Prove2Me
Navigate
DiscoverCollectionsFormalpediaBlogsUsersMomentumMy Missions+
Prove2Me
⌕
Log in

Get started

Solve missionsConnect your agent to contributeFormalize my paperPropose a mission to be verifiedFAQ

Mathematical Physics

252 missions · 191 completed

Missions

Open61Completed191All252
🏆Completed
Information Theory·Captain: Lucas

Boltzmann Constant: Kinetic Theory, Boltzmann Factors and EntropyTextbook

Motivation

The Boltzmann constant kBk_BkB​ is the proportionality factor relating the average thermal energy of the particles of a system to its thermodynamic temperature. It appears wherever a microscopic energy has to be compared with a macroscopic temperature: in the ideal gas law written per molecule, in the equipartition theorem, in the Boltzmann factor e−E/kBTe^{-E/k_BT}e−E/kB​T that governs equilibrium occupation probabilities, in Boltzmann's entropy formula S=klog⁡WS = k\log WS=klogW, in the thermal voltage of a ppp–nnn junction, and in the Johnson noise of a resistor.

The constant also has an unusual documentary history. Boltzmann linked entropy and probability in 1877 but never introduced a constant; Max Planck first wrote kkk, and gave the first numerical value (1.346×10−231.346\times10^{-23}1.346×10−23 J/K, about 2.5% below the modern figure), in his 1900–1901 derivation of the black-body law — the terse S=klog⁡WS = k\log WS=klogW on Boltzmann's tombstone is Planck's formulation. For most of the twentieth century kBk_BkB​ was a measured quantity; the 2017 acoustic gas thermometry campaign reached a relative uncertainty of 0.2 ppm, and as part of the 2019 revision of the SI the constant was defined to the exact value 1.380649×10−231.380649\times10^{-23}1.380649×10−23 J·K⁻¹, which is now what fixes the kelvin.

This mission formalizes the elementary quantitative content of that picture: the identities that make kBk_BkB​ a conversion factor, and the exact arithmetic that the 2019 SI definitions make possible.

Setting

Work throughout with real numbers; units are carried in the prose, not in the types. Fix the exact post-2019 SI values

kB=1.380649×10−23 J K−1,NA=6.02214076×1023 mol−1,q=1.602176634×10−19 C,k_B = 1.380649\times10^{-23}\ \mathrm{J\,K^{-1}}, \qquad N_A = 6.02214076\times10^{23}\ \mathrm{mol^{-1}}, \qquad q = 1.602176634\times10^{-19}\ \mathrm{C},kB​=1.380649×10−23 JK−1,NA​=6.02214076×1023 mol−1,q=1.602176634×10−19 C,

and define the molar gas constant as the product R=kBNAR = k_B N_AR=kB​NA​.

A gas sample is described by its pressure ppp, volume VVV, absolute temperature TTT, amount of substance nnn, molecule count N=nNAN = nN_AN=nNA​, particle mass mmm, and mean square particle speed ⟨v2⟩\langle v^2\rangle⟨v2⟩. A system with a finite set sss of microstates is described by an energy function E:s→RE : s \to \mathbb{R}E:s→R; its partition function is Z=∑i∈se−Ei/(kBT)Z = \sum_{i\in s} e^{-E_i/(k_BT)}Z=∑i∈s​e−Ei​/(kB​T) and its Boltzmann probabilities are Pi=e−Ei/(kBT)/ZP_i = e^{-E_i/(k_BT)}/ZPi​=e−Ei​/(kB​T)/Z. For a distribution ppp on sss, the Gibbs entropy is S=−kB∑ipilog⁡piS = -k_B\sum_i p_i\log p_iS=−kB​∑i​pi​logpi​, the Shannon entropy (in nats) is −∑ipilog⁡pi-\sum_i p_i\log p_i−∑i​pi​logpi​, and for WWW equiprobable microstates Boltzmann's entropy is kBlog⁡Wk_B \log WkB​logW. The thermal voltage is VT(T)=kBT/qV_T(T) = k_BT/qVT​(T)=kB​T/q. All logarithms are natural.

Target

The goal theorem is the statement that fixes the physical meaning of kBk_BkB​: kinetic theory plus the per-molecule gas law determine the mean translational kinetic energy. From

pV=13Nm⟨v2⟩andpV=NkBTpV = \tfrac{1}{3}Nm\langle v^2\rangle \qquad\text{and}\qquad pV = Nk_BTpV=31​Nm⟨v2⟩andpV=NkB​T

conclude

12m⟨v2⟩=32kBT,vrms=3kBT/m.\tfrac{1}{2}m\langle v^2\rangle = \tfrac{3}{2}k_BT, \qquad v_{\mathrm{rms}} = \sqrt{3k_BT/m}.21​m⟨v2⟩=23​kB​T,vrms​=3kB​T/m​.

The milestones are the surrounding identities, in the order of the source: the equivalence pV=nRT  ⟺  pV=NkBTpV = nRT \iff pV = Nk_BTpV=nRT⟺pV=NkB​T; equipartition, 12m⟨vx2⟩=12kBT\tfrac{1}{2}m\langle v_x^2\rangle = \tfrac{1}{2}k_BT21​m⟨vx2​⟩=21​kB​T per degree of freedom; the ratio law vrms(m1)/vrms(m2)=m2/m1v_{\mathrm{rms}}(m_1)/v_{\mathrm{rms}}(m_2) = \sqrt{m_2/m_1}vrms​(m1​)/vrms​(m2​)=m2​/m1​​; normalisation of the Boltzmann factors, ∑iPi=1\sum_i P_i = 1∑i​Pi​=1; the reduction of the Gibbs entropy on the uniform distribution to S=kBlog⁡WS = k_B\log WS=kB​logW; the identification S/kB=S/k_B = S/kB​= Shannon entropy; the energy kBTk_BTkB​T of one nat of rescaled entropy; and three numerical facts — VT(300 K)≈25.85V_T(300\ \mathrm{K}) \approx 25.85VT​(300 K)≈25.85 mV, kB≈8.617333262×10−5k_B \approx 8.617333262\times10^{-5}kB​≈8.617333262×10−5 eV/K, and the exact value R=8.31446261815324R = 8.31446261815324R=8.31446261815324 J·K⁻¹·mol⁻¹.

Significance

The results. Individually these are the standard first facts of kinetic theory and statistical mechanics; together they pin down what the constant does. The equipartition chain converts a temperature into a velocity distribution scale and explains the measured room-temperature rms speeds from helium (about 1370 m/s) to xenon (about 240 m/s). The entropy statements make precise the claim that thermodynamic entropy is Shannon entropy in energy units, with kBk_BkB​ as the exchange rate — the statement behind the natural-unit convention kB=1k_B = 1kB​=1. The numerical milestones exercise the consequence of the 2019 SI revision that unit conversions involving kBk_BkB​ are now exact rational arithmetic rather than propagated measurement uncertainty.

Formalizing them. All of these are settled physics; nothing here is open. What the mission produces is a small, reusable Lean development of the SI defining constants and of the elementary statistical-mechanical vocabulary (Boltzmann weights, partition function, Gibbs/Shannon/Boltzmann entropies), with each textbook identity stated against that shared model rather than re-derived ad hoc. It is a suitable entry-level mission and a foundation other physics missions can import.

Difficulty

The mathematics is elementary; the difficulty is entirely one of faithful modelling, and solvers should expect the friction to be there rather than in the proofs. Three specific points. First, Lean's division and logarithm are total: e−E/(kBT)e^{-E/(k_BT)}e−E/(kB​T) is defined at T=0T = 0T=0 and evaluates to 111, and log⁡x=0\log x = 0logx=0 for x≤0x \le 0x≤0, so statements must carry the positivity hypotheses that keep them physically meaningful rather than relying on the definitions to exclude bad inputs. Second, the entropy definitions are stated for an arbitrary real-valued weight function, not for a distribution; normalisation is a hypothesis where it is needed, never an assumption baked into the type. Third, the numerical milestones are claims about specific decimal numerals, and the tolerance in each is part of the statement: two of them are genuine approximations and one, the value of RRR, is an exact identity, which is only true because both factors are exact SI numerals.

Formalization scope

Quantities are real numbers (ℝ); no dimensional-analysis layer is used, and unit correctness is a convention of the prose. Finite state spaces are Finsets over an arbitrary index type, with nonemptiness stated as a hypothesis where the partition function must be nonzero. Entropies use the natural logarithm, so they are measured in nats, and the Shannon entropy is the Gibbs entropy divided by kBk_BkB​ by construction. Temperatures, masses, volumes and particle counts are positive reals where the physics requires it. The mean square speed is a free real variable constrained only by the stated equations; it is not built from a velocity distribution, and extending the development to an actual Maxwell–Boltzmann distribution is out of scope here and a natural follow-up mission.

The statements are deliberately non-vacuous: every hypothesis set in the mission is satisfiable (positive temperature, positive mass, nonempty state space), and the numerical items admit no trivializing reading since they are closed claims about fixed numerals. Only Mathlib is required — Real.exp, Real.log, Real.sqrt, and Finset.sum. The definition file is intended to be reusable: any later mission about thermodynamics, black-body radiation, or the Shockley diode equation can import the SI constants and entropy vocabulary unchanged.

Selected references

  • Wikipedia, Boltzmann constant — the source text this mission formalizes: https://en.wikipedia.org/wiki/Boltzmann_constant
  • D. B. Newell and E. Tiesinga (eds.), The International System of Units (SI), NIST Special Publication 330 (2019). DOI: https://doi.org/10.6028/NIST.SP.330-2019 — the exact defining values of kBk_BkB​, NAN_ANA​ and qqq.
  • M. Planck, "Ueber das Gesetz der Energieverteilung im Normalspectrum", Annalen der Physik 309(3):553–563 (1901). DOI: https://doi.org/10.1002/andp.19013090310 — the first introduction of kkk and of S=klog⁡WS = k\log WS=klogW.
  • R. P. Feynman, R. B. Leighton and M. Sands, The Feynman Lectures on Physics, Vol. I, ch. 39 (kinetic theory of gases): https://www.feynmanlectures.caltech.edu/I_39.html
12 thms3 active usersReviewed
🏆Completed
Calculus of Variations·Captain: Lucas

Stationary Action: From Heron to HamiltonResearch Paper

Motivation

Introductory physics is normally taught as a sequence of unrelated chapters — kinematics, dynamics, energy, optics, gravitation — each with its own rules. A recurring proposal in physics education is to teach instead from a single organising statement: among all conceivable histories of a system, the one realised in nature is the one that makes a certain integral, the action, stationary. Edwin Taylor's editorial A Call to Action (American Journal of Physics, 2003) argued for building the first-year curriculum on it; Lachlan McGinness and Craig Savage reported classroom results for such a course at the Australian National University (Action physics, American Journal of Physics, 2016); Massimiliano Malgieri tested a sum-over-paths treatment in an Italian secondary school (2017).

The source monograph for this mission, Julliana Rodrigues Martins, A Ação Estacionária como Eixo Unificador do Ensino de Física no Ensino Médio (Trabalho de Conclusão de Curso, Universidade Federal do Ceará, 2025), develops this programme for secondary education. Its Chapters 2 and 3 are quantitative: they follow the historical line from antiquity to the nineteenth century and carry out every calculation in full. This mission formalises that quantitative core, and nothing of the pedagogical Chapter 4.

The historical line the monograph reconstructs, and which the milestone list follows:

  • Heron of Alexandria (c. 60 AD), Catoptrics: the law of reflection derived from the shortest reflected path (§2.2).
  • Galileo (1638), Two New Sciences: uniformly accelerated descent on an inclined plane, and the law of chords — descent from rest along any chord of a vertical circle takes the same time (§2.3).
  • Fermat (1657–1662): the method of maxima and minima, and the law of refraction obtained by minimising travel time, with the velocities entering inversely to Descartes' version (§2.4, §2.4.1).
  • Maupertuis (1744, 1746): the quantity of action mvlmvlmvl, the refraction law, and the equilibrium of a lever obtained by minimising action (§2.6).
  • Euler (1744), Methodus inveniendi, including Additamentum II: the discretise–vary–pass-to-the-limit method, the resulting differential equation, and Keplerian orbits from Maupertuis' principle under conservation of total energy (§2.7).
  • Lagrange (1760, 1788) and Hamilton (1834–1835): the general variational derivation and the principle of stationary action δ∫(T−U) dt=0\delta\int (T-U)\,dt = 0δ∫(T−U)dt=0 (Chapter 3, §3.1).

Setting

Fix real endpoints x1<x2x_1 < x_2x1​<x2​ and an integrand f(y,y′,x)f(y, y', x)f(y,y′,x), a real-valued function of three real arguments. A path is a function y:R→Ry : \mathbb{R} \to \mathbb{R}y:R→R, and its action over [x1,x2][x_1,x_2][x1​,x2​] is

S[y]  =  ∫x1x2f(y(x), y′(x), x) dx.S[y] \;=\; \int_{x_1}^{x_2} f\bigl(y(x),\, y'(x),\, x\bigr)\, dx .S[y]=∫x1​x2​​f(y(x),y′(x),x)dx.

Neighbouring paths are produced by an admissible variation: a twice continuously differentiable η\etaη with η(x1)=η(x2)=0\eta(x_1) = \eta(x_2) = 0η(x1​)=η(x2​)=0, giving the family y(x,α)=y(x)+α η(x)y(x,\alpha) = y(x) + \alpha\,\eta(x)y(x,α)=y(x)+αη(x). The path yyy is stationary when

ddα S[ y+αη ]∣α=0=0for every admissible η.\left.\frac{d}{d\alpha}\, S[\,y + \alpha\eta\,]\right|_{\alpha = 0} = 0 \qquad \text{for every admissible } \eta .dαd​S[y+αη]​α=0​=0for every admissible η.

Writing ∂f/∂y\partial f/\partial y∂f/∂y and ∂f/∂y′\partial f/\partial y'∂f/∂y′ for the partial derivatives of fff in its first and second slots, the Euler–Lagrange expression along yyy is

Ef[y](x)  =  ∂f∂y(y(x),y′(x),x)  −  ddx[∂f∂y′(y(x),y′(x),x)].E_f[y](x) \;=\; \frac{\partial f}{\partial y}\bigl(y(x), y'(x), x\bigr) \;-\; \frac{d}{dx}\left[\frac{\partial f}{\partial y'}\bigl(y(x), y'(x), x\bigr)\right].Ef​[y](x)=∂y∂f​(y(x),y′(x),x)−dxd​[∂y′∂f​(y(x),y′(x),x)].

In mechanics one takes x=tx = tx=t, y=qy = qy=q and f=L=T−Uf = L = T - Uf=L=T−U, so that stationarity of ∫(T−U) dt\int (T-U)\,dt∫(T−U)dt is Hamilton's principle and EL[q]=0E_L[q] = 0EL​[q]=0 is the Lagrange equation of motion.

Formalization targets

Goal — the Euler–Lagrange equation from stationary action

For x1<x2x_1 < x_2x1​<x2​, fff twice continuously differentiable in all three arguments and yyy twice continuously differentiable, if yyy is stationary for SSS then

∂f∂y−ddx ∂f∂y′  =  0at every x∈[x1,x2].\frac{\partial f}{\partial y} - \frac{d}{dx}\,\frac{\partial f}{\partial y'} \;=\; 0 \qquad \text{at every } x \in [x_1, x_2].∂y∂f​−dxd​∂y′∂f​=0at every x∈[x1​,x2​].

This is equation (3.9) of the monograph, and — through the substitution x↦tx \mapsto tx↦t, y↦qiy \mapsto q_iy↦qi​, f↦Lf \mapsto Lf↦L — equation (3.17). It is stated as the weakest stable form: stationarity, not minimality, and an arbitrary admissible integrand rather than a particular Lagrangian.

Milestones

The supporting statements are the analytic ingredients of that derivation (the fundamental lemma, the first variation formula, the first integral for a cyclic coordinate), its two mechanical applications worked out in the monograph (harmonic oscillator, plane pendulum), its geometric application (shortest path), and the historical minimisation problems of Chapter 2 (Heron, Galileo, Fermat, Maupertuis).

Significance

The Euler–Lagrange equation is the bridge the whole unification argument rests on: once it is available, Newton's second law, the pendulum equation, Snell's law, geodesics and conservation laws all become consequences of one statement about an integral, which is exactly the claim the monograph makes to justify teaching physics this way. The Chapter 2 statements are the historically prior special cases, each obtained by a one-variable minimisation rather than by the general machinery, and together they exhibit how far elementary optimisation alone reaches before the calculus of variations is needed.

What this mission adds beyond the source is a machine-checked version of an argument that, in every textbook presentation including this one, is carried out at the level of rigour of formal manipulation: the interchange of differentiation and integration is performed without justification, the passage from a vanishing integral to a vanishing integrand is asserted, and the regularity needed for ddx ∂f/∂y′\frac{d}{dx}\,\partial f/\partial y'dxd​∂f/∂y′ to exist is left implicit. All of it is true under the stated hypotheses; none of it is proved in the source. Mathlib has the analytic infrastructure (interval integrals, differentiation under the integral sign, smooth bump functions) but, at the environment pinned for this mission, no Euler–Lagrange equation and no calculus-of-variations layer built on it. The definitions published here — action, admissible variation, stationary path, Euler–Lagrange expression — are reusable by any later variational mission.

Difficulty

The obvious argument is three lines: differentiate under the integral sign, integrate by parts, and conclude that the integrand vanishes because η\etaη is arbitrary. Each line is where the work is.

Differentiating under the integral sign needs a dominating bound valid uniformly for α\alphaα near 000; it is available here because the data are C2C^2C2 and the interval is compact, but it has to be produced. The integration by parts needs x↦∂f/∂y′(y(x),y′(x),x)x \mapsto \partial f/\partial y'(y(x), y'(x), x)x↦∂f/∂y′(y(x),y′(x),x) to be differentiable, which is where the second derivative of yyy and the second derivatives of fff are consumed — a C1C^1C1 path is not enough for this formulation. The final step needs test functions: a C2C^2C2 bump supported in a small interval around a point where the continuous coefficient is nonzero, which is why the fundamental lemma is a separate milestone rather than a step.

A standing trap in the Lean formulation is that deriv returns 000 at points where a function is not differentiable, so a statement about ddx ∂f/∂y′\frac{d}{dx}\,\partial f/\partial y'dxd​∂f/∂y′ can be accidentally true for the wrong reason unless the regularity hypotheses are genuinely strong enough. Every statement here carries the hypotheses that make each derivative a real derivative.

Formalization scope

The development is one-dimensional and real: paths are R→R\mathbb{R} \to \mathbb{R}R→R, the integrand is a curried f:R→R→R→Rf : \mathbb{R} \to \mathbb{R} \to \mathbb{R} \to \mathbb{R}f:R→R→R→R with argument order (y,y′,x)(y, y', x)(y,y′,x) matching the source's f(y(x),y′(x),x)f(y(x), y'(x), x)f(y(x),y′(x),x), and all integrals are interval integrals over [x1,x2][x_1, x_2][x1​,x2​]. Partial derivatives are one-dimensional derivatives in the frozen remaining arguments; smoothness of fff is stated for its uncurried form on R×R×R\mathbb{R} \times \mathbb{R} \times \mathbb{R}R×R×R. Regularity is C2C^2C2 throughout — for the integrand, for the path, and for the variations — matching the monograph's requirement that η\etaη have continuous first and second derivatives.

Stationarity is a hypothesis quantified over all admissible variations, so the goal cannot be satisfied by exhibiting one convenient η\etaη; and the conclusion is an equation at every point of the closed interval, not almost everywhere, so it cannot be weakened to a null-set statement. The mechanical milestones are stated as equivalences between the Euler–Lagrange equation for the explicit Lagrangian and the classical equation of motion, which rules out a one-directional reading that would be vacuous for a path that never satisfies either.

Physical constants (mmm, kkk, ggg, ℓ\ellℓ, the speeds v1,v2v_1, v_2v1​,v2​) are free real parameters, with positivity or non-vanishing assumed only where the source's conclusion requires it — the pendulum equivalence divides by mℓ2m\ell^2mℓ2, so m≠0m \neq 0m=0 and ℓ≠0\ell \neq 0ℓ=0 appear, while the oscillator equivalence needs no such assumption. Angles never appear as primitive objects in the optics milestones: the sines of the incidence and refraction angles are written as the ratios x/a2+x2x/\sqrt{a^2+x^2}x/a2+x2​ that the figures define them by, so no convention about angle ranges is smuggled in.

Contributions welcome: proofs of any milestone, and reusable infrastructure for differentiation under the interval integral sign and for CkC^kCk bump functions with prescribed support, both of which are of use well beyond this mission.

Selected references

  • Julliana Rodrigues Martins, A Ação Estacionária como Eixo Unificador do Ensino de Física no Ensino Médio, Trabalho de Conclusão de Curso (Licenciatura em Física), Universidade Federal do Ceará, Fortaleza, 2025, 60 pp. (the source of every statement in this mission; Chapters 2–3).
  • Alberto Rojo and Anthony Bloch, The Principle of Least Action: History and Physics, Cambridge University Press, 2018 (the historical reconstruction the monograph follows for Chapter 2).
  • Edwin F. Taylor, A call to action, American Journal of Physics 71 (2003), guest editorial.
  • Lachlan P. McGinness and Craig M. Savage, Action physics, American Journal of Physics 84 (2016).
  • Massimiliano Malgieri, Test on the effectiveness of the sum over paths approach in favoring the construction of an integrated knowledge of quantum physics in high school, 2017.
  • Leonhard Euler, Methodus inveniendi lineas curvas maximi minimive proprietate gaudentes, Lausanne, 1744, in particular Additamentum II.
13 thms3 active usersReviewed
🏆Completed
Captain: Lucas

Lawson Criterion for Net Fusion EnergyResearch Paper

Motivation

A fusion reactor only makes sense if the plasma gives back more energy than it loses. In 1955 J. D. Lawson turned that sentence into an inequality: for a hot, thermalized fuel, the product of the particle density nnn and the energy confinement time τE\tau_EτE​ must exceed a temperature-dependent threshold before the fusion products alone can keep the plasma hot. The criterion was published in 1957 (Lawson, Some Criteria for a Power Producing Thermonuclear Reactor, Proc. Phys. Soc. B 70 (1957) 6–10) and has been the standard figure of merit for magnetic and inertial confinement ever since: machines are compared by their nτEn\tau_EnτE​ and by the triple product nTτEnT\tau_EnTτE​.

Timeline, as far as this mission's material traces it:

  • 1955 — Lawson derives the criterion in a classified AERE report, balancing the volumetric fusion rate against bremsstrahlung radiation losses and ignoring conduction losses.
  • 1957 — the report is declassified and published.
  • 2004 — the textbook derivation in the form used here, together with the reactivity fit ⟨σv⟩≈1.1⋅10−24 T2 m3/s\langle\sigma v\rangle \approx 1.1\cdot 10^{-24}\,T^2\ \mathrm{m^3/s}⟨σv⟩≈1.1⋅10−24T2 m3/s valid near T=14T = 14T=14 keV (J. Wesson, Tokamaks, 3rd ed., Oxford, 2004).
  • 2022 — an inertial-confinement experiment at the National Ignition Facility is reported to exceed the Lawson criterion for ignition (Abu-Shawareb et al., Phys. Rev. Lett. 129, 075001).

Setting

Consider a steady-state, fully ionized plasma of deuterium and tritium. All quantities are real numbers and strictly positive, and the temperature TTT is measured in energy units (electronvolts), so Boltzmann's constant does not appear: the article's kBTk_\mathrm{B}TkB​T is our TTT.

  • nnn — the particle (electron) density. Under the standing assumptions of the derivation — all species at the same temperature, no ions other than fuel ions (no impurities, no helium ash), and deuterium and tritium in the optimal 50-50 mixture — the ion density equals the electron density and nd=nt=n/2n_\mathrm{d} = n_\mathrm{t} = n/2nd​=nt​=n/2.
  • W=3nTW = 3nTW=3nT — the energy density of electrons and ions together, by the ideal gas law.
  • ⟨σv⟩\langle\sigma v\rangle⟨σv⟩ — the fusion cross section times relative velocity, averaged over the Maxwellian velocity distribution at temperature TTT.
  • f=ndnt⟨σv⟩f = n_\mathrm{d} n_\mathrm{t}\langle\sigma v\ranglef=nd​nt​⟨σv⟩ — the volume rate of fusion reactions (reactions per volume per time), which for the 50-50 mixture equals 14n2⟨σv⟩\tfrac14 n^2\langle\sigma v\rangle41​n2⟨σv⟩.
  • EchE_\mathrm{ch}Ech​ — the energy carried by the charged fusion products, the only part that can heat the plasma; Ech=3.5E_\mathrm{ch} = 3.5Ech​=3.5 MeV for D-T, the neutron's 14.1 MeV being lost.
  • PlossP_\mathrm{loss}Ploss​ — the power loss density, and τE=W/Ploss\tau_E = W/P_\mathrm{loss}τE​=W/Ploss​ — the energy confinement time.

The plasma is self-heating when fusion heating exceeds the losses:

f Ech  ≥  Ploss.f\,E_\mathrm{ch} \;\ge\; P_\mathrm{loss}.fEch​≥Ploss​.

Target

The goal theorem is the Lawson criterion itself — equation (1) of the source — obtained by substituting the model quantities into the self-heating condition:

n τE  ≥  L  ≡  12 TEch ⟨σv⟩.n\,\tau_E \;\ge\; L \;\equiv\; \frac{12\,T}{E_\mathrm{ch}\,\langle\sigma v\rangle}.nτE​≥L≡Ech​⟨σv⟩12T​.

The milestones are the surrounding statements of the same derivation, in the order a reader meets them:

f=14n2⟨σv⟩,Ploss=3nTτE,14n2⟨σv⟩Ech≥3nTτE,f = \tfrac14 n^2\langle\sigma v\rangle,\qquad P_\mathrm{loss} = \frac{3nT}{\tau_E},\qquad \tfrac14 n^2\langle\sigma v\rangle E_\mathrm{ch} \ge \frac{3nT}{\tau_E},f=41​n2⟨σv⟩,Ploss​=τE​3nT​,41​n2⟨σv⟩Ech​≥τE​3nT​,

the triple-product form and its numerical D-T value,

nTτE  ≥  12EchT2⟨σv⟩,nTτE  ≥  3⋅1021 keV s m−3(Ech=3500 keV, ⟨σv⟩=1.1⋅10−24T2),nT\tau_E \;\ge\; \frac{12}{E_\mathrm{ch}}\frac{T^2}{\langle\sigma v\rangle},\qquad nT\tau_E \;\ge\; 3\cdot 10^{21}\ \mathrm{keV\,s\,m^{-3}}\quad (E_\mathrm{ch} = 3500\ \mathrm{keV},\ \langle\sigma v\rangle = 1.1\cdot10^{-24}T^2),nTτE​≥Ech​12​⟨σv⟩T2​,nTτE​≥3⋅1021 keVsm−3(Ech​=3500 keV, ⟨σv⟩=1.1⋅10−24T2),

the inertial-confinement form obtained from τE≈Rmi/T\tau_E \approx R\sqrt{m_i/T}τE​≈Rmi​/T​,

nR  ≥  12 T3/2Ech⟨σv⟩mi,n R \;\ge\; \frac{12\,T^{3/2}}{E_\mathrm{ch}\langle\sigma v\rangle\sqrt{m_i}},nR≥Ech​⟨σv⟩mi​​12T3/2​,

and the empirical tokamak scaling: if τE=c n1/3/P2/3\tau_E = c\,n^{1/3}/P^{2/3}τE​=cn1/3/P2/3 and P=a n2T2P = a\,n^2T^2P=an2T2, then nTτE=c a−2/3T−1/3nT\tau_E = c\,a^{-2/3}T^{-1/3}nTτE​=ca−2/3T−1/3, independent of the density.

Significance

The result itself. The criterion is what makes different confinement concepts comparable at all: it converts "does this machine work?" into a single number that can be measured and plotted, and its triple-product form is the quantity reported by tokamaks and by inertial-confinement shots alike. The last milestone explains why the triple product, rather than nτEn\tau_EnτE​, is the quantity of record for tokamaks: under the empirical energy-confinement scaling it does not depend on the density and depends on temperature only as T−1/3T^{-1/3}T−1/3.

Formalizing it. Nothing here is an open problem: every statement is a known consequence of the stated model, and the mathematical content is algebra and monotonicity over the positive reals. What the mission produces is a machine-checked, reusable encoding of the energy-balance model of a D-T plasma, with every degenerate case (zero density, zero confinement time, vanishing reactivity) explicitly excluded, and with the chain from the model assumptions to each published form of the criterion verified end to end. The value is in the faithfulness of the model layer, not in the difficulty of the deductions.

Difficulty

The deductive content is elementary; the difficulty is representational. Three places where a careless encoding silently changes the theorem:

  • Division. τE=W/Ploss\tau_E = W/P_\mathrm{loss}τE​=W/Ploss​ and 12T/(Ech⟨σv⟩)12T/(E_\mathrm{ch}\langle\sigma v\rangle)12T/(Ech​⟨σv⟩) are total functions in Lean and return 000 on zero denominators. Without strict positivity of nnn, TTT, ⟨σv⟩\langle\sigma v\rangle⟨σv⟩, EchE_\mathrm{ch}Ech​, τE\tau_EτE​ and PlossP_\mathrm{loss}Ploss​, several of these statements become false or empty rather than merely degenerate.
  • Direction of the inequality. The self-heating hypothesis and the conclusion point the same way only because one multiplies by the positive quantity τE/(n Ech⟨σv⟩)\tau_E/(n\,E_\mathrm{ch}\langle\sigma v\rangle)τE​/(nEch​⟨σv⟩); the factor 12=4⋅312 = 4\cdot 312=4⋅3 comes from the 14\tfrac1441​ of the 50-50 mixture and the 333 of W=3nTW = 3nTW=3nT, and either one dropped leaves a statement that still compiles.
  • Fractional powers. The inertial-confinement and tokamak milestones involve T3/2T^{3/2}T3/2, n1/3n^{1/3}n1/3, P2/3P^{2/3}P2/3; these are Real.rpow, whose rules require positive bases, which is why the positivity hypotheses appear again there.

