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Campaigns (experimental)

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Campaigns group missions around a shared mathematical goal. Each one tracks a quantity, such as an upper or lower bound. Have a good candidate in mind? Ping us on Slack, Zulip, or WeChat.

Block Sensitivity vs. Sensitivity

How much larger can block sensitivity be than sensitivity for a total Boolean function?

For a total Boolean function f:{0,1}n→{0,1}f:\{0,1\}^n\to\{0,1\}f:{0,1}n→{0,1}, a block of coordinates is sensitive at xxx if flipping every bit in that block changes f(x)f(x)f(x). Let s(f,x)s(f,x)s(f,x) count sensitive singletons and bs(f,x)bs(f,x)bs(f,x) be the maximum number of pairwise disjoint sensitive blocks. Define s(f)=max⁡xs(f,x)s(f)=\max_x s(f,x)s(f)=maxx​s(f,x) and bs(f)=max⁡xbs(f,x)bs(f)=\max_x bs(f,x)bs(f)=maxx​bs(f,x).

This campaign seeks larger exponents α\alphaα for which there exists an infinite family of total Boolean functions fk:{0,1}nk→{0,1}f_k:\{0,1\}^{n_k}\to\{0,1\}fk​:{0,1}nk​→{0,1}, indexed by k=1,2,…k=1,2,\ldotsk=1,2,…, satisfying

s(fk)→∞,bs(fk)≥s(fk)α−o(1)as k→∞.s(f_k)\to\infty,\qquad bs(f_k)\ge s(f_k)^{\alpha-o(1)}\quad\text{as }k\to\infty.s(fk​)→∞,bs(fk​)≥s(fk​)α−o(1)as k→∞.

Here o(1)o(1)o(1) denotes a quantity tending to zero as k→∞k\to\inftyk→∞. Higher is better. The classical exponent is 222, and Huang's bound gives a ceiling of 444.

OpenAI's construction achieves an exponent strictly greater than 222.

One sufficient way to establish an exponent α\alphaα is to find a single total Boolean function fff with s(f)>1s(f)>1s(f)>1 and bs(f)≥s(f)αbs(f)\ge s(f)^\alphabs(f)≥s(f)α. Input and output normalization followed by self-composition then yields the required asymptotic family.

≥ 2.13981Formalized record→≥ 2.15Open frontier
11 provers on it22 of 23 missions formalized

Integer Multiplication Below n log n

Turn proposed improvements to integer multiplication into complete Lean proofs, and push the exponent saving further.

Harvey and van der Hoeven established an O(nlog⁡n)O(n\log n)O(nlogn) algorithm in 2021. This campaign builds on that foundation, the OpenAI manuscript, and subsequent community constructions to pursue a strict asymptotic improvement.

For two nnn-bit integers, the target is

T(n)=O ⁣(n L(n)1−κ),L(n)=max⁡(⌈log⁡2n⌉,1).T(n)=O\!\left(n\,L(n)^{1-\kappa}\right),\qquad L(n)=\max(\lceil\log_2 n\rceil,1).T(n)=O(nL(n)1−κ),L(n)=max(⌈log2​n⌉,1).

A positive κ\kappaκ beats nlog⁡nn\log nnlogn asymptotically; larger κ\kappaκ is better. Every entry must exhibit one deterministic multitape Turing machine, with a fixed finite alphabet and tape count, that computes the exact product at every positive input length and meets the eventual worst-case time bound. The tracked number measures an asymptotic exponent saving.

≥ 3.6 × 10−5Formalized record→≥ 5.1 × 10−5Open frontier
8 provers on it4 of 7 missions formalized

3SUM Exponent

Classical algorithms solve 3SUM in O(n2)O(n^2)O(n2) time. In a 2026 breakthrough, Alman and Vassilevska Williams gave a deterministic O(n1.9992)O(n^{1.9992})O(n1.9992) algorithm, refuting the integer 3SUM hypothesis. How low can the exponent go?

