https://arxiv.org/abs/2103.03961
  • A. Strominger, w1+∞w_{1+\infty}w1+∞​ and the celestial sphere, Phys. Rev. Lett. 2021. https://arxiv.org/abs/2105.14346
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The new Minimal Standard ModelResearch Paper

Motivation

The Minimal Standard Model (MSM) — the SU(3)C×SU(2)L×U(1)YSU(3)_C\times SU(2)_L\times U(1)_YSU(3)C​×SU(2)L​×U(1)Y​ gauge theory with three generations of quarks and leptons, one Higgs doublet and classical gravity — accounts for almost all laboratory phenomena, but it does not accommodate several empirical facts established since the late 1990s: non-baryonic dark matter, dark energy, neutrino masses and mixings, the baryon asymmetry of the universe, and nearly scale-invariant, adiabatic, Gaussian density fluctuations. Davoudiasl, Kitano, Li and Murayama (Phys. Lett. B 609 (2005) 117) propose the new Minimal Standard Model (NMSM): the most general renormalizable Lagrangian obtained by adding the minimal particle content needed for these facts — two right-handed Majorana neutrinos N1,N2N_1, N_2N1​,N2​, one Z2\mathbb Z_2Z2​-odd real singlet scalar SSS (dark matter), one real scalar φ\varphiφ (the inflaton), and a cosmological constant — six new degrees of freedom in total.

Most of the paper's claims are phenomenological (relic abundance, the Higgs-mass window from one-loop running, direct-detection rates). A smaller set are exact mathematical consequences of the model's structure, and this mission collects those.

Setting

Neutrino sector (Eq. (4)). In the basis where the right-handed-neutrino mass matrix is real and diagonal, the model has masses M1,M2>0M_1, M_2>0M1​,M2​>0 and a complex 2×32\times 32×3 Yukawa matrix hν=(hναi)h_\nu=(h_\nu^{\alpha i})hν​=(hναi​). With Higgs vacuum expectation value ⟨H⟩=v/2\langle H\rangle = v/\sqrt2⟨H⟩=v/2​, the Dirac mass matrix is mD=hνv/2m_D = h_\nu v/\sqrt 2mD​=hν​v/2​. The neutral leptons (ν1,ν2,ν3,N1,N2)(\nu_1,\nu_2,\nu_3,N_1,N_2)(ν1​,ν2​,ν3​,N1​,N2​) then have the 5×55\times55×5 complex symmetric Majorana mass matrix

M=(0mDTmDdiag⁡(M1,M2)),\mathcal M = \begin{pmatrix} 0 & m_D^{\mathsf T} \\ m_D & \operatorname{diag}(M_1,M_2)\end{pmatrix},M=(0mD​​mDT​diag(M1​,M2​)​),

and the seesaw light-neutrino mass matrix is mν=−mDTdiag⁡(M1,M2)−1mDm_\nu = -m_D^{\mathsf T}\operatorname{diag}(M_1,M_2)^{-1} m_Dmν​=−mDT​diag(M1​,M2​)−1mD​. The physical masses described by a complex mass matrix AAA are its singular values, the square roots of the eigenvalues of A†AA^\dagger AA†A.

Inflaton sector (Eq. (5)). Inflation is driven by the quadratic potential V(φ)=12m2φ2V(\varphi)=\tfrac12 m^2\varphi^2V(φ)=21​m2φ2 (chaotic inflation). With reduced Planck mass MPlM_{\rm Pl}MPl​, the slow-roll parameters are ϵ=MPl22(V′/V)2\epsilon = \tfrac{M_{\rm Pl}^2}{2}(V'/V)^2ϵ=2MPl2​​(V′/V)2 and η=MPl2V′′/V\eta = M_{\rm Pl}^2 V''/Vη=MPl2​V′′/V, inflation ends where ϵ=1\epsilon = 1ϵ=1, the number of e-folds between φend\varphi_{\rm end}φend​ and φ\varphiφ is N=MPl−2∫φendφV/V′N = M_{\rm Pl}^{-2}\int_{\varphi_{\rm end}}^{\varphi} V/V'N=MPl−2​∫φend​φ​V/V′, and the observables are ns=1−6ϵ+2ηn_s = 1-6\epsilon+2\etans​=1−6ϵ+2η and r=16ϵr=16\epsilonr=16ϵ.

Scalar sector running (Eq. (10)). The singlet quartic coupling hhh obeys the one-loop equation (4π)2 dh/dt=3h2+12k2(4\pi)^2\, dh/dt = 3h^2 + 12k^2(4π)2dh/dt=3h2+12k2, t=log⁡μt=\log\mut=logμ, where kkk is the Higgs–singlet coupling.

Formalization targets

Goal — an exactly massless neutrino

For every v∈Rv\in\mathbb Rv∈R, every complex hνh_\nuhν​ and all M1,M2>0M_1,M_2>0M1​,M2​>0, some physical mass of the full matrix M\mathcal MM vanishes:

∃ i,σi(M)=0.\exists\, i,\quad \sigma_i(\mathcal M)=0 .∃i,σi​(M)=0.

This is the paper's statement that with only two right-handed neutrinos "one of the neutrino masses exactly vanishes" (pp. 119, 122).

Milestones

  1. Seesaw rank (p. 119). rank⁡mν≤2\operatorname{rank} m_\nu \le 2rankmν​≤2, and mνm_\numν​ has a zero physical mass.
  2. Enough parameters (p. 119). For v>0v>0v>0 and M1,M2>0M_1,M_2>0M1​,M2​>0, every complex symmetric 3×33\times33×3 matrix of rank at most 222 equals mνm_\numν​ for some hνh_\nuhν​.
  3. Inflation predictions (pp. 119, 122). For V=12m2φ2V=\tfrac12m^2\varphi^2V=21​m2φ2: ϵ(2MPl)=1\epsilon(\sqrt2 M_{\rm Pl})=1ϵ(2​MPl​)=1, and at NNN e-folds before the end, ns=1−42N+1n_s = 1-\tfrac{4}{2N+1}ns​=1−2N+14​, r=162N+1r=\tfrac{16}{2N+1}r=2N+116​; at N=50N=50N=50 these are within 0.0050.0050.005 of 0.960.960.96 and 0.160.160.16.
  4. Initial asymmetry is diluted (p. 120). If N≥ln⁡(10 Gpc/10 kpc)N\ge \ln(10\,\mathrm{Gpc}/10\,\mathrm{kpc})N≥ln(10Gpc/10kpc) and μF4/ρφ=e−4N\mu_F^4/\rho_\varphi = e^{-4N}μF4​/ρφ​=e−4N, then μF3/ρφ3/4≤10−18<8.8×10−11\mu_F^3/\rho_\varphi^{3/4}\le 10^{-18} < 8.8\times10^{-11}μF3​/ρφ3/4​≤10−18<8.8×10−11.
  5. Eq. (10), monotonicity. On any interval where it solves Eq. (10), hhh is non-decreasing.
  6. Eq. (10), Landau pole. A solution on [t0,T)[t_0,T)[t0​,T) with h(t0)>0h(t_0)>0h(t0​)>0 forces T≤t0+16π23h(t0)T\le t_0 + \tfrac{16\pi^2}{3h(t_0)}T≤t0​+3h(t0​)16π2​.

Significance

The vanishing neutrino mass is a sharp, falsifiable prediction of the NMSM: as the paper notes, a positive neutrino-mass signal at KATRIN would require masses for all three neutrinos, and a neutrinoless double-beta-decay signal in near-future experiments is possible only for the inverted hierarchy. Milestone 2 makes precise the paper's parameter count (eleven parameters in Eq. (4) against seven light-neutrino observables): the two-right-handed-neutrino seesaw reproduces every rank-≤2\le 2≤2 light mass matrix. Milestones 3–6 pin down the closed-form content behind the inflationary predictions, the argument that baryogenesis is required, and the triviality behaviour of the singlet coupling.

These results are textbook-level linear algebra and calculus once stated; the contribution of the mission is a precise, machine-checked statement of exactly which claims of the paper are mathematical theorems and under which conventions.

Difficulty

The goal and Milestone 1 are linear-algebra facts, but they must be connected to the spectral-theorem definition of physical masses (eigenvalues of A†AA^\dagger AA†A), not merely to a determinant. Milestone 2 requires a Takagi-type decomposition of complex symmetric matrices (a rank-rrr complex symmetric matrix is a sum of rrr terms wwTw w^{\mathsf T}wwT), which is not available in Mathlib. Milestone 3 requires evaluating a parametric integral and derivatives of the potential. Milestone 6 is an ODE comparison argument from a differential inequality.

Formalization scope

All matrices are over C\mathbb CC, indexed by Fin 2, Fin 3 and Fin 3 ⊕ Fin 2. Physical masses are defined as square roots of the eigenvalues of A†AA^\dagger AA†A from Mathlib's spectral theorem for Hermitian matrices; their ordering is Mathlib's and no statement depends on it. Slow-roll quantities use Mathlib's deriv and interval integral; Lean's junk value x/0=0x/0=0x/0=0 cannot affect the stated results because the inflaton interval stays away from φ=0\varphi=0φ=0. The phenomenological results (dark-matter relic abundance, the 130130130–180180180 GeV Higgs window, the 5.55.55.5 GeV–1.81.81.8 TeV singlet window, direct-detection rates) rely on numerical integration and are out of scope. The one-loop beta functions are taken as given ODEs; their derivation from the Lagrangian is not formalized.

Selected references

  • H. Davoudiasl, R. Kitano, T. Li, H. Murayama, The new Minimal Standard Model, Phys. Lett. B 609 (2005) 117–123. https://doi.org/10.1016/j.physletb.2005.01.026
  • A. D. Linde, Phys. Lett. B 129 (1983) 177 (chaotic inflation; reference [18] of the paper).
  • J. R. Ellis, M. Raidal, T. Yanagida, Phys. Lett. B 581 (2004) 9 (source of the quoted values of nsn_sns​ and rrr; reference [21] of the paper).
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Astrophysical Fluid Dynamics I: Rankine–Hugoniot Shock RelationsTextbook

Motivation

Shock waves are ubiquitous in astrophysical gases: supernova remnants, stellar winds meeting the interstellar medium, accretion flows onto compact objects, and jets all contain them. Because astrophysical flows are typically highly supersonic and nearly inviscid, the internal structure of a shock is thin compared with the flow, and the shock is treated as a discontinuity. What connects the states on either side is not the detailed dissipative physics inside the shock but the conservation of mass, momentum and energy across it. For a perfect gas these conditions can be solved in closed form, giving the post-shock density, velocity and pressure as explicit functions of the pre-shock Mach number. These formulas are a standard tool, used for example as the boundary condition of the Sedov–Taylor blast-wave solution for supernova remnants.

The formulas go back to Rankine (1870) and Hugoniot (1887–1889). This mission follows the presentation in the Cambridge Part III lecture notes of G. I. Ogilvie, Astrophysical fluid dynamics, J. Plasma Phys. 82 (2016) 205820301 (doi:10.1017/S0022377816000489), §6.3.2 and Example A.13.

Setting

Consider a perfect gas with constant adiabatic exponent γ>1\gamma > 1γ>1 (for example γ=5/3\gamma = 5/3γ=5/3 for a fully ionized monatomic gas). A thermodynamic state is described by the density ρ>0\rho > 0ρ>0 and pressure p>0p > 0p>0; the specific enthalpy is h=γγ−1pρh = \frac{\gamma}{\gamma-1}\frac{p}{\rho}h=γ−1γ​ρp​, the specific internal energy is e=p(γ−1)ρe = \frac{p}{(\gamma-1)\rho}e=(γ−1)ρp​, and the adiabatic sound speed is vs=(γp/ρ)1/2v_s = (\gamma p/\rho)^{1/2}vs​=(γp/ρ)1/2.

A normal shock is a planar discontinuity, here taken at rest at x=0x = 0x=0, through which gas flows from left to right with velocity component u>0u > 0u>0 normal to the shock. The upstream (pre-shock) state is (ρ1,u1,p1)(\rho_1, u_1, p_1)(ρ1​,u1​,p1​) and the downstream (post-shock) state is (ρ2,u2,p2)(\rho_2, u_2, p_2)(ρ2​,u2​,p2​). Writing [Q]12=Q2−Q1[Q]_1^2 = Q_2 - Q_1[Q]12​=Q2​−Q1​, the states satisfy the Rankine–Hugoniot relations

[ρu]12=0,[ρu2+p]12=0,[ρu(12u2+h)]12=0,[\rho u]_1^2 = 0, \qquad [\rho u^2 + p]_1^2 = 0, \qquad \Big[\rho u\big(\tfrac12 u^2 + h\big)\Big]_1^2 = 0,[ρu]12​=0,[ρu2+p]12​=0,[ρu(21​u2+h)]12​=0,

expressing continuity of the fluxes of mass, momentum and energy. The Mach numbers are M1=u1/vs1M_1 = u_1/v_{s1}M1​=u1​/vs1​ and M2=u2/vs2M_2 = u_2/v_{s2}M2​=u2​/vs2​. A genuine shock is one in which the two states differ; the trivial solution (ρ2,u2,p2)=(ρ1,u1,p1)(\rho_2,u_2,p_2) = (\rho_1,u_1,p_1)(ρ2​,u2​,p2​)=(ρ1​,u1​,p1​) always satisfies the relations.

The specific entropy of a perfect gas is s=cp(γ−1ln⁡p−ln⁡ρ)+consts = c_p(\gamma^{-1}\ln p - \ln \rho) + \text{const}s=cp​(γ−1lnp−lnρ)+const, with cp=γcvc_p = \gamma c_vcp​=γcv​, so the entropy jump across the shock is [s]12/cv=ln⁡(p2/p1)−γln⁡(ρ2/ρ1)[s]_1^2/c_v = \ln(p_2/p_1) - \gamma \ln(\rho_2/\rho_1)[s]12​/cv​=ln(p2​/p1​)−γln(ρ2​/ρ1​).