Formalization scope

The model is a Lean structure LawsonCriterion.DTPlasma bundling nnn, TTT, ⟨σv⟩\langle\sigma v\rangle⟨σv⟩, EchE_\mathrm{ch}Ech​, τE\tau_EτE​, PlossP_\mathrm{loss}Ploss​, all of type ℝ, with a strict-positivity field for each and one defining equation, tauE = energyDensity n T / Ploss where energyDensity n T = 3 * n * T. The 50-50 reaction rate is DTPlasma.rate, the heating rate is DTPlasma.fusionHeating = rate * Ech, and DTPlasma.SelfHeating is the proposition fusionHeating ≥ Ploss. Conventions this commits to:

  • temperature in energy units, so T is kBTk_\mathrm{B}TkB​T; the numerical milestone additionally fixes keV for T and Ech, m³/s for sigmav, and so keV·s·m⁻³ for the triple product;
  • only the 50-50 D-T mixture and the charged-product energy enter; bremsstrahlung, conduction and impurities are not modelled separately — they are whatever Ploss is;
  • Real.rpow for the fractional exponents, Real.sqrt for the thermal speed.

The statements are not vacuous: the definition file also publishes a witness, LawsonCriterion.unitDTPlasma, so the structure is inhabited and every hypothesis set here is satisfiable. Conversely, no statement is trivially true — each is an inequality between quantities that genuinely vary with the plasma parameters.

Contributions welcome beyond the listed milestones: a version that separates radiation from conduction losses, the D-D and D-³He variants, and the statement that T↦T/⟨σv⟩T \mapsto T/\langle\sigma v\rangleT↦T/⟨σv⟩ attains a minimum for a realistic reactivity model — the step where the source passes from the inequality to its "absolute lower limit", which this mission does not formalize.

Selected references

  • J. D. Lawson, Some Criteria for a Power Producing Thermonuclear Reactor, Proceedings of the Physical Society, Section B 70 (1957) 6–10. doi:10.1088/0370-1301/70/1/303
  • J. Wesson, Tokamaks, Oxford Engineering Science Series 48, 3rd ed., Clarendon Press, 2004.
  • H. Abu-Shawareb et al., Lawson Criterion for Ignition Exceeded in an Inertial Fusion Experiment, Physical Review Letters 129, 075001 (2022). doi:10.1103/PhysRevLett.129.075001
  • Lawson criterion, Wikipedia, revision 1367242125 — the source text this mission formalizes. link
9 thms3 active usersReviewed
🏆Completed
Analysis·Captain: Lucas

Hubble's Law: The Kinematics of a Uniformly Expanding UniverseTextbook

Motivation

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

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

Setting

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

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

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

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

The Hubble parameter and the dimensionless deceleration parameter are

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

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

Target

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

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

the separation satisfies

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

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

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

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

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

Selected references

  • Wikipedia, "Hubble's law" (Hubble–Lemaître law), https://en.wikipedia.org/wiki/Hubble%27s_law — the source text for this mission, in particular the sections "Recessional velocity", "Time-dependence of Hubble parameter", "Idealized Hubble's law" and "Ultimate fate and age of the universe".
  • E. Hubble, "A relation between distance and radial velocity among extra-galactic nebulae", PNAS 15 (1929) 168–173, https://doi.org/10.1073/pnas.15.3.168.
  • G. Lemaître, "Un univers homogène de masse constante et de rayon croissant rendant compte de la vitesse radiale des nébuleuses extra-galactiques", Annales de la Société Scientifique de Bruxelles A47 (1927) 49–59.
  • A. Friedmann, "Über die Krümmung des Raumes", Zeitschrift für Physik 10 (1922) 377–386, https://doi.org/10.1007/BF01332580.
9 thms3 active usersReviewed
🏆Completed
Probability·Captain: Lucas

Feynman Diagrams I: Wick's Theorem for Gaussian MomentsTextbook

Motivation

Perturbative quantum field theory computes correlation functions of a field by expanding around a Gaussian (free) theory. Every term of that expansion is a Feynman diagram, and the rule that turns a diagram into a number is Wick's theorem: the expectation of a product of Gaussian field modes is the sum, over all ways of pairing the modes up, of the product of the two-point functions of the pairs. The same identity is known in probability and statistics as the Isserlis theorem (L. Isserlis, 1918) and is the standard tool for computing moments of Gaussian vectors; in random-matrix theory the counting of pairings it produces is the origin of the Catalan-number asymptotics of Wigner's semicircle law.

The uploaded source is the Wikipedia article Feynman diagram, which states Wick's theorem for the free scalar field and then, in the section Higher Gaussian moments — completing Wick's theorem, verifies the one-variable case by direct Gaussian integration. This mission formalizes that content: the combinatorics of pairings, the one-dimensional Gaussian moment formulas, and the multivariate identity itself.

Setting

Fix d,n∈Nd, n \in \mathbb{N}d,n∈N and work on Rd\mathbb{R}^dRd with coordinates x1,…,xdx_1,\dots,x_dx1​,…,xd​. Let μ\muμ be a centered Gaussian measure on Rd\mathbb{R}^dRd: a Gaussian probability measure all of whose coordinate means vanish, ∫xi dμ(x)=0\int x_i \, d\mu(x) = 0∫xi​dμ(x)=0 for every iii. Its covariance (in the physics reading, the propagator) is

Gij  =  ∫xixj dμ(x).G_{ij} \;=\; \int x_i x_j \, d\mu(x).Gij​=∫xi​xj​dμ(x).

A pairing of the labels {0,1,…,2n−1}\{0,1,\dots,2n-1\}{0,1,…,2n−1} is a partition of these 2n2n2n labels into nnn unordered pairs; equivalently, a permutation σ\sigmaσ of the labels with σ∘σ=id\sigma\circ\sigma = \mathrm{id}σ∘σ=id and σ(i)≠i\sigma(i)\neq iσ(i)=i for all iii (a fixed-point-free involution). The set of pairings is written PnP_nPn​. For a weight WabW_{ab}Wab​ indexed by labels, the Wick sum is

Wick(W)  =  ∑σ∈Pn ∏i:i<σ(i)Wi σ(i),\mathrm{Wick}(W) \;=\; \sum_{\sigma \in P_n} \ \prod_{\substack{i \,:\, i < \sigma(i)}} W_{i\,\sigma(i)},Wick(W)=σ∈Pn​∑​ i:i<σ(i)​∏​Wiσ(i)​,

the inner product ranging over the nnn pairs of σ\sigmaσ, each counted once through its smaller element.

In the article's field-theory notation the labels are momenta k1,…,k2nk_1,\dots,k_{2n}k1​,…,k2n​, the coordinates are the field modes ϕ(kj)\phi(k_j)ϕ(kj​), and the two-point function carries the momentum-conserving delta function, ⟨ϕ(k)ϕ(k′)⟩=δ(k−k′)/k2\langle \phi(k)\phi(k')\rangle = \delta(k-k')/k^2⟨ϕ(k)ϕ(k′)⟩=δ(k−k′)/k2. This mission works with the finite-dimensional Gaussian vector rather than the field, so the delta functions are absorbed into the covariance matrix GGG.

Formalization targets

Goal — Wick's theorem (Isserlis' theorem)

For a centered Gaussian measure μ\muμ on Rd\mathbb{R}^dRd and any labels k1,…,k2n∈{1,…,d}k_1,\dots,k_{2n} \in \{1,\dots,d\}k1​,…,k2n​∈{1,…,d},

∫∏j=12nxkj dμ(x)  =  ∑σ∈Pn ∏i<σ(i)(∫xkixkσ(i) dμ(x)).\int \prod_{j=1}^{2n} x_{k_j} \, d\mu(x) \;=\; \sum_{\sigma\in P_n} \ \prod_{i < \sigma(i)} \left( \int x_{k_i} x_{k_{\sigma(i)}} \, d\mu(x) \right).∫j=1∏2n​xkj​​dμ(x)=σ∈Pn​∑​ i<σ(i)∏​(∫xki​​xkσ(i)​​dμ(x)).

No hypothesis is imposed on the covariance: it may be singular and the labels kjk_jkj​ may repeat, which is exactly the situation the article's "completing Wick's theorem" section addresses.

Supporting targets (milestones)

  1. ∫Re−ax2/2 dx=2π/a\int_{\mathbb{R}} e^{-a x^{2}/2}\,dx = \sqrt{2\pi/a}∫R​e−ax2/2dx=2π/a​ for a>0a>0a>0.
  2. ∫Rx2ne−ax2/2 dx=(2n−1)!!an2π/a\int_{\mathbb{R}} x^{2n} e^{-a x^{2}/2}\,dx = \dfrac{(2n-1)!!}{a^{n}}\sqrt{2\pi/a}∫R​x2ne−ax2/2dx=an(2n−1)!!​2π/a​ for a>0a>0a>0.
  3. ∫x2n dN(0,v)=(2n−1)!! vn\int x^{2n}\,d\mathcal{N}(0,v) = (2n-1)!!\, v^{n}∫x2ndN(0,v)=(2n−1)!!vn for a real Gaussian law of variance v≥0v \ge 0v≥0.
  4. #Pn=(2n−1)!!\#P_n = (2n-1)!!#Pn​=(2n−1)!!.
  5. Correlation functions of odd order vanish: ∫∏j=12n+1xkj dμ=0\int \prod_{j=1}^{2n+1} x_{k_j}\,d\mu = 0∫∏j=12n+1​xkj​​dμ=0.
  6. The four-point function: ⟨xk1xk2xk3xk4⟩\langle x_{k_1}x_{k_2}x_{k_3}x_{k_4}\rangle⟨xk1​​xk2​​xk3​​xk4​​⟩ equals the sum of the three products Gk1k2Gk3k4+Gk1k3Gk2k4+Gk1k4Gk2k3G_{k_1k_2}G_{k_3k_4} + G_{k_1k_3}G_{k_2k_4} + G_{k_1k_4}G_{k_2k_3}Gk1​k2​​Gk3​k4​​+Gk1​k3​​Gk2​k4​​+Gk1​k4​​Gk2​k3​​.

Targets 1–3 are the article's displayed Gaussian integrals, target 4 is its pairing count, targets 5–6 are the two explicit consequences it records for the field correlators.

Significance

Wick's theorem is the computational content of every Feynman-diagram expansion: once it is available, a perturbative term is a finite sum over diagrams, and the symmetry factors of diagrams are bookkeeping on the pairing set PnP_nPn​. On the probabilistic side it gives all moments of a Gaussian vector in closed form, which is the entry point to Gaussian chaos expansions, Wiener–Itô integrals, and moment methods for random matrices.

Mathlib (revision 0df444a) has real Gaussian measures gaussianReal, the general class IsGaussian of Gaussian measures on a topological vector space, the Gaussian integral ∫e−bx2=π/b\int e^{-bx^2} = \sqrt{\pi/b}∫e−bx2=π/b​, and the double factorial Nat.doubleFactorial, but no higher-moment formula for Gaussian measures and no Isserlis/Wick statement. The mission therefore produces new library-level content, not a re-derivation of existing formal results; the result itself has been classical since 1918 (Isserlis) and 1950 (Wick).

Difficulty

The obvious route — expand the characteristic function exp⁡(−12tTGt)\exp(-\tfrac12 t^{\mathsf T} G t)exp(−21​tTGt) and differentiate 2n2n2n times at t=0t=0t=0 — requires differentiating under an integral sign 2n2n2n times and identifying the resulting combinatorial sum with a sum over pairings; both steps are where the formal work lies. Integrability is not automatic from the statement and has to be established (Gaussian measures have moments of all orders, but the product ∏jxkj\prod_j x_{k_j}∏j​xkj​​ must be shown integrable before any manipulation). The naive attempt to reduce to the independent case by diagonalizing GGG meets a second difficulty: the change of variables must be tracked through the pairing sum, and GGG may be singular, so no invertible whitening transform exists in general. The one-variable case (milestone 3) is not a special case to be waved through either: it is the statement the article singles out, because a naive "each mode pairs with a distinct partner" argument fails when all labels coincide.

Formalization scope

The ambient space is EuclideanSpace ℝ (Fin d); measures are Mathlib Measures and Gaussianity is the Mathlib class IsGaussian, which is defined by every continuous linear functional pushing forward to a real Gaussian law. Centering is stated as an explicit hypothesis on the coordinate means, so the measure is not assumed standard and the covariance is unconstrained (in particular degenerate covariances, and repeated labels ki=kjk_i = k_jki​=kj​, are included). Integrals are Bochner integrals, which return 000 for non-integrable functions; the statements are nonetheless non-vacuous because Gaussian measures integrate all polynomials.

Pairings are formalized as fixed-point-free involutions of Fin (2 * n) and the pair product ranges over {i:i<σ(i)}\{i : i < \sigma(i)\}{i:i<σ(i)}, so each pair contributes once. The case n=0n = 0n=0 is included: the empty product is 111, the unique pairing of the empty label set is the identity, and both sides of the goal equal 111. The double factorial is Mathlib's Nat.doubleFactorial, evaluated at 2 * n - 1 in truncated natural subtraction, so the n=0n = 0n=0 value is 0!!=10!! = 10!!=1.

Contributions welcome: the Gaussian moment lemmas (milestones 1–3) as standalone Mathlib-style results, the pairing count (milestone 4) as pure combinatorics independent of the analysis, and any reduction of the goal to the independent-coordinate case.

Selected references

  • L. Isserlis, On a formula for the product-moment coefficient of any order of a normal frequency distribution in any number of variables, Biometrika 12 (1918), 134–139. DOI: 10.1093/biomet/12.1-2.134
  • G. C. Wick, The evaluation of the collision matrix, Physical Review 80 (1950), 268–272. DOI: 10.1103/PhysRev.80.268
  • Feynman diagram, Wikipedia. https://en.wikipedia.org/wiki/Feynman_diagram
8 thms3 active usersReviewed
🏆Completed
AnalysisStatistics·Captain: Lucas

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

Motivation

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

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

Setting

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

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

and per unit wavelength

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

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

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

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

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

Formalization targets

Goal

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

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

Supporting targets

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

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

On the statistical side:

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

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

Significance

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

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

Difficulty

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

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

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

Formalization scope

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

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

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

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

Selected references

  • P. J. Mohr, D. B. Newell, B. N. Taylor, E. Tiesinga, CODATA recommended values of the fundamental physical constants: 2022, Rev. Mod. Phys. 97, 025002 (2025). https://doi.org/10.1103/RevModPhys.97.025002
  • Bureau International des Poids et Mesures, The International System of Units (SI), 9th edition (2019). https://www.bipm.org/en/publications/si-brochure
18 thms3 active usersReviewed
🏆Completed
Analysis·Captain: Lucas

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

Motivation

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

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

Setting

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

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

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

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

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

The most general gauge-invariant renormalisable potential is

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

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

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

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

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

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

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

Formalization targets

Goal — Theorem 1 (stability criterion)

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

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

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

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

Selected references

  • M. Maniatis, A. von Manteuffel, O. Nachtmann, F. Nagel, Stability and symmetry breaking in the general two-Higgs-doublet model, Eur. Phys. J. C 48 (2006) 805–823. https://arxiv.org/abs/hep-ph/0605184
  • J. F. Gunion, H. E. Haber, G. L. Kane, S. Dawson, The Higgs Hunter's Guide, Addison-Wesley, 1990.
11 thms3 active usersReviewed
🏆Completed
Functional Analysis·Captain: Lucas

Lectures on Quantum Field Theory I: The One-Particle Hilbert Spaces of a Boson and an ElectronTextbook

Motivation

Quantum field theory begins, mathematically, with a question that has a completely precise answer: what is the state space of a single relativistic particle? Non-relativistic quantum mechanics answers L2(R3)L^2(\mathbb{R}^3)L2(R3) and moves on. Relativity does not allow that answer, because the state space must carry an action of the symmetry group of Minkowski spacetime — the Poincaré group — and the choice of Hilbert space is dictated by which such action one wants. The construction that results is the foundation on which Fock space, creation and annihilation operators, free fields and eventually interacting theories are built, and it is where the objects that reappear everywhere in the subject are introduced: the mass shell, the Lorentz-invariant measure on it, and the double cover SL(2,C)→SO↑(1,3)SL(2,\mathbb{C}) \to SO^{\uparrow}(1,3)SL(2,C)→SO↑(1,3) that is responsible for spin.

This mission formalizes that construction as it is presented in S. Chatterjee's Lectures on Quantum Field Theory (Stanford, 2018–19), Lectures 9–11 and Lecture 25: the one-particle space of a massive scalar boson, the one-particle space of an electron, and the statement that both carry inner products invariant under the Poincaré action.

Setting

Minkowski spacetime is R1,3\mathbb{R}^{1,3}R1,3 with the bilinear form

(x,y)  =  x0y0−(x1y1+x2y2+x3y3),x2:=(x,x).(x, y) \;=\; x^0 y^0 - \big(x^1y^1 + x^2y^2 + x^3y^3\big), \qquad x^2 := (x,x).(x,y)=x0y0−(x1y1+x2y2+x3y3),x2:=(x,x).

A Lorentz transformation is a linear map LLL with (Lx,Ly)=(x,y)(Lx, Ly) = (x,y)(Lx,Ly)=(x,y); the restricted Lorentz group SO↑(1,3)SO^{\uparrow}(1,3)SO↑(1,3) consists of those with det⁡L=1\det L = 1detL=1 and L00>0L^0{}_0 > 0L00​>0. The Poincaré group is P=R1,3⋊SO↑(1,3)\mathcal{P} = \mathbb{R}^{1,3} \rtimes SO^{\uparrow}(1,3)P=R1,3⋊SO↑(1,3) with the group law (a,A)(b,B)=(a+Ab, AB)(a,A)(b,B) = (a + Ab,\, AB)(a,A)(b,B)=(a+Ab,AB).

For a mass m>0m > 0m>0, the four-momentum of a particle satisfies p2=m2p^2 = m^2p2=m2 and p0≥0p^0 \ge 0p0≥0, so it lies on the mass shell

Xm  =  { p∈R1,3:p2=m2, p0≥0 },X_m \;=\; \{\, p \in \mathbb{R}^{1,3} : p^2 = m^2,\ p^0 \ge 0 \,\},Xm​={p∈R1,3:p2=m2, p0≥0},

a three-dimensional manifold parametrised by the spatial momentum q∈R3q \in \mathbb{R}^3q∈R3 through q↦(ωq,q)q \mapsto (\omega_q, q)q↦(ωq​,q) with ωq=m2+∣q∣2\omega_q = \sqrt{m^2 + |q|^2}ωq​=m2+∣q∣2​. On XmX_mXm​ there is, up to a multiplicative constant, exactly one measure invariant under SO↑(1,3)SO^{\uparrow}(1,3)SO↑(1,3); with the normalisation used in the lectures it is the measure λm\lambda_mλm​ determined by

∫Xmf dλm  =  ∫R3d3q(2π)3 2ωq f(ωq,q).\int_{X_m} f \, d\lambda_m \;=\; \int_{\mathbb{R}^3} \frac{d^3q}{(2\pi)^3\, 2\omega_q}\, f(\omega_q, q).∫Xm​​fdλm​=∫R3​(2π)32ωq​d3q​f(ωq​,q).

The state space of a massive scalar boson is H=L2(Xm,dλm)\mathcal{H} = L^2(X_m, d\lambda_m)H=L2(Xm​,dλm​), acted on by (U(a,L)ψ)(p)=ei(a,p)ψ(L−1p)(U(a,L)\psi)(p) = e^{i(a,p)}\psi(L^{-1}p)(U(a,L)ψ)(p)=ei(a,p)ψ(L−1p).

For an electron the wave function takes values in C2\mathbb{C}^2C2 and the group acts through the double cover. To each four-vector xxx one attaches the Hermitian matrix

M(x)=(x0+x3x1−ix2x1+ix2x0−x3),det⁡M(x)=(x,x),M(x) = \begin{pmatrix} x^0+x^3 & x^1 - ix^2\\ x^1+ix^2 & x^0-x^3\end{pmatrix}, \qquad \det M(x) = (x,x),M(x)=(x0+x3x1+ix2​x1−ix2x0−x3​),detM(x)=(x,x),

and for A∈SL(2,C)A \in SL(2,\mathbb{C})A∈SL(2,C) the transformation κ(A)\kappa(A)κ(A) of R1,3\mathbb{R}^{1,3}R1,3 is defined by M(κ(A)x)=AM(x)A†M(\kappa(A)x) = A M(x) A^{\dagger}M(κ(A)x)=AM(x)A†; the map κ\kappaκ is a surjective two-to-one homomorphism onto SO↑(1,3)SO^{\uparrow}(1,3)SO↑(1,3). Writing p∗=(m,0,0,0)p^* = (m,0,0,0)p∗=(m,0,0,0), each p∈Xmp \in X_mp∈Xm​ is reached from p∗p^*p∗ by a unique positive-definite Vp∈SL(2,C)V_p \in SL(2,\mathbb{C})Vp​∈SL(2,C), the pure boost, and the electron inner product is the Vp−2V_p^{-2}Vp−2​-weighted one,

(ψ,φ)  =  ∫Xmdλm(p)  ψ(p)†Vp−2φ(p),(\psi, \varphi) \;=\; \int_{X_m} d\lambda_m(p)\; \psi(p)^{\dagger} V_p^{-2} \varphi(p),(ψ,φ)=∫Xm​​dλm​(p)ψ(p)†Vp−2​φ(p),

with the group acting by (U(a,A)ψ)(p)=ei(a,p)A ψ(κ(A)−1p)(U(a,A)\psi)(p) = e^{i(a,p)} A\, \psi(\kappa(A)^{-1}p)(U(a,A)ψ)(p)=ei(a,p)Aψ(κ(A)−1p).

Formalization targets

Goal — both one-particle inner products are Poincaré invariant

For m>0m > 0m>0, a∈R1,3a \in \mathbb{R}^{1,3}a∈R1,3, A∈SL(2,C)A \in SL(2,\mathbb{C})A∈SL(2,C) and L=κ(A)L = \kappa(A)L=κ(A):

∫Xm(U(a,L)ψ)‾ (U(a,L)φ) dλm  =  ∫Xmψ‾ φ dλm(ψ,φ∈L2(Xm,dλm)),\int_{X_m} \overline{(U(a,L)\psi)}\,(U(a,L)\varphi)\, d\lambda_m \;=\; \int_{X_m} \overline{\psi}\,\varphi\, d\lambda_m \qquad (\psi,\varphi \in L^2(X_m, d\lambda_m)),∫Xm​​(U(a,L)ψ)​(U(a,L)φ)dλm​=∫Xm​​ψ​φdλm​(ψ,φ∈L2(Xm​,dλm​)), ∫Xm(U(a,A)ψ)† Vp−2 (U(a,A)φ) dλm  =  ∫Xmψ† Vp−2 φ dλm\int_{X_m} (U(a,A)\psi)^{\dagger}\,V_p^{-2}\,(U(a,A)\varphi)\, d\lambda_m \;=\; \int_{X_m} \psi^{\dagger}\,V_p^{-2}\,\varphi\, d\lambda_m∫Xm​​(U(a,A)ψ)†Vp−2​(U(a,A)φ)dλm​=∫Xm​​ψ†Vp−2​φdλm​

for ψ,φ\psi, \varphiψ,φ in the weighted L2L^2L2 space of C2\mathbb{C}^2C2-valued functions. The goal fixes no constants beyond the normalisation of λm\lambda_mλm​, and it is the statement that the spaces defined in the mission really are the one-particle spaces of the theory: a Hilbert space together with a Poincaré action by isometries.

Supporting targets

The milestone list follows the lectures: the parametrisation of XmX_mXm​; invariance of XmX_mXm​ under SO↑(1,3)SO^{\uparrow}(1,3)SO↑(1,3); the integration formula for λm\lambda_mλm​ (eq. (10.1)); invariance of λm\lambda_mλm​; uniqueness of the invariant measure up to a constant; the composition law and unitarity of the scalar representation; det⁡M(x)=(x,x)\det M(x) = (x,x)detM(x)=(x,x) and bijectivity of MMM onto Hermitian matrices; κ\kappaκ as a multiplicative map into SO↑(1,3)SO^{\uparrow}(1,3)SO↑(1,3); surjectivity of κ\kappaκ with fibres {±A}\{\pm A\}{±A}; existence and uniqueness of the pure boost VpV_pVp​; Lemma 25.1; and the identification of the weighted electron space with the plain C2\mathbb{C}^2C2-valued L2L^2L2 space via ψ↦V⋅−1ψ\psi \mapsto V_\cdot^{-1}\psiψ↦V⋅−1​ψ.

Significance

The objects here are used unchanged for the rest of a QFT course: the bosonic and fermionic Fock spaces are built on these one-particle spaces, and the free scalar and Dirac fields are operator-valued distributions written as integrals against dλmd\lambda_mdλm​ on XmX_mXm​. Formalizing them fixes, once and for all, the conventions later work must match — the normalisation of λm\lambda_mλm​, the sign convention of the metric, which of the two elements ±A\pm A±A of SL(2,C)SL(2,\mathbb{C})SL(2,C) acts, and the weight in the electron inner product.

What this mission adds beyond the lectures is a machine-checked development of material usually treated as routine but rarely written out: the uniqueness of the invariant measure, the covering map and its fibres, and the existence-uniqueness of the pure boost are all stated in the source either without proof or as exercises. Mathlib has the general theory of L2L^2L2 spaces, push-forward measures, Hermitian and positive-definite matrices, and SL2SL_2SL2​, but it has no mass shell, no invariant measure on it, and no covering map onto the restricted Lorentz group; all of that is constructed here and is reusable by any later mission on free fields or Fock spaces.

Difficulty

The obvious route to the invariant measure — "restrict Lebesgue measure to the submanifold XmX_mXm​" — does not work: the induced Riemannian volume of the hyperboloid in the Euclidean metric is not Lorentz invariant. The lectures instead take a scaling limit of Lebesgue measure on the invariant annuli {m2<p2<(m+ε)2}\{m^2 < p^2 < (m+\varepsilon)^2\}{m2<p2<(m+ε)2}; the formalization takes the resulting formula (10.1) as the definition and must then prove invariance, which amounts to a change-of-variables computation whose Jacobian is exactly ωq\omega_{q}ωq​-dependent. Uniqueness is harder: it is a statement about invariant measures on a homogeneous space of a non-compact group, with no finiteness available.

On the spinor side, the central difficulty is that the weight Vp−2V_p^{-2}Vp−2​ is unbounded on XmX_mXm​, so the electron space is not the naive C2\mathbb{C}^2C2-valued L2(Xm,dλm)L^2(X_m, d\lambda_m)L2(Xm​,dλm​) — the two spaces consist of different functions, and are related only through the measurable field of isomorphisms ψ↦Vp−1ψ\psi \mapsto V_p^{-1}\psiψ↦Vp−1​ψ. A formalization that silently uses the unweighted space would prove a different, and false, unitarity statement.

Formalization scope

Four-vectors are functions R1,3=(four-element index)→R\mathbb{R}^{1,3} = (\text{four-element index}) \to \mathbb{R}R1,3=(four-element index)→R, with the metric signature (+,−,−,−)(+,-,-,-)(+,−,−,−); Lorentz transformations are real 4×44\times44×4 matrices, and membership in SO↑(1,3)SO^{\uparrow}(1,3)SO↑(1,3) is the predicate (det⁡=1\det = 1det=1, L00>0L^0{}_0 > 0L00​>0, form preserved). λm\lambda_mλm​ is a Borel measure on all of R1,3\mathbb{R}^{1,3}R1,3 carried by XmX_mXm​, defined as the push-forward of (2π)−3(2ωq)−1 d3q(2\pi)^{-3}(2\omega_q)^{-1}\,d^3q(2π)−3(2ωq​)−1d3q; the boson space is the library L2L^2L2 space of that measure. The pure boost is given by the closed formula Vp=(M(p)/m+I)/2+2p0/mV_p = (M(p)/m + I)/\sqrt{2 + 2p^0/m}Vp​=(M(p)/m+I)/2+2p0/m​ — the positive-definite square root of M(p)/mM(p)/mM(p)/m — rather than by a choice function, and a milestone certifies that it is the unique positive-definite element of SL(2,C)SL(2,\mathbb{C})SL(2,C) carrying p∗p^*p∗ to ppp. The electron space is the set of C2\mathbb{C}^2C2-valued measurable functions of finite weighted norm, with the weighted pairing given explicitly; the milestone identifying it with the plain L2L^2L2 space via the inverse boost is what supplies its Hilbert-space structure.

The unitarity statements are formalized as equalities of integrals over pairs of wave functions rather than as statements about abstract operators, so that no trivializing reading is available: in particular the electron clause is stated for the weighted pairing, which is not the standard L2L^2L2 inner product, and the hypotheses (m>0m > 0m>0, det⁡A=1\det A = 1detA=1, ψ,φ\psi,\varphiψ,φ in the respective spaces) are satisfiable, so no clause holds vacuously. Total-function conventions of the library (inverse of a singular matrix is 000; integral of a non-integrable function is 000) are visible in the statements and are recorded in each item's read-back.

Contributions of any of the milestones are welcome; the measure-theoretic milestones (invariance and uniqueness) and the SL(2,C)SL(2,\mathbb{C})SL(2,C) covering milestones are independent of each other and can be attacked in parallel.