Building on existing Lean formalizations, this campaign tracks upper bounds for 3SUM on polynomially bounded integers, using a word RAM with O(log⁡n)O(\log n)O(logn)-bit words, and pursues smaller exponents.

≤ 1.960614Formalized record→≤ 1.9202796Open frontier
4 provers on it7 of 8 missions formalized

All-Pairs Shortest Paths (APSP) Exponent

Classical algorithms solve all-pairs shortest paths in O(n3)O(n^3)O(n3) time. In a 2026 breakthrough, Alman and Vassilevska Williams refuted the APSP conjecture with a deterministic O(n2.99942)O(n^{2.99942})O(n2.99942) algorithm. How low can the exponent go?

Building on existing Lean formalizations, this campaign tracks upper bounds for exact APSP and pursues smaller exponents.

≤ 2.995561Formalized record
3 provers on it5 of 5 missions formalized

The irrationality measure of π

The irrationality measure of π quantifies how closely rational numbers can approximate it. This campaign seeks formal proofs of sharper upper bounds, starting with Mahler’s bound of 42.

≤ 2Formalized record
19 provers on it9 of 9 missions formalized

Sharp diagonal Hlawka constant

The sharp Hlawka inequality for Schatten ppp-norms is a cousin of the triangle inequality: it relates the norms of three matrices to the norms of their pairwise sums and their total sum. For complex diagonal matrices, an exact formula for the best possible comparison constant has been proved in Lean for every real p≥256p\ge256p≥256. We conjecture that the same formula holds for all p≥2p\ge2p≥2.

What is the smallest cutoff p′p'p′ for which this formula holds for every real p≥p′p\ge p'p≥p′?

References:

  • Wolfram MathWorld, Hlawka's Inequality.
  • Audenaert and Kittaneh, Problems and Conjectures in Matrix and Operator Inequalities, §8.2 (2017).
  • Marinescu and Niculescu, A New Look at the Hornich–Hlawka Inequality (2025).
  • Analytic argument for p≥90p\ge90p≥90, awaiting formalization in Lean.
≤ 4Formalized record→≤ 2Open frontier
8 provers on it17 of 18 missions formalized

Odd numbers as sums of primes

Is every odd number a sum of kkk primes? This campaign tracks formalized proofs of the smallest kkk that suffices.

Schnirelmann (1930) showed some finite kkk works. Vinogradov (1937) showed that three is enough for all sufficiently large odd numbers. Tao (2012) proved k=5k = 5k=5 unconditionally. Helfgott (2013) proved that every odd number greater than 555 is a sum of three primes, though the proof is still unrefereed. Ideally, we can formalize this statement here. Note that three is optimal: 272727 is neither prime nor 222 + prime.

≤ 21Formalized record→≤ 5Open frontier
41 provers on it16 of 18 missions formalized

Matrix multiplication exponent

Schoolbook matrix multiplication takes n3n^3n3 operations. The exponent ω\omegaω is the infimum of all τ\tauτ such that two n×nn \times nn×n matrices can be multiplied in O(nτ)O(n^{\tau})O(nτ) arithmetic operations; trivially ω≥2\omega \geq 2ω≥2, and ω=2\omega = 2ω=2 is conjectured but open.

Strassen gave the first nontrivial bound, ω<2.81\omega < 2.81ω<2.81, in 1969, and introduced the laser method in 1986 to reach ω<2.48\omega < 2.48ω<2.48. Coppersmith and Winograd's 1990 bound of 2.3762.3762.376 stood for two decades. Every subsequent improvement comes from analyzing higher tensor powers of their construction with refined laser-method variants. That line reached ω<2.371339\omega < 2.371339ω<2.371339 in 2025, and the current record is ω<2.371177\omega < 2.371177ω<2.371177, from August 2026. See Computational complexity of matrix multiplication for the full table. Can we formalize these results and even improve on them?

≤ 2.25Formalized record
16 provers on it9 of 9 missions formalized

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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.