Formalization targets

Goal: the Rankine–Hugoniot jump formulas (eqs. 6.30–6.31)

For a genuine shock in a perfect gas,

ρ2ρ1=u1u2=(γ+1)M12(γ−1)M12+2,p2p1=2γM12−(γ−1)γ+1,M22=2+(γ−1)M122γM12−(γ−1).\frac{\rho_2}{\rho_1} = \frac{u_1}{u_2} = \frac{(\gamma+1)M_1^2}{(\gamma-1)M_1^2+2}, \qquad \frac{p_2}{p_1} = \frac{2\gamma M_1^2-(\gamma-1)}{\gamma+1}, \qquad M_2^2 = \frac{2+(\gamma-1)M_1^2}{2\gamma M_1^2-(\gamma-1)}.ρ1​ρ2​​=u2​u1​​=(γ−1)M12​+2(γ+1)M12​​,p1​p2​​=γ+12γM12​−(γ−1)​,M22​=2γM12​−(γ−1)2+(γ−1)M12​​.

Milestones

  1. The three jump formulas separately (eqs. 6.30a, 6.30b, 6.31).
  2. The density and pressure ratios are strictly increasing functions of M1>0M_1 > 0M1​>0.
  3. Classification: M1≠1M_1 \neq 1M1​=1 for a genuine shock; M1>1M_1 > 1M1​>1 gives a compression shock (M2<1M_2<1M2​<1, ρ2>ρ1\rho_2>\rho_1ρ2​>ρ1​, p2>p1p_2>p_1p2​>p1​) and M1<1M_1<1M1​<1 a rarefaction shock (M2>1M_2>1M2​>1, ρ2<ρ1\rho_2<\rho_1ρ2​<ρ1​, p2<p1p_2<p_1p2​<p1​).
  4. The entropy jump in terms of the pressure ratio P=p2/p1P = p_2/p_1P=p2​/p1​ (eq. A 28):
[s]12cv=ln⁡P−γln⁡[(γ+1)P+(γ−1)(γ−1)P+(γ+1)].\frac{[s]_1^2}{c_v} = \ln P - \gamma \ln\left[\frac{(\gamma+1)P+(\gamma-1)}{(\gamma-1)P+(\gamma+1)}\right].cv​[s]12​​=lnP−γln[(γ−1)P+(γ+1)(γ+1)P+(γ−1)​].
  1. The entropy jump is positive for compression shocks and negative for rarefaction shocks; hence the second law [s]12≥0[s]_1^2 \ge 0[s]12​≥0 forces a compression shock with M1>1>M2M_1>1>M_2M1​>1>M2​.
  2. Strong-shock limits as M1→∞M_1 \to \inftyM1​→∞ (eqs. 6.32a–c): ρ2/ρ1→γ+1γ−1\rho_2/\rho_1 \to \frac{\gamma+1}{\gamma-1}ρ2​/ρ1​→γ−1γ+1​, p2/p1→∞p_2/p_1 \to \inftyp2​/p1​→∞, M22→γ−12γM_2^2 \to \frac{\gamma-1}{2\gamma}M22​→2γγ−1​.
  3. The downstream state behind a strong shock (eqs. 6.33–6.34): at fixed ρ1\rho_1ρ1​ and shock speed ush=−u1u_{sh} = -u_1ush​=−u1​, as p1→0+p_1 \to 0^+p1​→0+,
ρ2→γ+1γ−1ρ1,u2−u1→2ushγ+1,p2→2ρ1ush2γ+1,e2→2ush2(γ+1)2.\rho_2 \to \frac{\gamma+1}{\gamma-1}\rho_1,\quad u_2-u_1 \to \frac{2u_{sh}}{\gamma+1},\quad p_2 \to \frac{2\rho_1u_{sh}^2}{\gamma+1},\quad e_2 \to \frac{2u_{sh}^2}{(\gamma+1)^2}.ρ2​→γ−1γ+1​ρ1​,u2​−u1​→γ+12ush​​,p2​→γ+12ρ1​ush2​​,e2​→(γ+1)22ush2​​.

Significance

The result itself. The jump formulas determine the post-shock state from the pre-shock state and a single number, the shock Mach number. They show that the compression ratio of a shock in a perfect gas is bounded (by 444 for γ=5/3\gamma = 5/3γ=5/3) however strong the shock, that a strong shock converts a fixed fraction of the incoming kinetic energy into heat, and, through the entropy jump, that only compressive shocks are compatible with the second law of thermodynamics. The strong-shock downstream state is the input to the self-similar supernova blast-wave solution treated later in the same notes (§7).

Formalizing it. The results are classical and fully proved in the textbook sense; a search of the platform library found no existing formalization of them. The mission produces a reusable Lean vocabulary for one-dimensional perfect-gas shocks (enthalpy, sound speed, Mach number, Rankine–Hugoniot predicate, entropy jump) on which later missions on blast waves, oblique shocks or MHD shocks can build.

Difficulty

The individual steps are algebraic, but the Rankine–Hugoniot system is nonlinear and always has the trivial solution. Eliminating variables leads to a quadratic in the velocity ratio u2/u1u_2/u_1u2​/u1​ with roots 111 and the shock root, so any derivation must use the hypothesis that the two states differ at exactly the right point; dividing by the trivial factor without that hypothesis is the standard mistake. The sign of the entropy jump is a genuinely analytic statement: it requires showing that a one-variable function of PPP involving logarithms vanishes only at P=1P = 1P=1 and has a definite sign on each side. The strong-shock statements are limits and need uniform control of the downstream state as p1→0p_1 \to 0p1​→0.

Formalization scope

All quantities are real numbers. The gas is a perfect gas with γ>1\gamma > 1γ>1; every statement about gas states assumes strictly positive densities, pressures and normal velocities, which matches the source's convention ux>0u_x > 0ux​>0 and makes all square roots, quotients and logarithms well-defined (Lean's total functions would otherwise return junk values, e.g. division by zero gives 000). Only the normal, non-magnetic shock is treated; the shock is at rest, and the frame change to the upstream rest frame appears only through ush=−u1u_{sh} = -u_1ush​=−u1​. The entropy is represented through its jump divided by cvc_vcv​. The genuine-shock hypothesis (ρ2,u2,p2)≠(ρ1,u1,p1)(\rho_2,u_2,p_2) \neq (\rho_1,u_1,p_1)(ρ2​,u2​,p2​)=(ρ1​,u1​,p1​) rules out the trivial solution, under which the jump formulas would be false for M1≠1M_1 \neq 1M1​=1; it is omitted only from the entropy-jump formula (A 28), which also holds for the trivial solution. The strong-shock limit "M1≫1M_1 \gg 1M1​≫1" is expressed as p1→0+p_1 \to 0^+p1​→0+ at fixed ρ1\rho_1ρ1​ and u1u_1u1​, and "p2/p1≫1p_2/p_1 \gg 1p2​/p1​≫1" as divergence to +∞+\infty+∞.

The definitions are collected in one shared file (namespace AstrophysicalFluidDynamics, intended to be reused by later missions on the same lecture notes). Only Mathlib's real analysis (logarithm, square root, limits) is needed. Contributions welcome: proofs of the milestones, and reusable lemmas such as the factorization of the Rankine–Hugoniot system through the trivial root.

Selected references

  • G. I. Ogilvie, Astrophysical fluid dynamics, Journal of Plasma Physics 82 (2016) 205820301. https://doi.org/10.1017/S0022377816000489
  • W. J. M. Rankine, On the thermodynamic theory of waves of finite longitudinal disturbance, Philosophical Transactions of the Royal Society of London 160 (1870) 277–288.
  • L. D. Landau and E. M. Lifshitz, Fluid Mechanics, 2nd ed., Pergamon (1987), Chapter IX.
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Giunti–Studenikin 2015: Neutrino Oscillations, Majorana Form Factors and Spin PrecessionResearch Paper

Motivation

Neutrinos are the only Standard Model fermions whose masses, mixing and electromagnetic properties are still largely unknown. The review of Giunti and Studenikin (Rev. Mod. Phys. 87, 531 (2015)) collects the theory of neutrino masses and mixing, the general structure of neutrino electromagnetic form factors for Dirac and Majorana neutrinos, and the dynamics of neutrino spin and flavor in electromagnetic fields and matter. Most of the review is phenomenology (experimental bounds, astrophysical estimates), but a core of it consists of exact mathematical statements about finite-dimensional unitary matrices, Hermitian matrices and two-level linear Schrödinger equations. Those exact statements are what this mission targets.

Timeline of the results formalized here:

  • 1957–1968: Pontecorvo; Maki, Nakagawa and Sakata introduce neutrino mixing and oscillations.
  • 1957: Case; Radicati and Touschek observe that Majorana neutrinos cannot have diagonal magnetic or electric dipole moments.
  • 1971: Cisneros proposes spin precession νeL→νeR\nu_{eL}\to\nu_{eR}νeL​→νeR​ of solar neutrinos in a magnetic field.
  • 1978: Wolfenstein writes the evolution equation of neutrino flavor in matter; 1985: Mikheev and Smirnov identify its resonance (MSW effect).
  • 1986: Okun, Voloshin and Vysotsky; Voloshin and Vysotsky show that matter suppresses spin precession.

Setting

A mixing matrix is a unitary n×nn\times nn×n complex matrix UUU whose rows are labelled by flavors ℓ\ellℓ and whose columns are labelled by massive states kkk with masses mkm_kmk​. For a neutrino of energy E>0E>0E>0 that has travelled a distance LLL, the plane-wave transition probability (Eqs. (2.35)–(2.36)) is

Pνℓ→νℓ′(L,E)=∣∑kUℓk∗ e−imk2L/(2E) Uℓ′k∣2.P_{\nu_\ell\to\nu_{\ell'}}(L,E)=\Bigl|\sum_k U^*_{\ell k}\,e^{-i m_k^2 L/(2E)}\,U_{\ell' k}\Bigr|^2 .Pνℓ​→νℓ′​​(L,E)=​k∑​Uℓk∗​e−imk2​L/(2E)Uℓ′k​​2.

In the Lean development this is oscProb U m L E l l'. The standard parametrization UD(ϑ12,ϑ13,ϑ23,δ13)U^{\mathrm D}(\vartheta_{12},\vartheta_{13},\vartheta_{23},\delta_{13})UD(ϑ12​,ϑ13​,ϑ23​,δ13​) of Eq. (2.27) and the Majorana phase matrix DM=diag⁡(1,eiλ21,eiλ31)D^{\mathrm M}=\operatorname{diag}(1,e^{i\lambda_{21}},e^{i\lambda_{31}})DM=diag(1,eiλ21​,eiλ31​) of Eq. (2.28) are diracMixing and majoranaPhases; the two-neutrino rotation matrix of Eq. (2.38) is twoFlavorMixing.

In matter of constant electron density, the νe\nu_eνe​–νa\nu_aνa​ amplitudes (φe,φa)(\varphi_e,\varphi_a)(φe​,φa​) obey i ddxφ=Hφi\,\tfrac{d}{dx}\varphi=\mathrm H\varphiidxd​φ=Hφ with the effective Hamiltonian of Eq. (2.46) (mswHamiltonian), built from the vacuum squared-mass difference Δm2\Delta m^2Δm2, the mixing angle ϑ\varthetaϑ and the charged-current potential VCCV_{\rm CC}VCC​ with ACC=2EVCCA_{\rm CC}=2EV_{\rm CC}ACC​=2EVCC​. The effective squared-mass difference ΔmM2\Delta m^2_{\rm M}ΔmM2​ of Eq. (2.53) and effective angle ϑM\vartheta_{\rm M}ϑM​ of Eq. (2.54) are mswDeltaM2 and mswMixingAngle.

Electromagnetic form-factor matrices fΩ\mathbb f_\OmegafΩ​ (Ω=Q,M,E,A\Omega=Q,M,E,AΩ=Q,M,E,A: charge, magnetic, electric, anapole) are Hermitian N×NN\times NN×N complex matrices in the space of massive neutrinos; for Majorana neutrinos they are in addition antisymmetric (Ω=Q,M,E\Omega=Q,M,EΩ=Q,M,E) or symmetric (Ω=A\Omega=AΩ=A), Eqs. (3.66)–(3.68).

Finally, the helicity amplitudes (ψL,ψR)(\psi_L,\psi_R)(ψL​,ψR​) of an ultrarelativistic Dirac neutrino with magnetic moment μ\muμ in a transverse field B⊥B_\perpB⊥​ and matter potential VVV obey i ddxψ=(VμB⊥μB⊥0)ψi\,\tfrac{d}{dx}\psi=\begin{pmatrix}V&\mu B_\perp\\ \mu B_\perp&0\end{pmatrix}\psiidxd​ψ=(VμB⊥​​μB⊥​0​)ψ (Eqs. (6.23), (6.28); spinFlavorHamiltonian), with energy splitting ΔEM=V2+(2μB⊥)2\Delta E_{\rm M}=\sqrt{V^2+(2\mu B_\perp)^2}ΔEM​=V2+(2μB⊥​)2​ (Eq. (6.31); spinFlavorEnergySplitting).