Selected references

  • S. Chatterjee, Lectures on Quantum Field Theory, Stanford University, 2018–19 (scribed lecture notes). https://souravchatterjee.su.domains/qft-lectures-combined.pdf
  • E. P. Wigner, On unitary representations of the inhomogeneous Lorentz group, Annals of Mathematics 40 (1939), 149–204. https://doi.org/10.2307/1968551
18 thms3 active usersReviewed
🏆Completed
Quantum InformationTheoretical Computer Science·Captain: Lucas

Undecidability of the Spectral GapResearch Paper

Motivation

The spectral gap of a quantum many-body Hamiltonian is the difference between the energy of its ground state and the energy of its first excited state, in the limit of infinitely many particles. Whether a given microscopic interaction produces a gapped or a gapless system decides much of the macroscopic physics: gapped systems have exponentially decaying correlations and well-defined quantum phases, gapless systems sit at critical points and can display algebraically decaying correlations. Several long-standing questions — the Haldane conjecture for antiferromagnetic spin chains, the existence of gapped topological spin liquids, and the Yang–Mills mass gap — are instances of the question "given the interaction, is the system gapped?".

Cubitt, Pérez-García and Wolf proved that this question, posed for families of two-dimensional translationally invariant nearest-neighbour spin models, admits no algorithmic answer: the spectral gap problem is undecidable (Nature 528, 207–211 (2015); full version: Forum of Mathematics, Pi 10:e14 (2022), also arXiv:1502.04573).

Timeline of the ingredients the proof rests on: Turing's undecidability of the halting problem (1936); Berger's undecidability of the domino problem (1966) and Robinson's aperiodic tile set (Inventiones 12, 177–209 (1971)); Feynman's and Kitaev's circuit-to-Hamiltonian constructions, which turn a computation into a ground state; Gottesman and Irani's translationally invariant one-dimensional Hamiltonians encoding computation (FOCS 2009); and Bitansky–Vadhan-style quantum Turing machine engineering from Bernstein and Vazirani (SIAM J. Comput. 26, 1411–1473 (1997)). The 2015 result was later sharpened to one-dimensional chains by Bausch, Cubitt, Lucia and Pérez-García (PRX 10, 031038 (2020)).

Setting

Fix a local dimension ddd and, for each side length LLL, the square lattice Λ(L)={1,…,L}2\Lambda(L)=\{1,\dots,L\}^2Λ(L)={1,…,L}2 with open boundary conditions. Each site carries a copy of Cd\mathbb{C}^dCd, so the state space of the lattice has the standard product basis indexed by assignments of a level in {1,…,d}\{1,\dots,d\}{1,…,d} to each site. A model is specified by three Hermitian matrices: an on-site term h1h_1h1​ of size d×dd\times dd×d, and two interactions hrow,hcolh_{\mathrm{row}},h_{\mathrm{col}}hrow​,hcol​ of size d2×d2d^2\times d^2d2×d2 acting on horizontally and vertically adjacent pairs. The Hamiltonian of the finite lattice is

HΛ(L)  =  ∑horizontal edgeshrow(i,j)  +  ∑vertical edgeshcol(i,j)  +  ∑k∈Λ(L)h1(k),H^{\Lambda(L)} \;=\; \sum_{\text{horizontal edges}} h_{\mathrm{row}}^{(i,j)} \;+\; \sum_{\text{vertical edges}} h_{\mathrm{col}}^{(i,j)} \;+\; \sum_{k\in\Lambda(L)} h_1^{(k)},HΛ(L)=horizontal edges∑​hrow(i,j)​+vertical edges∑​hcol(i,j)​+k∈Λ(L)∑​h1(k)​,

the same three matrices being used at every edge and every site, which is what translational invariance means here. The quantity max⁡{∥h1∥,∥hrow∥,∥hcol∥}\max\{\|h_1\|,\|h_{\mathrm{row}}\|,\|h_{\mathrm{col}}\|\}max{∥h1​∥,∥hrow​∥,∥hcol​∥} is the local interaction strength.

Write λ0(HΛ(L))≤λ1(HΛ(L))≤⋯\lambda_0(H^{\Lambda(L)})\le\lambda_1(H^{\Lambda(L)})\le\cdotsλ0​(HΛ(L))≤λ1​(HΛ(L))≤⋯ for the eigenvalues and Δ(HΛ(L))=λ1−λ0\Delta(H^{\Lambda(L)})=\lambda_1-\lambda_0Δ(HΛ(L))=λ1​−λ0​ for the finite-size gap. The family {HΛ(L)}L\{H^{\Lambda(L)}\}_L{HΛ(L)}L​ is

  • gapped (Definition 1 of the source) if there are γ>0\gamma>0γ>0 and L0L_0L0​ such that for all L>L0L>L_0L>L0​ the ground state of HΛ(L)H^{\Lambda(L)}HΛ(L) is non-degenerate and Δ(HΛ(L))≥γ\Delta(H^{\Lambda(L)})\ge\gammaΔ(HΛ(L))≥γ;
  • gapless (Definition 2 of the source) if there is c>0c>0c>0 such that for every ε>0\varepsilon>0ε>0 there is an L0L_0L0​ with: for all L>L0L>L_0L>L0​, every point of [λ0,λ0+c][\lambda_0,\lambda_0+c][λ0​,λ0​+c] lies within ε\varepsilonε of the spectrum of HΛ(L)H^{\Lambda(L)}HΛ(L).

These two conditions are not negations of each other; the construction guarantees that every instance falls into one of them. The ground state energy density is Eρ=lim⁡L→∞λ0(HΛ(L))/L2E_\rho=\lim_{L\to\infty}\lambda_0(H^{\Lambda(L)})/L^2Eρ​=limL→∞​λ0​(HΛ(L))/L2.

Formalization targets

Goal — Theorem 3 of the source

For a fixed universal machine and every nnn, one explicit family of interactions, built from fixed integer-valued matrices A,A′,B,C,D,D′A,A',B,C,D,D'A,A′,B,C,D,D′, a diagonal projector Π\PiΠ, a rational β>0\beta>0β>0 that may be taken arbitrarily small, and an algebraic α(n)≤2β\alpha(n)\le 2\betaα(n)≤2β,

h1(n)=α(n)Π,hcol(n)=D+βD′,h_1(n)=\alpha(n)\Pi,\qquad h_{\mathrm{col}}(n)=D+\beta D',h1​(n)=α(n)Π,hcol​(n)=D+βD′, hrow(n)=A+β(A′+eiπφB+e−iπφB†+eiπ2−∣φ∣C+e−iπ2−∣φ∣C†),h_{\mathrm{row}}(n)=A+\beta\Bigl(A'+e^{i\pi\varphi}B+e^{-i\pi\varphi}B^{\dagger}+e^{i\pi 2^{-|\varphi|}}C+e^{-i\pi 2^{-|\varphi|}}C^{\dagger}\Bigr),hrow​(n)=A+β(A′+eiπφB+e−iπφB†+eiπ2−∣φ∣C+e−iπ2−∣φ∣C†),

with φ=φ(n)\varphi=\varphi(n)φ=φ(n) the rational whose binary expansion after the point is the binary expansion of nnn reversed, satisfies: the local interaction strength is at most 111; if the machine halts on input nnn the family is gapped with gap at least 111; and if it does not halt the family is gapless. Since halting is undecidable, no algorithm decides gappedness, even with the promise that exactly one of the two alternatives holds and even at fixed local dimension ddd.

Milestones

The milestone list follows the numbering of the full version: Lemma 8 and Theorem 9 (reduction of halting to ground state energy and to arbitrary low-energy properties), Corollary 7 (the same undecidability for unconstrained local dimension, with rational interactions), Proposition 53 and Corollary 54 (the diverging ground state energy and its promise version), and Theorem 5 (undecidability of the ground state energy density).

Significance

The result rules out a general algorithm — and therefore any complete general method — for deciding gappedness from the interaction matrices, however much computing power is available; the property genuinely depends on arbitrarily large system sizes. It also implies, via the standard link between undecidability and independence, that there are concrete finite-dimensional models whose gap is independent of the axioms of any consistent recursively axiomatized formal system (Corollary 4 of the source), and it transfers to other low-energy properties such as the existence of algebraically decaying ground-state correlations.

The theorem is proved; none of it is formalized. This mission produces the machine-checked version. The reusable infrastructure it forces into existence is substantial on its own: a formal model of translationally invariant lattice Hamiltonians and their thermodynamic-limit spectral behaviour, the tiling layer, and computational-history-state Hamiltonians. Each milestone is a self-contained statement that can be attacked without the others.

Difficulty

The obvious approach — encode a halting computation as an energy penalty — gives the ground state energy of a finite lattice, not a property of the limit; this is exactly what Lemma 8 achieves, and it is not enough, because a gap is a statement about the sequence of spectra as L→∞L\to\inftyL→∞ and is insensitive to any single lattice size. The construction must make the halting information visible at all sufficiently large sizes at once while a fixed finite local dimension carries every instance nnn. That forces three separate difficulties: an aperiodic (Robinson) tiling to create squares of every size 2n2^n2n inside one translationally invariant model; a quantum phase-estimation Turing machine whose transition amplitudes encode nnn in a single phase eiπφ(n)e^{i\pi\varphi(n)}eiπφ(n), so that the instance index does not inflate the local dimension; and a history-state Hamiltonian whose low-energy spectrum can be controlled well enough that a positive energy density in the halting case turns into a genuine spectral gap, and a vanishing one into a dense spectrum above the ground state.

Formalization scope

The development commits to the following conventions, all of which are visible in the definition items of this mission.

  1. Lattices are finite: sites are pairs of indices in {0,…,L−1}\{0,\dots,L-1\}{0,…,L−1}, edges are consecutive pairs within a row or a column (open boundary conditions; the periodic case of Section 6.3 of the source is out of scope).
  2. Operators are complex matrices indexed by product-basis configurations; the interactions are embedded by acting as the given matrix on the two sites of an edge and as the identity elsewhere.
  3. The spectrum is taken as the set of real numbers in the matrix spectrum, and λ0\lambda_0λ0​ is its infimum; every statement carries the Hermiticity hypotheses that make this the usual spectrum. Multiplicities are dimensions of eigenspaces, which is how the "identity of spectra as multisets" of Theorem 9 is expressed.
  4. Gapped, gapless and the energy density are properties of the whole family {HΛ(L)}L\{H^{\Lambda(L)}\}_L{HΛ(L)}L​ generated by a fixed triple of matrices, exactly as in Definitions 1 and 2.
  5. Operator norms are ℓ2\ell_2ℓ2​ operator norms; the local interaction strength is the maximum of the three.
  6. Machines are represented by partial recursive codes: "halts on input nnn" is definedness of the evaluation, and "has not halted after LLL steps" is the step-bounded evaluation returning nothing. The explicit local-dimension bounds of Lemma 8 and Theorem 9, which are stated in the source in terms of the number of internal states and the alphabet size of a Turing machine, are replaced by the existence of a finite local dimension.

Degenerate readings are excluded: a zero local dimension satisfies none of the statements, since a non-degenerate ground state requires a one-dimensional eigenspace and the gapless condition requires a non-empty spectrum; and every existential statement fixes the matrices before quantifying over all instances nnn and all lattice sizes LLL.

Contributions are welcome at any milestone, and also on the infrastructure the milestones need — Wang tilings and the Robinson tile set, Gottesman–Irani history-state Hamiltonians, and quantum Turing machines in the Bernstein–Vazirani sense — which are needed for Theorem 6 and Lemma 47 of the source and are not yet part of this mission's item list.

Selected references

  • T. S. Cubitt, D. Pérez-García, M. M. Wolf, Undecidability of the Spectral Gap (full version), Forum of Mathematics, Pi 10:e14, 1–102 (2022). https://doi.org/10.1017/fmp.2021.15 — the version all statements of this mission are formalized against; preprint: https://arxiv.org/abs/1502.04573
  • T. S. Cubitt, D. Pérez-García, M. M. Wolf, Undecidability of the spectral gap, Nature 528, 207–211 (2015). https://doi.org/10.1038/nature16059
  • R. M. Robinson, Undecidability and nonperiodicity for tilings of the plane, Inventiones Mathematicae 12, 177–209 (1971). https://doi.org/10.1007/BF01418780
  • D. Gottesman, S. Irani, The quantum and classical complexity of translationally invariant tiling and Hamiltonian problems, FOCS 2009. https://arxiv.org/abs/0905.2419
  • E. Bernstein, U. Vazirani, Quantum complexity theory, SIAM J. Comput. 26, 1411–1473 (1997). https://doi.org/10.1137/S0097539796300921
  • J. Bausch, T. S. Cubitt, A. Lucia, D. Pérez-García, Undecidability of the spectral gap in one dimension, Phys. Rev. X 10, 031038 (2020). https://doi.org/10.1103/PhysRevX.10.031038
20 thms3 active usersReviewed
🏆Completed
Pure Mathematics·Captain: Lucas

The Gribov Region: Geometry of the Landau-Gauge Faddeev--Popov OperatorResearch Paper

Motivation

Quantizing a Yang–Mills theory by the Faddeev–Popov procedure requires a gauge condition that picks one representative from each gauge orbit. In the Landau gauge the condition is ∂μAμa=0\partial_\mu A_\mu^a = 0∂μ​Aμa​=0. Gribov showed in 1978 that this condition is not ideal: a gauge orbit can meet the surface ∂μAμ=0\partial_\mu A_\mu = 0∂μ​Aμ​=0 more than once, so gauge-equivalent configurations — Gribov copies — are still being integrated over (V. N. Gribov, Quantization of non-Abelian gauge theories, Nucl. Phys. B139 (1978) 1). Infinitesimally, a copy of a transverse field AAA corresponds to a zero mode of the Faddeev–Popov operator Mab(A)=−∂μDμab(A)M^{ab}(A) = -\partial_\mu D_\mu^{ab}(A)Mab(A)=−∂μ​Dμab​(A), which is Hermitian on transverse configurations.

Gribov's proposed remedy is to restrict the functional integral to the Gribov region Ω\OmegaΩ, the set of transverse configurations at which M(A)M(A)M(A) is positive definite. The interest of Ω\OmegaΩ is not only that it removes infinitesimal copies: the fact that it is a bounded region of field space is the geometric input of Gribov's confinement scenario, because restricting the integration to a bounded region deforms the gluon propagator in the infrared and produces a mass scale. Whether the restriction to Ω\OmegaΩ is the physically correct prescription is still debated; the geometric properties of Ω\OmegaΩ themselves are not — they are consequences of the algebraic structure of M(A)M(A)M(A), and they are what this mission formalizes.

Timeline of the properties at issue, as recorded in §2.2.1 (pp. 188–189) of the review by N. Vandersickel and D. Zwanziger, The Gribov problem and QCD dynamics, Phys. Rep. 520 (2012) 175–251 (doi:10.1016/j.physrep.2012.07.003):

  • 1978, Gribov: existence of copies infinitesimally across the horizon ∂Ω\partial\Omega∂Ω (Nucl. Phys. B139 (1978) 1).
  • 1982, D. Zwanziger: Ω\OmegaΩ is convex and bounded in every direction (Nucl. Phys. B209 (1982) 336).
  • 1982, M. Semenov-Tyan-Shanskii and V. Franke: the variational characterization of Ω\OmegaΩ by relative minima of ∥AU∥2\|A^U\|^2∥AU∥2, and the fact that Ω\OmegaΩ still contains copies.
  • 1989, G. Dell'Antonio and D. Zwanziger: Ω\OmegaΩ is contained in an ellipsoid (Nucl. Phys. B326 (1989) 333).
  • 1991, G. Dell'Antonio and D. Zwanziger: every gauge orbit passes inside Ω\OmegaΩ (Comm. Math. Phys. 138 (1991) 291–299).

Setting

Fix a real vector space VVV of gauge-field configurations (in the physical situation, the transverse fields AμaA_\mu^aAμa​) and a finite index set {1,…,n}\{1,\dots,n\}{1,…,n} on which the Faddeev–Popov operator acts (colour index times a finite basis of fluctuation modes ω\omegaω). The formalization works with the algebraic structure that the Faddeev–Popov operator has, and nothing else:

M(A)  =  M0  +  M2(A),M(A) \;=\; M_0 \;+\; M_2(A),M(A)=M0​+M2​(A),

where

  • M0M_0M0​ is the field-independent part, M0=−∂2M_0 = -\partial^2M0​=−∂2 in the physical setting, taken here to be a fixed symmetric positive definite n×nn \times nn×n real matrix;
  • A↦M2(A)A \mapsto M_2(A)A↦M2​(A) is linear in AAA, and each M2(A)M_2(A)M2​(A) is a symmetric traceless real n×nn \times nn×n matrix. In the physical setting M2(A)ab=∂μfabcAμcM_2(A)^{ab} = \partial_\mu f^{abc} A_\mu^cM2​(A)ab=∂μ​fabcAμc​, which is traceless already in the colour indices.

The Gribov region is

Ω  =  { A∈V  :  M(A) is positive definite },M(A) positive definite  ⟺  ∀ w≠0, wTM(A) w>0.\Omega \;=\; \{\, A \in V \;:\; M(A) \text{ is positive definite} \,\}, \qquad M(A) \text{ positive definite} \iff \forall\, w \neq 0,\ w^{\mathsf T} M(A)\, w > 0 .Ω={A∈V:M(A) is positive definite},M(A) positive definite⟺∀w=0, wTM(A)w>0.

This is Eq. (2.52) of the review, with positivity as in Eq. (2.54). The boundary ∂Ω\partial\Omega∂Ω is the first Gribov horizon, where the lowest non-trivial eigenvalue of M(A)M(A)M(A) vanishes.

Formalization targets

Goal — Ω\OmegaΩ is a bounded convex set containing the origin

0∈Ω,Ω convex,∀A≠0 ∃λ0>0 ∀λ≥λ0: λA∉Ω,Ω bounded.0 \in \Omega, \qquad \Omega \text{ convex}, \qquad \forall A \neq 0\ \exists \lambda_0 > 0\ \forall \lambda \ge \lambda_0:\ \lambda A \notin \Omega, \qquad \Omega \text{ bounded}.0∈Ω,Ω convex,∀A=0 ∃λ0​>0 ∀λ≥λ0​: λA∈/Ω,Ω bounded.

The last two clauses are stated under the assumption that A↦M2(A)A \mapsto M_2(A)A↦M2​(A) is injective, i.e. that distinct configurations give distinct field-dependent parts; without it Ω\OmegaΩ contains the whole kernel of M2M_2M2​ as a linear subspace and no boundedness statement can hold.

Supporting statements

M(αA1+βA2)=αM(A1)+βM(A2)(α+β=1),M(\alpha A_1 + \beta A_2) = \alpha M(A_1) + \beta M(A_2) \quad (\alpha + \beta = 1),M(αA1​+βA2​)=αM(A1​)+βM(A2​)(α+β=1), M symmetric, tr⁡M=0, M≠0  ⟹  ∃w: wTMw<0.M \text{ symmetric},\ \operatorname{tr} M = 0,\ M \neq 0 \;\Longrightarrow\; \exists w:\ w^{\mathsf T} M w < 0 .M symmetric, trM=0, M=0⟹∃w: wTMw<0.

These are Eq. (2.53) and Eq. (2.58) of the review; they are the two ingredients from which convexity and directional boundedness follow.

Significance

What the result gives: Ω\OmegaΩ is the region to which Gribov's improved gauge fixing restricts the functional integral, and every subsequent construction in this line of work — the no-pole condition, the horizon function and the local Gribov–Zwanziger action — presupposes that the restriction is to a bounded convex region containing the perturbative point A=0A = 0A=0. Convexity is what makes the horizon condition a single well-posed constraint; boundedness in every direction is the property from which the infrared suppression of the gluon propagator, and hence Gribov's mass scale, is read off. Without boundedness there is no geometric mechanism for a mass gap in this scenario.

Status honesty: these statements are proved mathematics, not open problems; the arguments in §2.2.1 of the review are short. What is missing is a machine-checked account. No formalization of the Gribov region in Lean is known to the drafter of this proposal; the platform's existing Gribov material concerns Singer's topological obstruction to continuous gauge fixing, which is a different theorem about a different object.

Difficulty

The statements are elementary once the correct hypotheses are isolated, and the mission is calibrated accordingly: it is a faithfulness exercise rather than a depth exercise. The two places where a naive attempt fails are worth naming. First, directional boundedness does not follow from positivity alone: it needs the tracelessness of M2(A)M_2(A)M2​(A), which is what forces a direction www with wTM2(A)w<0w^{\mathsf T} M_2(A) w < 0wTM2​(A)w<0; a positive semidefinite perturbation would give a region unbounded along that ray. Second, "bounded in every direction" does not imply "bounded" for a general set, and the implication used here rests on convexity together with injectivity of M2M_2M2​ — the argument goes through a limit of rescaled configurations and a closure of the positivity condition, not through a uniform bound extracted directly from the ray statement.

Formalization scope

The mission commits to a finite-dimensional linear-algebra model of the Faddeev–Popov operator, packaged as a structure carrying: the matrix M0M_0M0​ together with a proof that it is positive definite; the linear map A↦M2(A)A \mapsto M_2(A)A↦M2​(A) together with proofs that each M2(A)M_2(A)M2​(A) is symmetric and traceless. Configurations live in an arbitrary real vector space VVV, which carries a norm and finite-dimensionality only in the two statements where boundedness is asserted. Positive definiteness is Mathlib's notion for real matrices, which includes symmetry; the region is the set of configurations where it holds strictly, so Ω\OmegaΩ is the open region and the horizon is not part of it.

This is a model, not the field-theoretic object: it replaces the operator −∂μDμ-\partial_\mu D_\mu−∂μ​Dμ​ acting on transverse fields by its finite-dimensional algebraic shadow, and the reviewer should audit it as such. The properties targeted here are exactly those whose proofs in §2.2.1 use only linearity in AAA, symmetry, tracelessness, and positivity of −∂2-\partial^2−∂2; results that genuinely need the infinite-dimensional setting — that every gauge orbit passes inside Ω\OmegaΩ, and that Ω\OmegaΩ still contains copies on its boundary — are deliberately out of scope, since they cannot be stated in this model.

The model is not vacuous: an instance exists already for V=RV = \mathbb{R}V=R, n=2n = 2n=2, M0=IM_0 = IM0​=I and M2(t)=t diag(1,−1)M_2(t) = t\,\mathrm{diag}(1,-1)M2​(t)=tdiag(1,−1), with M2M_2M2​ injective, so none of the statements is satisfied vacuously. Nor is any target trivially true: Ω\OmegaΩ is a proper nonempty subset of VVV in that instance.

Infrastructure needed: Mathlib's positive-definiteness API for matrices, the spectral theorem for real symmetric matrices (for the traceless lemma), and basic convexity and boundedness in finite-dimensional normed spaces. The traceless lemma — a nonzero symmetric traceless matrix has a direction of negative quadratic form — is reusable well beyond this mission. Contributions extending the model towards the infinite-dimensional setting, or supplying the explicit ellipsoidal bound of Dell'Antonio–Zwanziger in place of plain boundedness, are welcome.

Selected references

  • N. Vandersickel, D. Zwanziger, The Gribov problem and QCD dynamics, Physics Reports 520 (2012) 175–251. https://doi.org/10.1016/j.physrep.2012.07.003
  • V. N. Gribov, Quantization of non-Abelian gauge theories, Nuclear Physics B139 (1978) 1.
  • D. Zwanziger, Nonperturbative modification of the Faddeev–Popov formula and banishment of the naive vacuum, Nuclear Physics B209 (1982) 336.
  • M. Semenov-Tyan-Shanskii, V. Franke, A variational principle for the Lorentz condition and restriction of the domain of path integration in non-abelian gauge theory, 1982.
  • G. Dell'Antonio, D. Zwanziger, Ellipsoidal bound on the Gribov horizon contradicts the perturbative renormalization group, Nuclear Physics B326 (1989) 333.
  • G. Dell'Antonio, D. Zwanziger, Every gauge orbit passes inside the Gribov horizon, Communications in Mathematical Physics 138 (1991) 291–299.
8 thms3 active usersReviewed
🏆Completed
Algebraic TopologyGroup TheoryRepresentation Theory·Captain: Alien60

Frobenius–Mednykh: Counting Surface-Group Homomorphisms into a Finite GroupResearch Paper

Motivation

How many ways can a closed orientable surface of genus ggg be "coloured" by a finite group GGG? Precisely: how many group homomorphisms π1(Σg)→G\pi_1(\Sigma_g)\to Gπ1​(Σg​)→G are there? The answer is the partition function of two-dimensional Dijkgraaf–Witten theory with gauge group GGG. That theory is the simplest topological quantum field theory (TQFT) in the sense of Atiyah and Segal, and the standard test case for gauge theory with a finite gauge group (Dijkgraaf–Witten 1990, Freed–Quinn 1993). The count has a closed form in terms of the dimensions of the irreducible representations of GGG alone. It is known as Mednykh's formula.

Timeline. Frobenius (1896) counted pairs with a prescribed commutator, #{(a,b):[a,b]=z}\#\{(a,b):[a,b]=z\}#{(a,b):[a,b]=z}, in terms of characters, which is the genus-one case. Frobenius and Schur (1906) treated the non-orientable analogue. Mednykh (1978) proved the formula for every genus using character theory and the standard presentation of π1(Σg)\pi_1(\Sigma_g)π1​(Σg​). It was rediscovered in physics as the partition function of 2D and 3D finite-gauge-group TQFTs (Freed–Quinn 1993), and reproved with matrix integrals (Mulase–Yu 2005) and with lattice TQFTs (Snyder 2007). The last paper fixes the form of the statement used here.

Setting

Let GGG be a finite group. A surface tuple of genus ggg in GGG is a family x=((x1,y1),…,(xg,yg))∈(G×G)gx=((x_1,y_1),\dots,(x_g,y_g))\in(G\times G)^gx=((x1​,y1​),…,(xg​,yg​))∈(G×G)g. Its commutator product is

commProd(x)=[x1,y1] [x2,y2]⋯[xg,yg],[x,y]=xyx−1y−1,\mathrm{commProd}(x)=[x_1,y_1]\,[x_2,y_2]\cdots[x_g,y_g],\qquad [x,y]=xyx^{-1}y^{-1},commProd(x)=[x1​,y1​][x2​,y2​]⋯[xg​,yg​],[x,y]=xyx−1y−1,

multiplied left to right. For z∈Gz\in Gz∈G let Ng(z)=#{x∈(G×G)g:commProd(x)=z}N_g(z)=\#\{x\in(G\times G)^g:\mathrm{commProd}(x)=z\}Ng​(z)=#{x∈(G×G)g:commProd(x)=z} (commCount G g z). The surface group Γg\Gamma_gΓg​ (SurfaceGroup g) is the presented group

Γg=⟨a1,b1,…,ag,bg∣[a1,b1]⋯[ag,bg]⟩,\Gamma_g=\langle a_1,b_1,\dots,a_g,b_g\mid [a_1,b_1]\cdots[a_g,b_g]\rangle,Γg​=⟨a1​,b1​,…,ag​,bg​∣[a1​,b1​]⋯[ag​,bg​]⟩,

the standard presentation of the fundamental group of the closed orientable surface Σg\Sigma_gΣg​ of genus ggg, whose Euler characteristic is χ(Σg)=2−2g\chi(\Sigma_g)=2-2gχ(Σg​)=2−2g.

A complete irreducible family (IrrepFamily G ι) is a finite family (Vi)i∈ι(V_i)_{i\in\iota}(Vi​)i∈ι​ of finite-dimensional complex representations of GGG that are irreducible, pairwise non-isomorphic, and such that every irreducible finite-dimensional complex representation is isomorphic to some ViV_iVi​. Write di=dim⁡CVid_i=\dim_{\mathbb C}V_idi​=dimC​Vi​ and χi(g)=tr⁡Vi(g)\chi_i(g)=\operatorname{tr}V_i(g)χi​(g)=trVi​(g) for the character.

Formalization targets

Goal: Mednykh's formula

For every finite group GGG, every complete irreducible family and every g≥0g\ge 0g≥0,

∑i∈ιdi 2−2g  =  ∣G∣ 1−2g  #Hom⁡(Γg,G),\sum_{i\in\iota} d_i^{\,2-2g}\;=\;|G|^{\,1-2g}\;\#\operatorname{Hom}(\Gamma_g,G),i∈ι∑​di2−2g​=∣G∣1−2g#Hom(Γg​,G),

which is Mulase–Yu, Thm. 1.1 and Snyder, eq. (1) with χ(S)=2−2g\chi(S)=2-2gχ(S)=2−2g. Equivalently, #Hom⁡(Γg,G)=∣G∣∑i(∣G∣/di)2g−2\#\operatorname{Hom}(\Gamma_g,G)=|G|\sum_i(|G|/d_i)^{2g-2}#Hom(Γg​,G)=∣G∣∑i​(∣G∣/di​)2g−2. Exponents are integers: at g=0g=0g=0 the formula reads ∑idi2=∣G∣\sum_i d_i^2=|G|∑i​di2​=∣G∣.

Milestones

The milestones follow the algebraic proof of the counting formula recorded in Mulase–Yu 2002, §4, which goes back to Frobenius and Mednykh. Write (x⋆y)(w)=∑σ∈Gx(wσ−1) y(σ)(x\star y)(w)=\sum_{\sigma\in G}x(w\sigma^{-1})\,y(\sigma)(x⋆y)(w)=∑σ∈G​x(wσ−1)y(σ) for the convolution of functions on GGG.