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Mathematical Physics·Captain: Lucas

Weinberg 1967: A Model of Leptons — tree-level electroweak boson spectrumResearch Paper

Motivation

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

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

Setting

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

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

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

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

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

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

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

Target

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

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

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

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

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

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

Significance

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

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

Difficulty

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

Formalization scope

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

Selected references

  • S. Weinberg, A Model of Leptons, Phys. Rev. Lett. 19, 1264–1266 (1967). doi:10.1103/PhysRevLett.19.1264
13 thms2 active usersReviewed
Bandit AlgorithmsMachine Learning·Captain: mikedeng1

An Optimal Algorithm for Stochastic and Adversarial Bandits III: α-Tsallis-INF With Gap-Tuned Asymmetric Regularization Has Logarithmic Pseudo-Regret When the Best Arm Is UniqueResearch Paper

Motivation

In the multi-armed bandit problem a learner repeatedly chooses one of KKK actions and observes only the loss of the action it chose. Two models of the environment dominate the literature. In the stochastic model the losses of each arm are drawn i.i.d. from a fixed distribution, and the optimal pseudo-regret grows like ∑i≠i∗log⁡(T)/Δi\sum_{i\ne i^*}\log(T)/\Delta_i∑i=i∗​log(T)/Δi​, where Δi\Delta_iΔi​ is the gap between the mean loss of arm iii and that of the best arm i∗i^*i∗ (Lai and Robbins, 1985). In the adversarial model the losses are arbitrary and the optimal rate is Θ(KT)\Theta(\sqrt{KT})Θ(KT​) (Audibert and Bubeck, 2010). Algorithms that are near-optimal in both models without knowing which one they face are called best of both worlds.

Timeline:

  • Bubeck and Slivkins (2012) gave the first best-of-both-worlds algorithm and asked whether one algorithm could be optimal in both regimes.
  • Seldin and Slivkins (2014) and Auer and Chiang (2016) obtained log⁡2T\log^2 Tlog2T or log⁡3T\log^3 Tlog3T stochastic rates with KT\sqrt{KT}KT​-type adversarial guarantees.
  • Wei and Luo (2018) introduced the stochastically constrained adversarial regime and the log-barrier algorithm BROAD.
  • Zimmert and Seldin (2021) showed that online mirror descent with the 12\tfrac1221​-Tsallis entropy (Tsallis-INF) is optimal in both regimes up to constants. Their Theorem 4, the subject of this mission, studies the whole family of α\alphaα-Tsallis regularizers with gap-dependent tuning in the stochastically constrained regime.

Setting

There are K≥2K\ge2K≥2 arms and rounds t=1,2,…t=1,2,\dotst=1,2,…. In round ttt the learner draws an arm ItI_tIt​ from a probability vector wtw_twt​ in the simplex ΔK−1\Delta^{K-1}ΔK−1, the environment fixes losses ℓt∈[0,1]K\ell_t\in[0,1]^Kℓt​∈[0,1]K, and only ℓt,It\ell_{t,I_t}ℓt,It​​ is observed. The environment may adapt to the past actions I1,…,It−1I_1,\dots,I_{t-1}I1​,…,It−1​ and use its own randomization, modelled by a seed ω\omegaω drawn once from a probability measure μ\muμ. The pseudo-regret is

Reg‾T=E[∑t=1Tℓt,It]−min⁡iE[∑t=1Tℓt,i],\overline{Reg}_T=\mathbb E\Big[\sum_{t=1}^T\ell_{t,I_t}\Big]-\min_i\mathbb E\Big[\sum_{t=1}^T\ell_{t,i}\Big],Reg​T​=E[t=1∑T​ℓt,It​​]−imin​E[t=1∑T​ℓt,i​],

with the expectation over the seed and the learner's draws; a minimizing arm is a best arm in hindsight iT∗i^*_TiT∗​.

α-Tsallis-INF is online mirror descent on the simplex. With α∈(0,1)\alpha\in(0,1)α∈(0,1), regularization parameters ξi>0\xi_i>0ξi​>0 and learning rates ηt>0\eta_t>0ηt​>0, set

Ψ(w)=−∑iwiα−αwiα(1−α)ξi,Ψt=Ψ/ηt.\Psi(w)=-\sum_i\frac{w_i^\alpha-\alpha w_i}{\alpha(1-\alpha)\xi_i},\qquad\Psi_t=\Psi/\eta_t .Ψ(w)=−i∑​α(1−α)ξi​wiα​−αwi​​,Ψt​=Ψ/ηt​.