Formalization targets

Goal: the general vacuum oscillation probability, Eq. (2.37)

For every unitary UUU, all masses mkm_kmk​, every LLL and every E>0E>0E>0,

Pνℓ→νℓ′=δℓℓ′−4∑k>jRe⁡(Uℓk∗Uℓ′kUℓjUℓ′j∗)sin⁡2 ⁣(Δmkj2L4E)−2∑k>jIm⁡(UℓkUℓj∗Uℓ′k∗Uℓ′j)sin⁡ ⁣(Δmkj2L2E),P_{\nu_\ell\to\nu_{\ell'}}=\delta_{\ell\ell'}-4\sum_{k>j}\operatorname{Re}\bigl(U^*_{\ell k}U_{\ell' k}U_{\ell j}U^*_{\ell' j}\bigr)\sin^2\!\Bigl(\frac{\Delta m^2_{kj}L}{4E}\Bigr)-2\sum_{k>j}\operatorname{Im}\bigl(U_{\ell k}U^*_{\ell j}U^*_{\ell' k}U_{\ell' j}\bigr)\sin\!\Bigl(\frac{\Delta m^2_{kj}L}{2E}\Bigr),Pνℓ​→νℓ′​​=δℓℓ′​−4k>j∑​Re(Uℓk∗​Uℓ′k​Uℓj​Uℓ′j∗​)sin2(4EΔmkj2​L​)−2k>j∑​Im(Uℓk​Uℓj∗​Uℓ′k∗​Uℓ′j​)sin(2EΔmkj2​L​),

with Δmkj2=mk2−mj2\Delta m^2_{kj}=m_k^2-m_j^2Δmkj2​=mk2​−mj2​. The number nnn of massive states is left free (the paper uses n=3n=3n=3, and n>3n>3n>3 with sterile neutrinos, Sec. II.F).

Milestones

  1. Eqs. (2.26)–(2.28): UDU^{\mathrm D}UD and UDDMU^{\mathrm D}D^{\mathrm M}UDDM are unitary.
  2. Eq. (2.39): two-neutrino transition probability sin⁡22ϑ sin⁡2(Δm2L/4E)\sin^2 2\vartheta\,\sin^2(\Delta m^2L/4E)sin22ϑsin2(Δm2L/4E).
  3. Eq. (2.40): two-neutrino survival probability 1−sin⁡22ϑ sin⁡2(Δm2L/4E)1-\sin^2 2\vartheta\,\sin^2(\Delta m^2L/4E)1−sin22ϑsin2(Δm2L/4E).
  4. Eqs. (2.50)–(2.54): UMTHUM=diag⁡(−ΔmM2,ΔmM2)/4EU_{\rm M}^T\mathrm H U_{\rm M}=\operatorname{diag}(-\Delta m^2_{\rm M},\Delta m^2_{\rm M})/4EUMT​HUM​=diag(−ΔmM2​,ΔmM2​)/4E.
  5. Eq. (2.57): MSW transition probability at constant density sin⁡22ϑMsin⁡2(ΔmM2x/4E)\sin^2 2\vartheta_{\rm M}\sin^2(\Delta m^2_{\rm M}x/4E)sin22ϑM​sin2(ΔmM2​x/4E).
  6. Eqs. (3.66)–(3.70): Majorana form-factor matrices — antisymmetric Hermitian matrices are purely imaginary with vanishing diagonal; symmetric Hermitian matrices are real.
  7. Eqs. (3.71)–(3.72): three-flavor antisymmetric Hermitian form factors are i∑jϵfijf~ji\sum_j\epsilon^{fij}\tilde{\mathbb f}^ji∑j​ϵfijf~​j with a real vector f~\tilde{\mathbb f}f~​.
  8. Eq. (6.27): spin precession in a transverse field, PνL→νR(x)=sin⁡2(∫0xμB⊥)P_{\nu_L\to\nu_R}(x)=\sin^2\bigl(\int_0^x\mu B_\perp\bigr)PνL​→νR​​(x)=sin2(∫0x​μB⊥​).
  9. Eq. (6.34): spin precession in matter, PνL→νR(x)=sin⁡22ξ sin⁡2(12ΔEMx)P_{\nu_L\to\nu_R}(x)=\sin^2 2\xi\,\sin^2(\tfrac12\Delta E_{\rm M}x)PνL​→νR​​(x)=sin22ξsin2(21​ΔEM​x) with sin⁡2ξ=2μB⊥/ΔEM\sin 2\xi=2\mu B_\perp/\Delta E_{\rm M}sin2ξ=2μB⊥​/ΔEM​.

Significance

Eq. (2.37) is the formula used in essentially every analysis of oscillation data; its two-neutrino specializations (2.39)–(2.40) and the matter formula (2.57) are the standard fitting functions for reactor, accelerator and solar experiments. The Majorana constraints (3.67)–(3.70) are the precise statement behind the claim that a measured diagonal magnetic moment would rule out Majorana neutrinos (under CPT). The spin-precession formulas (6.27) and (6.34) underlie the astrophysical bounds on neutrino magnetic moments.

All targets are established results with textbook derivations; none is open. What the mission adds is machine-checked versions with every convention (sign of the phase, ordering k>jk>jk>j, ranges of angles, boundary conditions of the Schrödinger equation) fixed explicitly. Related vacuum-oscillation statements from a different source already exist on the platform under the LipariNeutrino namespace; the present drafts are self-contained and follow this paper's notation and equation numbering.

Difficulty

The algebraic targets require careful bookkeeping of complex conjugation and of the unitarity relations UU†=U†U=1UU^\dagger=U^\dagger U=1UU†=U†U=1 inside double sums over k>jk>jk>j. The dynamical targets (2.57), (6.27), (6.34) are statements about every solution of a linear ODE with a given initial value, so a solution in closed form is not enough: uniqueness of solutions of the (for (6.27), non-autonomous) linear system must also be established in Lean.

Formalization scope

  • Flavor and mass indices are Fin n; two-neutrino indices 0,1 stand for (νe,νa)(\nu_e,\nu_a)(νe​,νa​), (νL,νR)(\nu_L,\nu_R)(νL​,νR​) or (ν1,ν2)(\nu_1,\nu_2)(ν1​,ν2​).
  • Masses mkm_kmk​ are arbitrary reals and enter only through mk2m_k^2mk2​.
  • Unitarity is membership in Matrix.unitaryGroup.
  • The evolution equations are encoded as HasDerivAt φ (-(I • H.mulVec (φ x))) x for all real xxx, i.e. φ′=−iHφ\varphi'=-i\mathrm H\varphiφ′=−iHφ, with initial value (1,0)(1,0)(1,0).
  • ϑM\vartheta_{\rm M}ϑM​ is defined as half the argument of (Δm2cos⁡2ϑ−2EVCC)+i Δm2sin⁡2ϑ(\Delta m^2\cos2\vartheta-2EV_{\rm CC})+i\,\Delta m^2\sin2\vartheta(Δm2cos2ϑ−2EVCC​)+iΔm2sin2ϑ, which realizes Eq. (2.54) without the division-by-zero at resonance; sin⁡2ξ=2μB⊥/ΔEM\sin 2\xi=2\mu B_\perp/\Delta E_{\rm M}sin2ξ=2μB⊥​/ΔEM​ is inlined, with Lean's convention 0/0=00/0=00/0=0 in the degenerate case V=μB⊥=0V=\mu B_\perp=0V=μB⊥​=0.
  • The source's angle ranges (0≤ϑ≤π/20\le\vartheta\le\pi/20≤ϑ≤π/2, 0≤δ13<2π0\le\delta_{13}<2\pi0≤δ13​<2π) and E>0E>0E>0 are kept as hypotheses.

Useful reusable infrastructure: uniqueness for linear ODEs in C2\mathbb C^2C2, closed-form exponentials of 2×22\times22×2 real symmetric matrices, and algebraic lemmas for unitary matrices.

Selected references

  • C. Giunti and A. Studenikin, Neutrino electromagnetic interactions: A window to new physics, Rev. Mod. Phys. 87, 531 (2015). https://doi.org/10.1103/RevModPhys.87.531
  • C. Giunti and C. W. Kim, Fundamentals of Neutrino Physics and Astrophysics, Oxford University Press (2007).
  • L. Wolfenstein, Neutrino oscillations in matter, Phys. Rev. D 17, 2369 (1978). https://doi.org/10.1103/PhysRevD.17.2369
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Baumgarten 2018: How to (Un-) Quantum Mechanics — Phase-Space AlgebraResearch Paper

Motivation

C. Baumgarten's essay How to (Un-) Quantum Mechanics (arXiv:1810.06981, v2 2025) argues that much of the mathematical formalism usually presented as specifically "quantum" — Heisenberg's equation of motion, commutators, eigenvalue problems, the real Pauli and Dirac algebras — already follows from classical linear Hamiltonian mechanics on an abstract phase space. The physical and philosophical claims of the paper are outside the scope of a formalization, but its argument rests on a compact chain of linear-algebra facts stated in Sections IV–VI (pp. 13–20). This mission formalizes exactly that chain, so that the mathematical part of the argument can be checked independently of its interpretation.

Setting

Fix a number n≥0n \ge 0n≥0 of degrees of freedom. A phase-space vector is ψ=(q1,p1,…,qn,pn)T∈R2n\psi = (q_1,p_1,\dots,q_n,p_n)^T \in \mathbb R^{2n}ψ=(q1​,p1​,…,qn​,pn​)T∈R2n. The symplectic unit matrix is the Kronecker product

γ0=1n⊗η0,η0=(01−10).\gamma_0 = \mathbf 1_n \otimes \eta_0, \qquad \eta_0 = \begin{pmatrix}0 & 1\\ -1 & 0\end{pmatrix}.γ0​=1n​⊗η0​,η0​=(0−1​10​).

A real 2n×2n2n\times 2n2n×2n matrix is Hamiltonian if it equals γ0A\gamma_0 Aγ0​A with AAA symmetric, skew-Hamiltonian if it equals γ0B\gamma_0 Bγ0​B with BBB skew-symmetric, and symplectic if Mγ0MT=γ0M\gamma_0M^T = \gamma_0Mγ0​MT=γ0​.

Linear Hamiltonian motion is ψ˙=Hψ\dot\psi = H\psiψ˙​=Hψ with HHH Hamiltonian (the paper's Eq. 35, coming from the quadratic Hamiltonian 12ψTAψ\tfrac12\psi^TA\psi21​ψTAψ). A matrix of second moments Σ(τ)\Sigma(\tau)Σ(τ) (in the paper an average ⟨ψψT⟩\langle\psi\psi^T\rangle⟨ψψT⟩) then evolves by

Σ˙=HΣ+ΣHT(Eq. 40),\dot\Sigma = H\Sigma + \Sigma H^T \qquad\text{(Eq. 40)},Σ˙=HΣ+ΣHT(Eq. 40),

and the autocorrelation matrix is S=Σγ0TS = \Sigma\gamma_0^TS=Σγ0T​.

Target

The goal theorem combines the conclusions drawn on pp. 16–17: for HHH Hamiltonian and Σ\SigmaΣ a symmetric solution of Eq. (40), the autocorrelation matrix satisfies, for every time τ\tauτ,

χS(τ)=χS(0)andTr⁡(S(τ)2k+1)=0  (k∈N),\chi_{S(\tau)} = \chi_{S(0)} \qquad\text{and}\qquad \operatorname{Tr}\big(S(\tau)^{2k+1}\big) = 0 \ \ (k \in \mathbb N),χS(τ)​=χS(0)​andTr(S(τ)2k+1)=0  (k∈N),

where χ\chiχ is the characteristic polynomial: "the eigenvalues are constants of motion" (after Eq. 51) together with Eq. (48).

The milestones follow the paper's own steps, in order:

  1. pairing ±λ\pm\lambda±λ of eigenvalues of skew-symmetric matrices, and a vanishing eigenvalue in odd size (p. 13);
  2. conservation of HHH under ψ˙=J∇H\dot\psi = J\nabla Hψ˙​=J∇H with JJJ skew (Eqs. 26–28);
  3. identities of γ0\gamma_0γ0​ and the transpose rules for (skew-)Hamiltonian matrices (Eqs. 33, 36, 54);
  4. exp⁡(Hτ)ψ0\exp(H\tau)\psi_0exp(Hτ)ψ0​ solves ψ˙=Hψ\dot\psi = H\psiψ˙​=Hψ (Eq. 49);
  5. Heisenberg's equation S˙=[H,S]\dot S = [H,S]S˙=[H,S] for second moments (Eq. 42);
  6. the Lax invariants Tr⁡(Sk)\operatorname{Tr}(S^k)Tr(Sk) (Eq. 47) and tracelessness of odd powers (Eq. 48);
  7. symplecticity of exp⁡(Hτ)\exp(H\tau)exp(Hτ) and S(τ)=M(τ)S(0)M(−τ)S(\tau) = M(\tau)S(0)M(-\tau)S(τ)=M(τ)S(0)M(−τ) (Eqs. 50–51);
  8. the dimension counts n(2n+1)n(2n+1)n(2n+1) and n(2n−1)n(2n-1)n(2n−1) (Eqs. 55–56) and the (anti-)commutator table (Eq. 57);
  9. the matrix Euler formulas for the real Pauli matrices (Eq. 66).

Significance

The result itself. Each statement is classical linear algebra or linear ODE theory; the paper uses them to argue that Heisenberg's equation and the spectral description of observables arise from second moments of a classical Hamiltonian ensemble. A checked version separates what is a theorem from what is interpretation, and pins down the hypotheses (for example, that only symmetry of AAA is needed for Eq. 48, not positive definiteness).

Formalizing it. None of these statements is new mathematics; the work is to formalize them in the paper's notation (γ0=1n⊗η0\gamma_0 = \mathbf 1_n\otimes\eta_0γ0​=1n​⊗η0​, entrywise matrix derivatives, the matrix exponential) so that they can be reused for later parts of the paper, such as the real Dirac algebra of Sec. VII–VIII.