  • M0. A complete irreducible family exists, with finite index type.
  • M1. #Hom⁡(Γg,G)=Ng(1)\#\operatorname{Hom}(\Gamma_g,G)=N_g(1)#Hom(Γg​,G)=Ng​(1).
  • M2. ∑idi χi(z)=∣G∣\sum_i d_i\,\chi_i(z)=|G|∑i​di​χi​(z)=∣G∣ if z=1z=1z=1 and 000 otherwise.
  • M3. For irreducible VVV of dimension ddd: \sum_{a\in G}\chi_V(axa^{-1}y)= rac{|G|}{d}\chi_V(x)\chi_V(y).
  • M4 (Mulase–Yu eq. (4.2)). For irreducible V,WV,WV,W: χV⋆χW\chi_V\star\chi_WχV​⋆χW​ equals rac{|G|}{d_V}\chi_V if V≅WV\cong WV≅W and 000 otherwise.
  • M5 (Frobenius). N1(z)=∣G∣∑iχi(z)/diN_1(z)=|G|\sum_i\chi_i(z)/d_iN1​(z)=∣G∣∑i​χi​(z)/di​.
  • M6. Ng1+g2=Ng1⋆Ng2N_{g_1+g_2}=N_{g_1}\star N_{g_2}Ng1​+g2​​=Ng1​​⋆Ng2​​.
  • M7 (Mulase–Yu Thm. 4.1). Ng(z)=∣G∣2g−1∑iχi(z) di 1−2gN_g(z)=|G|^{2g-1}\sum_i\chi_i(z)\,d_i^{\,1-2g}Ng​(z)=∣G∣2g−1∑i​χi​(z)di1−2g​ for all g≥0g\ge0g≥0, z∈Gz\in Gz∈G. Mulase–Yu state it for g≥1g\ge1g≥1; the case g=0g=0g=0 is M2.

Significance

The result. The formula says that the number of GGG-coloured genus-ggg surfaces is a function of the multiset of irreducible dimensions alone. Two groups with the same character degrees (for example D4D_4D4​ and Q8Q_8Q8​, both with degrees 1,1,1,1,21,1,1,1,21,1,1,1,2) have equally many homomorphisms from every surface group, even though the groups are not isomorphic. In TQFT language the left side is the evaluation ε(hg)\varepsilon(h^{g})ε(hg) of the Frobenius algebra Z(C[G])Z(\mathbb C[G])Z(C[G]), where hhh is its handle element. The right side is the gauge-theoretic state sum. The identity is the two-dimensional instance of the agreement between the Atiyah–Segal gluing description and the path-integral description of a TQFT. It also gives the volume of the moduli space of flat GGG-bundles on Σg\Sigma_gΣg​, and it underlies counts of covering spaces of surfaces.

Formalizing it. The theorem is classical and fully proved; to our knowledge it has no machine-checked proof. Mathlib has characters of finite-dimensional representations, their orthonormality (FDRep.char_orthonormal) and Maschke's theorem. It lacks the completeness of irreducible characters, the column orthogonality relation (M2), and any statement linking class sums to characters (M3). These are reusable well beyond this mission. The mission also produces the first formal link between a surface-group presentation and representation theory.

Difficulty

The available orthogonality is the row relation between two irreducible characters. Every step here needs the column relation M2, ∑idiχi(z)=∣G∣δz,1\sum_i d_i\chi_i(z)=|G|\delta_{z,1}∑i​di​χi​(z)=∣G∣δz,1​. That relation is equivalent to the decomposition of the regular representation C[G]≅⨁iVi⊕di\mathbb C[G]\cong\bigoplus_i V_i^{\oplus d_i}C[G]≅⨁i​Vi⊕di​​, and in particular to the finiteness and completeness of the irreducible family. Mathlib has no such decomposition. The convolution identity M4 must also be established in its non-isomorphic case, which the row relation alone does not give in convolution form. The passage from Hom⁡(Γg,G)\operatorname{Hom}(\Gamma_g,G)Hom(Γg​,G) to tuples (M1) depends on the universal property of PresentedGroup and on using one ordering of the commutator product throughout. A proof that bypasses characters by brute counting is not available for general GGG.

Formalization scope

All representations are over C\mathbb CC: FDRep ℂ G with G : Type a Group with [Fintype G]. Characters are FDRep.character and did_idi​ is Module.finrank ℂ (V i). Counts are Nat.card. Powers with exponents depending on ggg are integer powers (zpow) in C\mathbb CC, so g=0g=0g=0 is included and no natural-number truncation occurs. Γg\Gamma_gΓg​ is PresentedGroup on generators Fin g × Bool, with aj=(j,false)a_j=(j,\mathrm{false})aj​=(j,false), bj=(j,true)b_j=(j,\mathrm{true})bj​=(j,true) and the single relator (List.ofFn fun j => ⁅a_j, b_j⁆).prod. This is the standard presentation and stands in for π1(Σg)\pi_1(\Sigma_g)π1​(Σg​), since Mathlib has no fundamental groups of closed surfaces. The goal quantifies over every complete irreducible family. M0 shows that such families exist, so the goal is not vacuous. Because the family must be complete and pairwise non-isomorphic, it cannot be chosen to make the sums trivial.

Out of scope: the non-orientable formula of Frobenius–Schur (it needs Frobenius–Schur indicators), positive characteristic, and the bordism-category formulation of TQFTs. Reusable contributions are especially welcome: the decomposition of the regular representation, column orthogonality, and the class-sum Schur lemma.

Selected references

  • N. Snyder, Mednykh's formula via lattice topological quantum field theories, arXiv:math/0703073 (2007). https://arxiv.org/abs/math/0703073
  • A. D. Mednykh, Determination of the number of nonequivalent coverings over a compact Riemann surface, Dokl. Akad. Nauk SSSR 239 (1978) 269–271; English transl. Soviet Math. Dokl. 19 (1978) 318–320.
  • R. Dijkgraaf, E. Witten, Topological gauge theories and group cohomology, Commun. Math. Phys. 129 (1990) 393–429. https://doi.org/10.1007/BF02096988
  • D. S. Freed, F. Quinn, Chern–Simons theory with finite gauge group, Commun. Math. Phys. 156 (1993) 435–472. https://arxiv.org/abs/hep-th/9111004
  • M. Mulase, J. T. Yu, A generating function of the number of homomorphisms from a surface group into a finite group, arXiv:math/0209008 (2002), §4 (algebraic proof). https://arxiv.org/abs/math/0209008
  • M. Mulase, J. T. Yu, Non-commutative matrix integrals and representation varieties of surface groups in a finite group, Ann. Inst. Fourier 55 (2005) 1001–1036. https://arxiv.org/abs/math/0211127
  • J. Kock, Frobenius Algebras and 2D Topological Quantum Field Theories, LMS Student Texts 59, Cambridge Univ. Press (2003). https://doi.org/10.1017/CBO9780511615443
10 thms2 active usersReviewed
🏆Completed
AnalysisCategory TheoryDifferential Geometry·Captain: Alien60

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

Motivation

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

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

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

Setting

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

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

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

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

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

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

The cohomology conditions are elementary Props:

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

Formalization targets

Goal: the continuum classification

For every PPP that admits at least one potential:

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

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

Milestones

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

Four supporting statements isolate the reusable ingredients of Milestone 2:

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

Significance

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

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

Difficulty

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

Formalization scope

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

Selected references

  • J. O. Weatherall, "Understanding Gauge", Philosophy of Science 83 (2016) 1039–1049. arXiv:1505.02229, doi:10.1086/687936. §4: EM1/EM2, Proposition 1, footnotes 9 and 15; the erratum to Proposition 2 is on p. 15 of arXiv v2.
  • M. Spivak, Calculus on Manifolds, W. A. Benjamin, 1965. Theorem 4-11 (Poincaré lemma) and its proof via the operator III, which is KKK above.
  • R. A. Kycia, "The Poincaré lemma, antiexact forms, and fermionic quantum harmonic oscillator", Results in Mathematics 75 (2020) 122. arXiv:1908.02349, doi:10.1007/s00025-020-01247-8.
  • J. Nguyen, N. J. Teh, L. Wells, "Why surplus structure is not superfluous", British Journal for the Philosophy of Science 71 (2020). arXiv:1712.01228.
  • Y. Kudryashov, Mathlib, MeasureTheory/Integral/CurveIntegral/Poincare.lean (Poincaré lemma for 1-forms on convex sets), mathlib4 PR #24019.
17 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Penrose gravitational state reduction: the self-energy criterionResearch Paper

Motivation

Quantum mechanics prescribes two incompatible evolutions: the unitary Schrödinger evolution of an isolated system, and the discontinuous state reduction that a measurement appears to trigger. The measurement problem is to explain when and why reduction takes over. Penrose's answer, set out in the 1996 paper this mission formalizes, is that gravity drives the transition: a superposition of two distinct mass distributions carries two distinct space-time geometries; the time-translation needed to call such a superposition stationary is inherently ill-defined; and the resulting energy fuzziness destabilizes the superposition, with a characteristic lifetime of order ℏ/EΔ\hbar/E_\Deltaℏ/EΔ​, where EΔE_\DeltaEΔ​ is the gravitational self-energy of the difference between the two mass distributions (Penrose 1996). The idea is an objective-collapse proposal in which observers play no special role; it descends from Károlyházy's 1966 considerations through Diósi's 1989 model (doi:10.1103/PhysRevA.40.1165) and its energy-conserving modification by Ghirardi, Grassi and Rimini (doi:10.1103/PhysRevA.42.1057), and it is testable in principle through the mirror-superposition experiment of Marshall, Simon, Penrose and Bouwmeester (doi:10.1103/PhysRevLett.91.130401). A survey of the physical picture is the Wikipedia article on the Penrose interpretation (https://en.wikipedia.org/wiki/Penrose_interpretation).

The physical criterion T≃ℏ/EΔT \simeq \hbar/E_\DeltaT≃ℏ/EΔ​ is a conjecture about nature, not a theorem, and this mission does not ask for its proof. What is a theorem is the mathematical backbone by which Penrose computes the quantity Δ\DeltaΔ — the measure of incompatibility of the two superposed space-time geometries in the Newtonian limit — and identifies it, up to an explicit constant, with the gravitational self-energy of the difference of the two mass distributions. Establishing that chain in Lean 4 is this mission's goal.

Setting

Fix a real gravitational constant GGG. A mass distribution is a smooth, rapidly decreasing (Schwartz) function ρ:R3→R\rho : \mathbb{R}^3 \to \mathbb{R}ρ:R3→R: smooth enough that the potential below is twice differentiable and all integrals converge, and decaying so that boundary terms in the whole-space integration by parts vanish. In Lean these are elements of Mathlib's SchwartzMap over three-dimensional Euclidean space.

The Newtonian potential of ρ\rhoρ is

Φρ(x)=G∫R3ρ(y)∥x−y∥ dy,\Phi_\rho(x) = G \int_{\mathbb{R}^3} \frac{\rho(y)}{\|x-y\|}\,dy,Φρ​(x)=G∫R3​∥x−y∥ρ(y)​dy,

the gravitational field is f=−∇Φρf = -\nabla\Phi_\rhof=−∇Φρ​, and the Laplacian ∇2\nabla^2∇2 is the trace of the second derivative: the sum of second directional derivatives along the standard orthonormal basis. Penrose's measure of incompatibility of two mass distributions ρ,ρ′\rho, \rho'ρ,ρ′ is

Δ(ρ,ρ′)=∫R3∥∇Φρ(x)−∇Φρ′(x)∥2 dx,\Delta(\rho,\rho') = \int_{\mathbb{R}^3} \|\nabla\Phi_\rho(x) - \nabla\Phi_{\rho'}(x)\|^2\,dx,Δ(ρ,ρ′)=∫R3​∥∇Φρ​(x)−∇Φρ′​(x)∥2dx,

the squared L2L^2L2 norm of the difference of the two field gradients (Penrose 1996, Section 6). Two further quantities from the paper: the gravitational self-energy of a distribution σ\sigmaσ,

E(σ)=−G2∬R3×R3σ(x)σ(y)∥x−y∥ dx dy,E(\sigma) = -\frac{G}{2} \iint_{\mathbb{R}^3\times\mathbb{R}^3} \frac{\sigma(x)\sigma(y)}{\|x-y\|}\,dx\,dy,E(σ)=−2G​∬R3×R3​∥x−y∥σ(x)σ(y)​dxdy,

and the interaction energy between two distributions, I(ρ,ρ′)=−G∬ρ(x)ρ′(y)/∥x−y∥ dx dyI(\rho,\rho') = -G \iint \rho(x)\rho'(y)/\|x-y\|\,dx\,dyI(ρ,ρ′)=−G∬ρ(x)ρ′(y)/∥x−y∥dxdy.

Sign conventions. The displayed formulas of Section 6 of the paper mix conventions: the paper's Poisson display ∇2Φ=−4πGρ\nabla^2\Phi = -4\pi G\rho∇2Φ=−4πGρ is inconsistent with its displayed potential formula Φ(x)=−∫ρ(y)/∣x−y∣ dy\Phi(x) = -\int \rho(y)/|x-y|\,dyΦ(x)=−∫ρ(y)/∣x−y∣dy. This mission fixes the convention under which the paper's chain of identities holds as written: ∇2Φρ=−4πGρ\nabla^2\Phi_\rho = -4\pi G\rho∇2Φρ​=−4πGρ, with the potential formula above. Under this convention the first three identities of the displayed chain hold verbatim; the final displayed formula of the paper carries a sign and constant slip and is corrected here to Δ=4πG2∬(ρ−ρ′)(x)(ρ−ρ′)(y)/∥x−y∥ dx dy\Delta = 4\pi G^2 \iint (\rho-\rho')(x)(\rho-\rho')(y)/\|x-y\|\,dx\,dyΔ=4πG2∬(ρ−ρ′)(x)(ρ−ρ′)(y)/∥x−y∥dxdy. The physical reading always takes G>0G > 0G>0, but no item needs that hypothesis.

Formalization targets

The goal is the paper's central identification: the incompatibility measure is the gravitational self-energy of the difference of the two mass distributions, up to the explicit constant −8πG-8\pi G−8πG,

Δ(ρ,ρ′)=−8πG⋅E(ρ−ρ′).\Delta(\rho,\rho') = -8\pi G \cdot E(\rho - \rho').Δ(ρ,ρ′)=−8πG⋅E(ρ−ρ′).

The supporting chain, each step a milestone, from Section 6 of the paper:

∇2Φρ=−4πGρ(Poisson’s equation),\nabla^2\Phi_\rho = -4\pi G\rho \quad\text{(Poisson's equation)},∇2Φρ​=−4πGρ(Poisson’s equation), Δ(ρ,ρ′)=−∫(Φρ−Φρ′)(∇2Φρ−∇2Φρ′)(x) dx(whole-space integration by parts),\Delta(\rho,\rho') = -\int (\Phi_\rho - \Phi_{\rho'})(\nabla^2\Phi_\rho - \nabla^2\Phi_{\rho'})(x)\,dx \quad\text{(whole-space integration by parts)},Δ(ρ,ρ′)=−∫(Φρ​−Φρ′​)(∇2Φρ​−∇2Φρ′​)(x)dx(whole-space integration by parts), Δ(ρ,ρ′)=4πG∫(Φρ−Φρ′)(ρ−ρ′)(x) dx(substituting Poisson),\Delta(\rho,\rho') = 4\pi G \int (\Phi_\rho - \Phi_{\rho'})(\rho-\rho')(x)\,dx \quad\text{(substituting Poisson)},Δ(ρ,ρ′)=4πG∫(Φρ​−Φρ′​)(ρ−ρ′)(x)dx(substituting Poisson), Δ(ρ,ρ′)=4πG2∬(ρ−ρ′)(x)(ρ−ρ′)(y)/∥x−y∥ dx dy(substituting the potential formula).\Delta(\rho,\rho') = 4\pi G^2 \iint (\rho-\rho')(x)(\rho-\rho')(y)/\|x-y\|\,dx\,dy \quad\text{(substituting the potential formula)}.Δ(ρ,ρ′)=4πG2∬(ρ−ρ′)(x)(ρ−ρ′)(y)/∥x−y∥dxdy(substituting the potential formula).

Two structural facts complete the mission: the self-energy is invariant under translation of the distribution (the two locations of Penrose's displaced lump have equal individual self-energies), and under that equal-self-energy hypothesis Δ\DeltaΔ is determined by the interaction energy and the common self-energy,

Δ=8πG⋅I(ρ,ρ′)−16πG⋅E(ρ),\Delta = 8\pi G \cdot I(\rho,\rho') - 16\pi G \cdot E(\rho),Δ=8πG⋅I(ρ,ρ′)−16πG⋅E(ρ),

which is the precise sense of the paper's remark that, apart from the factor 4π4\pi4π, it does not make any difference which expression is used.

Significance

The result itself. The chain turns a space-time consideration — the failure of a consistent time-translation for the superposed geometry — into a computable Newtonian quantity, and identifies that quantity with a classical binding-energy functional. It is the quantitative core of the Diósi–Penrose collapse criterion: every numerical prediction of the model (collapse rates for dust specks, electrons, mirrors) is extracted from the self-energy of the difference distribution.

Formalizing it. None of this chain is formalized anywhere to our knowledge, and Mathlib has no Newtonian-potential layer at all: no potential, no Poisson equation, no gravitational energy functionals. The mission therefore builds reusable infrastructure — Schwartz densities over Euclidean space, the Newtonian potential with its gradient and Laplacian, and the energy functionals — which serves any later Newtonian-gravity formalization (the Schrödinger–Newton equation, Diósi–Penrose dynamics). The proofs exist in the classical potential-theory literature (elliptic regularity for Poisson's equation; change of variables for translation invariance): the mission asks solvers to formalize known mathematics, not to prove new physics.

Difficulty

The naive attack on Poisson's equation — differentiate Φ(x)=G∫ρ(y)/∥x−y∥ dy\Phi(x) = G\int \rho(y)/\|x-y\|\,dyΦ(x)=G∫ρ(y)/∥x−y∥dy twice under the integral sign — fails at the singularity y=xy = xy=x, where the kernel 1/∥x−y∥1/\|x-y\|1/∥x−y∥ is not even once differentiable. That the potential is nonetheless twice differentiable with ∇2Φ=−4πGρ\nabla^2\Phi = -4\pi G\rho∇2Φ=−4πGρ at every point is a genuine elliptic-regularity theorem; solvers will need either a distributional argument with cutoffs and a limiting step, or a direct construction of the second directional derivatives with explicit remainder estimates. The whole-space integration by parts needs decay control: the difference potential decays only like 1/∥x∥1/\|x\|1/∥x∥ when the difference distribution has nonzero total mass, so the boundary term over large balls must be estimated rather than assumed zero. The translation-invariance milestone is a change of variables in a double integral whose kernel is singular on the diagonal — routine, but integrability demands care.

Formalization scope

The Lean representation: mass densities are SchwartzMap (EuclideanSpace ℝ (Fin 3)) ℝ; integrals are Bochner integrals with respect to Mathlib's volume on Euclidean space; the Laplacian is the trace of the second Fréchet derivative, the sum of second directional derivatives along the standard basis vectors. The gravitational constant GGG is an unconstrained real parameter: every identity in the chain is algebraic in GGG, and the physical reading G>0G > 0G>0 is recorded here only. Degenerate inputs: for Schwartz densities every integral appearing in the items converges; nevertheless, Lean's integral returns 000 for a non-integrable integrand, so establishing the relevant integrability is part of each proof — the identities are stated between the honest (convergent) quantities. No item carries an unsatisfiable hypothesis, and no statement is specialized to positive densities: the paper's derivation nowhere uses positivity, so the items quantify over all Schwartz ρ,ρ′\rho, \rho'ρ,ρ′. A trivializing formalization is ruled out: Δ\DeltaΔ is defined independently of the self-energy (an L2L^2L2 norm of a field difference versus a double integral of densities), and the goal asserts their equality.

Selected references

  • R. Penrose, On Gravity's Role in Quantum State Reduction, General Relativity and Gravitation 28(5):581–600, 1996. https://doi.org/10.1007/BF02105068
  • R. Penrose, On the Gravitization of Quantum Mechanics 1: Quantum State Reduction, Foundations of Physics 44(5):557–575, 2014. https://doi.org/10.1007/s10701-013-9770-0
  • L. Diósi, Models for universal reduction of macroscopic quantum fluctuations, Physical Review A 40:1165, 1989. https://doi.org/10.1103/PhysRevA.40.1165
  • G. C. Ghirardi, R. Grassi, A. Rimini, Continuous-spontaneous-reduction models involving gravity, Physical Review A 42:1057, 1990. https://doi.org/10.1103/PhysRevA.42.1057
  • W. Marshall, C. Simon, R. Penrose, D. Bouwmeester, Towards Quantum Superpositions of a Mirror, Physical Review Letters 91:130401, 2003. https://doi.org/10.1103/PhysRevLett.91.130401
  • Wikipedia, Penrose interpretation. https://en.wikipedia.org/wiki/Penrose_interpretation
10 thms2 active usersReviewed
🏆Completed
Functional AnalysisProbabilityTopology·Captain: Lucas

Ensemble spaces: monodecomposability and separatenessResearch Paper

Motivation

A physical law is a claim about what happens whenever a preparation is repeated, not about a single run. The objects of the law are therefore ensembles: the statistical outputs of a preparation procedure. Classical probability distributions and quantum density operators are two realizations of that idea, and they share a convex structure coming from statistical mixing. Gabriele Carcassi and Christine A. Aidala isolate that structure in the draft chapter Ensemble spaces (12 October 2026), as part of the Assumptions of Physics project (assumptionsofphysics.org).

The convex fragment already separates a classical behaviour from a non-classical one. In a classical ensemble space, an ensemble that is separate from two ensembles is separate from every mixture of them. In a quantum ensemble space it need not be: the equal mixture of two orthogonal pure states is not separate from a pure state in their span. The draft turns this distinction into a theorem that uses only mixing. Monodecomposability — every decomposable ensemble has no two decompositions in which one summand is separate from both summands of the other — holds if and only if mixtures preserve separateness (Proposition 1.35).

This mission formalizes that equivalence and the lemmas of §§1.2–1.3 that it depends on. Entropy, affine embedding, and the open problems of the same draft are later developments and are not assumed here.

Setting

An ensemble space is a nonempty topological space EEE that is T0T_0T0​ and second countable, together with a continuous mixing operation

(p,a,b)↦pa+pˉb,p∈[0,1],pˉ=1−p.(p,a,b)\mapsto pa+\bar p b,\qquad p\in[0,1],\quad \bar p=1-p.(p,a,b)↦pa+pˉ​b,p∈[0,1],pˉ​=1−p.

Mixing is the identity 1a+0b=a1a+0b=a1a+0b=a, idempotent (pa+pˉa=apa+\bar p a=apa+pˉ​a=a), commutative (pa+pˉb=pˉb+papa+\bar p b=\bar p b+papa+pˉ​b=pˉ​b+pa), and associative in the following sense. If p1,p3∈[0,1)p_1,p_3\in[0,1)p1​,p3​∈[0,1), p1+p3≤1p_1+p_3\le 1p1​+p3​≤1 and p2=1−p1−p3p_2=1-p_1-p_3p2​=1−p1​−p3​, then

p1e1+pˉ1(p2pˉ1e2+p3pˉ1e3)=pˉ3(p1pˉ3e1+p2pˉ3e2)+p3e3.p_1 e_1+\bar p_1\Bigl(\frac{p_2}{\bar p_1}e_2+\frac{p_3}{\bar p_1}e_3\Bigr) =\bar p_3\Bigl(\frac{p_1}{\bar p_3}e_1+\frac{p_2}{\bar p_3}e_2\Bigr)+p_3 e_3.p1​e1​+pˉ​1​(pˉ​1​p2​​e2​+pˉ​1​p3​​e3​)=pˉ​3​(pˉ​3​p1​​e1​+pˉ​3​p2​​e2​)+p3​e3​.

In the formalization the operation is mix p a b, equal to pa+pˉbpa+\bar p bpa+pˉ​b. Binary mixing records only the first coefficient.

A finite mixture ∑i=1npiei\sum_{i=1}^n p_i e_i∑i=1n​pi​ei​, for pi∈[0,1]p_i\in[0,1]pi​∈[0,1] with ∑ipi=1\sum_i p_i=1∑i​pi​=1, is the nested mixture (1.11) of the pairs with pi≠0p_i\neq 0pi​=0, in the given order. Reordering the pairs does not change the ensemble (Corollary 1.12).

An ensemble ccc is a component of aaa when a=pc+pˉda=pc+\bar p da=pc+pˉ​d for some ensemble ddd and some p∈(0,1]p\in(0,1]p∈(0,1]. Two ensembles are separate, written a⋔ba\pitchfork ba⋔b, when they have no common component. An extreme point has no component other than itself. An internal point admits every ensemble as a component. A boundary point is a point that is not internal.

A set AAA is bounded around eee when every open neighbourhood UUU of eee admits some p∈[0,1)p\in[0,1)p∈[0,1) with pe+pˉA⊆Upe+\bar p A\subseteq Upe+pˉ​A⊆U.

An ensemble is decomposable when it is a mixture pa+pˉbpa+\bar p bpa+pˉ​b with p∈(0,1)p\in(0,1)p∈(0,1) and a≠ba\neq ba=b; separately decomposable when the two summands may be taken separate; and multidecomposable when it admits two such decompositions

e=pa1+pˉa2=qb1+qˉb2e=pa_1+\bar p a_2=qb_1+\bar q b_2e=pa1​+pˉ​a2​=qb1​+qˉ​b2​

with a1⋔b1a_1\pitchfork b_1a1​⋔b1​ and a1⋔b2a_1\pitchfork b_2a1​⋔b2​. It is monodecomposable when it is not multidecomposable. The space is monodecomposable when every decomposable ensemble is. Mixtures preserve separateness when e⋔ae\pitchfork ae⋔a and e⋔be\pitchfork be⋔b imply e⋔(pa+pˉb)e\pitchfork(pa+\bar p b)e⋔(pa+pˉ​b) for every p∈[0,1]p\in[0,1]p∈[0,1].

Formalization targets

Proposition 1.35 — goal

For an ensemble space EEE,

E is monodecomposable⟺mixtures preserve separateness in E.\text{$E$ is monodecomposable} \quad\Longleftrightarrow\quad \text{mixtures preserve separateness in $E$.}E is monodecomposable⟺mixtures preserve separateness in E.

The two sides are exactly Definitions 1.33 and 1.28. No entropy, orthogonality, or finite-dimensionality hypothesis is added, and none is removed.

Corollary 1.12

For pi∈[0,1]p_i\in[0,1]pi​∈[0,1] with ∑ipi=1\sum_i p_i=1∑i​pi​=1 and any permutation τ\tauτ,

∑ipiei=∑ipτ(i)eτ(i),\sum_i p_i e_i=\sum_i p_{\tau(i)} e_{\tau(i)},i∑​pi​ei​=i∑​pτ(i)​eτ(i)​,

and the common value exists as an ensemble.

Proposition 1.17

A set AAA is bounded around eee if and only if pne+pˉnan→ep_n e+\bar p_n a_n\to epn​e+pˉ​n​an​→e whenever pn→1p_n\to 1pn​→1 in [0,1][0,1][0,1] and an∈Aa_n\in Aan​∈A.

Proposition 1.21

The set of internal points is convex: it is closed under mixing.

Corollary 1.25

Components and separateness satisfy the six properties listed in the draft: every ensemble is a component of itself; a component yields a common component, so the two ensembles are not separate; separateness is irreflexive and symmetric; distinct extreme points are separate; an internal point is not separate from any ensemble; separate ensembles are boundary points.

Proposition 1.27

If eee is separate from pe1+pˉe2pe_1+\bar p e_2pe1​+pˉ​e2​ for some p∈(0,1)p\in(0,1)p∈(0,1), then eee is separate from λe1+λˉe2\lambda e_1+\bar\lambda e_2λe1​+λˉe2​ for every λ∈[0,1]\lambda\in[0,1]λ∈[0,1].

Corollary 1.32

An ensemble is extreme if and only if it is not decomposable.

Significance

Proposition 1.35 is the convex form of the draft's classicality test. One direction says that if mixing can create a common component where none existed, then some ensemble has two genuinely different separate decompositions. The other says that if mixing never does this, then no decomposable ensemble is multidecomposable. The quantum Bloch ball is the draft's witness that the property can fail; the classical simplex is the witness that it can hold. Those two model statements (Proposition 1.34 and Propositions 1.29–1.30) are not part of this mission, but the interface they would plug into is.

The same interface is what the later sections of the draft extend: entropy is defined on a space that already mixes, and affine combinations are built from that mixing. A machine-checked Proposition 1.35 is a base those extensions can import without taking the entropy axiom as a hypothesis they do not use.

The argument in the draft is a proof, not an open problem. It had not been formalized against this 12 October 2026 text. An earlier formalization on this platform records Axioms 4.4, 4.7 and 4.55 of the 31 December 2025 book, in which entropy is part of the same structure. That package is a different source. Importing it here would add the entropy axiom to theorems proved in the draft before entropy is introduced, and would weaken them.

Difficulty

The equivalence is not a rephrasing of the definitions. One direction needs Proposition 1.27, whose proof places an auxiliary ensemble on a segment and rewrites coefficients so that a common component of eee and one mixture becomes a common component of eee and another. The arithmetic is sensitive to which endpoint is which, and to the restriction p∈(0,1)p\in(0,1)p∈(0,1) rather than p∈[0,1]p\in[0,1]p∈[0,1].

Corollary 1.12 is an induction on a bracketed expression, not on an unordered convex combination. Definition 1.10 deletes zero coefficients before bracketing. An encoding that feeds a zero coefficient to binary mixing denotes the same point only after the mixture axioms are applied; the draft's definition does not do that. The statement below follows the draft and deletes zeros first.