The learner keeps importance-weighted loss estimates ℓ^t,i=1(It=i)ℓt,i/wt,i\hat\ell_{t,i}=\mathbb 1(I_t=i)\ell_{t,i}/w_{t,i}ℓ^t,i​=1(It​=i)ℓt,i​/wt,i​, their sums L^t\hat L_tL^t​, and plays wt=arg⁡max⁡w∈ΔK−1⟨w,−L^t−1⟩−Ψt(w)w_t=\arg\max_{w\in\Delta^{K-1}}\langle w,-\hat L_{t-1}\rangle-\Psi_t(w)wt​=argmaxw∈ΔK−1​⟨w,−L^t−1​⟩−Ψt​(w). The potential Φt(Y)=max⁡w∈ΔK−1⟨w,Y⟩−Ψt(w)\Phi_t(Y)=\max_{w\in\Delta^{K-1}}\langle w,Y\rangle-\Psi_t(w)Φt​(Y)=maxw∈ΔK−1​⟨w,Y⟩−Ψt​(w) splits the regret into a stability term E[∑tℓt,It+Φt(−L^t)−Φt(−L^t−1)]\mathbb E[\sum_t\ell_{t,I_t}+\Phi_t(-\hat L_t)-\Phi_t(-\hat L_{t-1})]E[∑t​ℓt,It​​+Φt​(−L^t​)−Φt​(−L^t−1​)] and a penalty term E[∑tΦt(−L^t−1)−Φt(−L^t)−ℓt,iT∗]\mathbb E[\sum_t\Phi_t(-\hat L_{t-1})-\Phi_t(-\hat L_t)-\ell_{t,i^*_T}]E[∑t​Φt​(−L^t−1​)−Φt​(−L^t​)−ℓt,iT∗​​].

In the stochastically constrained regime the loss differences have fixed means, E[ℓt,i−ℓt,i∗]=Δi\mathbb E[\ell_{t,i}-\ell_{t,i^*}]=\Delta_iE[ℓt,i​−ℓt,i∗​]=Δi​, with a unique best arm i∗i^*i∗ (Δi>0\Delta_i>0Δi​>0 for i≠i∗i\ne i^*i=i∗). Then Reg‾T=E[∑t∑i≠i∗wt,iΔi]\overline{Reg}_T=\mathbb E[\sum_t\sum_{i\ne i^*}w_{t,i}\Delta_i]Reg​T​=E[∑t​∑i=i∗​wt,i​Δi​] and iT∗=i∗i^*_T=i^*iT∗​=i∗. Write Δmin⁡=min⁡i≠i∗Δi\Delta_{\min}=\min_{i\ne i^*}\Delta_iΔmin​=mini=i∗​Δi​. Theorem 4 uses

ηt=16α4 1−tˉ−1+α(1−α)tα,tˉ=max⁡{e,t},ξi=Δi1−2α (i≠i∗),ξi∗=Δmin⁡1−2α.\eta_t=\frac{16^\alpha}{4}\,\frac{1-\bar t^{-1+\alpha}}{(1-\alpha)t^\alpha},\quad\bar t=\max\{e,t\},\qquad\xi_i=\Delta_i^{1-2\alpha}\ (i\ne i^*),\quad\xi_{i^*}=\Delta_{\min}^{1-2\alpha}.ηt​=416α​(1−α)tα1−tˉ−1+α​,tˉ=max{e,t},ξi​=Δi1−2α​ (i=i∗),ξi∗​=Δmin1−2α​.