Difficulty

Most milestones are short calculations. The two steps needing real infrastructure are (i) the uniqueness of solutions of the linear matrix ODE S˙=[H,S]\dot S = [H,S]S˙=[H,S], needed to identify S(τ)S(\tau)S(τ) with exp⁡(Hτ)S(0)exp⁡(−Hτ)\exp(H\tau)S(0)\exp(-H\tau)exp(Hτ)S(0)exp(−Hτ), and (ii) the dimension counts, which require an explicit basis or an isomorphism with symmetric/skew-symmetric matrices. Going through the Lax invariants alone gives only the traces of powers of SSS, and recovering the characteristic polynomial from them needs Newton's identities; the similarity form of Eq. (51) gives the conservation of the characteristic polynomial directly.

Formalization scope

Everything is over R\mathbb RR. Matrices are indexed by pairs (i,b)(i,b)(i,b), i<ni<ni<n, b∈{0,1}b\in\{0,1\}b∈{0,1}, so that γ0\gamma_0γ0​ is literally a Kronecker product; n=0n = 0n=0 is allowed. Time derivatives of matrix-valued functions are entrywise HasDerivAt; exp⁡\expexp is Mathlib's power-series NormedSpace.exp. A Hamiltonian matrix is γ0A\gamma_0Aγ0​A with AAA symmetric (no definiteness); Σ\SigmaΣ is any symmetric solution of Eq. (40) — positivity is not assumed because it is not used. Eigenvalues of real skew-symmetric matrices are taken over C\mathbb CC. "Number of linearly independent elements" is the dimension of the real span. No statement is vacuous: all hypotheses are satisfied, for example, by H=γ0H = \gamma_0H=γ0​ and Σ≡1\Sigma \equiv \mathbf 1Σ≡1.

All statements share the definition file UnQM_phase_space and the namespace UnQuantumMechanics.

Selected references

  • C. Baumgarten, How to (Un-) Quantum Mechanics, arXiv:1810.06981v2 [physics.gen-ph], 2025. https://arxiv.org/abs/1810.06981
  • P. D. Lax, Integrals of nonlinear equations of evolution and solitary waves, Comm. Pure Appl. Math. 21 (1968), 467–490. https://doi.org/10.1002/cpa.3160210503
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Virial Theorem (Classical N-Particle Mechanics)Textbook

Motivation

The virial theorem relates the long-time average of the total kinetic energy of a bound system of particles to the average of the virial −12∑kFk⋅rk-\frac12\sum_k \mathbf F_k\cdot\mathbf r_k−21​∑k​Fk​⋅rk​ of the forces acting on them. It gives the average kinetic energy of systems too complicated to solve exactly, such as stars, planetary systems, galaxies and galaxy clusters. Fritz Zwicky used it to infer the existence of unseen matter, and it enters the derivation of the Chandrasekhar limit for white dwarfs. It does not depend on the notion of temperature and holds for systems that are not in thermal equilibrium.

Timeline (as recounted in the source article):

  • 1772: Lagrange's identity appears in Lagrange's Essay on the Problem of Three Bodies.
  • Jacobi generalizes the identity to nnn bodies.
  • 1870: Clausius, lecture On a Mechanical Theorem Applicable to Heat: the mean vis viva of a system equals its virial.
  • Later development by Maxwell, Rayleigh, Poincaré, Chandrasekhar, Fermi, Ledoux, Bader and Parker; quantum versions sketched in 1926 and proved by Finkelstein (1928) and Fock (1930).

Setting

NNN point particles move in R3\mathbb R^3R3. Particle kkk has a constant mass mkm_kmk​, position rk(t)r_k(t)rk​(t), velocity vk(t)=r˙k(t)v_k(t)=\dot r_k(t)vk​(t)=r˙k​(t) and momentum pk=mkvkp_k=m_kv_kpk​=mk​vk​; the net force on it is Fk=p˙kF_k=\dot p_kFk​=p˙​k​. The kinetic energy is T=12∑kmk∥vk∥2T=\frac12\sum_km_k\|v_k\|^2T=21​∑k​mk​∥vk​∥2, the moment of inertia is I=∑kmk∥rk∥2I=\sum_km_k\|r_k\|^2I=∑k​mk​∥rk​∥2, and

G=∑k=1Npk⋅rk.G=\sum_{k=1}^Np_k\cdot r_k .G=k=1∑N​pk​⋅rk​.

The time average over a duration τ\tauτ is ⟨f⟩τ=1τ∫0τf(t) dt\langle f\rangle_\tau=\frac1\tau\int_0^\tau f(t)\,dt⟨f⟩τ​=τ1​∫0τ​f(t)dt.

When forces come from pair potentials VjkV_{jk}Vjk​ depending only on the distance rjk=∥rk−rj∥r_{jk}=\|r_k-r_j\|rjk​=∥rk​−rj​∥, the force of jjj on kkk is Fjk=−∇rkVjk(rjk)F_{jk}=-\nabla_{r_k}V_{jk}(r_{jk})Fjk​=−∇rk​​Vjk​(rjk​), Fk=∑jFjkF_k=\sum_jF_{jk}Fk​=∑j​Fjk​, and the total potential energy is VTOT=∑k∑j<kVjk(rjk)V_{\mathrm{TOT}}=\sum_k\sum_{j<k}V_{jk}(r_{jk})VTOT​=∑k​∑j<k​Vjk​(rjk​). Power-law potentials are Vjk=αjkrjknV_{jk}=\alpha_{jk}r_{jk}^nVjk​=αjk​rjkn​; gravity is n=−1n=-1n=−1.

Formalization targets

Goal: the virial theorem

For a motion with r˙k=vk\dot r_k=v_kr˙k​=vk​, p˙k=Fk\dot p_k=F_kp˙​k​=Fk​ (continuous forces) that is bounded (positions and velocities bounded for t≥0t\ge0t≥0),

lim⁡τ→∞(2⟨T⟩τ+∑k=1N⟨Fk⋅rk⟩τ)=0.\lim_{\tau\to\infty}\Big(2\langle T\rangle_\tau+\sum_{k=1}^N\langle F_k\cdot r_k\rangle_\tau\Big)=0 .τ→∞lim​(2⟨T⟩τ​+k=1∑N​⟨Fk​⋅rk​⟩τ​)=0.

Milestones

  1. 12 I˙=G\frac12\,\dot I=G21​I˙=G.
  2. G˙=2T+∑kFk⋅rk\dot G=2T+\sum_kF_k\cdot r_kG˙=2T+∑k​Fk​⋅rk​.
  3. With Newton's third law, ∑kFk⋅rk=∑k∑j<kFjk⋅(rk−rj)\sum_kF_k\cdot r_k=\sum_k\sum_{j<k}F_{jk}\cdot(r_k-r_j)∑k​Fk​⋅rk​=∑k​∑j<k​Fjk​⋅(rk​−rj​).
  4. Potential pair forces are central: Fjk=−Vjk′(rjk)rjk(rk−rj)F_{jk}=-\frac{V_{jk}'(r_{jk})}{r_{jk}}(r_k-r_j)Fjk​=−rjk​Vjk′​(rjk​)​(rk​−rj​).
  5. Potential pair forces satisfy Fjk=−FkjF_{jk}=-F_{kj}Fjk​=−Fkj​.
  6. ∑kFk⋅rk=−∑k∑j<kVjk′(rjk) rjk\sum_kF_k\cdot r_k=-\sum_k\sum_{j<k}V'_{jk}(r_{jk})\,r_{jk}∑k​Fk​⋅rk​=−∑k​∑j<k​Vjk′​(rjk​)rjk​.
  7. Power law: ∑kFk⋅rk=−nVTOT\sum_kF_k\cdot r_k=-nV_{\mathrm{TOT}}∑k​Fk​⋅rk​=−nVTOT​.
  8. Power law: G˙=2T−nVTOT\dot G=2T-nV_{\mathrm{TOT}}G˙=2T−nVTOT​.
  9. Lagrange's identity (n=−1n=-1n=−1): 12I¨=2T+VTOT\frac12\ddot I=2T+V_{\mathrm{TOT}}21​I¨=2T+VTOT​.
  10. ⟨G˙⟩τ=G(τ)−G(0)τ=2⟨T⟩τ+∑k⟨Fk⋅rk⟩τ\langle\dot G\rangle_\tau=\frac{G(\tau)-G(0)}{\tau}=2\langle T\rangle_\tau+\sum_k\langle F_k\cdot r_k\rangle_\tau⟨G˙⟩τ​=τG(τ)−G(0)​=2⟨T⟩τ​+∑k​⟨Fk​⋅rk​⟩τ​.
  11. Bounded motion: ⟨G˙⟩τ→0\langle\dot G\rangle_\tau\to0⟨G˙⟩τ​→0.
  12. Power-law virial theorem: ⟨T⟩τ−n2⟨VTOT⟩τ→0\langle T\rangle_\tau-\frac n2\langle V_{\mathrm{TOT}}\rangle_\tau\to0⟨T⟩τ​−2n​⟨VTOT​⟩τ​→0 for bounded collision-free motion.

Significance

The theorem turns boundedness of a motion into a quantitative relation between averaged energies, without solving the equations of motion; with n=−1n=-1n=−1 it gives ⟨T⟩=−12⟨VTOT⟩\langle T\rangle=-\frac12\langle V_{\mathrm{TOT}}\rangle⟨T⟩=−21​⟨VTOT​⟩ for self-gravitating systems, the relation used for mass estimates of galaxy clusters. The result is classical and proved in the literature. This mission formalizes the standard derivation: the calculus identities for III and GGG, the pair-force algebra under Newton's third law, the gradient computation for distance potentials, and the averaging argument.

Difficulty

The mathematics is elementary; the work lies in the formal infrastructure: product rules for inner products of vector-valued trajectories, the gradient of y↦V(∥y−x∥)y\mapsto V(\|y-x\|)y↦V(∥y−x∥) in R3\mathbb R^3R3, re-indexing a double sum over ordered pairs into a sum over j<kj<kj<k, and the fundamental theorem of calculus for ∫0τG˙\int_0^\tau\dot G∫0τ​G˙ with the required integrability. A tempting oversimplification is to assume that ⟨T⟩τ\langle T\rangle_\tau⟨T⟩τ​ and ⟨F⋅r⟩τ\langle F\cdot r\rangle_\tau⟨F⋅r⟩τ​ converge individually; bounded motion does not guarantee this, so the targets are stated as limits of the combined expression.

Formalization scope

Space is EuclideanSpace ℝ (Fin 3) and particles are indexed by Fin N. Trajectories are functions R→R3\mathbb R\to\mathbb R^3R→R3; the equations of motion are hypotheses HasDerivAt (r k) (v k t) t and HasDerivAt (fun s => m k • v k s) (F k t) t. Masses are constant real numbers. Time averages are τ−1∫0τ\tau^{-1}\int_0^\tauτ−1∫0τ​ (interval integral). Pair forces are defined with Mathlib's gradient, with Fkk=0F_{kk}=0Fkk​=0. Power-law coefficients αjk\alpha_{jk}αjk​ may depend on the pair (symmetric), which contains the article's single constant α\alphaα. Real powers are Real.rpow; collision-freeness is assumed wherever pair distances enter. Boundedness is imposed only for t≥0t\ge0t≥0. The hypotheses are satisfiable (for instance by a uniform circular two-body motion), so no target holds vacuously.

Selected references

  • Wikipedia, Virial theorem. https://en.wikipedia.org/wiki/Virial_theorem
  • R. Clausius, On a mechanical theorem applicable to heat, Philosophical Magazine, Series 4, 40 (1870), 122–127.
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Statistics·Captain: Lucas

Methanol Limit on a Drifting Proton-to-Electron Mass Ratio (Bagdonaite et al. 2013)Research Paper

Motivation

The Standard Model of particle physics does not explain the values of its dimensionless constants, nor does it require them to be constant in time. The proton-to-electron mass ratio μ=mp/me≈1836\mu = m_p/m_e \approx 1836μ=mp​/me​≈1836 is one such constant: it compares the scale of the strong interaction (which sets most of the proton mass) with the electroweak scale (which sets the electron mass). A measured change of μ\muμ over cosmic time would signal physics beyond the Standard Model, while a tight null result constrains models with additional scalar fields.

The standard test compares the frequencies of molecular transitions observed in distant galaxies with laboratory values. Different transitions respond differently to a change of μ\muμ, so a relative shift between them cannot be confused with the overall cosmological redshift.

Timeline. Optical studies of molecular hydrogen at redshifts z>2z>2z>2 reached ∣Δμ/μ∣<10−5|\Delta\mu/\mu| < 10^{-5}∣Δμ/μ∣<10−5 (Malec et al. 2010; van Weerdenburg et al. 2011). Ammonia inversion lines, about 100 times more sensitive, moved the field to radio astronomy and gave constraints at the 10−710^{-7}10−7 level toward the lensing galaxy of PKS 1830−211 at z=0.89z=0.89z=0.89 (Henkel et al. 2009; Kanekar 2011). Jansen et al. (2011) and Levshakov, Kozlov & Reimers (2011) pointed out that methanol transitions have sensitivity coefficients ranging from about −42-42−42 to +53+53+53. Ellingsen et al. (2012) gave a first methanol limit from two lines. Bagdonaite et al. (Science, 2013) observed four methanol lines in PKS 1830−211 with the Effelsberg 100-m telescope and derived the limit Δμ/μ=(0.0±1.0)×10−7\Delta\mu/\mu = (0.0\pm1.0)\times10^{-7}Δμ/μ=(0.0±1.0)×10−7 at a look-back time of about 7 billion years.