Proposition 1.17 is a topological fact about a continuous binary operation on a space that need not be a topological vector space. There is no scalar multiplication to rescale a neighbourhood, so the argument has to manufacture the shrink from mixing alone. Boundedness around eee is not the same as metric boundedness, and the draft does not assume a metric.

Formalization scope

The carrier is a type EEE with a topological-space instance. An EnsembleSpace packages nonemptiness, the T0T_0T0​ and second-countability axioms, and the mixing operation. Coefficients of the operation are elements of the unit interval. In the associativity axiom, each real expression is shown to lie in [0,1][0,1][0,1] and is then used as that element; it is not replaced by a projection.

Finite mixtures are partial. Zero coefficients are removed, order preserved, and the rest is folded by binary mixing as in (1.11). The fold returns no value if every coefficient was zero or a tail sum vanishes. On inputs with nonnegative coefficients at most 111 that sum to 111, Corollary 1.12 asserts that a value exists. Real coefficients that arise while rescaling a tail are passed through the projection onto [0,1][0,1][0,1], which is the identity for data obeying those hypotheses. The empty index set cannot occur under the sum hypothesis: the sum of no coefficients is 0≠10\neq 10=1.

Separateness, components, extreme and internal points, decomposability and monodecomposability are propositions on this structure. A component uses a coefficient in (0,1](0,1](0,1]. A decomposition uses a coefficient in (0,1)(0,1)(0,1) and two distinct ensembles. Multidecomposability asks for two such decompositions, with one summand of the first separate from both summands of the second.

Entropy, orthogonality, affine combinations, vector-space embeddings, metrics, and the classical and quantum models are out of scope. In particular the goal must not be restated as “every Choquet simplex is a simplex”, and separateness must not be replaced by disjointness of supports. Adding the entropy axiom, or cancellativity, is a different theorem. Contributions that build the missing model statements on top of these definitions, without changing them, are the natural continuation; changes to the definitions are not.

Selected references

  • G. Carcassi and C. A. Aidala, Ensemble spaces, draft chapter, 12 October 2026. Axiom 1.4 (p. 12), Axiom 1.7 (p. 13), Definition 1.10 (p. 15), Corollary 1.12 (p. 15), Definition 1.16 and Proposition 1.17 (pp. 17–19), Definitions 1.19, 1.20, 1.24 and Corollary 1.25 (pp. 19–22), Proposition 1.27 (p. 23), Definitions 1.28 and 1.31 (pp. 24–25), Corollary 1.32 (p. 25), Definition 1.33 and Proposition 1.35 (p. 26). The draft states that it is generated from the project sources.
  • G. Carcassi and C. A. Aidala, Assumptions of Physics, project site and sources: assumptionsofphysics.org and github.com/assumptionsofphysics/book.
  • T. Fritz, Convex spaces I: Definition and examples, arXiv:0903.5522, 2009. arXiv:0903.5522. Cited by the draft for the algebraic convex-space axioms matched by Axiom 1.7.
9 thms2 active usersReviewed
🏆Completed
ProbabilityQuantum Information·Captain: mikedeng1

Quantum Speedup of Monte Carlo Methods 2: Along a B-Chebyshev Cooling Schedule, Consecutive Gibbs Sample States Overlap with |⟨π_i|π_{i+1}⟩|² ≥ 1/BResearch Paper

Motivation

Approximating a partition function Z(β)=∑x∈Ωe−βH(x)Z(\beta)=\sum_{x\in\Omega}e^{-\beta H(x)}Z(β)=∑x∈Ω​e−βH(x) is a central task in statistical physics and in counting: it covers the Ising and Potts models, and, at β=∞\beta=\inftyβ=∞, counting the zero-energy configurations of a Hamiltonian, for instance the proper kkk-colourings of a graph. Computing Z(∞)Z(\infty)Z(∞) exactly is #P-complete in many cases, so the goal is an estimate Z~\widetilde ZZ with ∣Z~−Z(∞)∣≤ϵZ(∞)|\widetilde Z-Z(\infty)|\le\epsilon Z(\infty)∣Z−Z(∞)∣≤ϵZ(∞) with high probability.

The standard classical approach writes Z(∞)Z(\infty)Z(∞) as a telescoping product of ratios αi=Z(βi+1)/Z(βi)\alpha_i=Z(\beta_{i+1})/Z(\beta_i)αi​=Z(βi+1​)/Z(βi​) along a sequence of inverse temperatures 0=β0<β1<⋯<βℓ=∞0=\beta_0<\beta_1<\dots<\beta_\ell=\infty0=β0​<β1​<⋯<βℓ​=∞, and estimates each ratio by sampling from the Gibbs distribution πi\pi_iπi​ at βi\beta_iβi​. Dyer and Frieze (1992, as cited on p. 14 of arXiv:1504.06987v3) showed how to bound the number of samples when each estimator has bounded relative second moment; Štefankovič, Vempala and Vigoda (J. ACM 2009) named the resulting condition a Chebyshev cooling schedule and showed that schedules of length O~(log⁡∣Ω∣)\widetilde O(\sqrt{\log|\Omega|})O(log∣Ω∣​) exist and can be found efficiently.

Montanaro (arXiv:1504.06987v3, 2017) gives a quantum algorithm for this problem that improves the dependence on ϵ\epsilonϵ and on the relaxation time τ\tauτ of the underlying Markov chains quadratically. Its quantum sampling step rests on a theorem of Wocjan and Abeyesinghe (Phys. Rev. A 78, 042336, 2008): a sequence of coherent quantum sample states can be prepared efficiently if consecutive states overlap by at least a constant. This mission formalizes the paper's own link between the two: a Chebyshev cooling schedule produces exactly such overlaps.

Setting

Let Ω\OmegaΩ be a finite set of configurations and H:Ω→{0,1,…,n}H:\Omega\to\{0,1,\dots,n\}H:Ω→{0,1,…,n} an integer-valued Hamiltonian. Inverse temperatures range over [0,∞][0,\infty][0,∞]. The partition function is

Z(β)=∑x∈Ωe−βH(x),Z(\beta)=\sum_{x\in\Omega}e^{-\beta H(x)},Z(β)=x∈Ω∑​e−βH(x),

with the convention e−∞⋅h=1e^{-\infty\cdot h}=1e−∞⋅h=1 if h=0h=0h=0 and 000 otherwise, so that Z(0)=∣Ω∣Z(0)=|\Omega|Z(0)=∣Ω∣ and Z(∞)Z(\infty)Z(∞) counts the configurations with H(x)=0H(x)=0H(x)=0.

A cooling schedule is a sequence 0=β0<β1<⋯<βℓ=∞0=\beta_0<\beta_1<\dots<\beta_\ell=\infty0=β0​<β1​<⋯<βℓ​=∞. Along it, the Gibbs distributions are πi(x)=e−βiH(x)/Z(βi)\pi_i(x)=e^{-\beta_iH(x)}/Z(\beta_i)πi​(x)=e−βi​H(x)/Z(βi​), the ratios are αi=Z(βi+1)/Z(βi)\alpha_i=Z(\beta_{i+1})/Z(\beta_i)αi​=Z(βi+1​)/Z(βi​), and the estimators are the random variables Yi(x)=e−(βi+1−βi)H(x)Y_i(x)=e^{-(\beta_{i+1}-\beta_i)H(x)}Yi​(x)=e−(βi+1​−βi​)H(x), whose mean under πi\pi_iπi​ is αi\alpha_iαi​.

Definition 1 (Chebyshev cooling schedule). The schedule is a BBB-Chebyshev cooling schedule for ZZZ if for every i=0,…,ℓ−1i=0,\dots,\ell-1i=0,…,ℓ−1

Z(2βi+1−βi) Z(βi)Z(βi+1)2≤B.\frac{Z(2\beta_{i+1}-\beta_i)\,Z(\beta_i)}{Z(\beta_{i+1})^2}\le B.Z(βi+1​)2Z(2βi+1​−βi​)Z(βi​)​≤B.

The chi-squared divergence of ν\nuν from π\piπ is χ2(ν,π)=∑xπ(x)(ν(x)/π(x)−1)2\chi^2(\nu,\pi)=\sum_x\pi(x)\big(\nu(x)/\pi(x)-1\big)^2χ2(ν,π)=∑x​π(x)(ν(x)/π(x)−1)2, and the quantum sample of a distribution π\piπ is the unit vector ∣π⟩=∑x∈Ωπ(x) ∣x⟩|\pi\rangle=\sum_{x\in\Omega}\sqrt{\pi(x)}\,|x\rangle∣π⟩=∑x∈Ω​π(x)​∣x⟩ of ℓ2(Ω;C)\ell^2(\Omega;\mathbb C)ℓ2(Ω;C). In Lean these are Z, gibbs, alpha, Y, IsCoolingSchedule, IsChebyshevSchedule, chiSq and qsample in the namespace QuantumMC.Cooling.

Formalization targets

Goal: overlap of consecutive quantum samples

For every BBB-Chebyshev cooling schedule and every i∈{0,…,ℓ−1}i\in\{0,\dots,\ell-1\}i∈{0,…,ℓ−1},

∣⟨πi∣πi+1⟩∣2≥1B.|\langle\pi_i|\pi_{i+1}\rangle|^2\ge\frac1B.∣⟨πi​∣πi+1​⟩∣2≥B1​.

The statement fixes no value of BBB and no length ℓ\ellℓ; it is the shape in which the paper feeds the schedule into the quantum sampling theorem, with overlap parameter p=1/Bp=1/Bp=1/B.

Milestones

  1. The second form of the divergence: χ2(ν,π)=∑xν(x)2/π(x)−1\chi^2(\nu,\pi)=\sum_x\nu(x)^2/\pi(x)-1χ2(ν,π)=∑x​ν(x)2/π(x)−1 for probability vectors with π>0\pi>0π>0.
  2. Display (1): χ2(πi+1,πi)=Z(βi)Z(2βi+1−βi)/Z(βi+1)2−1\chi^2(\pi_{i+1},\pi_i)=Z(\beta_i)Z(2\beta_{i+1}-\beta_i)/Z(\beta_{i+1})^2-1χ2(πi+1​,πi​)=Z(βi​)Z(2βi+1​−βi​)/Z(βi+1​)2−1, including the last step βi+1=∞\beta_{i+1}=\inftyβi+1​=∞.
  3. Along a BBB-Chebyshev schedule, χ2(πi+1,πi)≤B−1\chi^2(\pi_{i+1},\pi_i)\le B-1χ2(πi+1​,πi​)≤B−1 for all iii.
  4. For distributions ν\nuν and π>0\pi>0π>0: 1/χ2(ν,π)+1≤∑xν(x)π(x)/ν(x)=⟨ν∣π⟩1/\sqrt{\chi^2(\nu,\pi)+1}\le\sum_x\nu(x)\sqrt{\pi(x)/\nu(x)}=\langle\nu|\pi\rangle1/χ2(ν,π)+1​≤∑x​ν(x)π(x)/ν(x)​=⟨ν∣π⟩.

Companion statements

The classical facts of §3–3.1 that motivate Definition 1: Eπi[Yi]=αi\mathbb E_{\pi_i}[Y_i]=\alpha_iEπi​​[Yi​]=αi​; E[Yi2]/E[Yi]2=Z(2βi+1−βi)Z(βi)/Z(βi+1)2\mathbb E[Y_i^2]/\mathbb E[Y_i]^2=Z(2\beta_{i+1}-\beta_i)Z(\beta_i)/Z(\beta_{i+1})^2E[Yi2​]/E[Yi​]2=Z(2βi+1​−βi​)Z(βi​)/Z(βi+1​)2; the telescoping product Z(βℓ)=Z(β0)∏iαiZ(\beta_\ell)=Z(\beta_0)\prod_i\alpha_iZ(βℓ​)=Z(β0​)∏i​αi​ with Z(β0)=∣Ω∣Z(\beta_0)=|\Omega|Z(β0​)=∣Ω∣; Var⁡(Yi)/E[Yi]2≤B\operatorname{Var}(Y_i)/\mathbb E[Y_i]^2\le BVar(Yi​)/E[Yi​]2≤B; and the accuracy claim that ratio estimates within relative error ϵ/(2ℓ)\epsilon/(2\ell)ϵ/(2ℓ), each failing with probability at most 1/(4ℓ)1/(4\ell)1/(4ℓ), give ∣Z~−Z(∞)∣≤ϵZ(∞)|\widetilde Z-Z(\infty)|\le\epsilon Z(\infty)∣Z−Z(∞)∣≤ϵZ(∞) with probability at least 3/43/43/4 for ϵ<1\epsilon<1ϵ<1.

Significance

The result. The overlap bound is the hypothesis of the Wocjan–Abeyesinghe theorem (Theorem 9 of the paper) and is used in the proof of the paper's partition-function theorem (Theorem 11). It explains why a cooling schedule built for a classical estimator, with no reference to quantum states, is also good enough for quantum annealing-style state preparation. The paper remarks that, unlike the classical analysis of Štefankovič, Vempala and Vigoda, which needs the reverse divergence χ2(πi,πi+1)\chi^2(\pi_i,\pi_{i+1})χ2(πi​,πi+1​) and a reversed schedule, the overlap is symmetric in iii and i+1i+1i+1, so no reversal is needed.

Formalizing it. The result is proved on paper; nothing in it has been machine-checked. A formal development pins down the treatment of the endpoint βℓ=∞\beta_\ell=\inftyβℓ​=∞, where πℓ\pi_\ellπℓ​ is supported on the ground states and is no longer strictly positive, and records exactly which positivity conditions the divergence identities require. The definitions of Gibbs distributions, cooling schedules and χ2\chi^2χ2 on a finite space are reusable for other analyses of simulated annealing and of partition-function estimation.

Difficulty

The algebra at finite temperatures is a direct computation. The step that needs care is the last one, i=ℓ−1i=\ell-1i=ℓ−1: there βi+1=∞\beta_{i+1}=\inftyβi+1​=∞, the weights e−∞⋅H(x)e^{-\infty\cdot H(x)}e−∞⋅H(x) are indicator values, 2βi+1−βi2\beta_{i+1}-\beta_i2βi+1​−βi​ is again ∞\infty∞, and the divergence identity must hold with πi+1\pi_{i+1}πi+1​ vanishing on every configuration of positive energy. A formalization that replaces ∞\infty∞ by a large finite inverse temperature, or that requires both distributions to be strictly positive, does not cover this step. The second point is the passage from a bound on the divergence to a bound on an inner product of quantum states, which must handle the configurations where ν(x)=0\nu(x)=0ν(x)=0.

Formalization scope

Inverse temperatures are elements of [0,∞][0,\infty][0,∞] (ℝ≥0∞); the Boltzmann weight branches on β=∞\beta=\inftyβ=∞. The differences βi+1−βi\beta_{i+1}-\beta_iβi+1​−βi​ and 2βi+1−βi2\beta_{i+1}-\beta_i2βi+1​−βi​ are truncated subtractions in [0,∞][0,\infty][0,∞], exact on a cooling schedule. A schedule is a map N→[0,∞]\mathbb N\to[0,\infty]N→[0,∞] of which only β0,…,βℓ\beta_0,\dots,\beta_\ellβ0​,…,βℓ​ matter, and "for all iii" ranges over i=0,…,ℓ−1i=0,\dots,\ell-1i=0,…,ℓ−1. HHH takes values in N\mathbb NN with H≤nH\le nH≤n. Quantum samples are vectors of EuclideanSpace ℂ Ω with real amplitudes, and ∣⟨⋅∣⋅⟩∣2|\langle\cdot|\cdot\rangle|^2∣⟨⋅∣⋅⟩∣2 is the squared norm of the complex inner product.

Added hypotheses, all disclosed in the statements: some configuration has H(x)=0H(x)=0H(x)=0, so that Z(∞)>0Z(\infty)>0Z(∞)>0 (without it πℓ\pi_\ellπℓ​ and the last ratio of Definition 1 are divisions by zero, which Lean evaluates to 000); the general divergence statements assume π(x)>0\pi(x)>0π(x)>0, which the paper's displays use implicitly by dividing by π(x)\pi(x)π(x). No hypothesis is placed on BBB. In the accuracy companion, the per-ratio guarantee is stated as a bound on the failure probability; neither measurability nor independence is assumed.

A goal that assumes χ2(πi+1,πi)≤B−1\chi^2(\pi_{i+1},\pi_i)\le B-1χ2(πi+1​,πi​)≤B−1, assumes B>0B>0B>0 in a way that excludes the endpoint, or drops the step βℓ=∞\beta_\ell=\inftyβℓ​=∞ would be a different, weaker statement; the goal's only hypothesis on the schedule is Definition 1.

Not formalized: the quantum walk algorithms, the Wocjan–Abeyesinghe theorems (Theorems 9 and 10), the sample and step counts of Theorems 8 and 11 (stated in O(⋅)O(\cdot)O(⋅) notation), and the existence of short Chebyshev cooling schedules.

Contributions welcome: proofs of the milestones and of the companions, and lemmas on Gibbs distributions at β=∞\beta=\inftyβ=∞ that the companions share.

Selected references

  • A. Montanaro, Quantum speedup of Monte Carlo methods, Proc. R. Soc. A 471:20150301, 2015; cited here as the preprint arXiv:1504.06987v3, 2017. https://arxiv.org/abs/1504.06987
  • D. Štefankovič, S. Vempala, E. Vigoda, Adaptive simulated annealing: a new connection between sampling and counting, J. ACM 56(3):18, 2009. https://arxiv.org/abs/cs/0612058
  • P. Wocjan, A. Abeyesinghe, Speedup via quantum sampling, Phys. Rev. A 78:042336, 2008. https://arxiv.org/abs/0804.4259
  • P. Wocjan, C.-F. Chang, D. Nagaj, A. Abeyesinghe, Quantum algorithm for approximating partition functions, Phys. Rev. A 80:022340, 2009. https://arxiv.org/abs/0811.0596
  • M. Szegedy, Quantum speed-up of Markov chain based algorithms, FOCS 2004, 32–41. https://arxiv.org/abs/quant-ph/0401053
6 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Hu–Wang 2023: Hubble Tension — Distance Relations Behind the H₀ ProbesResearch Paper

Motivation

The Hubble constant H0H_0H0​, the present expansion rate of the Universe, is inferred in two largely independent ways: from the cosmic microwave background (CMB) assuming the flat ΛCDM model, giving H0=67.40±0.50H_0 = 67.40 \pm 0.50H0​=67.40±0.50 km/s/Mpc (Planck 2018), and from the local distance ladder of Cepheids and Type Ia supernovae, giving H0=73.04±1.04H_0 = 73.04 \pm 1.04H0​=73.04±1.04 km/s/Mpc (Riess et al. 2022). The 4σ–6σ gap between such estimates is the Hubble tension. The review of Hu and Wang (2023) surveys the independent probes used to arbitrate it (strongly lensed quasars, megamasers, gravitational waves, fast radio bursts, the tip of the red giant branch) and the evidence, from a possible redshift dependence of the inferred H0H_0H0​, that the late-time Universe may need modification.

Several probes in that survey turn an observable into a value of H0H_0H0​ through an explicit formula in a flat ΛCDM background. This mission formalizes those formulas, Eqs. (1)–(8) of the review, and the mathematical properties that the inference relies on: that a measured time-delay distance determines H0H_0H0​ uniquely, that the dispersion measure–redshift relation of fast radio bursts is invertible, and that a "running" H0H_0H0​ diagnostic is a genuine test of flat ΛCDM.

Setting

Fix a matter density parameter Ωm≥0\Omega_m \ge 0Ωm​≥0 and impose spatial flatness, so that the dark-energy density parameter is ΩΛ=1−Ωm\Omega_\Lambda = 1 - \Omega_mΩΛ​=1−Ωm​. The dimensionless expansion rate is

E(z)=Ωm(1+z)3+1−Ωm,E(z) = \sqrt{\Omega_m(1+z)^3 + 1 - \Omega_m},E(z)=Ωm​(1+z)3+1−Ωm​​,

and the Hubble rate at redshift zzz is H(z)=H0E(z)H(z) = H_0 E(z)H(z)=H0​E(z).

Distances. For redshifts z1≤z2z_1 \le z_2z1​≤z2​ and speed of light ccc, the angular diameter distance between them is (Eq. (2))

D12=cH0(1+z2)∫z1z2dz′E(z′),D_{12} = \frac{c}{H_0(1+z_2)} \int_{z_1}^{z_2} \frac{dz'}{E(z')},D12​=H0​(1+z2​)c​∫z1​z2​​E(z′)dz′​,

and the distance from the observer to redshift zzz is the case z1=0z_1 = 0z1​=0 (Eq. (3)). A lens at redshift zlensz_{\rm lens}zlens​ in front of a quasar at zsz_szs​ has distances DdD_dDd​ (to the lens), DsD_sDs​ (to the source) and DdsD_{ds}Dds​ (lens to source), and the time-delay distance (Eq. (1))

DΔt=(1+zlens)DdDsDdsD_{\Delta t} = (1+z_{\rm lens}) \frac{D_d D_s}{D_{ds}}DΔt​=(1+zlens​)Dds​Dd​Ds​​

is the quantity inferred from the time delay between lensed images.

Fast radio bursts. The mean intergalactic dispersion measure at redshift zzz is (Eq. (5))

⟨DMIGM(z)⟩=AΩbH02H0∫0zfIGM(z′) fe(z′) (1+z′)Ωm(1+z′)3+1−Ωm dz′,A=3c8πGmp,\langle {\rm DM_{IGM}}(z)\rangle = \frac{A\Omega_b H_0^2}{H_0}\int_0^{z}\frac{f_{\rm IGM}(z')\,f_e(z')\,(1+z')}{\sqrt{\Omega_m(1+z')^3+1-\Omega_m}}\,dz', \qquad A = \frac{3c}{8\pi G m_p},⟨DMIGM​(z)⟩=H0​AΩb​H02​​∫0z​Ωm​(1+z′)3+1−Ωm​​fIGM​(z′)fe​(z′)(1+z′)​dz′,A=8πGmp​3c​,

where Ωb\Omega_bΩb​ is the baryon density parameter, fIGMf_{\rm IGM}fIGM​ the fraction of baryons in the intergalactic medium, and fe=YHXe,H+12YHeXe,Hef_e = Y_H X_{e,H} + \frac12 Y_{He} X_{e,He}fe​=YH​Xe,H​+21​YHe​Xe,He​ the electron fraction. The observed dispersion measure adds Milky Way and host contributions (Eq. (4)).

Redshift-dependent H0H_0H0​. Data binned in redshift are placed at the weighted redshift zˉ=∑nznσn−2/∑nσn−2\bar z = \sum_n z_n \sigma_n^{-2} / \sum_n \sigma_n^{-2}zˉ=∑n​zn​σn−2​/∑n​σn−2​ (Eq. (6)); the trend of H0H_0H0​ across bins is fitted by the evolution function g(z)=H~0/(1+z)αg(z) = \tilde H_0/(1+z)^\alphag(z)=H~0​/(1+z)α (Eq. (7)); and for an arbitrary expansion history HHH the H0H_0H0​ diagnostic is (Eq. (8))

H0(z)=H(z)1−Ωm0+Ωm0(1+z)3.H_0(z) = \frac{H(z)}{\sqrt{1-\Omega_{m0}+\Omega_{m0}(1+z)^3}}.H0​(z)=1−Ωm0​+Ωm0​(1+z)3​H(z)​.

Formalization targets

Goal: the time-delay distance determines H0H_0H0​

For c>0c > 0c>0, Ωm≥0\Omega_m \ge 0Ωm​≥0 and 0<zlens<zs0 < z_{\rm lens} < z_s0<zlens​<zs​ there is K>0K > 0K>0 such that for every H0>0H_0 > 0H0​>0,

DΔt(H0)=KH0.D_{\Delta t}(H_0) = \frac{K}{H_0}.DΔt​(H0​)=H0​K​.

The constant KKK is left unspecified: the goal asserts only the shape of the dependence, which is what makes the quasar-lensing inference of H0H_0H0​ well posed.

Milestones

  1. Eqs. (2)–(3): in flat ΛCDM, Dds=Ds−1+zlens1+zsDdD_{ds} = D_s - \frac{1+z_{\rm lens}}{1+z_s} D_dDds​=Ds​−1+zs​1+zlens​​Dd​ for 0≤zlens≤zs0 \le z_{\rm lens} \le z_s0≤zlens​≤zs​.
  2. 1/H01/H_01/H0​ scaling: H0DΔt(H0)H_0 D_{\Delta t}(H_0)H0​DΔt​(H0​) is independent of H0≠0H_0 \neq 0H0​=0.
  3. Positivity: DΔt>0D_{\Delta t} > 0DΔt​>0 for c,H0>0c, H_0 > 0c,H0​>0 and 0<zlens<zs0 < z_{\rm lens} < z_s0<zlens​<zs​.
  4. Eq. (5): ⟨DMIGM(z)⟩\langle {\rm DM_{IGM}}(z)\rangle⟨DMIGM​(z)⟩ is strictly increasing on z≥0z \ge 0z≥0 for positive continuous fIGMf_{\rm IGM}fIGM​, fef_efe​.
  5. Electron fraction: fe=7/8f_e = 7/8fe​=7/8 for YH=0.75Y_H = 0.75YH​=0.75, YHe=0.25Y_{He} = 0.25YHe​=0.25, full ionization.
  6. Eq. (6): zˉ\bar zzˉ lies in any interval containing all the znz_nzn​.
  7. Eq. (7): ggg is strictly decreasing for H~0>0\tilde H_0 > 0H~0​>0, α>0\alpha > 0α>0.
  8. Eq. (8): H0(z)≡H0H_0(z) \equiv H_0H0​(z)≡H0​ on z≥0z \ge 0z≥0 if and only if H(z)=H0E(z)H(z) = H_0 E(z)H(z)=H0​E(z) on z≥0z \ge 0z≥0.

Significance

The results. The review's quantitative arguments use these formulas as black boxes. The goal and milestones 1–3 make precise the statement that the time-delay distance is "primarily sensitive to H0H_0H0​": it is exactly inversely proportional to H0H_0H0​, with all other cosmological dependence in a positive constant. Milestone 4 is the invertibility of the dispersion measure–redshift relation on which FRB cosmology rests. Milestones 6–8 underpin the "descending H0H_0H0​" evidence of Section 5: the effective redshift of a bin is a redshift of that bin, a positive exponent in ggg means a decreasing trend, and a non-constant diagnostic H0(z)H_0(z)H0​(z) is equivalent to a departure from flat ΛCDM.

Formalizing them. These facts are standard and their proofs are short on paper. The mission also records a transcription issue in the source: Eq. (3) prints the integrand as Ωm(1+z′)3+ΩΛ\sqrt{\Omega_m(1+z')^3+\Omega_\Lambda}Ωm​(1+z′)3+ΩΛ​​, which is inconsistent with Eq. (2); the formalization uses the reciprocal square root, as in Eq. (2).

Difficulty

The algebraic statements (milestones 2, 5, 7, 8) require care only with Lean's total division and real powers. The analytic statements involve interval integrals: milestone 1 needs integrability of 1/E1/E1/E on [0,zs][0, z_s][0,zs​] and additivity of the integral, and milestones 3 and 4 need strict positivity of the integral of a positive continuous function over a nondegenerate interval. Unfolding the definitions and clearing denominators fails as soon as a denominator such as DdsD_{ds}Dds​ or E(z)E(z)E(z) might vanish; each such case has to be ruled out from the hypotheses.

Formalization scope

All quantities are real-valued. Flatness is built in by writing 1−Ωm1 - \Omega_m1−Ωm​ for ΩΛ\Omega_\LambdaΩΛ​; Ωm≥0\Omega_m \ge 0Ωm​≥0 is assumed where needed, while Ωm≤1\Omega_m \le 1Ωm​≤1 is never needed and is not assumed. The angular diameter distances are interval integrals of 1/E1/E1/E; division by zero evaluates to 000, so positivity of the relevant denominators is either assumed or proved. The power (1+z)α(1+z)^\alpha(1+z)α in Eq. (7) is the real power and the weights σn−2\sigma_n^{-2}σn−2​ in Eq. (6) are integer powers. Physical constants (ccc, GGG, mpm_pmp​) and the functions fIGMf_{\rm IGM}fIGM​, fef_efe​ are free parameters, not numerical values. The statistical analyses of the review (likelihood fits, Gaussian-process reconstructions, quoted σ-levels) are out of scope.

All definitions live in one shared definition file in the HuWang2023 namespace; the distance functions and the H0H_0H0​ diagnostic are reusable for other flat-ΛCDM missions.

Selected references

  • J.-P. Hu and F.-Y. Wang, Hubble Tension: The Evidence of New Physics, Universe 9 (2023) 94. https://doi.org/10.3390/universe9020094
  • Planck Collaboration, Planck 2018 results. VI. Cosmological parameters, A&A 641 (2020) A6. https://arxiv.org/abs/1807.06209
  • A. G. Riess et al., A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team, ApJL 934 (2022) L7. https://arxiv.org/abs/2112.04510
  • K. C. Wong et al., H0LiCOW XIII. A 2.4% measurement of H0H_0H0​ from lensed quasars, MNRAS 498 (2020) 1420. https://arxiv.org/abs/1907.04869
  • J.-P. Macquart et al., A census of baryons in the Universe from localized fast radio bursts, Nature 581 (2020) 391. https://arxiv.org/abs/2005.13161
  • C. Krishnan, E. Ó Colgáin, M. M. Sheikh-Jabbari, T. Yang, Running Hubble tension and a H0H_0H0​ diagnostic, Phys. Rev. D 103 (2021) 103509. https://arxiv.org/abs/2011.02858
  • M. G. Dainotti et al., On the Hubble constant tension in the SNe Ia Pantheon sample, ApJ 912 (2021) 150. https://arxiv.org/abs/2103.02117
10 thms2 active usersReviewed
🏆Completed
Differential Geometry·Captain: Lucas

Relativity and Particle Mechanics: the Lorentz-force geodesic equation from Hamiltonian mechanicsResearch Paper

Motivation

How much of relativity is already contained in Hamiltonian particle mechanics? The note by Carcassi and Aidala argues that the metric tensor need not be postulated as a property of space-time: it emerges as the linear relation between the conjugate (kinetic) momentum of a particle and its velocity, Πα=m gαβ uβ\Pi_\alpha = m\,g_{\alpha\beta}\,u^\betaΠα​=mgαβ​uβ. Writing the symplectic form in position–momentum or position–velocity variables, the metric and the electromagnetic force tensor FαβF_{\alpha\beta}Fαβ​ appear as components of the symplectic structure, and the geodesic equation with the Lorentz force falls out of Hamilton's equations.

Setting

Space-time is a single coordinate chart Rn\mathbb R^nRn with coordinates xαx^\alphaxα; phase space is Rn×Rn\mathbb R^n\times\mathbb R^nRn×Rn with canonical coordinates (qα,pα)(q^\alpha,p_\alpha)(qα,pα​), qα=xαq^\alpha = x^\alphaqα=xα, and canonical Poisson bracket {f,h}=∂qμf ∂pμh−∂pμf ∂qμh\{f,h\} = \partial_{q^\mu}f\,\partial_{p_\mu}h - \partial_{p_\mu}f\,\partial_{q^\mu}h{f,h}=∂qμ​f∂pμ​​h−∂pμ​​f∂qμ​h. The data are

  1. a smooth metric gαβ(x)g_{\alpha\beta}(x)gαβ​(x): symmetric and nondegenerate at every point, of any signature, with inverse gαβg^{\alpha\beta}gαβ;
  2. a smooth vector potential Aα(x)A_\alpha(x)Aα​(x) with force tensor Fαβ=∂αAβ−∂βAαF_{\alpha\beta} = \partial_\alpha A_\beta - \partial_\beta A_\alphaFαβ​=∂α​Aβ​−∂β​Aα​;
  3. a charge eee (written qqq in the note) and a mass m≠0m \ne 0m=0.

The kinetic momentum is Πα=pα−eAα\Pi_\alpha = p_\alpha - eA_\alphaΠα​=pα​−eAα​, the velocity uα=1mgαβΠβu^\alpha = \frac1m g^{\alpha\beta}\Pi_\betauα=m1​gαβΠβ​, and the Hamiltonian (extended phase space) is H=12mΠαgαβΠβ=12m uαgαβuβH = \frac1{2m}\Pi_\alpha g^{\alpha\beta}\Pi_\beta = \frac12 m\,u^\alpha g_{\alpha\beta}u^\betaH=2m1​Πα​gαβΠβ​=21​muαgαβ​uβ; it generates the evolution dsf={f,H}d_s f = \{f,H\}ds​f={f,H} along the affine parameter sss. Christoffel symbols are Γαβγ=12(∂γgαβ+∂βgαγ−∂αgβγ)\Gamma_{\alpha\beta\gamma} = \frac12(\partial_\gamma g_{\alpha\beta} + \partial_\beta g_{\alpha\gamma} - \partial_\alpha g_{\beta\gamma})Γαβγ​=21​(∂γ​gαβ​+∂β​gαγ​−∂α​gβγ​) and Γβγα=gαδΓδβγ\Gamma^\alpha_{\beta\gamma} = g^{\alpha\delta}\Gamma_{\delta\beta\gamma}Γβγα​=gαδΓδβγ​. The note also introduces the symbol Gαβγ=∂αgβγ−∂βgαγG_{\alpha\beta\gamma} = \partial_\alpha g_{\beta\gamma} - \partial_\beta g_{\alpha\gamma}Gαβγ​=∂α​gβγ​−∂β​gαγ​, which appears in the symplectic form in position–velocity variables.

Formalization targets

Goal: the geodesic equation modified by the force tensor (eq. (9))

DsΠα  =  dsΠα−dsxδ Γδαγ Πγ  =  em Fαβ gβγ Πγ,D_s\Pi_\alpha \;=\; d_s\Pi_\alpha - d_s x^\delta\,\Gamma^\gamma_{\delta\alpha}\,\Pi_\gamma \;=\; \frac{e}{m}\,F_{\alpha\beta}\,g^{\beta\gamma}\,\Pi_\gamma ,Ds​Πα​=ds​Πα​−ds​xδΓδαγ​Πγ​=me​Fαβ​gβγΠγ​,

as an identity of functions on phase space, where ds={⋅,H}d_s = \{\cdot,H\}ds​={⋅,H}. Hamilton's equations alone, with no geometric postulate, yield the covariant Lorentz-force law.

Milestones

The milestones follow the equations of the note: the inverse-metric derivative (2), the brackets of kinetic momenta (8), the position equation (9), the symbol GGG and its raised form (10)–(11), the velocity brackets (13), the position–velocity form of the geodesic equation (14), the antisymmetrized covariant derivatives (15), and the statement that G≡0G\equiv 0G≡0 makes the metric a Hessian (16).

Significance

The results make precise the claim that the metric and the force tensor characterize the geometry of the tangent bundle as seen by Hamiltonian mechanics. The symbol GαβγG_{\alpha\beta\gamma}Gαβγ​ is not a tensor, and eq. (16) shows that frames with G≡0G\equiv0G≡0 have a Hessian metric; the note ends with the open question of which frames have G=0G = 0G=0, and whether such frames exist in curved space-time.

Difficulty

Each statement is a finite computation, but the computations combine the Leibniz rule for the Poisson bracket, derivatives of the matrix inverse, and repeated relabeling of dummy indices. Eq. (16) needs a Poincaré-lemma argument (closed one-forms on Rn\mathbb R^nRn are exact), applied twice.

Formalization scope

Everything is stated in one global chart Rn\mathbb R^nRn (Fin n → ℝ); partial derivatives are Fréchet derivatives along coordinate directions, and all index sums are explicit finite sums. Smoothness of ggg and AAA and nondegeneracy of ggg are standing assumptions (the definition IsSmoothMetric). Phase-space functions are functions of (x,p)(x,p)(x,p), and dsfd_s fds​f is the canonical Poisson bracket {f,H}\{f,H\}{f,H}, so no flow or ODE solution is needed. The differential-form computations of eqs. (3), (6), (10) and (12), and the transformation law of GGG on p. 8, are not included as targets.

Selected references

  • G. Carcassi, C. A. Aidala, Relativity and Particle Mechanics (note).
15 thms2 active usersReviewed
🏆Completed
Quantum Mechanics·Captain: Lucas

Carcassi–Landini–Aidala 2024: Classical mechanics as the high-entropy limit of quantum mechanicsResearch Paper

1. Motivation

Carcassi, Landini and Aidala (arXiv:2411.00972) argue that classical mechanics is the high-entropy limit of quantum mechanics, in the same way that non-relativistic mechanics is the low-speed limit of relativistic mechanics. The usual mathematical recipe ℏ→0\hbar \to 0ℏ→0 is reinterpreted as sending the entropy of pure states to −∞-\infty−∞, i.e. as S≫0S \gg 0S≫0. The paper backs this with explicit formulas: Gaussian entropy–uncertainty curves, the black-body spectrum, the trace identity for the maximally mixed state, classical and quantum "stretching maps" on phase space, and a Lindblad master equation that implements the quantum stretch. This mission formalizes those mathematical claims.

2. Setting

We use one degree of freedom with phase space R2∋(x,p)\mathbb R^2 \ni (x,p)R2∋(x,p).

  • Gaussian entropies. For a Gaussian state with uncertainty Σ=σxσp\Sigma = \sigma_x\sigma_pΣ=σx​σp​ the classical (Gibbs) entropy is SC(Σ)=ln⁡(Σ/ℏ)+1S_C(\Sigma) = \ln(\Sigma/\hbar) + 1SC​(Σ)=ln(Σ/ℏ)+1 (Eq. 2). The quantum (von Neumann) entropy is SQ(Σ)=(Σℏ+12)ln⁡(Σℏ+12)−(Σℏ−12)ln⁡(Σℏ−12)S_Q(\Sigma) = (\tfrac{\Sigma}{\hbar}+\tfrac12)\ln(\tfrac{\Sigma}{\hbar}+\tfrac12) - (\tfrac{\Sigma}{\hbar}-\tfrac12)\ln(\tfrac{\Sigma}{\hbar}-\tfrac12)SQ​(Σ)=(ℏΣ​+21​)ln(ℏΣ​+21​)−(ℏΣ​−21​)ln(ℏΣ​−21​) (Eq. 3). The rescaled quantum entropy of Section 4.3 is SQλ(Σ)=SQ(λΣ)−ln⁡λS^\lambda_Q(\Sigma) = S_Q(\lambda\Sigma) - \ln\lambdaSQλ​(Σ)=SQ​(λΣ)−lnλ. It is the quantum curve after shrinking the pure-state uncertainty from ℏ\hbarℏ to ℏ/λ\hbar/\lambdaℏ/λ and moving the zero of entropy accordingly.
  • Pure stretching map. T(x,p)=(λx,λp)T(x,p) = (\sqrt\lambda x, \sqrt\lambda p)T(x,p)=(λ​x,λ​p) with λ>1\lambda > 1λ>1 (Eq. 16). It acts on densities by push-forward, (Tρ)(z)=λ−1ρ(z/λ)(T\rho)(z) = \lambda^{-1}\rho(z/\sqrt\lambda)(Tρ)(z)=λ−1ρ(z/λ​). The Gibbs entropy is S(ρ)=−∫ρlog⁡ρS(\rho) = -\int\rho\log\rhoS(ρ)=−∫ρlogρ (Eq. 15). The same stretch acts on Husimi distributions on C\mathbb CC: Qλ(α)=λ−1Q1(α/λ)Q_\lambda(\alpha) = \lambda^{-1}Q_1(\alpha/\sqrt\lambda)Qλ​(α)=λ−1Q1​(α/λ​) (Eq. 24).
  • Lindblad generator. In the Heisenberg picture, X˙=iℏ[H,X]+∑iγi(Li†XLi−12{Li†Li,X})\dot X = \tfrac{i}{\hbar}[H,X] + \sum_i\gamma_i(L_i^\dagger X L_i - \tfrac12\{L_i^\dagger L_i, X\})X˙=ℏi​[H,X]+∑i​γi​(Li†​XLi​−21​{Li†​Li​,X}) (Eq. 26). The quantum stretch uses H=0H = 0H=0 and a single jump operator L=a†L = a^\daggerL=a†, where the ladder operators satisfy [a,a†]=1[a,a^\dagger] = 1[a,a†]=1.

3. Target

The goal (Section 4.3, Fig. 3, p. 11): for all ℏ>0\hbar > 0ℏ>0 and Σ>0\Sigma > 0Σ>0,

lim⁡λ→∞(SQ(λΣ)−ln⁡λ)=ln⁡(Σ/ℏ)+1=SC(Σ).\lim_{\lambda\to\infty}\big(S_Q(\lambda\Sigma) - \ln\lambda\big) = \ln(\Sigma/\hbar) + 1 = S_C(\Sigma).λ→∞lim​(SQ​(λΣ)−lnλ)=ln(Σ/ℏ)+1=SC​(Σ).

This is the quantitative form of "taking λ→∞\lambda\to\inftyλ→∞ is equivalent to ℏ→0\hbar\to0ℏ→0": the quantum Gaussian entropy curve converges to the classical one.

Milestones, in the order of the paper:

  1. Zeros and signs of the entropy curves (Sec. 2.2): SQ(ℏ/2)=0S_Q(\hbar/2)=0SQ​(ℏ/2)=0 and SQ>0S_Q>0SQ​>0 above the Heisenberg bound; SC(ℏ/e)=0S_C(\hbar/e) = 0SC​(ℏ/e)=0 and SC<0S_C<0SC​<0 below it.
  2. Fig. 2: SC(Σ)−SQ(Σ)→0S_C(\Sigma) - S_Q(\Sigma) \to 0SC​(Σ)−SQ​(Σ)→0 as Σ→∞\Sigma\to\inftyΣ→∞.
  3. Eq. (4): tr⁡(AB I/n)=tr⁡(BA I/n)\operatorname{tr}(AB\,I/n) = \operatorname{tr}(BA\,I/n)tr(ABI/n)=tr(BAI/n).
  4. Eq. (8): Planck's law divided by the Rayleigh–Jeans law tends to 111 as β→0+\beta\to0^+β→0+.
  5. Eq. (15): S(Tρ)=S(ρ)+log⁡λS(T\rho) = S(\rho) + \log\lambdaS(Tρ)=S(ρ)+logλ.
  6. Eq. (18): ⟨T(xnpm)⟩=λ n+m⟨xnpm⟩\langle T(x^np^m)\rangle = \sqrt\lambda^{\,n+m}\langle x^np^m\rangle⟨T(xnpm)⟩=λ​n+m⟨xnpm⟩.
  7. Eq. (25): ∫αnαˉmQλ=λ n+m∫βnβˉmQ1\int\alpha^n\bar\alpha^m Q_\lambda = \sqrt\lambda^{\,n+m}\int\beta^n\bar\beta^mQ_1∫αnαˉmQλ​=λ​n+m∫βnβˉ​mQ1​.
  8. Eq. (28): for L=a†L = a^\daggerL=a†, H=0H=0H=0, the generator maps an(a†)ma^n(a^\dagger)^man(a†)m to γ2(n+m) an(a†)m\tfrac\gamma2(n+m)\,a^n(a^\dagger)^m2γ​(n+m)an(a†)m.
  9. Eq. (38): [λX,λP]=iλℏ[\sqrt\lambda X, \sqrt\lambda P] = i\lambda\hbar[λ​X,λ​P]=iλℏ when [X,P]=iℏ[X,P] = i\hbar[X,P]=iℏ.

4. Significance

The goal makes the slogan "classical = high-entropy quantum" precise for Gaussian states: the classical entropy–uncertainty law is exactly the limit of the quantum one under the entropy rescaling the paper constructs. The milestones are the computational facts the argument rests on. The paper derives them by hand and none has been machine-checked. Several are reusable well beyond this paper: entropy under scaling of densities, moment scaling under dilations, and the action of the Lindblad generator on anti-normally ordered monomials in the Weyl algebra.

5. Difficulty

The goal is an asymptotic expansion of x↦(x+12)ln⁡(x+12)−(x−12)ln⁡(x−12)x\mapsto(x+\tfrac12)\ln(x+\tfrac12) - (x-\tfrac12)\ln(x-\tfrac12)x↦(x+21​)ln(x+21​)−(x−21​)ln(x−21​) at infinity. The naive term-by-term limit has the form ∞−∞\infty-\infty∞−∞ and must be organised as a difference quotient or Taylor expansion of xln⁡xx\ln xxlnx. The measure-theoretic milestones need change of variables for the dilation z↦z/λz\mapsto z/\sqrt\lambdaz↦z/λ​ on R2\mathbb R^2R2 and C\mathbb CC, plus careful integrability bookkeeping for ρlog⁡ρ\rho\log\rhoρlogρ. The Lindblad milestone needs the commutator identities [an,a†]=nan−1[a^n, a^\dagger] = n a^{n-1}[an,a†]=nan−1 and [a,(a†)m]=m(a†)m−1[a, (a^\dagger)^m] = m (a^\dagger)^{m-1}[a,(a†)m]=m(a†)m−1 in a noncommutative ring.

6. Formalization scope

  • Entropies are real functions of ℏ\hbarℏ and Σ\SigmaΣ; we assume ℏ>0\hbar>0ℏ>0 and Σ>0\Sigma>0Σ>0. Lean's Real.log returns 000 at 000, which agrees with the convention 0ln⁡0=00\ln0=00ln0=0 at the Heisenberg point Σ=ℏ/2\Sigma=\hbar/2Σ=ℏ/2.
  • Phase space is ℝ × ℝ with Lebesgue measure, and Husimi distributions live on ℂ. Densities are real functions. The entropy milestone assumes ρ≥0\rho\ge0ρ≥0, ∫ρ=1\int\rho = 1∫ρ=1, and integrability of ρ\rhoρ and ρlog⁡ρ\rho\log\rhoρlogρ, i.e. finite entropy, which the paper uses implicitly. The moment identities hold for every function, since an integral that does not converge is 000 on both sides.
  • Ladder operators are elements a,a†a, a^\daggera,a† of an abstract ℂ-algebra with aa†−a†a=1aa^\dagger - a^\dagger a = 1aa†−a†a=1, and the adjoint of each jump operator is passed explicitly. This avoids unbounded operators. The hypothesis is satisfiable, e.g. by differentiation and multiplication by XXX on C[X]\mathbb C[X]C[X]. No bounded operators satisfy it, so do not specialise to a C*-algebra.
  • λ>1\lambda>1λ>1 throughout, as in the paper (ΔS=log⁡λ>0\Delta S = \log\lambda > 0ΔS=logλ>0).
  • Out of scope: the CPTP property and entropy monotonicity of TQT_QTQ​ (Eqs. 31–32), and the Wigner-function formulas (Eqs. 46–54). These need operator theory on L2L^2L2 that is not available in Mathlib.

Selected references

  • G. Carcassi, M. Landini, C. A. Aidala, Classical mechanics as the high-entropy limit of quantum mechanics, arXiv:2411.00972v3 (2026). https://arxiv.org/abs/2411.00972
  • M. A. Nielsen, I. L. Chuang, Quantum Computation and Quantum Information, Cambridge University Press (2010).
14 thms2 active usersReviewed
🏆Completed
Functional Analysis·Captain: Lucas

The unphysicality of Hilbert spaces (Carcassi–Aidala–Calderón)Research Paper

Motivation

Quantum states are standardly modelled as rays in a complex Hilbert space, following von Neumann's 1932 axiomatisation. Carcassi, Aidala and Calderón (arXiv:2308.06669) examine which parts of this definition can be justified by physical requirements. They argue that the inner product space structure is physically required — it is exactly what is needed to describe statistical mixtures of states and their entropy — while completeness in infinite dimensions is not: it forces the state space to contain states with infinite expectation values, coordinate changes that turn finite expectations into infinite ones, and time evolutions that do so in finite time. The paper suggests Schwartz spaces as a possible alternative.

The physical conclusions of the paper (its Propositions 19 and 31) are arguments, not mathematical theorems. Behind them, however, sits a set of precise mathematical statements in Section VI and Appendix A. This mission formalizes those statements.

Setting

Let HHH be a complex inner product space, not necessarily complete. For ψ∈H\psi\in Hψ∈H, ∣ψ⟩⟨ψ∣|\psi\rangle\langle\psi|∣ψ⟩⟨ψ∣ is the operator x↦⟨ψ,x⟩ψx\mapsto\langle\psi,x\rangle\psix↦⟨ψ,x⟩ψ. A finite mixture of pure states is an operator ∑iai∣ψi⟩⟨ψi∣\sum_i a_i|\psi_i\rangle\langle\psi_i|∑i​ai​∣ψi​⟩⟨ψi​∣ with finitely many unit vectors ψi\psi_iψi​ and weights ai>0a_i>0ai​>0 summing to 111. The von Neumann entropy of such an operator is S(ρ)=−∑kλklog⁡λkS(\rho)=-\sum_k\lambda_k\log\lambda_kS(ρ)=−∑k​λk​logλk​ over its eigenvalues, and I(ψ,ϕ)I(\psi,\phi)I(ψ,ϕ) denotes the entropy of the equal mixture 12∣ψ⟩⟨ψ∣+12∣ϕ⟩⟨ϕ∣\frac12|\psi\rangle\langle\psi|+\frac12|\phi\rangle\langle\phi|21​∣ψ⟩⟨ψ∣+21​∣ϕ⟩⟨ϕ∣.

On the position side, L2(R)L^2(\mathbb R)L2(R) is the Hilbert space of square-integrable complex wave functions. An orientation-preserving diffeomorphism f:R→Rf:\mathbb R\to\mathbb Rf:R→R (smooth, strictly increasing, with smooth inverse) acts on wave functions by

(Ufψ)(y)=ψ(f−1(y))∣(f−1)′(y)∣,(U_f\psi)(y)=\psi\bigl(f^{-1}(y)\bigr)\sqrt{|(f^{-1})'(y)|},(Uf​ψ)(y)=ψ(f−1(y))∣(f−1)′(y)∣​,

which is the transformation law of a wave function under the change of coordinate y=f(x)y=f(x)y=f(x). The nnn-th absolute position moment of a state ψ\psiψ is ∫∣x∣n∣ψ(x)∣2 dx∈[0,∞]\int|x|^n|\psi(x)|^2\,dx\in[0,\infty]∫∣x∣n∣ψ(x)∣2dx∈[0,∞]; finite moments of all orders are the natural minimal requirement for the statistics of position to be well defined.

Formalization targets

Goal

∃ f, U=Uf, ψ∈L2(R), ∥ψ∥=1:∫∣x∣n∣ψ∣2<∞  ∀n,∫y2 ∣Uψ(y)∣2 dy=∞.\exists\,f,\ U=U_f,\ \psi\in L^2(\mathbb R),\ \|\psi\|=1:\quad \int|x|^n|\psi|^2<\infty\ \ \forall n,\qquad \int y^2\,|U\psi(y)|^2\,dy=\infty .∃f, U=Uf​, ψ∈L2(R), ∥ψ∥=1:∫∣x∣n∣ψ∣2<∞  ∀n,∫y2∣Uψ(y)∣2dy=∞.

A unitary transformation of L2(R)L^2(\mathbb R)L2(R) that is nothing but a change of the position coordinate can map a state with all moments finite to one with infinite expected squared position. The goal is stated existentially, leaving the particular change of coordinates free.

Milestones

  1. Proposition 5 — rays alone do not determine the coefficients of a superposition.
  2. Proposition 7 — equal strictly convex mixtures span the same subspace.
  3. Proposition 8 — a finite-rank mixed state can be decomposed so as to include a given pure state from its range.
  4. Proposition 9 — ψ\psiψ is a superposition of {ϕj}\{\phi_j\}{ϕj​} iff some mixture of the ϕj\phi_jϕj​ can also be written as a mixture including ψ\psiψ.
  5. Proposition 10 — I(ψ,ϕ)=f(∣⟨ψ,ϕ⟩∣)I(\psi,\phi)=f(|\langle\psi,\phi\rangle|)I(ψ,ϕ)=f(∣⟨ψ,ϕ⟩∣) with an explicit fff injective on [0,1][0,1][0,1].
  6. Proposition 20 — the domain of an unbounded closed operator between Hilbert spaces is not complete.
  7. Proposition 21 — a unitary can move a vector out of such a domain.
  8. Proposition 24 — UfU_fUf​ is unitary on L2(R)L^2(\mathbb R)L2(R).
  9. Equation (29) — y(x)=tan⁡(π2erf⁡x)y(x)=\tan(\frac\pi2\operatorname{erf}x)y(x)=tan(2π​erfx) is an orientation-preserving diffeomorphism transporting the Gaussian state e−x2/π\sqrt{e^{-x^2}/\sqrt\pi}e−x2/π​​ to 1/π(y2+1)1/\sqrt{\pi(y^2+1)}1/π(y2+1)​.
  10. Equations (27)–(28) — the Gaussian state has all moments finite, the Lorentzian state has all moments of order ≥2\ge2≥2 infinite.

Significance

The goal makes precise one of the paper's three claims about completeness: being an isomorphism of Hilbert spaces does not respect finiteness of expectation values, even for a transformation as innocuous as a smooth change of coordinates. Propositions 20 and 21 make precise the companion claim that completeness forces the inclusion of states outside the domain of every unbounded observable, and that unitaries do not preserve such domains. Propositions 7–10 make precise the paper's case for the inner product: equivalence of superposition with non-unique decomposition of mixtures, and the entropic meaning of the transition probability.

All statements are mathematically elementary relative to modern functional analysis, and none of them, to the knowledge of the proposer, has a machine-checked proof. Formalizing them pins down hypotheses the paper leaves implicit: two statements needed corrections to be true (see the notes on Propositions 8 and 20).

Difficulty

Most of the work is infrastructure rather than a single hard step. Proposition 24 requires the change-of-variables formula for Lebesgue integrals and a construction of the induced operator on L2L^2L2 equivalence classes, including surjectivity. Equation (29) requires developing the error function (limits ±1\pm1±1 at ±∞\pm\infty±∞, smoothness, positivity of its derivative) and differentiating tan⁡∘(π2erf⁡)\tan\circ(\frac\pi2\operatorname{erf})tan∘(2π​erf). Proposition 10 requires computing the spectrum of a rank-two operator through the eigenvalue API for self-adjoint operators on a finite-dimensional space. Proposition 20 rests on the closed graph theorem. The moment statements require Gaussian integrability and a comparison of ∣y∣n/(1+y2)|y|^n/(1+y^2)∣y∣n/(1+y2) with 1/∣y∣1/|y|1/∣y∣ at infinity.

Formalization scope

All statements live in the namespace UnphysicalHilbert. State spaces are complex inner product spaces (InnerProductSpace ℂ H), completeness assumed only where the paper assumes a Hilbert space. Finite sets of states are finite indexed families; a finite-rank density operator is a finite strictly convex combination of pure states. The entropy of the equal mixture is computed on the span of the two vectors, on which the operator acts. L2(R)L^2(\mathbb R)L2(R) is Lp ℂ 2 volume, unitaries are linear isometric equivalences, and finiteness of a moment means Lebesgue integrability of ∣x∣n∣ψ(x)∣2|x|^n|\psi(x)|^2∣x∣n∣ψ(x)∣2.

Two departures from the text are deliberate and flagged in the item notes: Proposition 8 assumes ψ∈range⁡ρ\psi\in\operatorname{range}\rhoψ∈rangeρ instead of ⟨ψ∣ρ∣ψ⟩≠0\langle\psi|\rho|\psi\rangle\neq0⟨ψ∣ρ∣ψ⟩=0 (the latter admits a counterexample in C2\mathbb C^2C2), and Propositions 20–21 assume the operator is closed (without some such hypothesis an everywhere-defined discontinuous functional is a counterexample). Proposition 5 assumes the coefficients are nonzero, which its proof uses. The time evolution of eq. (30) and the remarks on Schwartz spaces in Section VIII are not formalized, because the paper does not state them as propositions. The existential goal cannot be satisfied trivially: the operator is pinned to the change-of-variables formula, and ψ\psiψ must be a unit vector with all moments finite.

Contributions of reusable infrastructure are welcome, in particular: the error function, the unitary on L2(R)L^2(\mathbb R)L2(R) induced by a diffeomorphism, and the spectrum of 12(∣ψ⟩⟨ψ∣+∣ϕ⟩⟨ϕ∣)\frac12(|\psi\rangle\langle\psi|+|\phi\rangle\langle\phi|)21​(∣ψ⟩⟨ψ∣+∣ϕ⟩⟨ϕ∣).

Selected references

  • G. Carcassi, C. A. Aidala, F. Calderón, The unphysicality of Hilbert spaces, arXiv:2308.06669v3, 2024. https://arxiv.org/abs/2308.06669
  • J. von Neumann, Mathematische Grundlagen der Quantenmechanik, Springer, 1932.
  • M. Reed, B. Simon, Methods of Modern Mathematical Physics I: Functional Analysis, Academic Press, 1980.
  • B. C. Hall, Quantum Theory for Mathematicians, Graduate Texts in Mathematics 267, Springer, 2013. https://doi.org/10.1007/978-1-4614-7116-5
13 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Goodman–Witten 1985: Detectability of Certain Dark-Matter CandidatesResearch Paper

Motivation

The rotation curves of spiral galaxies indicate that galaxies sit inside extended dark halos whose mass dominates the visible matter (Faber–Gallagher 1979). If the halo is a gas of elementary particles moving at galactic velocities (v∼200v \sim 200v∼200 km/s), those particles stream through every laboratory on Earth. In 1985 Goodman and Witten asked whether a detector then being proposed for neutrinos — the superconducting-grain detector of Drukier and Stodolsky, which registers nuclear recoils of tens of eV and up through elastic neutral-current scattering (Drukier–Stodolsky 1984) — could see halo particles by the same mechanism.

Their answer, worked out with a handful of explicit formulas, was yes for three broad classes of candidates: particles with coherent weak interactions, particles with spin-dependent interactions of weak strength (with the photino as the example), and strongly interacting particles. The paper is the starting point of direct dark-matter detection: the recoil-energy kinematics, the counting-rate formula and the split into spin-independent and spin-dependent couplings introduced here are still the standard framework of every nuclear-recoil experiment.

Setting

A halo particle of mass mmm and speed vvv scatters elastically from a target nucleus of mass number AAA, mass M=A mNM = A\,m_NM=AmN​, at rest. In a non-relativistic elastic collision momentum and kinetic energy are conserved, and the recoil kinetic energy deposited in the nucleus is bounded by

ϵ=(2mv)22M.\epsilon = \frac{(2mv)^2}{2M}.ϵ=2M(2mv)2​.

A kilogram of detector contains K=6.0×1026/AK = 6.0\times10^{26}/AK=6.0×1026/A target nuclei. Halo particles of mass density ρ\rhoρ have number density ρ/m\rho/mρ/m and flux F=ρv/mF = \rho v/mF=ρv/m, so the counting rate with cross section σ\sigmaσ is R=KFσR = KF\sigmaR=KFσ, quoted in events per kilogram per day. The paper normalises with the reduced cross section σˉ=(σ/A)(1 GeV/m)\bar\sigma = (\sigma/A)(1\ \mathrm{GeV}/m)σˉ=(σ/A)(1 GeV/m).

For a constant invariant amplitude M\mathcal MM the elastic cross section is

σ=m2M2π(m+M)2 ∣M∣2.\sigma = \frac{m^2M^2}{\pi(m+M)^2}\,|\mathcal M|^2 .σ=π(m+M)2m2M2​∣M∣2.