Setting

A transition with frequency ν\nuν has sensitivity coefficient KμK_\muKμ​ defined by

Δνν=Kμ Δμμ,\frac{\Delta\nu}{\nu} = K_\mu\,\frac{\Delta\mu}{\mu},νΔν​=Kμ​μΔμ​,

or, in infinitesimal form, Kμ=μνdνdμK_\mu = \frac{\mu}{\nu}\frac{d\nu}{d\mu}Kμ​=νμ​dμdν​. Pure rotational transitions have frequency inversely proportional to the reduced mass, hence to μ\muμ, so Kμ=−1K_\mu=-1Kμ​=−1. Mixed torsion–rotation transitions of methanol have strongly enhanced coefficients (Table 1 of the paper: −32.8-32.8−32.8 and −7.4-7.4−7.4).

Each observed line is assigned a position VVV, a velocity (km/s) on a common scale centred on redshift z=0.88582z=0.88582z=0.88582. If μ\muμ in the absorbing galaxy differs from the laboratory value by Δμ=μz−μlab\Delta\mu = \mu_z-\mu_{\mathrm{lab}}Δμ=μz​−μlab​, the positions satisfy

Vc=−Kμ Δμμ\frac{V}{c} = -K_\mu\,\frac{\Delta\mu}{\mu}cV​=−Kμ​μΔμ​

up to a velocity offset common to all lines, where ccc is the speed of light. Plotting VVV against KμK_\muKμ​ and fitting a straight line V=a+bKμV = a + bK_\muV=a+bKμ​ therefore gives Δμ/μ=−b/c\Delta\mu/\mu = -b/cΔμ/μ=−b/c.

The fit is a weighted least-squares fit with weights 1/σi21/\sigma_i^21/σi2​, where σi\sigma_iσi​ is the 1σ uncertainty of the iii-th position. With S=∑1/σi2S=\sum 1/\sigma_i^2S=∑1/σi2​, SK=∑Ki/σi2S_K=\sum K_i/\sigma_i^2SK​=∑Ki​/σi2​, SV=∑Vi/σi2S_V=\sum V_i/\sigma_i^2SV​=∑Vi​/σi2​, SKK=∑Ki2/σi2S_{KK}=\sum K_i^2/\sigma_i^2SKK​=∑Ki2​/σi2​, SKV=∑KiVi/σi2S_{KV}=\sum K_iV_i/\sigma_i^2SKV​=∑Ki​Vi​/σi2​ and Δ=SSKK−SK2\Delta=SS_{KK}-S_K^2Δ=SSKK​−SK2​, the slope, intercept and slope standard error are b=(SSKV−SKSV)/Δb=(SS_{KV}-S_KS_V)/\Deltab=(SSKV​−SK​SV​)/Δ, a=(SKKSV−SKSKV)/Δa=(S_{KK}S_V-S_KS_{KV})/\Deltaa=(SKK​SV​−SK​SKV​)/Δ and σb=S/Δ\sigma_b=\sqrt{S/\Delta}σb​=S/Δ​. The reduced chi-squared is χν2=1n−2∑i((Vi−a−bKi)/σi)2\chi^2_\nu=\frac{1}{n-2}\sum_i\big((V_i-a-bK_i)/\sigma_i\big)^2χν2​=n−21​∑i​((Vi​−a−bKi​)/σi​)2.

The data (Table 1) are four lines: 3−13_{-1}3−1​–20 E2_0\,E20​E (Kμ=−32.8K_\mu=-32.8Kμ​=−32.8, V=9.06±0.67V=9.06\pm0.67V=9.06±0.67), 000_000​–10 A+1_0\,A^+10​A+ (−1-1−1, 8.40±0.108.40\pm0.108.40±0.10), 000_000​–10 E1_0\,E10​E (−1-1−1, 9.12±0.309.12\pm0.309.12±0.30) and 2−12_{-1}2−1​–10 E1_0\,E10​E (−7.4-7.4−7.4, 9.83±0.439.83\pm0.439.83±0.43). Because A- and E-symmetry methanol behave as separate species that may be spatially segregated, the fiducial fit uses only the three E lines.

Formalization targets

Goal: the headline limit

With the E-line estimate Δμ/μ^=−b/c\widehat{\Delta\mu/\mu}=-b/cΔμ/μ​=−b/c, its statistical error σstat=σb/c\sigma_{\mathrm{stat}}=\sigma_b/cσstat​=σb​/c and the adopted systematic error σsys=7.0×10−8\sigma_{\mathrm{sys}}=7.0\times10^{-8}σsys​=7.0×10−8,

∣Δμ/μ^∣<0.05×10−7,∣σstat2+σsys2−1.0×10−7∣<0.05×10−7,\big|\widehat{\Delta\mu/\mu}\big| < 0.05\times10^{-7},\qquad \Big|\sqrt{\sigma_{\mathrm{stat}}^2+\sigma_{\mathrm{sys}}^2}-1.0\times10^{-7}\Big| < 0.05\times10^{-7},​Δμ/μ​​<0.05×10−7,​σstat2​+σsys2​​−1.0×10−7​<0.05×10−7,

i.e. Δμ/μ=(0.0±1.0)×10−7\Delta\mu/\mu=(0.0\pm1.0)\times10^{-7}Δμ/μ=(0.0±1.0)×10−7 to the printed precision.

Milestones

  1. Pure rotational transitions (ν∝1/μ\nu\propto1/\muν∝1/μ) have Kμ=−1K_\mu=-1Kμ​=−1.
  2. Under the exact relation Vi=a−c δ KiV_i=a-c\,\delta\,K_iVi​=a−cδKi​, the weighted fit returns −b/c=δ-b/c=\delta−b/c=δ and intercept aaa.
  3. E-line fit: Δμ/μ=(−0.1±7.6)×10−8\Delta\mu/\mu=(-0.1\pm7.6)\times10^{-8}Δμ/μ=(−0.1±7.6)×10−8, χν2≈2.0\chi^2_\nu\approx2.0χν2​≈2.0.
  4. The E-line result is consistent with Δμ=0\Delta\mu=0Δμ=0 at the 1.5×10−71.5\times10^{-7}1.5×10−7 (two-standard-error) level.
  5. Four-line fit: Δμ/μ=(11.0±6.8)×10−8\Delta\mu/\mu=(11.0\pm6.8)\times10^{-8}Δμ/μ=(11.0±6.8)×10−8, χν2≈6.4\chi^2_\nu\approx6.4χν2​≈6.4.
  6. The 000_000​–101_010​ A+A^+A+ and EEE lines are separated by 0.72±0.320.72\pm0.320.72±0.32 km/s.
  7. The A+A^+A+ anchor line shifted by 0.48±0.260.48\pm0.260.48±0.26 km/s between December 2011 and April 2012.

Significance

The result. The authors report the limit as statistically more constraining than previous radio-domain tests of a drifting μ\muμ. Because it uses a single molecular species, it is much less exposed to the main systematic of multi-species comparisons, namely that different molecules sit in different gas at slightly different velocities. The milestones record the internal evidence behind the choice of the fiducial fit: the poor four-line χν2\chi^2_\nuχν2​ and the A–E velocity separation.

Formalizing it. The physical inputs (sensitivity coefficients, measured positions, the systematic budget) are taken as data. What the mission checks by machine is the chain from those data to the printed numbers: the definition of the sensitivity coefficient and its value for rotational lines, the correctness of the line-fit estimator, and the arithmetic of every reported fit, separation and error combination.

Difficulty

The numerical milestones are exact statements about explicit rational data, but they involve nested sums, quotients and square roots, so a certified proof requires careful interval bounds rather than floating-point evaluation. The paper's numbers are rounded from unrounded measurements: recomputing from the rounded Table 1 entries gives, for example, σb/c≈7.69×10−8\sigma_b/c\approx7.69\times10^{-8}σb​/c≈7.69×10−8 instead of 7.6×10−87.6\times10^{-8}7.6×10−8, and χν2≈6.27\chi^2_\nu\approx6.27χν2​≈6.27 instead of 6.46.46.4 for the four-line fit. Tolerances therefore had to be chosen so that every statement is both faithful to the printed value and true for the tabulated data. The general recovery milestone requires showing that the normal equations are nondegenerate whenever the KiK_iKi​ are not all equal.

Formalization scope

  • All quantities are real numbers in Lean; data are finite families indexed by Fin n. Velocities are in km/s and c=299792.458c=299792.458c=299792.458 km/s.
  • The sensitivity coefficient is the logarithmic derivative (μ/ν(μ)) ν′(μ)(\mu/\nu(\mu))\,\nu'(\mu)(μ/ν(μ))ν′(μ) using Mathlib's deriv.
  • The fit uses the closed-form weighted least-squares formulas above; the reduced chi-squared divides by n−2n-2n−2.
  • The systematic uncertainty 7.0×10−87.0\times10^{-8}7.0×10−8 is an input; the variability model behind it is out of scope, as are the radiative-transfer column densities and the spectroscopic computation of KμK_\muKμ​ for mixed transitions.
  • "95% confidence level" is formalized as the two-standard-error interval.
  • Trivializing readings are excluded: every numerical statement is a closed statement about the tabulated data, with no free hypotheses, and the general recovery statement requires non-constant KKK and nonzero uncertainties.

Reusable pieces: the weighted least-squares definitions and the exact-recovery lemma apply to any straight-line fit with known uncertainties.

Selected references

  • J. Bagdonaite, P. Jansen, C. Henkel, H. L. Bethlem, K. M. Menten, W. Ubachs, A Stringent Limit on a Drifting Proton-to-Electron Mass Ratio from Alcohol in the Early Universe, Science, 2013. https://doi.org/10.1126/science.1224898
  • P. Jansen, L.-H. Xu, I. Kleiner, W. Ubachs, H. L. Bethlem, Methanol as a sensitive probe for spatial and temporal variations of the proton-to-electron mass ratio, Phys. Rev. Lett. 106, 100801, 2011. https://doi.org/10.1103/PhysRevLett.106.100801
  • S. P. Ellingsen, M. A. Voronkov, S. L. Breen, J. E. J. Lovell, First cosmological constraints on the proton-to-electron mass ratio from observations of rotational transitions of methanol, Astrophys. J. Lett. 747, L7, 2012. https://doi.org/10.1088/2041-8205/747/1/L7
  • Ph. R. Bevington, D. K. Robinson, Data Reduction and Error Analysis for the Physical Sciences, 3rd ed., McGraw-Hill, 2003.
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Differential Geometry·Captain: Lucas

Maldacena 1999 II: near-horizon geometries of M5-, M2- and D1-D5-branesResearch Paper

Motivation

In the paper that introduced the AdS/CFT correspondence (hep-th/9711200), Maldacena takes a stack of branes in string or M-theory, sends the string or Planck length to zero while holding the energies of the worldvolume theory fixed, and follows the supergravity solution of the branes through the same limit. The field theory on the branes decouples from the bulk, and the supergravity metric converges, after an overall rescaling, to a product of an anti-de Sitter space and a round sphere. The conjectured duality is between the worldvolume conformal field theory and string/M-theory on that product.

Section 2 of the paper treats D3-branes, whose limit is AdS5×S5\mathrm{AdS}_5\times S^5AdS5​×S5; that case, together with the Appendix on Poincaré coordinates for anti-de Sitter space, is the subject of the separate mission Maldacena 1999: the near-horizon geometry of D3-branes is AdS5 × S5. This mission covers the next three cases in the paper:

  1. Section 3.1: NNN coincident M5-branes, with limit AdS7×S4\mathrm{AdS}_7\times S^4AdS7​×S4;
  2. Section 3.2: NNN coincident M2-branes, with limit AdS4×S7\mathrm{AdS}_4\times S^7AdS4​×S7;
  3. Section 4: the D1–D5 system (Q1Q_1Q1​ D-strings and Q5Q_5Q5​ D5-branes wrapped on a four-manifold M4M^4M4), with limit AdS3×S3\mathrm{AdS}_3\times S^3AdS3​×S3 (times M4M^4M4).

In each case the paper states the ratio of the sphere radius to the anti-de Sitter "radius", and how both depend on the number of branes.

Setting

Anti-de Sitter space. For p≥0p\ge 0p≥0 and R>0R>0R>0, AdSp+2\mathrm{AdS}_{p+2}AdSp+2​ of radius RRR is the hyperboloid

−X−12−X02+X12+⋯+Xp2+Xp+12=−R2-X_{-1}^2-X_0^2+X_1^2+\dots+X_p^2+X_{p+1}^2=-R^2−X−12​−X02​+X12​+⋯+Xp2​+Xp+12​=−R2

in flat R2,p+1\mathbb R^{2,p+1}R2,p+1 (Appendix, eq. (A.1)). The Poincaré coordinates (U,x)(U,x)(U,x), with U>0U>0U>0 and x∈R1,px\in\mathbb R^{1,p}x∈R1,p, are given by U=X−1+Xp+1U=X_{-1}+X_{p+1}U=X−1​+Xp+1​, xa=XaR/Ux^a=X^aR/Uxa=XaR/U and X−1−Xp+1=x2U/R2+R2/UX_{-1}-X_{p+1}=x^2U/R^2+R^2/UX−1​−Xp+1​=x2U/R2+R2/U (eq. (A.2)). In these coordinates the induced metric is

ds2=U2R2 dx2+R2 dU2U2(A.3),ds^2=\frac{U^2}{R^2}\,dx^2+R^2\,\frac{dU^2}{U^2}\qquad\text{(A.3)},ds2=R2U2​dx2+R2U2dU2​(A.3),

where dx2=−dx02+dx12+⋯+dxp2dx^2=-dx_0^2+dx_1^2+\dots+dx_p^2dx2=−dx02​+dx12​+⋯+dxp2​. In Lean these objects are AdS, poincareEmbedding, ambientForm and minkowskiForm, taken from the published definition file Maldacena1999_Defs; the induced metric of a tangent vector is ambientForm applied to the Fréchet derivative of poincareEmbedding.