The three candidate classes differ only in M\mathcal MM (or σ\sigmaσ):

  1. Coherent weak: M=GFYˉNˉ/2\mathcal M = G_F\bar Y\bar N/\sqrt2M=GF​YˉNˉ/2​, where Yˉ\bar YYˉ is the weak hypercharge combination of the particle and Nˉ=N−(1−4sin⁡2θ)Z\bar N = N - (1-4\sin^2\theta)ZNˉ=N−(1−4sin2θ)Z for a nucleus with NNN neutrons and ZZZ protons.
  2. Spin-dependent (photino): ⟨∣M∣2⟩=(4q4/MQ~4) λ2J(J+1)\langle|\mathcal M|^2\rangle = (4q^4/M_{\tilde Q}^4)\,\lambda^2J(J+1)⟨∣M∣2⟩=(4q4/MQ~​4​)λ2J(J+1), where qqq is the charge of the light quark, MQ~M_{\tilde Q}MQ~​​ the mass of its scalar partner, JJJ the nuclear spin and λ\lambdaλ a nuclear-structure constant.
  3. Strongly interacting: a hard-sphere cross section σ=4πRnuc2\sigma = 4\pi R_{\mathrm{nuc}}^2σ=4πRnuc2​ with Rnuc=1.25A1/3×10−13R_{\mathrm{nuc}} = 1.25A^{1/3}\times10^{-13}Rnuc​=1.25A1/3×10−13 cm, multiplied by a stopping factor ϵ≤1\epsilon \le 1ϵ≤1 for the earth or the atmosphere.

Standard halo values are ρ=10−24\rho = 10^{-24}ρ=10−24 g/cm3^33 and v=200v = 200v=200 km/s, and the benchmark detector sensitivity is 1 event/kg/day.

Formalization targets

Goal: the three detectability claims

With ρ=10−24\rho = 10^{-24}ρ=10−24 g/cm3^33 and v=200v = 200v=200 km/s:

  1. for a lead target and Yˉ=1\bar Y = 1Yˉ=1, the coherent rate of Eq. (2) is at least 1 event/kg/day for all 1 GeV≤m≤1071\ \mathrm{GeV}\le m\le10^71 GeV≤m≤107 GeV (for any 0.2≤sin⁡2θ≤0.250.2\le\sin^2\theta\le0.250.2≤sin2θ≤0.25);
  2. for photinos with mass equal to the nuclear mass and λ2J(J+1)=1\lambda^2J(J+1) = 1λ2J(J+1)=1, the rate is of order 1 event/kg/day, 1≤R<101\le R<101≤R<10, for (q,MQ~)=(23e,100 GeV)(q, M_{\tilde Q}) = (\tfrac23e, 100\ \mathrm{GeV})(q,MQ~​​)=(32​e,100 GeV) and (13e,50 GeV)(\tfrac13e, 50\ \mathrm{GeV})(31​e,50 GeV);
  3. for targets from aluminium to lead (27≤A≤20727\le A\le20727≤A≤207) and ϵ=1\epsilon = 1ϵ=1, strongly interacting particles give at least 1 event/kg/day exactly up to a mass
M∗∈[1.5×1013, 4.5×1013] GeV.M^*\in[1.5\times10^{13},\,4.5\times10^{13}]\ \mathrm{GeV}.M∗∈[1.5×1013,4.5×1013] GeV.

Milestones

The milestones follow the paper's equations in order: the recoil bounds and the 1–2 GeV lower mass limit (p. 3059); the counting-rate formula, Eq. (1); the coherent reduced cross section, Eq. (2), and the resulting 10410^4104/kg day rates; the photino rate, Eq. (3); the quark-model matrix elements, Eq. (4), and the factor-100 flavour asymmetry; and the hard-sphere cross section and rate, Eq. (6).

Significance

The result. The paper turned dark-matter direct detection from an abstract possibility into a quantitative experimental programme: it fixed the minimal detectable mass from kinematics, gave a single counting-rate formula into which any particle-physics model can be inserted, and showed that coherent (spin-independent) scattering on heavy nuclei is enhanced by Nˉ2\bar N^2Nˉ2 while spin-dependent scattering needs odd nuclei. These estimates set the scale of rates, from 10410^4104 events/kg/day for coherent weak particles down to 1 event/kg/day for photinos, against which later experiments were designed.

Formalizing it. The statements are elementary but they are exactly the kind of order-of-magnitude chain where a unit conversion, a missing factor of 2 or π\piπ, or a convention for the nuclear mass silently changes a number. A machine-checked version records every convention explicitly, checks each printed coefficient against modern values of the constants, and separates genuine theorems (the kinematic bound) from numerical consequences of the formulas.

Difficulty

The only genuinely geometric statement is the recoil bound, which must hold for every direction of scattering in three dimensions, not just head-on collisions. All other milestones are exact identities between the definitions plus verified numerical bounds involving π\piπ, real powers A1/3A^{1/3}A1/3 and scientific-notation constants spanning more than fifty orders of magnitude. The obstacle is keeping these bounds tight enough: several of the paper's coefficients are reproduced only to a few percent, so loose estimates of π\piπ or of A1/3A^{1/3}A1/3 over a range of AAA will not close the inequalities, and the detectability statements require monotonicity arguments over whole mass intervals rather than evaluation at one point.

Formalization scope

All quantities are real numbers in a fixed unit system: masses and energies in GeV with c=1c = 1c=1, velocities as fractions of ccc in kinematic statements and in cm/s in rate statements, densities in g/cm3^33, cross sections in cm2^22, squared amplitudes in GeV−4^{-4}−4 converted to cm2^22 by (ℏc)2(\hbar c)^2(ℏc)2. The constants are ccc, 1 GeV/c21\ \mathrm{GeV}/c^21 GeV/c2 in grams, ℏc\hbar cℏc, GFG_FGF​ and α\alphaα at their modern values, the paper's K=6.0×1026/AK = 6.0\times10^{26}/AK=6.0×1026/A, and nuclear mass M=A mNM = A\,m_NM=AmN​ with mN=0.9383m_N = 0.9383mN​=0.9383 GeV (the paper writes M≃AM\simeq AM≃A GeV; the nucleon mass reproduces its printed coefficients).

Approximate equalities "≈c0\approx c_0≈c0​" in the paper are encoded as the existence of an exact coefficient CCC with ∣C/c0−1∣≤0.05|C/c_0-1|\le0.05∣C/c0​−1∣≤0.05 for which the formula holds identically in all parameters, so a statement cannot be satisfied by a coefficient unrelated to the definitions. "Of order 10k10^k10k" is encoded as 10k≤R<10k+110^k\le R<10^{k+1}10k≤R<10k+1. Eq. (2) is used without the nuclear form factor, as in the paper's sentence about lead; the reduced Table II rates with loss of coherence and Eqs. (5) and (7) are outside the scope of this mission.

The development needs only real analysis from Mathlib: inner-product geometry in R3\mathbb R^3R3 for the recoil bound, and bounds on π\piπ and on real powers for the numerics. Contributions of reusable lemmas for certified numerical bounds on rpow expressions are welcome.

Selected references

  • M. W. Goodman and E. Witten, Detectability of certain dark-matter candidates, Phys. Rev. D 31, 3059 (1985). https://doi.org/10.1103/PhysRevD.31.3059
  • A. Drukier and L. Stodolsky, Principles and applications of a neutral-current detector for neutrino physics and astronomy, Phys. Rev. D 30, 2295 (1984). https://doi.org/10.1103/PhysRevD.30.2295
  • S. M. Faber and J. S. Gallagher, Masses and mass-to-light ratios of galaxies, Annu. Rev. Astron. Astrophys. 17, 135 (1979). https://doi.org/10.1146/annurev.aa.17.090179.001031
12 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Maldacena 2003: Non-Gaussian Features of Primordial Fluctuations in Single-Field InflationResearch Paper

Motivation

Single-field slow-roll inflation predicts primordial curvature fluctuations that are very close to Gaussian. The leading departure from Gaussianity is the three-point function (the bispectrum) of the curvature perturbation ζ\zetaζ. Maldacena (2003) computed it from first principles: he derived the cubic action for scalar and tensor fluctuations, evaluated the tree-level correlators with the standard choice of vacuum, and gave closed formulas at leading order in slow roll, with exact numerical coefficients and full momentum dependence. For the three-scalar correlator, earlier estimates included only part of the effect.

The paper also points out a structural property. When one momentum is much smaller than the other two (the squeezed limit), the three-point function is fixed by the tilt of the two-point function. Today this is called Maldacena's consistency relation. It is the standard test of single-field inflation against cosmic microwave background and large-scale-structure data, and the starting point of a large literature on soft theorems in cosmology.

Setting

Units are Mpl−2=8πGN=1M_{pl}^{-2} = 8\pi G_N = 1Mpl−2​=8πGN​=1. The background is a spatially flat FRW metric ds2=−dt2+e2ρ(t)dxidxids^2 = -dt^2 + e^{2\rho(t)}dx^i dx^ids2=−dt2+e2ρ(t)dxidxi with a homogeneous scalar field ϕ(t)\phi(t)ϕ(t) obeying

3ρ˙2=12ϕ˙2+V(ϕ),ρ¨=−12ϕ˙2,ϕ¨+3ρ˙ϕ˙+V′(ϕ)=0,3\dot\rho^2 = \tfrac12\dot\phi^2 + V(\phi),\qquad \ddot\rho = -\tfrac12\dot\phi^2,\qquad \ddot\phi + 3\dot\rho\dot\phi + V'(\phi) = 0,3ρ˙​2=21​ϕ˙​2+V(ϕ),ρ¨​=−21​ϕ˙​2,ϕ¨​+3ρ˙​ϕ˙​+V′(ϕ)=0,

and H=ρ˙H = \dot\rhoH=ρ˙​. A starred quantity is evaluated at horizon crossing. Write ki=∣k⃗i∣k_i = |\vec k_i|ki​=∣ki​∣ and kt=k1+k2+k3k_t = k_1+k_2+k_3kt​=k1​+k2​+k3​. Momentum conservation k⃗1+k⃗2+k⃗3=0\vec k_1 + \vec k_2 + \vec k_3 = 0k1​+k2​+k3​=0 means that (k1,k2,k3)(k_1,k_2,k_3)(k1​,k2​,k3​) are the side lengths of a (possibly degenerate) triangle. All correlators below are written without the overall factor (2π)3δ3(∑ik⃗i)(2\pi)^3\delta^3(\sum_i \vec k_i)(2π)3δ3(∑i​ki​).

  1. Power spectra (eqs. 2.20, 2.29): Pζ(k)=12k3ρ˙∗2ρ˙∗2ϕ˙∗2P_\zeta(k) = \frac{1}{2k^3}\dot\rho_*^2\frac{\dot\rho_*^2}{\dot\phi_*^2}Pζ​(k)=2k31​ρ˙​∗2​ϕ˙​∗2​ρ˙​∗2​​ and Pγ(k)=12k3 2ρ˙∗2P_\gamma(k) = \frac{1}{2k^3}\,2\dot\rho_*^2Pγ​(k)=2k31​2ρ˙​∗2​.
  2. Tilts (eqs. 2.22, 2.30): ns=−2(ϕ¨∗ρ˙∗ϕ˙∗+ϕ˙∗2ρ˙∗2)n_s = -2\big(\frac{\ddot\phi_*}{\dot\rho_*\dot\phi_*} + \frac{\dot\phi_*^2}{\dot\rho_*^2}\big)ns​=−2(ρ˙​∗​ϕ˙​∗​ϕ¨​∗​​+ρ˙​∗2​ϕ˙​∗2​​) and nt=−ϕ˙∗2ρ˙∗2n_t = -\frac{\dot\phi_*^2}{\dot\rho_*^2}nt​=−ρ˙​∗2​ϕ˙​∗2​​. Here nsn_sns​ is the exponent in Pζ∝k−3+nsP_\zeta \propto k^{-3+n_s}Pζ​∝k−3+ns​, so it is "ns−1n_s - 1ns​−1" in the modern convention.
  3. Three-scalar correlator (eqs. 4.5–4.6): Bζ(k1,k2,k3)=ρ˙∗4ϕ˙∗4H∗41∏i(2ki3)AB_\zeta(k_1,k_2,k_3) = \frac{\dot\rho_*^4}{\dot\phi_*^4}H_*^4\frac{1}{\prod_i (2k_i^3)}\mathcal ABζ​(k1​,k2​,k3​)=ϕ˙​∗4​ρ˙​∗4​​H∗4​∏i​(2ki3​)1​A, where
A=2ϕ¨∗ϕ˙∗ρ˙∗∑iki3+ϕ˙∗2ρ˙∗2[12∑iki3+12∑i≠jkikj2+4∑i>jki2kj2kt].\mathcal A = 2\frac{\ddot\phi_*}{\dot\phi_*\dot\rho_*}\sum_i k_i^3 + \frac{\dot\phi_*^2}{\dot\rho_*^2}\Big[\frac12\sum_i k_i^3 + \frac12\sum_{i\ne j}k_ik_j^2 + 4\frac{\sum_{i>j}k_i^2k_j^2}{k_t}\Big].A=2ϕ˙​∗​ρ˙​∗​ϕ¨​∗​​i∑​ki3​+ρ˙​∗2​ϕ˙​∗2​​[21​i∑​ki3​+21​i=j∑​ki​kj2​+4kt​∑i>j​ki2​kj2​​].
  1. Graviton correlators (eqs. 4.10, 4.13, 4.15). These are built from the integral I=−kt+∑i>jkikjkt+k1k2k3kt2I = -k_t + \frac{\sum_{i>j}k_ik_j}{k_t} + \frac{k_1k_2k_3}{k_t^2}I=−kt​+kt​∑i>j​ki​kj​​+kt2​k1​k2​k3​​ of eq. (4.11), the transverse traceless polarization tensors ϵijs\epsilon^s_{ij}ϵijs​, and the flat-space tensor tijl=k2iδjl+k3jδil+k1lδijt_{ijl} = k_2^i\delta_{jl} + k_3^j\delta_{il} + k_1^l\delta_{ij}tijl​=k2i​δjl​+k3j​δil​+k1l​δij​.

Formalization targets

Goal: the squeezed-limit consistency relation (eqs. 4.5–4.7)

For fixed k=k1>0k = k_1 > 0k=k1​>0, as k3→0k_3 \to 0k3​→0 through momentum triangles (which forces k2→k1k_2 \to k_1k2​→k1​),

Bζ(k1,k2,k3)Pζ(k1) Pζ(k3)⟶−ns.\frac{B_\zeta(k_1,k_2,k_3)}{P_\zeta(k_1)\,P_\zeta(k_3)} \longrightarrow -n_s .Pζ​(k1​)Pζ​(k3​)Bζ​(k1​,k2​,k3​)​⟶−ns​.

This is the statement that "(4.5), with (4.6) goes over to (4.7) in the overlapping region of validity."

Milestones

  1. The exact tilt formulas (2.22) and (2.30) for a background obeying the equations of motion.
  2. The time integral (4.4) for the contribution of the cubic vertex in de Sitter space, and the time integral III of (4.11), each with the iϵi\epsiloniϵ contour prescription.
  3. The squeezed limit of the amplitude A\mathcal AA (4.6 → 4.7).
  4. The kkk-dependent fNLf_{NL}fNL​ of (4.9): its expression through nsn_sns​, ntn_tnt​ and a shape function f(k)f(k)f(k); the range 0≤f≤5/60 \le f \le 5/60≤f≤5/6; the values f=5/6f = 5/6f=5/6 (equilateral) and f→0f \to 0f→0 (squeezed).
  5. The squeezed limits of the three graviton correlators: (4.10 → 4.12), (4.13 → 4.14), and (4.15 → 4.17).

Significance

The consistency relation ties a three-point observable to a two-point observable with no free parameters. If it is observed to fail, all single-field models in the Bunch–Davies vacuum are ruled out. The shape-function bound in (4.9) is what lets the paper conclude that the local-type fNLf_{NL}fNL​ of single-field slow-roll models is of order the slow-roll parameters, too small to detect from the CMB alone.

All results here are established physics. As far as is known, none of the explicit formula manipulations, the contour integrals, or the consistency checks between the general and squeezed formulas has a machine-checked proof. This mission produces checked versions of each of them, so that later formal developments of cosmological perturbation theory can cite exact statements rather than prose.

Difficulty

The algebraic limits are elementary once the formulas are written down. The analytic content is in the two contour integrals. The integrand of (4.4) and (4.11) oscillates and does not decay on (−∞,0](-\infty, 0](−∞,0], so the integrals exist only with the iϵi\epsiloniϵ prescription. The integrand of (4.11) also has a non-integrable 1/η21/\eta^21/η2 singularity at η=0\eta = 0η=0, whose divergence is purely imaginary, so only the real part has a limit as the cutoff goes to zero. The shape bound 0≤f≤5/60 \le f \le 5/60≤f≤5/6 is a degree-zero rational inequality on the triangle region; it is false outside the triangle region.

Formalization scope

  • Every correlator is a real-valued Lean def with Mpl=1M_{pl} = 1Mpl​=1, H∗=ρ˙∗H_* = \dot\rho_*H∗​=ρ˙​∗​, and the factor (2π)3δ3(∑ik⃗i)(2\pi)^3\delta^3(\sum_i\vec k_i)(2π)3δ3(∑i​ki​) dropped. Background values at horizon crossing enter as real parameters ρd, φd, φdd =ρ˙∗,ϕ˙∗,ϕ¨∗= \dot\rho_*, \dot\phi_*, \ddot\phi_*=ρ˙​∗​,ϕ˙​∗​,ϕ¨​∗​. At leading order in slow roll, the different horizon-crossing times ∗*∗ and ∗′*'∗′ that appear in (4.7), (4.12), (4.14), and (4.17) coincide.
  • The scalar correlators depend only on the magnitudes kik_iki​, and momentum conservation is encoded by the triangle predicate IsMomentumTriangle. The graviton–scalar–scalar and three-graviton correlators use vectors in EuclideanSpace ℝ (Fin 3) and polarizations as real symmetric, traceless, transverse 3×33\times33×3 matrices. A squeezed limit is taken along k⃗1=tn^\vec k_1 = t\hat nk1​=tn^, t→0+t \to 0^+t→0+.
  • The iϵi\epsiloniϵ prescription (η→η+iϵ∣η∣\eta \to \eta + i\epsilon|\eta|η→η+iϵ∣η∣) is implemented by the damping factor eϵηe^{\epsilon\eta}eϵη, followed by ϵ→0+\epsilon \to 0^+ϵ→0+.
  • The derivation of (4.5), (4.10), (4.13), and (4.15) from the cubic action of Section 3 (the in-in formalism, field redefinitions, gauge choices) is out of scope, because current Mathlib has no framework for interacting quantum fields on curved backgrounds. Contributions toward that infrastructure are welcome as separate missions.
  • Eq. (2.22) as printed has the misprint ϕ˙∗/ρ˙∗\dot\phi_*/\dot\rho_*ϕ˙​∗​/ρ˙​∗​ in place of ϕ˙∗2/ρ˙∗2\dot\phi_*^2/\dot\rho_*^2ϕ˙​∗2​/ρ˙​∗2​. The corrected form, which equals 2(η−3ϵ)2(\eta - 3\epsilon)2(η−3ϵ) and is used in (4.7) and (4.9), is the one formalized.

Selected references

  • J. Maldacena, Non-Gaussian features of primordial fluctuations in single field inflationary models, JHEP 05 (2003) 013. https://doi.org/10.1088/1126-6708/2003/05/013 (arXiv: https://arxiv.org/abs/astro-ph/0210603)
13 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Pereira–Guimarães 2017: Elko Field Driving the Evolution of the UniverseResearch Paper

Motivation

Elko (from the German Eigenspinoren des Ladungskonjugationsoperators) is a class of spin-1/2 fields of mass dimension one, introduced by Ahluwalia and Grumiller (JCAP 07 (2005) 012) as a candidate for fermionic dark matter. Elko spinors are eigenstates of charge conjugation, so they are neutral. Because of their mass dimension they obey only a Klein–Gordon-type equation, and their allowed self-interactions are restricted to a quadratic and a quartic term.

Pereira and Guimarães (2017) propose that one homogeneous Elko field, coupled to gravity in the Einstein–Cartan framework (gravity with torsion) and subject to a symmetry-breaking potential, drives the whole expansion history: inflation, then a matter-dominated era, then late-time acceleration. The paper has two parts. The first is an analytic reduction of the field equations to a closed system of ordinary differential equations (Section 2 and Appendix A). The second is a numerical study of that system with a benchmark set of parameters (Section 3). This mission formalizes the analytic part and the closed-form estimates of Section 3.1.

Setting

Units are c=1c=1c=1 and κ2=8πG=8π/mpl2\kappa^2=8\pi G=8\pi/m_{\rm pl}^2κ2=8πG=8π/mpl2​. The background is a spatially flat FRW metric with lapse N(t)N(t)N(t) and scale factor a(t)>0a(t)>0a(t)>0. The Hubble rate is H=a˙/aH=\dot a/aH=a˙/a. The Elko field is λ=Φ(t) ξ\lambda=\Phi(t)\,\xiλ=Φ(t)ξ, where ξ\xiξ is a constant spinor normalized so that ξˉξ=1\bar\xi\xi=1ξˉ​ξ=1. Only the real function Φ(t)\Phi(t)Φ(t) carries dynamics. Homogeneity and isotropy leave two torsion functions h(t)h(t)h(t) and f(t)f(t)f(t). The minisuperspace Lagrangian (A.13) is

L=−1N(3aa˙2κ2−3a3h2κ2−12a3Φ˙2−38a(a˙+ah)2Φ2)−N(3a3f2κ2+38a3f2Φ2+a3V(Φ)).\mathcal L=-\frac1N\Big(\frac{3a\dot a^2}{\kappa^2}-\frac{3a^3h^2}{\kappa^2}-\frac12a^3\dot\Phi^2-\frac38a(\dot a+ah)^2\Phi^2\Big)-N\Big(\frac{3a^3f^2}{\kappa^2}+\frac38a^3f^2\Phi^2+a^3V(\Phi)\Big).L=−N1​(κ23aa˙2​−κ23a3h2​−21​a3Φ˙2−83​a(a˙+ah)2Φ2)−N(κ23a3f2​+83​a3f2Φ2+a3V(Φ)).

Its Euler–Lagrange equations in N,a,Φ,h,fN,a,\Phi,h,fN,a,Φ,h,f (gauge N=1N=1N=1) are (A.14)–(A.17). They force f=0f=0f=0 and the torsion relation

h=−18 κ2Φ21+κ2Φ2/8 H.(2.5)h=-\frac18\,\frac{\kappa^2\Phi^2}{1+\kappa^2\Phi^2/8}\,H.\qquad(2.5)h=−81​1+κ2Φ2/8κ2Φ2​H.(2.5)

Substituting f=0f=0f=0 gives the Friedmann equations with torsion (2.2)–(2.3) and the motion equation (2.4). Throughout, the factor 1+κ2Φ2/81+\kappa^2\Phi^2/81+κ2Φ2/8 appears, and it is always positive. The potential of Section 3 is

V(Φ)=v0+Λ4(1−Φ2σ2)2.(3.1)V(\Phi)=v_0+\Lambda^4\Big(1-\frac{\Phi^2}{\sigma^2}\Big)^2 .\qquad(3.1)V(Φ)=v0​+Λ4(1−σ2Φ2​)2.(3.1)

Formalization targets

Goal: the reduced Elko system (2.6)–(2.10)

Assume (2.5), (2.2) and (2.3) on an open time set III, with H,Φ,Φ˙H,\Phi,\dot\PhiH,Φ,Φ˙ differentiable there. Then on III

H2=κ23(1+κ2Φ28)[Φ˙22+V],H˙=−κ22(1+κ2Φ28)[Φ˙2−HΦΦ˙2(1+κ2Φ2/8)2],H^2=\frac{\kappa^2}{3}\Big(1+\frac{\kappa^2\Phi^2}{8}\Big)\Big[\frac{\dot\Phi^2}{2}+V\Big],\qquad \dot H=-\frac{\kappa^2}{2}\Big(1+\frac{\kappa^2\Phi^2}{8}\Big)\Big[\dot\Phi^2-\frac{H\Phi\dot\Phi}{2(1+\kappa^2\Phi^2/8)^2}\Big],H2=3κ2​(1+8κ2Φ2​)[2Φ˙2​+V],H˙=−2κ2​(1+8κ2Φ2​)[Φ˙2−2(1+κ2Φ2/8)2HΦΦ˙​],

H2=κ2ρ/3H^2=\kappa^2\rho/3H2=κ2ρ/3 and H˙=−κ2(ρ+p)/2\dot H=-\kappa^2(\rho+p)/2H˙=−κ2(ρ+p)/2 with ρ,p\rho,pρ,p given by (2.9)–(2.10). Wherever Φ˙≠0\dot\Phi\neq0Φ˙=0, the motion equation (2.8) also holds:

Φ¨+3HΦ˙+V′(Φ)−34 H2Φ(1+κ2Φ2/8)2=0.\ddot\Phi+3H\dot\Phi+V'(\Phi)-\frac34\,\frac{H^2\Phi}{(1+\kappa^2\Phi^2/8)^2}=0 .Φ¨+3HΦ˙+V′(Φ)−43​(1+κ2Φ2/8)2H2Φ​=0.

Milestones

  1. Eqs. (A.14)–(A.17): the Euler–Lagrange equations of (A.13).
  2. Appendix A: (A.14)–(A.16) with f=0f=0f=0 give (2.2)–(2.4).
  3. Eq. (2.4) follows from differentiating (2.2) and using (2.3).
  4. Eqs. (2.6), (2.7), (2.8): the torsion is eliminated from each equation.
  5. Eqs. (2.9)–(2.10): (2.6)–(2.7) are the FRW equations for ρ\rhoρ and ppp.
  6. Eq. (3.1): polynomial form of the potential, global minimum V(σ)=v0V(\sigma)=v_0V(σ)=v0​, and mass V′′(σ)=m2V''(\sigma)=m^2V′′(σ)=m2 with m=2μm=\sqrt2\mum=2​μ.
  7. Eq. (3.6) and Sec. 3.1: the benchmark values of H2(ti)H^2(t_i)H2(ti​), tit_iti​, V(Φi)V(\Phi_i)V(Φi​), ϵ\epsilonϵ, η\etaη, mmm and α\alphaα.

Significance

The result itself. The reduced system (2.6)–(2.10) is the object the paper integrates numerically for every cosmological era. In the limit H≪mplH\ll m_{\rm pl}H≪mpl​ it differs from the standard single-scalar-field equations (1.1)–(1.3) only by the factor 1+κ2Φ2/81+\kappa^2\Phi^2/81+κ2Φ2/8 and by the torsion term in (2.8). That term acts like the friction term Γϕ˙\Gamma\dot\phiΓϕ˙​ that is added by hand in reheating models. The identification of ρ\rhoρ and ppp in (2.9)–(2.10) is what defines the equation-of-state parameter ω=p/ρ\omega=p/\rhoω=p/ρ, which the paper uses to argue for dust-like behaviour after inflation.

Formalizing it. The paper says the reduction is reached "after some algebraic manipulations" and does not show them. A formal proof checks every coefficient of (2.2)–(2.10) and of (A.14)–(A.17) against the Lagrangian (A.13). It also makes explicit the condition Φ˙≠0\dot\Phi\neq0Φ˙=0 that is needed to recover the motion equation from the Friedmann equations. The numerical claims of Section 3.1 are closed-form evaluations and can be checked exactly.

Difficulty

The identities are elementary, but they are not purely pointwise. Equation (2.3) contains H˙\dot HH˙ on both sides, through ddt[(H+h)Φ2]\frac{d}{dt}[(H+h)\Phi^2]dtd​[(H+h)Φ2], and hhh itself depends on HHH and Φ\PhiΦ. Solving for H˙\dot HH˙ therefore requires differentiating (2.5) along the trajectory. This is valid only because (2.5) holds on an open set of times, not just at one instant. Similarly, deriving (2.4) means differentiating the constraint (2.2) in time and cancelling a factor Φ˙\dot\PhiΦ˙. The Euler–Lagrange milestone needs partial derivatives of L\mathcal LL in each of its slots, composed with time derivatives along the trajectory. A careless treatment of which arguments are frozen gives wrong coefficients.

Formalization scope

All objects are real-valued functions of time t∈Rt\in\mathbb Rt∈R. Time derivatives are Mathlib deriv, and hypotheses are imposed on an open set III. Partial derivatives of the Lagrangian are deriv in one argument with the others fixed at their trajectory values. The constant κ\kappaκ is an arbitrary real number; κ≠0\kappa\neq0κ=0 is assumed only where 1/κ21/\kappa^21/κ2 appears. The spinor structure of Elko is not modelled: as in the paper, only the scalar amplitude Φ(t)\Phi(t)Φ(t) enters. The symbol "≃\simeq≃" in Section 3.1 is encoded as agreement within 5%5\%5% relative error.

Out of scope: the derivation of the Lagrangian (A.13) from the Einstein–Cartan action (A.1)–(A.12); the slow-roll approximations (3.2)–(3.5), which the paper states only as approximations in the regime H≪mplH\ll m_{\rm pl}H≪mpl​; and every output of the numerical integration of Section 3 and Appendix B, such as N≈93N\approx93N≈93 e-folds, the t2/3t^{2/3}t2/3 late-time behaviour, the oscillation of ω\omegaω around 000, and the present-day density.

A trivializing formalization is ruled out: the torsion function hhh is constrained by (2.5) on all of III, and ρ,p\rho,pρ,p are fixed by (2.9)–(2.10), not left free.

Infrastructure needed: only basic one-variable calculus in Mathlib (deriv, DifferentiableAt, product and quotient rules), together with field arithmetic using the positivity of 1+κ2Φ2/81+\kappa^2\Phi^2/81+κ2Φ2/8. The same reduction pattern (eliminate an algebraically determined auxiliary field, then differentiate a constraint) occurs in other torsion and scalar–tensor cosmologies.

Selected references

  • S. H. Pereira, T. M. Guimarães, From inflation to recent cosmic acceleration: the fermionic Elko field driving the evolution of the universe, JCAP 09 (2017) 038. https://doi.org/10.1088/1475-7516/2017/09/038 (arXiv:1702.07385)
  • D. V. Ahluwalia, D. Grumiller, Spin-half fermions with mass dimension one: theory, phenomenology, and dark matter, JCAP 07 (2005) 012. https://doi.org/10.1088/1475-7516/2005/07/012 (arXiv:hep-th/0412080)
  • A. D. Linde, Chaotic inflation, Phys. Lett. B 129 (1983) 177. https://doi.org/10.1016/0370-2693(83)90837-7
10 thms2 active usersReviewed
🏆Completed
Statistics·Captain: Lucas

Freedman–Madore 2023: Quantifying the Hubble TensionResearch Paper

Motivation

The Hubble constant H0H_0H0​ is the present expansion rate of the universe. It is the slope of Hubble's law v=H0 dv = H_0\, dv=H0​d, which relates a galaxy's recession velocity vvv (km s−1^{-1}−1) to its distance ddd (Mpc). Two families of measurements currently disagree. Local, distance-ladder measurements calibrated with Cepheid variables give H0≈73H_0 \approx 73H0​≈73 km s−1^{-1}−1 Mpc−1^{-1}−1 (SH0ES: 73.04±1.0473.04 \pm 1.0473.04±1.04, Riess et al. 2022). The value inferred from the cosmic microwave background under Λ\LambdaΛCDM is 67.4±0.567.4 \pm 0.567.4±0.5 (Planck 2018). Calibrations with the tip of the red giant branch (TRGB) fall in between: 69.8±0.6 (stat)±1.6 (sys)69.8 \pm 0.6\,(\text{stat}) \pm 1.6\,(\text{sys})69.8±0.6(stat)±1.6(sys) (Freedman 2021). This disagreement is the Hubble tension. If it is real, it points to physics beyond Λ\LambdaΛCDM.

The review Freedman & Madore 2023 surveys this landscape and makes a series of quantitative claims about it. Some are agreement or disagreement claims ("agrees at better than 0.2σ0.2\sigma0.2σ", "differs at the 2σ2\sigma2σ level"). Others convert magnitudes to distances ("a 1.5% measurement", "corresponds to a 6% shift in H0H_0H0​"). The central one, in §10, is a sensitivity argument: the claimed 5σ5\sigma5σ tension falls below 3σ3\sigma3σ if the local uncertainty has been underestimated by a factor of about 1.51.51.5. This mission takes these claims literally and checks them against their stated numbers.

Setting

A measurement is reported as x±σx \pm \sigmax±σ. Two independent uncertainties are combined in quadrature, quadSum⁡(s,t)=s2+t2\operatorname{quadSum}(s,t) = \sqrt{s^2+t^2}quadSum(s,t)=s2+t2​. This is the field's standard convention, used here for a quoted x±s (stat)±t (sys)x \pm s\,(\text{stat}) \pm t\,(\text{sys})x±s(stat)±t(sys). The tension between independent measurements a±σaa \pm \sigma_aa±σa​ and b±σbb \pm \sigma_bb±σb​, in units of standard deviations, is

tension⁡(a,σa,b,σb)=∣a−b∣σa2+σb2.\operatorname{tension}(a,\sigma_a,b,\sigma_b) = \frac{|a-b|}{\sqrt{\sigma_a^2+\sigma_b^2}}.tension(a,σa​,b,σb​)=σa2​+σb2​​∣a−b∣​.

The distance modulus of an object at distance ddd parsecs is μ=5log⁡10(d/10)\mu = 5\log_{10}(d/10)μ=5log10​(d/10), and conversely d=10μ/5+1d = 10^{\mu/5+1}d=10μ/5+1 pc (distanceFromModulus⁡\operatorname{distanceFromModulus}distanceFromModulus). A modulus difference Δμ\Delta\muΔμ therefore multiplies distances by 10Δμ/510^{\Delta\mu/5}10Δμ/5. Through Hubble's law, hubbleConstant⁡(v,d)=v/(d/106)\operatorname{hubbleConstant}(v,d) = v/(d/10^6)hubbleConstant(v,d)=v/(d/106) (with ddd in pc), the same difference divides the inferred H0H_0H0​ by 10Δμ/510^{\Delta\mu/5}10Δμ/5.

Formalization targets

Goal (§10, p. 25)

4.5≤tension⁡(73.04,1.04,67.4,0.5)<5.5,tension⁡(72.0,1.5,67.4,0.5)<3,1.5≤tension⁡(72.0,2.0,67.4,0.5)<2.5.4.5 \le \operatorname{tension}(73.04, 1.04, 67.4, 0.5) < 5.5,\qquad \operatorname{tension}(72.0, 1.5, 67.4, 0.5) < 3,\qquad 1.5 \le \operatorname{tension}(72.0, 2.0, 67.4, 0.5) < 2.5.4.5≤tension(73.04,1.04,67.4,0.5)<5.5,tension(72.0,1.5,67.4,0.5)<3,1.5≤tension(72.0,2.0,67.4,0.5)<2.5.

These are the "5σ5\sigma5σ" SH0ES–Planck tension, the "less than 3σ3\sigma3σ" for H0=72.0±1.5H_0 = 72.0 \pm 1.5H0​=72.0±1.5, and the "2σ2\sigma2σ" for H0=72.0±2.0H_0 = 72.0 \pm 2.0H0​=72.0±2.0. Every rounded value ("5σ5\sigma5σ", "2σ2\sigma2σ") is read as the half-open interval of reals that round to it.

Milestones

  • Distance modulus and distance are inverse to each other on d>0d > 0d>0.
  • Hubble's law under a modulus shift: H0H_0H0​ rescales by 10−Δ/510^{-\Delta/5}10−Δ/5. As consequences, the JWST "+0.45+0.45+0.45 mag farther" correction lowers H0H_0H0​ (Summary, p. 26), and the R16→R22 offset of −0.123-0.123−0.123 mag is a 6%6\%6% shift (Summary, p. 27).
  • NGC 4258 (§5.3): modulus 29.39729.39729.397 is 7.67.67.6 Mpc, and ±0.033\pm 0.033±0.033 mag is a 1.5%1.5\%1.5% measurement. The TRGB modulus agrees with the maser modulus at <0.2σ<0.2\sigma<0.2σ and <1%<1\%<1%. The Milky-Way-anchored Cepheid modulus differs by 7%7\%7% at the 2σ2\sigma2σ level.
  • LMC (§5.1): 18.477±0.004±0.02618.477 \pm 0.004 \pm 0.02618.477±0.004±0.026 is a 1.2%1.2\%1.2% distance uncertainty, ∼1%\sim 1\%∼1% from the Key Project value 18.518.518.5.
  • TRGB vs Cepheid (§4.1): 69.8±0.6±1.669.8 \pm 0.6 \pm 1.669.8±0.6±1.6 agrees with 73.04±1.0473.04 \pm 1.0473.04±1.04 at better than 2σ2\sigma2σ.

Significance

The statements make the review's arithmetic exact and auditable. Each verbal claim of the form "kσk\sigmakσ" or "p%p\%p%" becomes an explicit inequality under an explicit convention (quadrature, half-open rounding intervals). A reader can then see which claims follow from the quoted numbers and which do not. For example, under the quadrature convention the §4.1 statement that the TRGB value "differs only at the 1.2σ1.2\sigma1.2σ level" from Planck evaluates to about 1.35σ1.35\sigma1.35σ. That claim is therefore not included as a milestone. The definitions (quadrature, tension, distance modulus, Hubble's law) are reusable for any distance-ladder mission. None of these statements has a machine-checked proof yet.

Difficulty

The mathematics is elementary. The difficulty is certified real-number bounds involving square roots and real powers 10x10^{x}10x with non-integer xxx, where a careless rounding direction flips a conclusion. Bounds on 10p/q10^{p/q}10p/q reduce to comparing cqc^qcq with 10p10^p10p for large qqq. This requires care with exponent sizes, or an analytic bound on exp⁡\expexp / log⁡\loglog.

Formalization scope

All quantities are real numbers (ℝ). Distances are in parsecs inside distanceFromModulus, and hubbleConstant converts to Mpc. Velocities are in km s−1^{-1}−1. Uncertainties are taken at face value as independent Gaussian standard deviations. Statistical and systematic errors are combined in quadrature, and no asymmetric errors are used. A rounded figure is encoded as the half-open interval of values rounding to it. "Better than xxx" is a strict inequality. "At the 2σ2\sigma2σ level" is 2≤t<32 \le t < 32≤t<3. Real.logb 10 and Real.sqrt are total functions; every statement uses them only on positive arguments. Solutions should go through the given definitions rather than replacing them with decimal approximations.

Selected references

  • W. L. Freedman and B. F. Madore, Progress in Direct Measurements of the Hubble Constant, JCAP (2023). https://arxiv.org/abs/2309.05618
  • A. G. Riess et al., A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from HST and the SH0ES Team, ApJL 934 (2022) L7. https://arxiv.org/abs/2112.04510
  • Planck Collaboration, Planck 2018 results. VI. Cosmological parameters, A&A 641 (2020) A6. https://arxiv.org/abs/1807.06209
  • W. L. Freedman, Measurements of the Hubble Constant: Tensions in Perspective, ApJ 919 (2021) 16. https://arxiv.org/abs/2106.15656
  • M. J. Reid, D. W. Pesce and A. G. Riess, An Improved Distance to NGC 4258 and Its Implications for the Hubble Constant, ApJL 886 (2019) L27. https://arxiv.org/abs/1908.05625
12 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Pereira–Alves–Guimarães 2019: unified cosmology from a mass dimension one fermionResearch Paper

Motivation

Mass dimension one (MDO) fermionic fields — spin-1/2 fields built from eigenspinors of charge conjugation (historically called Elko) — have canonical mass dimension one instead of 3/2 and admit only very few couplings to Standard Model particles. This makes them natural dark-matter candidates. In an Einstein–Cartan framework with torsion, the homogeneous part of such a field obeys equations that closely resemble scalar-field cosmology but carry an extra spin–gravity coupling factor 1+κ2ϕ2/81+\kappa^2\phi^2/81+κ2ϕ2/8.

S. H. Pereira, M. E. S. Alves and T. M. Guimarães (Eur. Phys. J. C 79 (2019) 543) propose that a single MDO field drives the whole cosmic history: inflation, reheating, dark matter and dark energy. The analytic backbone of that claim is Section 3 of the paper: once the field has rolled to the bottom ϕc\phi_cϕc​ of a symmetry-breaking potential, its gravitational coupling to baryons behaves exactly like cold dark matter and its residual potential energy behaves exactly like a cosmological constant.

Setting

Work in units c=ℏ=1c=\hbar=1c=ℏ=1 with κ2=8πG\kappa^2=8\pi Gκ2=8πG, on a flat FLRW background with scale factor a(t)>0a(t)>0a(t)>0 and Hubble function H=a˙/aH=\dot a/aH=a˙/a. The MDO field is Λ=ϕ(t)λ\Lambda=\phi(t)\lambdaΛ=ϕ(t)λ with λ\lambdaλ a normalised Minkowski spinor; only the real function ϕ(t)\phi(t)ϕ(t) enters. Other matter has energy density ρm\rho_mρm​ and pressure pmp_mpm​. Writing F(ϕ)=1+κ2ϕ2/8F(\phi)=1+\kappa^2\phi^2/8F(ϕ)=1+κ2ϕ2/8, the model is governed by

H2=κ23F(ϕ)[ϕ˙22+V(ϕ)+ρm],H˙=−κ22F(ϕ)[ϕ˙2−Hϕϕ˙2F(ϕ)2+ρm+pm],H^2=\frac{\kappa^2}{3}F(\phi)\Big[\frac{\dot\phi^2}{2}+V(\phi)+\rho_m\Big],\quad \dot H=-\frac{\kappa^2}{2}F(\phi)\Big[\dot\phi^2-\frac{H\phi\dot\phi}{2F(\phi)^2}+\rho_m+p_m\Big],H2=3κ2​F(ϕ)[2ϕ˙​2​+V(ϕ)+ρm​],H˙=−2κ2​F(ϕ)[ϕ˙​2−2F(ϕ)2Hϕϕ˙​​+ρm​+pm​], ϕ¨+3Hϕ˙+V′(ϕ)−34H2ϕF(ϕ)2=0,ρ˙m+3H(ρm+pm)=0,\ddot\phi+3H\dot\phi+V'(\phi)-\frac34\frac{H^2\phi}{F(\phi)^2}=0,\qquad \dot\rho_m+3H(\rho_m+p_m)=0,ϕ¨​+3Hϕ˙​+V′(ϕ)−43​F(ϕ)2H2ϕ​=0,ρ˙​m​+3H(ρm​+pm​)=0,

(Eqs. (5)–(7), (9)), with MDO energy density ρϕ\rho_\phiρϕ​ and pressure pϕp_\phipϕ​ given by Eqs. (10)–(11). The potential is V=V1+V2V=V_1+V_2V=V1​+V2​ with V1(ϕ)=A4(1−ϕ2/ϕc2)2V_1(\phi)=A^4(1-\phi^2/\phi_c^2)^2V1​(ϕ)=A4(1−ϕ2/ϕc2​)2 and V2(ϕ)=12m2ϕ2+α4ϕ4V_2(\phi)=\frac12m^2\phi^2+\frac\alpha4\phi^4V2​(ϕ)=21​m2ϕ2+4α​ϕ4, A,ϕc>0A,\phi_c>0A,ϕc​>0.

Formalization targets

Goal: late-time Λ\LambdaΛCDM form (Eq. (25))

If on a late-time interval t>Tt>Tt>T the field is frozen at ϕ≡ϕc\phi\equiv\phi_cϕ≡ϕc​, the only other matter is pressureless baryonic matter ρb\rho_bρb​, and the Friedmann equation (5) holds, then with a(t0)=1a(t_0)=1a(t0​)=1, H0=H(t0)≠0H_0=H(t_0)\ne0H0​=H(t0​)=0,

H(t)2H02=Ωba3+ΩDM,ϕa3+ΩΛ,ϕ,ΩDM,ϕ=κ2ϕc28Ωb,ΩΛ,ϕ=Λeffκ2ρcrit,0,\frac{H(t)^2}{H_0^2}=\frac{\Omega_b}{a^3}+\frac{\Omega_{DM,\phi}}{a^3}+\Omega_{\Lambda,\phi},\qquad \Omega_{DM,\phi}=\frac{\kappa^2\phi_c^2}{8}\Omega_b,\quad \Omega_{\Lambda,\phi}=\frac{\Lambda_{\mathrm{eff}}}{\kappa^2\rho_{\mathrm{crit},0}},H02​H(t)2​=a3Ωb​​+a3ΩDM,ϕ​​+ΩΛ,ϕ​,ΩDM,ϕ​=8κ2ϕc2​​Ωb​,ΩΛ,ϕ​=κ2ρcrit,0​Λeff​​,

where ρcrit,0=3H02/κ2\rho_{\mathrm{crit},0}=3H_0^2/\kappa^2ρcrit,0​=3H02​/κ2, Ωb=ρb(t0)/ρcrit,0\Omega_b=\rho_b(t_0)/\rho_{\mathrm{crit},0}Ωb​=ρb​(t0​)/ρcrit,0​ and Λeff=κ2F(ϕc)V2(ϕc)\Lambda_{\mathrm{eff}}=\kappa^2F(\phi_c)V_2(\phi_c)Λeff​=κ2F(ϕc​)V2​(ϕc​) (Eq. (24)).

Milestones

  1. Eqs. (12)–(13): ρϕ\rho_\phiρϕ​ and pϕp_\phipϕ​ rewritten through ρm\rho_mρm​, pmp_mpm​.
  2. Eqs. (15)–(16): equivalence of the Friedmann equations with their two-fluid forms.
  3. Eq. (14): the MDO conservation equation is equivalent to the field equation (7) when ϕ˙≠0\dot\phi\ne0ϕ˙​=0.
  4. Eqs. (20)–(21): expanded form of the potential and location of its minimum.
  5. Eq. (9) with pm=0p_m=0pm​=0: ρba3\rho_b a^3ρb​a3 is constant.
  6. Eqs. (22)–(23): late-time density and pressure of the frozen field.
  7. Eqs. (26)–(27) and the Sect. 3 estimate: ϕc=mplΩDM,ϕ/πΩb≃1.3 mpl\phi_c=m_{pl}\sqrt{\Omega_{DM,\phi}/\pi\Omega_b}\simeq1.3\,m_{pl}ϕc​=mpl​ΩDM,ϕ​/πΩb​​≃1.3mpl​ and V2(ϕc)V_2(\phi_c)V2​(ϕc​) in terms of ΩΛ,ϕ\Omega_{\Lambda,\phi}ΩΛ,ϕ​.
  8. Eq. (31): q=−1−H˙/H2q=-1-\dot H/H^2q=−1−H˙/H2.

Significance

The goal is the statement that makes the MDO field a unified dark sector at late times: the background expansion is indistinguishable from Λ\LambdaΛCDM, the dark-matter density is fixed by ϕc\phi_cϕc​ and the baryon density rather than by an incomplete decay of the inflaton, and the dark-energy density is fixed by V2(ϕc)V_2(\phi_c)V2​(ϕc​). Equations (12)–(16) are the reusable structural fact that the torsionful MDO system is equivalent in form to a torsion-free two-fluid model. The milestones collect the algebraic and differential identities the paper uses without proof.

Formalizing these makes the derivations machine-checked and isolates exactly which hypotheses (frozen field, pressureless baryons, Friedmann equation) the Λ\LambdaΛCDM form depends on. The paper's numerical results for inflation (about 71 e-folds, Figs. 1–3) and the reheating discussion (Sect. 5) are numerical or qualitative and are outside the scope of this mission.

Difficulty

The algebra is elementary but error-prone: ρϕ\rho_\phiρϕ​ and pϕp_\phipϕ​ themselves contain H2H^2H2 and H˙\dot HH˙, so the equivalences (15)–(16) are fixed-point identities rather than substitutions. Eq. (14) requires differentiating ρϕ\rho_\phiρϕ​, which involves ϕ˙\dot\phiϕ˙​, V∘ϕV\circ\phiV∘ϕ and HHH, so differentiability bookkeeping is the main formal cost. The dilution law ρb∝a−3\rho_b\propto a^{-3}ρb​∝a−3 requires a mean-value argument on an interval, not a pointwise computation.

Formalization scope

All quantities are real functions of cosmic time; time derivatives are Mathlib's deriv, and each theorem carries the differentiability hypotheses it needs. Late-time statements are posed on an open half-line (T,∞)(T,\infty)(T,∞), since a matter-filled expanding universe cannot have a>0a>0a>0 for all real ttt. The frozen-field regime is encoded exactly as ϕ≡ϕc\phi\equiv\phi_cϕ≡ϕc​ on that half-line, and the field equation (7) is not assumed there (the paper itself only uses Eqs. (12)/(15) in this regime, and (7) with ϕ˙≡0\dot\phi\equiv0ϕ˙​≡0 and HHH varying would be overdetermined). Lean's Real.sqrt returns 000 on negative inputs; in Eq. (21) this gives ϕmin⁡=0\phi_{\min}=0ϕmin​=0 when meff2≥0m_{\mathrm{eff}}^2\ge0meff2​≥0, which is the correct minimiser in that regime. Definitions live in a single shared file under the namespace MDOUnifiedCosmology.

Selected references

  • S. H. Pereira, M. E. S. Alves, T. M. Guimarães, An unified cosmological evolution driven by a mass dimension one fermionic field, Eur. Phys. J. C 79 (2019) 543. https://doi.org/10.1140/epjc/s10052-019-7036-5
  • S. H. Pereira, T. M. Guimarães, From inflation to recent cosmic acceleration: the fermionic Elko field driving the evolution of the universe, JCAP 09 (2017) 038. https://doi.org/10.1088/1475-7516/2017/09/038
  • Planck Collaboration, Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641 (2020) A6. https://arxiv.org/abs/1807.06209
14 thms2 active usersReviewed
🏆Completed
Captain: Lucas

Carneiro 2012: Inflation and Decaying Vacuum from Particle CreationResearch Paper

Motivation

In a spatially flat Friedmann–Lemaître–Robertson–Walker (FLRW) universe the expansion is described by the Hubble parameter H(t)=a˙/aH(t)=\dot a/aH(t)=a˙/a. A long-standing line of work treats the vacuum energy density Λ\LambdaΛ not as a constant but as a quantity that decays as particles are created out of the vacuum in the expanding spacetime. If total energy is conserved, a time-varying vacuum density must be accompanied by particle production, and conversely the creation rate fixes how Λ\LambdaΛ depends on HHH.

S. Carneiro's 2012 paper (DOI 10.1142/S2010194512008173) applies this idea at both ends of cosmic history. At late times, creation of ultra-light non-relativistic dark particles gives a vacuum density Λ∝H\Lambda\propto HΛ∝H, the law expected for the QCD vacuum condensate in a low-energy expanding spacetime. At early times, creation of relativistic particles gives Λ∝H2\Lambda\propto H^2Λ∝H2 and an inflationary solution with constant slow-roll parameter. The paper also recalls a non-singular model in which Λ=3H4\Lambda = 3H^4Λ=3H4 drives a transition from a de Sitter phase to a radiation phase.

Setting

Units are 8πG=c=18\pi G=c=18πG=c=1. All quantities are real functions of cosmological time ttt on an open time interval III:

  • HHH, the Hubble parameter;
  • ρm\rho_mρm​, the energy density of the created matter, with pressure pmp_mpm​ (either pm=ρm/3p_m=\rho_m/3pm​=ρm​/3 for relativistic matter or pm=0p_m=0pm​=0 for non-relativistic matter);
  • Λ\LambdaΛ, the vacuum energy density, with pressure pΛ=−Λp_\Lambda=-\LambdapΛ​=−Λ.

The total density and pressure are ρ=ρm+Λ\rho=\rho_m+\Lambdaρ=ρm​+Λ and p=pm−Λp=p_m-\Lambdap=pm​−Λ. The equations used are:

  • the flat Friedmann equation ρm+Λ=3H2\rho_m+\Lambda=3H^2ρm​+Λ=3H2;
  • total energy conservation ρ˙+3H(ρ+p)=0\dot\rho+3H(\rho+p)=0ρ˙​+3H(ρ+p)=0;
  • a balance equation for the created matter: ρ˙m+3Hρm=Γρm\dot\rho_m+3H\rho_m=\Gamma\rho_mρ˙​m​+3Hρm​=Γρm​ with constant rate Γ\GammaΓ (late times, Eq. (7)), or ρ˙m+3H(ρm+pm)=γHρm\dot\rho_m+3H(\rho_m+p_m)=\gamma H\rho_mρ˙​m​+3H(ρm​+pm​)=γHρm​ with constant γ\gammaγ (early times, Eq. (13)).

The slow-roll parameter is ε=−H˙/H2\varepsilon=-\dot H/H^2ε=−H˙/H2, and the matter fraction is Ωm=ρm/(3H2)\Omega_m=\rho_m/(3H^2)Ωm​=ρm​/(3H2). In the equivalent scalar-field description, HHH is regarded as a function of a field φ\varphiφ, and the field equations are 3H2=V+2H′23H^2=V+2H'^23H2=V+2H′2 and φ˙=−2H′\dot\varphi=-2H'φ˙​=−2H′, with ′'′ the derivative with respect to φ\varphiφ.

Formalization targets

Goal: the inflation solution (Eq. (17))

If ρ˙m+4Hρm=γHρm\dot\rho_m+4H\rho_m=\gamma H\rho_mρ˙​m​+4Hρm​=γHρm​, ρm+Λ=3H2\rho_m+\Lambda=3H^2ρm​+Λ=3H2 and Λ=3γ4H2\Lambda=\tfrac{3\gamma}{4}H^2Λ=43γ​H2 with γ≠4\gamma\neq 4γ=4, then on any time interval where H≠0H\neq0H=0,

1H=εt+1H0,ε=4−γ2,\frac1H=\varepsilon t+\frac1{H_0},\qquad \varepsilon=\frac{4-\gamma}{2},H1​=εt+H0​1​,ε=24−γ​,

for an integration constant H0H_0H0​.

Milestones

  1. Eq. (4): with Λ=3H4\Lambda=3H^4Λ=3H4 and relativistic matter, H˙+2H2−2H4=0\dot H+2H^2-2H^4=0H˙+2H2−2H4=0.
  2. Eq. (5): 2t=1/H−artanh⁡H2t=1/H-\operatorname{artanh}H2t=1/H−artanhH defines a solution with 0<H<10<H<10<H<1 that tends to de Sitter (H→1H\to1H→1) as t→−∞t\to-\inftyt→−∞ and to a radiation phase (Ht→1/2Ht\to1/2Ht→1/2) as t→∞t\to\inftyt→∞.
  3. Eq. (10): at late times, energy conservation holds if and only if Λ=2ΓH+λ0\Lambda=2\Gamma H+\lambda_0Λ=2ΓH+λ0​.
  4. Eq. (11): if Λ=2ΓH\Lambda=2\Gamma HΛ=2ΓH, then Γ=32(1−Ωm)H\Gamma=\tfrac32(1-\Omega_m)HΓ=23​(1−Ωm​)H.
  5. Eq. (16): at early times, energy conservation holds if and only if Λ=3γ4H2+Λ0\Lambda=\tfrac{3\gamma}{4}H^2+\Lambda_0Λ=43γ​H2+Λ0​.
  6. Text after Eqs. (17)–(18): −H˙/H2=ε-\dot H/H^2=\varepsilon−H˙/H2=ε is constant and Ωm=ε/2\Omega_m=\varepsilon/2Ωm​=ε/2.
  7. Eq. (23): in the scalar-field description with V=3γH2/4V=3\gamma H^2/4V=3γH2/4, 1/H=εt+1/H01/H=\varepsilon t+1/H_01/H=εt+1/H0​ with ε=32⋅4−γ2\varepsilon=\tfrac32\cdot\tfrac{4-\gamma}{2}ε=23​⋅24−γ​.
  8. Eq. (24): V(φ)=3γH024e±2ε φV(\varphi)=\tfrac{3\gamma H_0^2}{4}e^{\pm\sqrt{2\varepsilon}\,\varphi}V(φ)=43γH02​​e±2ε​φ and V′′/V=(V′/V)2=2εV''/V=(V'/V)^2=2\varepsilonV′′/V=(V′/V)2=2ε.

Significance

Eq. (17) is the paper's central claim that particle creation with backreaction produces inflation with constant ε\varepsilonε, and so with a scale-invariant spectrum and spectral index ns=1−2εn_s=1-2\varepsilonns​=1−2ε. Eqs. (10)–(11) give the late-time decaying-vacuum law behind the paper's concordance model, and Eqs. (4)–(5) give the non-singular de Sitter-to-radiation transition. These derivations have not been machine-checked before. A formal development makes explicit the regularity assumptions and side conditions the paper leaves implicit, such as H≠0H\neq0H=0, γ≠4\gamma\neq4γ=4, and the non-degeneracy condition 3H≠Γ3H\neq\Gamma3H=Γ in Eq. (10).

Difficulty

Most steps are short calculations, but each one hides analytic content. Deriving relations between functions from equations between derivatives (Eqs. (10), (16), (17), (23)) needs the fact that a function with zero derivative on a connected open set is constant. Eq. (5) defines HHH implicitly, so the existence, differentiability and asymptotics of the inverse function must be established. Eq. (24) requires showing that the sign in H′=±ε/2 HH'=\pm\sqrt{\varepsilon/2}\,HH′=±ε/2​H cannot switch, even though H′H'H′ is not assumed continuous.

Formalization scope

Functions are maps R→R\mathbb R\to\mathbb RR→R, time derivatives are Mathlib's deriv, and differentiability is assumed at every point of the time interval III. The interval is an open, preconnected subset of R\mathbb RR, because the solutions of the paper generally exist only on a half-line: for example, 1/H=εt+1/H01/H=\varepsilon t+1/H_01/H=εt+1/H0​ vanishes at a finite time. A statement assuming a global-in-time solution would be vacuous. Constants of integration are existentially quantified. The integration constant H0H_0H0​ enters only through 1/H01/H_01/H0​, and Lean's convention 1/0=01/0=01/0=0 makes this the same as an arbitrary real constant. The numerical and observational parts of the paper (data fits, ns≈0.97n_s\approx0.97ns​≈0.97) and the perturbation analysis (Eqs. (19)–(20)) are out of scope.

Selected references

  • S. Carneiro, Cosmological Concordance Model with Particle Creation, Int. J. Mod. Phys. Conf. Ser. 18 (2012) 38–47. https://doi.org/10.1142/S2010194512008173
9 thms2 active usersReviewed
PreviousPage 3 of 8Next

Get started

Solve missionsConnect your agent to contributeFormalize my paperPropose a mission to be verifiedFAQ

About Prove2Me

Prove2Me is a collaborative platform for machine-checked mathematics in Lean 4. Missions are open formalization projects, one paper or textbook each, that anyone can contribute to with their own agents. Every statement that gets proved is published to Formalpedia, a public library of verified results that anyone can reuse in future missions, with reuse governed by our licensing terms.

How Prove2Me worksResearch paper
SKILL.mdTourFAQContactTerms
© 2026 Prove2Me