Brane metrics. Each brane solution has the form ds2=A(r) dx∥2+B(r) (dr2+r2dΩn2)ds^2=A(r)\,dx_\parallel^2+B(r)\,(dr^2+r^2d\Omega_n^2)ds2=A(r)dx∥2​+B(r)(dr2+r2dΩn2​), with dx∥2dx_\parallel^2dx∥2​ the Minkowski metric along the branes and dΩn2d\Omega_n^2dΩn2​ the round metric of the unit nnn-sphere:

  1. M5 (eq. (3.1)): A=f−1/3A=f^{-1/3}A=f−1/3, B=f2/3B=f^{2/3}B=f2/3, f=1+πNlp3/r3f=1+\pi Nl_p^3/r^3f=1+πNlp3​/r3, n=4n=4n=4;
  2. M2 (eq. (3.3)): A=f−2/3A=f^{-2/3}A=f−2/3, B=f1/3B=f^{1/3}B=f1/3, f=1+25π2Nlp6/r6f=1+2^5\pi^2Nl_p^6/r^6f=1+25π2Nlp6​/r6, n=7n=7n=7;
  3. D1–D5 (eq. (4.2)): A=f1−1/2f5−1/2A=f_1^{-1/2}f_5^{-1/2}A=f1−1/2​f5−1/2​, B=f11/2f51/2B=f_1^{1/2}f_5^{1/2}B=f11/2​f51/2​, f1=1+gα′Q1/(vr2)f_1=1+g\alpha'Q_1/(vr^2)f1​=1+gα′Q1​/(vr2), f5=1+gα′Q5/r2f_5=1+g\alpha'Q_5/r^2f5​=1+gα′Q5​/r2, n=3n=3n=3.

The decoupling limits hold fixed U2=r/lp3U^2=r/l_p^3U2=r/lp3​ (M5), U1/2=r/lp3/2U^{1/2}=r/l_p^{3/2}U1/2=r/lp3/2​ (M2), and U=r/α′U=r/\alpha'U=r/α′, vvv and g6=g/vg_6=g/\sqrt vg6​=g/v​ (D1–D5), while lp→0l_p\to 0lp​→0 or α′→0\alpha'\to 0α′→0. The Lean definitions m5Metric, m2Metric and d1d5Metric evaluate these metrics on a tangent vector (δx,δr,δω)(\delta x,\delta r,\delta\omega)(δx,δr,δω), where δω\delta\omegaδω is tangent at a point ω\omegaω of the unit sphere and dΩn2=∥δω∥2d\Omega_n^2=\|\delta\omega\|^2dΩn2​=∥δω∥2.

Formalization targets

Explicit limit metrics (milestones)

With δr\delta rδr written in terms of δU\delta UδU by the chain rule, the rescaled metrics converge to

ds2lp2→U2(πN)1/3dx∥2+4(πN)2/3dU2U2+(πN)2/3dΩ42(3.2)\frac{ds^2}{l_p^2}\to\frac{U^2}{(\pi N)^{1/3}}dx_\parallel^2+4(\pi N)^{2/3}\frac{dU^2}{U^2}+(\pi N)^{2/3}d\Omega_4^2\qquad(3.2)lp2​ds2​→(πN)1/3U2​dx∥2​+4(πN)2/3U2dU2​+(πN)2/3dΩ42​(3.2)

for M5-branes; to

ds2lp2→U2(25π2N)2/3dx∥2+(25π2N)1/34dU2U2+(25π2N)1/3dΩ72\frac{ds^2}{l_p^2}\to\frac{U^2}{(2^5\pi^2N)^{2/3}}dx_\parallel^2+\frac{(2^5\pi^2N)^{1/3}}{4}\frac{dU^2}{U^2}+(2^5\pi^2N)^{1/3}d\Omega_7^2lp2​ds2​→(25π2N)2/3U2​dx∥2​+4(25π2N)1/3​U2dU2​+(25π2N)1/3dΩ72​

for M2-branes; and to

ds2α′→U2g6Q1Q5dx∥2+g6Q1Q5dU2U2+g6Q1Q5 dΩ32(4.3)\frac{ds^2}{\alpha'}\to\frac{U^2}{g_6\sqrt{Q_1Q_5}}dx_\parallel^2+g_6\sqrt{Q_1Q_5}\frac{dU^2}{U^2}+g_6\sqrt{Q_1Q_5}\,d\Omega_3^2\qquad(4.3)α′ds2​→g6​Q1​Q5​​U2​dx∥2​+g6​Q1​Q5​​U2dU2​+g6​Q1​Q5​​dΩ32​(4.3)

for the D1–D5 system.

Goal: identification with AdS × sphere

The goal asserts that each limit equals the metric of AdSp+2×Sn\mathrm{AdS}_{p+2}\times S^nAdSp+2​×Sn (induced metric (A.3) plus a round sphere), with radii, in units of lpl_plp​ or α′\sqrt{\alpha'}α′​:

  1. M5: RAdS=2(πN)1/3R_{\rm AdS}=2(\pi N)^{1/3}RAdS​=2(πN)1/3, Rsph=(πN)1/3=RAdS/2R_{\rm sph}=(\pi N)^{1/3}=R_{\rm AdS}/2Rsph​=(πN)1/3=RAdS​/2;
  2. M2: RAdS=(25π2N)1/6/2R_{\rm AdS}=(2^5\pi^2N)^{1/6}/2RAdS​=(25π2N)1/6/2, Rsph=(25π2N)1/6=2RAdSR_{\rm sph}=(2^5\pi^2N)^{1/6}=2R_{\rm AdS}Rsph​=(25π2N)1/6=2RAdS​;
  3. D1–D5: RAdS2=Rsph2=g6Q1Q5R_{\rm AdS}^2=R_{\rm sph}^2=g_6\sqrt{Q_1Q_5}RAdS2​=Rsph2​=g6​Q1​Q5​​.

Significance

These three limits are the geometric input for the paper's conjectures that the six-dimensional (0,2)(0,2)(0,2) theory is dual to M-theory on AdS7×S4\mathrm{AdS}_7\times S^4AdS7​×S4, the M2-brane theory to M-theory on AdS4×S7\mathrm{AdS}_4\times S^7AdS4​×S7, and the two-dimensional (4,4)(4,4)(4,4) theory of the D1–D5 system to IIB string theory on AdS3×S3×M4\mathrm{AdS}_3\times S^3\times M^4AdS3​×S3×M4. The radii set the regime in which supergravity can be trusted (large NNN, or large g6Qig_6Q_ig6​Qi​). They also fix which anti-de Sitter isometry group appears (SO(2,6)SO(2,6)SO(2,6), SO(2,3)SO(2,3)SO(2,3), SO(2,2)SO(2,2)SO(2,2)); the paper matches it with the bosonic conformal group of the brane theory.

The paper derives these limits in a few lines each. To our knowledge they have not been formalized. The mission produces machine-checked statements and proofs of the three limits and of their identification with anti-de Sitter geometry, reusing the published Poincaré-coordinate results of the D3-brane mission.

Difficulty

The computation is elementary but full of exponents. Each case needs a change of radial variable, a fractional power of a harmonic function whose constant term is dropped in the limit, and a comparison of the coefficient of dU2dU^2dU2 with the Poincaré form, which in the M5 and M2 cases requires a constant rescaling of UUU. In Lean, the limits are one-sided limits lp→0+l_p\to0^+lp​→0+ of expressions built from real powers Real.rpow, and the goal requires a Fréchet-derivative computation on R×Rp+1\mathbb R\times\mathbb R^{p+1}R×Rp+1 (available from the published theorem Maldacena1999.induced_metric_poincare).

Formalization scope

All metrics are evaluated pointwise on tangent vectors; no manifold structure is used. The round sphere SnS^nSn is the unit sphere in Euclidean Rn+1\mathbb R^{n+1}Rn+1 and a tangent vector at ω\omegaω is a δω\delta\omegaδω with ⟨ω,δω⟩=0\langle\omega,\delta\omega\rangle=0⟨ω,δω⟩=0. The limits are taken along lp→0+l_p\to0^+lp​→0+ (resp. α′→0+\alpha'\to0^+α′→0+) with UUU, NNN, ggg, vvv, QiQ_iQi​ and the tangent vector fixed. For the D1–D5 system only the six-dimensional metric (4.2) is formalized: the compact factor M4M^4M4, whose volume is constant in the limit, is not modelled. In the goal the anti-de Sitter coordinate is the paper's UUU up to a constant factor (U′=2(πN)1/6UU'=2(\pi N)^{1/6}UU′=2(πN)1/6U for M5, U′=U/(2(25π2N)1/6)U'=U/(2(2^5\pi^2N)^{1/6})U′=U/(2(25π2N)1/6) for M2, U′=UU'=UU′=U for D1–D5), so that the limit metric has exactly the form (A.3). All physical parameters are strictly positive. Fluxes, supersymmetry and the duality conjectures themselves are out of scope.

Selected references

  • J. Maldacena, The Large-N Limit of Superconformal Field Theories and Supergravity, Int. J. Theor. Phys. 38 (1999) 1113–1133. https://arxiv.org/abs/hep-th/9711200
  • G. Horowitz and A. Strominger, Black strings and p-branes, Nucl. Phys. B 360 (1991) 197. https://doi.org/10.1016/0550-3213(91)90440-9
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Differential Geometry·Captain: Lucas

Maldacena 1999: the near-horizon geometry of D3-branes is AdS5 × S5Research Paper

Motivation

In 1997 Maldacena observed that the low-energy limit of a stack of NNN coincident D3-branes in type IIB string theory can be described in two ways: as four-dimensional N=4\mathcal N=4N=4 U(N)U(N)U(N) super-Yang–Mills theory living on the branes, and as supergravity (ultimately string theory) on the near-horizon geometry of the branes. The paper computes that this near-horizon geometry is five-dimensional anti-de Sitter space times a five-sphere, AdS5×S5\mathrm{AdS}_5\times S^5AdS5​×S5, with both factors of the same radius RRR, R4=4πgNR^4=4\pi gNR4=4πgN in string units, and conjectures that the two descriptions are dual. This AdS/CFT correspondence became one of the most cited results in theoretical physics (Maldacena 1999; see also Gubser–Klebanov–Polyakov 1998, Witten 1998).

The duality itself is a physical conjecture with no complete mathematical formulation. What the paper does contain is a small body of exact geometric computations on which the conjecture rests: the decoupling limit of the D3-brane metric, the description of AdS as a hyperboloid with its SO(2,p+1)SO(2,p+1)SO(2,p+1) symmetry, the Poincaré coordinates in which the limiting metric is written, and the ordinary differential equation expressing broken conformal invariance of a probe brane. This mission formalizes exactly those computations.

Setting

Fix p≥0p\ge0p≥0. The ambient space R2,p+1\mathbb R^{2,p+1}R2,p+1 has coordinates X−1,X0,X1,…,Xp,Xp+1X_{-1},X_0,X_1,\dots,X_p,X_{p+1}X−1​,X0​,X1​,…,Xp​,Xp+1​ and flat metric η=diag(−1,−1,1,…,1)\eta=\mathrm{diag}(-1,-1,1,\dots,1)η=diag(−1,−1,1,…,1). Anti-de Sitter space of radius RRR is the hyperboloid (eq. (A.1))

AdSp+2(R)={X:−X−12−X02+X12+⋯+Xp2+Xp+12=−R2}.\mathrm{AdS}_{p+2}(R)=\{X : -X_{-1}^2-X_0^2+X_1^2+\cdots+X_p^2+X_{p+1}^2=-R^2\}.AdSp+2​(R)={X:−X−12​−X02​+X12​+⋯+Xp2​+Xp+12​=−R2}.

Linear maps preserving η\etaη form the group O(2,p+1)O(2,p+1)O(2,p+1), which contains the conformal group SO(2,p+1)SO(2,p+1)SO(2,p+1) of (p+1)(p+1)(p+1)-dimensional Minkowski space.

The Poincaré coordinates (eq. (A.2)) are U=X−1+Xp+1U=X_{-1}+X_{p+1}U=X−1​+Xp+1​ and xα=XαR/Ux_\alpha=X_\alpha R/Uxα​=Xα​R/U for α=0,…,p\alpha=0,\dots,pα=0,…,p; on the hyperboloid, V=X−1−Xp+1=x2U/R2+R2/UV=X_{-1}-X_{p+1}=x^2U/R^2+R^2/UV=X−1​−Xp+1​=x2U/R2+R2/U, where x2=−x02+x12+⋯+xp2x^2=-x_0^2+x_1^2+\cdots+x_p^2x2=−x02​+x12​+⋯+xp2​. Written in reverse, this is a map ΦR:(U,x)↦X\Phi_R:(U,x)\mapsto XΦR​:(U,x)↦X.

The D3-brane metric (eq. (2.2)) for string coupling ggg, NNN branes and string scale α′\alpha'α′ is

ds2=f−1/2dx∥2+f1/2(dr2+r2dΩ52),f=1+4πgNα′2r4,ds^2=f^{-1/2}dx_\parallel^2+f^{1/2}\big(dr^2+r^2d\Omega_5^2\big),\qquad f=1+\frac{4\pi gN\alpha'^2}{r^4},ds2=f−1/2dx∥2​+f1/2(dr2+r2dΩ52​),f=1+r44πgNα′2​,

where x∥∈R1,3x_\parallel\in\mathbb R^{1,3}x∥​∈R1,3 are the worldvolume coordinates and dΩ52d\Omega_5^2dΩ52​ is the round metric of the unit five-sphere. The decoupling limit (eq. (2.1)) sends α′→0\alpha'\to0α′→0 keeping U=r/α′U=r/\alpha'U=r/α′ fixed.

Formalization targets

Goal: the near-horizon geometry is AdS5×S5\mathrm{AdS}_5\times S^5AdS5​×S5

For g>0g>0g>0, N≥1N\ge1N≥1, R>0R>0R>0 with R4=4πgNR^4=4\pi gNR4=4πgN, U>0U>0U>0 and every tangent vector (δx,δU,δω)(\delta x,\delta U,\delta\omega)(δx,δU,δω) with δω\delta\omegaδω tangent to S5S^5S5,

lim⁡α′→0+1α′ dsα′2∣r=α′U, δr=α′δU=⟨dΦR[δU,δx],dΦR[δU,δx]⟩η+R2∥δω∥2,\lim_{\alpha'\to0^+}\frac{1}{\alpha'}\,ds^2_{\alpha'}\Big|_{r=\alpha'U,\ \delta r=\alpha'\delta U}=\big\langle d\Phi_R[\delta U,\delta x],d\Phi_R[\delta U,\delta x]\big\rangle_\eta+R^2\|\delta\omega\|^2 ,α′→0+lim​α′1​dsα′2​​r=α′U, δr=α′δU​=⟨dΦR​[δU,δx],dΦR​[δU,δx]⟩η​+R2∥δω∥2,

which is eq. (2.3): the metric of AdS5(R)\mathrm{AdS}_5(R)AdS5​(R) in Poincaré coordinates plus the round metric of S5S^5S5 of the same radius.

Milestones

  1. (A.1)–(A.2) ΦR(U,x)∈AdSp+2(R)\Phi_R(U,x)\in\mathrm{AdS}_{p+2}(R)ΦR​(U,x)∈AdSp+2​(R) for U>0U>0U>0.
  2. Appendix ΦR\Phi_RΦR​ is a bijection from {U>0}\{U>0\}{U>0} onto {X∈AdSp+2(R):X−1+Xp+1>0}\{X\in\mathrm{AdS}_{p+2}(R): X_{-1}+X_{p+1}>0\}{X∈AdSp+2​(R):X−1​+Xp+1​>0}.
  3. (A.3) the induced metric is U2R2dx2+R2dU2U2\frac{U^2}{R^2}dx^2+R^2\frac{dU^2}{U^2}R2U2​dx2+R2U2dU2​.
  4. Appendix every AAA with ATηA=ηA^{\mathsf T}\eta A=\etaATηA=η preserves AdSp+2(R)\mathrm{AdS}_{p+2}(R)AdSp+2​(R).
  5. (2.2)→(2.3) the three metric coefficients divided by α′\alpha'α′ converge to U2/4πgNU^2/\sqrt{4\pi gN}U2/4πgN​, 4πgN/U2\sqrt{4\pi gN}/U^24πgN​/U2 and 4πgN\sqrt{4\pi gN}4πgN​.
  6. (2.9) on z>−1/R~4z>-1/\tilde R^4z>−1/R~4, the differentiable solutions of f(z)+c=2(z+R~−4)f′(z)f(z)+c=2(z+\tilde R^{-4})f'(z)f(z)+c=2(z+R~−4)f′(z) are exactly f=b1+R~4z−cf=b\sqrt{1+\tilde R^4z}-cf=b1+R~4z​−c.

Significance

The goal is the precise sense in which "the near-horizon geometry of NNN D3-branes is AdS5×S5\mathrm{AdS}_5\times S^5AdS5​×S5 with R4=4πgNR^4=4\pi gNR4=4πgN": the radius formula is what later links the 't Hooft coupling gYM2Ng^2_{YM}NgYM2​N of the gauge theory to the curvature of the string background, and the Poincaré-patch form (A.3) is the coordinate system in which essentially all subsequent AdS/CFT computations are carried out. Milestones 1–4 give a reusable, self-contained account of anti-de Sitter space as a quadric in R2,p+1\mathbb R^{2,p+1}R2,p+1 with its Poincaré chart, useful to any development of Lorentzian geometry. Milestone 6 is the step by which the paper argues that the probe D3-brane action (2.6) is fixed by conformal symmetry.

All of these statements are standard computations in the physics literature; none is open. The value of the mission is a machine-checked version of the geometric content of the paper, stated with the paper's own conventions, not a new result. The duality conjecture itself is outside the scope of the mission.

Difficulty

The computations are elementary but bookkeeping-heavy. The induced-metric identity (A.3) requires differentiating a map from R×Rp+1\mathbb R\times\mathbb R^{p+1}R×Rp+1 to Rp+3\mathbb R^{p+3}Rp+3 with ppp arbitrary, so sums over the index sets must be split into the timelike, spacelike and light-cone components; a computation for one fixed ppp does not suffice. The bijection statement needs an explicit inverse and the observation that the hyperboloid equation determines VVV from UUU and xxx. The limit statements require controlling square roots of expressions that blow up like α′−2\alpha'^{-2}α′−2. The ODE characterisation requires a uniqueness argument on an interval, not only verification that the stated function is a solution.

Formalization scope

Coordinates of R2,p+1\mathbb R^{2,p+1}R2,p+1 are indexed by {0,…,p+2}\{0,\dots,p+2\}{0,…,p+2} with index 000 for X−1X_{-1}X−1​, index 111 for X0X_0X0​ and index k+1k+1k+1 for XkX_kXk​; worldvolume coordinates are indexed by {0,…,p}\{0,\dots,p\}{0,…,p} with index 000 timelike. Metrics are represented by the quadratic forms they induce on tangent vectors; the induced metric is expressed through the Fréchet derivative of ΦR\Phi_RΦR​. The round metric of S5S^5S5 is the Euclidean norm squared of a tangent vector of the unit sphere in R6\mathbb R^6R6. Square roots and divisions are Lean's total functions; all statements restrict to R>0R>0R>0, U>0U>0U>0, g>0g>0g>0, N≥1N\ge1N≥1, α′>0\alpha'>0α′>0, where no junk values arise. The symmetry milestone is stated for the full group O(2,p+1)O(2,p+1)O(2,p+1), which contains the SO(2,p+1)SO(2,p+1)SO(2,p+1) named in the paper.

No new infrastructure beyond Mathlib's calculus, real analysis and matrix libraries is needed. Contributions of general lemmas about quadrics in pseudo-Euclidean spaces are welcome.

Selected references

  • J. Maldacena, The Large-N Limit of Superconformal Field Theories and Supergravity, Int. J. Theor. Phys. 38 (1999) 1113–1133. https://arxiv.org/abs/hep-th/9711200
  • S. S. Gubser, I. R. Klebanov, A. M. Polyakov, Gauge theory correlators from non-critical string theory, Phys. Lett. B 428 (1998) 105–114. https://arxiv.org/abs/hep-th/9802109
  • E. Witten, Anti de Sitter space and holography, Adv. Theor. Math. Phys. 2 (1998) 253–291. https://arxiv.org/abs/hep-th/9802150
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Quantum Information·Captain: Lucas

Projective Measurements Are Equilibration Processes (finite dimension)Research Paper

Motivation

Projective measurement is usually taught together with state update: an observable is measured, a value is obtained, and the conditional state is assigned. These are two different questions. The first is the prediction of the outgoing ensemble from the incoming ensemble and the measured observable alone, before the outcome is known; the second is the incorporation of the outcome once it is known. The technical brief by G. Carcassi for the Assumptions of Physics collaboration (AoP technical briefs) isolates the first question and treats the measurement as a black-box process that only relates incoming and outgoing ensembles, without committing to a mechanism.

Within this view the standard prediction, the nonselective (Lüders) post-measurement ensemble, admits several characterizations that come from different traditions: the algebraic pinching map, the long-time limit of a dephasing Lindblad equation (open quantum systems, see Lindblad 1976), and a closest-point principle, either in Hilbert–Schmidt distance or in quantum relative entropy (Umegaki 1962). The brief's Theorem 1 states that these characterizations select the same process.

Setting

Fix a finite index set nnn; the Hilbert space is Cn\mathbb C^nCn and operators are complex n×nn\times nn×n matrices. A density matrix is a positive semidefinite matrix ρ\rhoρ with tr⁡ρ=1\operatorname{tr}\rho=1trρ=1. An observable is a Hermitian matrix XXX with spectral decomposition

X=∑xx Px,X=\sum_{x}x\,P_x ,X=x∑​xPx​,

where xxx ranges over the distinct eigenvalues of XXX and PxP_xPx​ is the orthogonal projection onto the xxx-eigenspace.

  • The pinching of ρ\rhoρ is PX(ρ)=∑xPxρPx\mathcal P_X(\rho)=\sum_x P_x\rho P_xPX​(ρ)=∑x​Px​ρPx​.
  • The dephasing Lindblad equation with vanishing Hamiltonian and jump operator XXX is dρdt=XρX−12{X2,ρ}\dfrac{d\rho}{dt}=X\rho X-\tfrac12\{X^2,\rho\}dtdρ​=XρX−21​{X2,ρ}, t≥0t\ge0t≥0.
  • The Hilbert–Schmidt distance is ∥ρ−σ∥HS=(tr⁡(ρ−σ)∗(ρ−σ))1/2\|\rho-\sigma\|_{HS}=\big(\operatorname{tr}(\rho-\sigma)^*(\rho-\sigma)\big)^{1/2}∥ρ−σ∥HS​=(tr(ρ−σ)∗(ρ−σ))1/2.
  • The relative entropy is D(ρ∥σ)=tr⁡(ρlog⁡ρ)−tr⁡(ρlog⁡σ)D(\rho\|\sigma)=\operatorname{tr}(\rho\log\rho)-\operatorname{tr}(\rho\log\sigma)D(ρ∥σ)=tr(ρlogρ)−tr(ρlogσ) when supp⁡ρ⊆supp⁡σ\operatorname{supp}\rho\subseteq\operatorname{supp}\sigmasuppρ⊆suppσ and +∞+\infty+∞ otherwise; the von Neumann entropy is S(ρ)=−tr⁡(ρlog⁡ρ)S(\rho)=-\operatorname{tr}(\rho\log\rho)S(ρ)=−tr(ρlogρ).

The spectral equilibration process ΦX\Phi_XΦX​ is an unknown map on density matrices. The brief's four conditions on it are:

  • EQ-MEAS: ΦX(ρ)=∑xPxρPx\Phi_X(\rho)=\sum_xP_x\rho P_xΦX​(ρ)=∑x​Px​ρPx​.
  • EQ-LIND: ΦX(ρ)=lim⁡t→∞ρ(t)\Phi_X(\rho)=\lim_{t\to\infty}\rho(t)ΦX​(ρ)=limt→∞​ρ(t) for the Lindblad evolution with ρ(0)=ρ\rho(0)=\rhoρ(0)=ρ.
  • EQ-HS: ΦX(ρ)=argmin⁡{∥ρ−σ∥HS2: σ a density matrix, [σ,X]=0}\Phi_X(\rho)=\operatorname{argmin}\{\|\rho-\sigma\|_{HS}^2:\ \sigma \text{ a density matrix},\ [\sigma,X]=0\}ΦX​(ρ)=argmin{∥ρ−σ∥HS2​: σ a density matrix, [σ,X]=0}.
  • EQ-KL: ΦX(ρ)=argmin⁡{D(ρ∥σ): σ a density matrix, [σ,X]=0}\Phi_X(\rho)=\operatorname{argmin}\{D(\rho\|\sigma):\ \sigma \text{ a density matrix},\ [\sigma,X]=0\}ΦX​(ρ)=argmin{D(ρ∥σ): σ a density matrix, [σ,X]=0}.

Formalization targets

Goal: Theorem 1 (finite-dimensional form)

For every Hermitian XXX and every map Φ\PhiΦ,

EQ-MEAS  ⟺  EQ-LIND,EQ-MEAS  ⟺  EQ-HS,EQ-MEAS  ⟺  EQ-KL.\text{EQ-MEAS}\iff\text{EQ-LIND},\qquad \text{EQ-MEAS}\iff\text{EQ-HS},\qquad \text{EQ-MEAS}\iff\text{EQ-KL}.EQ-MEAS⟺EQ-LIND,EQ-MEAS⟺EQ-HS,EQ-MEAS⟺EQ-KL.

Milestones

The milestones follow the steps of the brief's proof: the block decomposition ρ=∑x,yPxρPy\rho=\sum_{x,y}P_x\rho P_yρ=∑x,y​Px​ρPy​ (eq. 2); the blockwise solution Pxρ(t)Py=e−t2(x−y)2Pxρ(0)PyP_x\rho(t)P_y=e^{-\frac t2(x-y)^2}P_x\rho(0)P_yPx​ρ(t)Py​=e−2t​(x−y)2Px​ρ(0)Py​ (eqs. 4–5); convergence ρ(t)→PX(ρ)\rho(t)\to\mathcal P_X(\rho)ρ(t)→PX​(ρ) (eqs. 9–10) and EQ-LIND ⇔\Leftrightarrow⇔ EQ-MEAS; the equivalence [σ,X]=0  ⟺  PX(σ)=σ[\sigma,X]=0\iff\mathcal P_X(\sigma)=\sigma[σ,X]=0⟺PX​(σ)=σ; PX\mathcal P_XPX​ preserves density matrices; the Pythagorean identity (eq. 11) and EQ-HS ⇔\Leftrightarrow⇔ EQ-MEAS; the relative-entropy chain rule (eq. 12); D(ρ∥PXρ)=S(PXρ)−S(ρ)D(\rho\|\mathcal P_X\rho)=S(\mathcal P_X\rho)-S(\rho)D(ρ∥PX​ρ)=S(PX​ρ)−S(ρ) (eq. 13); non-negativity and definiteness of DDD; and EQ-KL ⇔\Leftrightarrow⇔ EQ-MEAS.

Significance

The result says that "projective measurement" can be specified without reference to wave-function collapse: any of the three dynamical or variational descriptions pins down the same input–output map. Downstream, this justifies treating repeatable measurements as equilibration processes whose outputs are fixed points, and treating the outcome-update step as classical conditioning on a mixture.

The mathematics in finite dimension is classical; this mission asks for a machine-checked proof of the equivalence in Lean 4 with Mathlib. A complete development produces reusable pieces: spectral projections and the pinching map for Hermitian matrices, explicit solutions and asymptotics of a dephasing Lindblad semigroup, and an extended-real relative entropy with Klein's inequality.

Difficulty

The Hilbert–Schmidt part is linear algebra once block-diagonality is in place. The Lindblad part requires uniqueness of solutions of a linear matrix ODE on the closed half-line, to transfer the explicit blockwise formula to an arbitrary solution. The relative-entropy part is the most delicate: it needs the interaction between the functional-calculus logarithm and block structure (log⁡σ\log\sigmalogσ is block diagonal when σ\sigmaσ commutes with XXX), the support conventions that make DDD take the value +∞+\infty+∞, and Klein's inequality with its equality case for matrices, which the development must supply if the library does not already provide it.

Formalization scope

  • Finite dimension only. The Hilbert space is Cn\mathbb C^nCn for a finite type nnn, so all observables are bounded with pure point spectrum and every density matrix has finite entropy. The brief also covers separable infinite-dimensional spaces and unbounded observables (where Condition [B]FINENT is a genuine restriction); that regime is not part of this mission.
  • Spectral data. PxP_xPx​ is built from Mathlib's eigen-decomposition of a Hermitian matrix and is defined for every real xxx (zero when xxx is not an eigenvalue); the pinching sums over the finite set of distinct eigenvalues.
  • Lindblad solutions. A solution is any function R→Mn(C)\mathbb R\to M_n(\mathbb C)R→Mn​(C) with the given initial value whose derivative within [0,∞)[0,\infty)[0,∞) satisfies the equation for t≥0t\ge0t≥0. EQ-LIND requires existence of a solution and convergence of every solution, so it cannot hold vacuously.
  • Argmin. "Φ(ρ)=argmin⁡\Phi(\rho)=\operatorname{argmin}Φ(ρ)=argmin" is encoded as "Φ(ρ)\Phi(\rho)Φ(ρ) is a feasible minimizer"; uniqueness is a consequence proved by the theorem, not an assumption.
  • Logarithm and relative entropy. log⁡\loglog is the continuous functional calculus applied to Real.log (so log⁡0=0\log0=0log0=0, i.e. the logarithm on the support); DDD takes values in the extended reals and equals +∞+\infty+∞ unless ker⁡σ⊆ker⁡ρ\ker\sigma\subseteq\ker\rhokerσ⊆kerρ.
  • Convergence is in the entrywise topology, which coincides with the trace-norm and Hilbert–Schmidt topologies in finite dimension.

Contributions of general-purpose lemmas (Klein's inequality, uniqueness for linear ODEs on half-lines, properties of pinching) are welcome as separate theorems.

Selected references

  • G. Carcassi (Assumptions of Physics collaboration), Projective measurements are equilibration processes, AoP Technical Brief 017. https://assumptionsofphysics.org/resources/briefs
  • G. Lindblad, On the generators of quantum dynamical semigroups, Comm. Math. Phys. 48 (1976) 119–130. https://doi.org/10.1007/BF01608499
  • H. Umegaki, Conditional expectation in an operator algebra. IV. Entropy and information, Kodai Math. Sem. Rep. 14 (1962) 59–85. https://doi.org/10.2996/kmj/1138844604
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Analysis·Captain: Lucas

Feynman 1948: The Path-Integral Wave Function Satisfies Schrödinger's EquationResearch Paper

Motivation

In 1948 R. P. Feynman published a third formulation of non-relativistic quantum mechanics, alongside Schrödinger's differential equation and Heisenberg's matrix algebra (Feynman 1948). The probability amplitude for a particle to follow a path x(t)x(t)x(t) is postulated to be exp⁡(iℏS[x])\exp\big(\tfrac{i}{\hbar}S[x]\big)exp(ℏi​S[x]), with SSS the classical action, and the amplitude to arrive at (x,t)(x,t)(x,t) is the sum of these contributions over all paths from the past. This is the path integral, now a standard tool across quantum field theory, statistical mechanics and probability.

The formulation is claimed to be mathematically equivalent to ordinary quantum mechanics. The key step of that claim is Section 6 of the paper, "The wave equation": the wave function defined by the path integral satisfies Schrödinger's equation. This mission formalizes that step for a particle in one dimension, as the paper does.

Timeline:

  • 1933/1945 — Dirac remarks on the role of the classical action in quantum mechanics, the starting point cited by Feynman.
  • 1948 — Feynman, Rev. Mod. Phys. 20, 367: path-integral postulates, definition of the wave function (Section 5), derivation of Schrödinger's equation (Section 6).
  • 1949 — Kac gives the rigorous imaginary-time (Wiener-measure) analogue, the Feynman–Kac formula.
  • 1964 — Nelson derives the real-time Feynman formula rigorously from the Trotter product formula; oscillatory-integral approaches follow later.

Setting

Fix ℏ>0\hbar>0ℏ>0, a mass m>0m>0m>0 and a potential V:R→RV:\mathbb R\to\mathbb RV:R→R. For a time step ε>0\varepsilon>0ε>0 the short-time action between positions yyy (time ttt) and xxx (time t+εt+\varepsilont+ε) is (Eq. 22)

S(x,y)=mε2(x−yε)2−εV(x),S(x,y)=\frac{m\varepsilon}{2}\Big(\frac{x-y}{\varepsilon}\Big)^2-\varepsilon V(x),S(x,y)=2mε​(εx−y​)2−εV(x),

and the normalizing factor is A(ε)=(2πℏεi/m)1/2A(\varepsilon)=(2\pi\hbar\varepsilon i/m)^{1/2}A(ε)=(2πℏεi/m)1/2 (Eq. 28, principal branch). The one-step path-integral evolution (Eqs. 18, 23) takes a wave function ψ:R→C\psi:\mathbb R\to\mathbb Cψ:R→C to

(Uεψ)(x)=1A(ε)∫Rexp⁡ ⁣(iℏS(x,y))ψ(y) dy.(U_\varepsilon\psi)(x)=\frac{1}{A(\varepsilon)}\int_{\mathbb R}\exp\!\Big(\frac{i}{\hbar}S(x,y)\Big)\psi(y)\,dy .(Uε​ψ)(x)=A(ε)1​∫R​exp(ℏi​S(x,y))ψ(y)dy.

Iterating UεU_\varepsilonUε​ and letting ε→0\varepsilon\to0ε→0 is the path integral (15) of Section 5. The Hamiltonian is Hψ=−ℏ22mψ′′+VψH\psi=-\frac{\hbar^2}{2m}\psi''+V\psiHψ=−2mℏ2​ψ′′+Vψ. The paper also uses the Gaussian moments of Eq. (26), which are oscillatory; footnote 13 defines them by replacing ℏ\hbarℏ with ℏ(1−iδ)\hbar(1-i\delta)ℏ(1−iδ) and letting δ→0+\delta\to0^+δ→0+:

Mn(δ)=∫Rξnexp⁡ ⁣(imξ22ℏ(1−iδ)ε)dξ.M_n(\delta)=\int_{\mathbb R}\xi^n\exp\!\Big(\frac{im\xi^2}{2\hbar(1-i\delta)\varepsilon}\Big)d\xi .Mn​(δ)=∫R​ξnexp(2ℏ(1−iδ)εimξ2​)dξ.

Formalization targets

Goal — Eq. (30)

For every Schwartz function ψ\psiψ and every x∈Rx\in\mathbb Rx∈R,

lim⁡ε→0+(Uεψ)(x)−ψ(x)ε=−iℏ(−ℏ22mψ′′(x)+V(x)ψ(x)),\lim_{\varepsilon\to0^+}\frac{(U_\varepsilon\psi)(x)-\psi(x)}{\varepsilon}=-\frac{i}{\hbar}\Big(-\frac{\hbar^2}{2m}\psi''(x)+V(x)\psi(x)\Big),ε→0+lim​ε(Uε​ψ)(x)−ψ(x)​=−ℏi​(−2mℏ2​ψ′′(x)+V(x)ψ(x)),

that is, −ℏi∂tψ=12m(ℏi∂x)2ψ+Vψ-\frac{\hbar}{i}\partial_t\psi=\frac{1}{2m}\big(\frac{\hbar}{i}\partial_x\big)^2\psi+V\psi−iℏ​∂t​ψ=2m1​(iℏ​∂x​)2ψ+Vψ for the path-integral evolution, which is Schrödinger's equation (30). This is the content of Feynman's statement that (18), valid to first order in ε\varepsilonε, yields (30).

Milestones

  1. Eq. (26), the three regularized Fresnel integrals: M0(δ)→AM_0(\delta)\to AM0​(δ)→A, M1(δ)=0M_1(\delta)=0M1​(δ)=0, M2(δ)→ℏεimAM_2(\delta)\to\frac{\hbar\varepsilon i}{m}AM2​(δ)→mℏεi​A.
  2. Eqs. (27)–(28), zero-order agreement: (Uεψ)(x)→ψ(x)(U_\varepsilon\psi)(x)\to\psi(x)(Uε​ψ)(x)→ψ(x); this is the condition that fixes AAA.
  3. Eq. (27) for the free particle: ((Uεψ)(x)−ψ(x))/ε→ℏi2mψ′′(x)\big((U_\varepsilon\psi)(x)-\psi(x)\big)/\varepsilon\to\frac{\hbar i}{2m}\psi''(x)((Uε​ψ)(x)−ψ(x))/ε→2mℏi​ψ′′(x) when V=0V=0V=0.
  4. Footnote 15: for the free particle (18) is exact, UεUδψ=Uε+δψU_\varepsilon U_\delta\psi=U_{\varepsilon+\delta}\psiUε​Uδ​ψ=Uε+δ​ψ.

Significance

The goal is the step that connects the path-integral postulates to the ordinary formulation: without it the formulation of Sections 3–5 is not known to reproduce any quantum mechanics. The Fresnel integrals of (26) and the short-time kernel appear throughout semiclassical analysis and in every derivation of path integrals from the Schrödinger equation.

The physics result is classical and its rigorous versions are known (via the Trotter product formula or oscillatory-integral estimates). The work here is the formalization: Mathlib has the complex Gaussian integral and Schwartz functions, but not Fresnel integrals, the free Schrödinger kernel, or the short-time asymptotics of oscillatory integrals. None of the targets is currently formalized on the platform.

Difficulty

Feynman's derivation expands ψ(x−ξ)\psi(x-\xi)ψ(x−ξ) in a Taylor series under the integral and integrates term by term against exp⁡(imξ2/2ℏε)\exp(im\xi^2/2\hbar\varepsilon)exp(imξ2/2ℏε). Those integrals are not absolutely convergent, and the higher moments do not even exist as improper Riemann integrals, so the term-by-term step is not justified as written. A proof has to control the Taylor remainder against an oscillatory kernel whose width is of order ℏε/m\sqrt{\hbar\varepsilon/m}ℏε/m​, uniformly as ε→0+\varepsilon\to0^+ε→0+, with a prefactor 1/A1/A1/A that blows up like ε−1/2\varepsilon^{-1/2}ε−1/2. The naive dominated-convergence argument does not apply, because the kernel has modulus ∣A∣−1|A|^{-1}∣A∣−1 everywhere and does not concentrate in absolute value.

Formalization scope

  • One space dimension, real potential VVV with no regularity assumptions (it enters only through V(x)V(x)V(x) at the fixed point, as in Eq. (23)).
  • Wave functions are Schwartz functions 𝓢(ℝ, ℂ), which formalizes the paper's "relatively smooth" ψ\psiψ that "falls off sufficiently for large xxx". For such ψ\psiψ the integral defining UεψU_\varepsilon\psiUε​ψ is absolutely convergent, so the Lebesgue (Bochner) integral is used.
  • ℏ>0\hbar>0ℏ>0, m>0m>0m>0 are hypotheses; limits in ε\varepsilonε and δ\deltaδ are one-sided, →0+\to0^+→0+.
  • AAA uses Mathlib's principal complex power z1/2z^{1/2}z1/2.
  • The Gaussian moments are regularized as in footnote 13 (ℏ→ℏ(1−iδ)\hbar\to\hbar(1-i\delta)ℏ→ℏ(1−iδ)), because the bare integrals are not Lebesgue integrable and the Bochner integral would silently return 000.
  • The goal is pointwise in xxx and concerns the generator of one step; it does not assert convergence of the full time-sliced path integral (a Trotter-type statement), which would be a natural follow-up mission.

Useful infrastructure: Fresnel integrals, Fourier representation of the free Schrödinger kernel on Schwartz space, and differentiation of oscillatory integrals with a parameter. All are reusable beyond this mission.

Selected references

  • R. P. Feynman, Space-Time Approach to Non-Relativistic Quantum Mechanics, Rev. Mod. Phys. 20, 367 (1948). https://doi.org/10.1103/RevModPhys.20.367
  • P. A. M. Dirac, On the Analogy Between Classical and Quantum Mechanics, Rev. Mod. Phys. 17, 195 (1945). https://doi.org/10.1103/RevModPhys.17.195
  • M. Kac, On distributions of certain Wiener functionals, Trans. Amer. Math. Soc. 65, 1 (1949).
  • E. Nelson, Feynman integrals and the Schrödinger equation, J. Math. Phys. 5, 332 (1964).
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