Formalization targets

Goal: Theorem 4 (p. 12)

With T0=16Δmin⁡2log⁡216Δmin⁡2T_0=\frac{16}{\Delta_{\min}^2}\log^2\frac{16}{\Delta_{\min}^2}T0​=Δmin2​16​log2Δmin2​16​, for every T≥1T\ge1T≥1,

Reg‾T≤∑i≠i∗(8min⁡{11−α,log⁡T}+64)(log⁡T+1)Δi+16log⁡4(T0)Δmin⁡+4.\overline{Reg}_T\le\sum_{i\ne i^*}\frac{\big(8\min\{\frac1{1-\alpha},\log T\}+64\big)(\log T+1)}{\Delta_i}+\frac{16\log^4(T_0)}{\Delta_{\min}}+4 .Reg​T​≤i=i∗∑​Δi​(8min{1−α1​,logT}+64)(logT+1)​+Δmin​16log4(T0​)​+4.

Milestones

Lemma 17 (Hessian control along a mirror step); Lemma 11, cases 1 and 4 (instantaneous stability); Lemma 20 and Lemma 12, part 2 (penalty); Lemmas 14 and 16 (scalar inequalities for the learning-rate factors); displays (26) and (30) of Appendix D, the stability and penalty bounds under the parameters of Theorem 4.

Lemmas 20 and 12 cover any causal unbiased loss estimator satisfying the bandit feedback assumptions; the other bandit bounds use the importance-weighted estimator.

Significance

The theorem shows that the logarithmic stochastic rate is not special to the 12\tfrac1221​-Tsallis entropy: for every α∈(0,1)\alpha\in(0,1)α∈(0,1), tuning the regularizer to the gaps gives pseudo-regret of order ∑i≠i∗min⁡{11−α,log⁡T}log⁡T/Δi\sum_{i\ne i^*}\min\{\frac1{1-\alpha},\log T\}\log T/\Delta_i∑i=i∗​min{1−α1​,logT}logT/Δi​ in stochastically constrained environments. This places the log-barrier (α→0\alpha\to0α→0) and entropic (α→1\alpha\to1α→1) regularizers of earlier algorithms in one family, and isolates the role of asymmetric regularization. Unlike Theorem 1, it needs the gaps to tune ξ\xiξ, so it is a statement about the reach of the method rather than a practical algorithm.

The result is proved in the paper; no part of it has a machine-checked proof. Formalizing it produces a complete verified analysis of an online-mirror-descent bandit algorithm with time-varying, non-monotone learning rates, including the stability–penalty decomposition, the Hessian control of Lemma 17 and the explicit constant chase of Appendix D. The analysis also checks two points the paper leaves open: the printed bound has log⁡T\log TlogT where its proof gives log⁡T+1\log T+1logT+1, and Appendix D applies Lemma 12, which assumes non-increasing learning rates, to a rate that increases for a few early rounds when α\alphaα is small.

Difficulty

The obvious argument bounds each round's stability by ∑iηtξi2E[wt,i]1−α\sum_i\frac{\eta_t\xi_i}2\mathbb E[w_{t,i}]^{1-\alpha}∑i​2ηt​ξi​​E[wt,i​]1−α (Lemma 11, case 1) and sums. That bound contains the best arm, whose weight tends to one, so it grows polynomially in TTT and cannot give a logarithmic rate. The arm i∗i^*i∗ has to be removed from the stability, which needs a shifted second-order expansion where losses become slightly negative, and that is only controlled once ηtξi≤14\eta_t\xi_i\le\frac14ηt​ξi​≤41​ (Lemma 17). The early rounds before T0T_0T0​ must be paid for separately, and the asymmetric ξ\xiξ and the learning rate interact through constants that must be tracked exactly for the self-bounding step to close.

Formalization scope

Arms are Fin K with K≥2K\ge2K≥2 and the paper's arm iii is i - 1. Rounds start at 1; an action sequence is h : ℕ → Fin K with h 0 unused. The adversary is the published RegretBandits.Adversarial.Adversary (losses in [0,1][0,1][0,1] depending on past actions only) composed with a seed drawn from a probability measure, with losses measurable in the seed. Expectations are explicit: an integral over the seed of a finite sum over action paths weighted by ∏twt,It\prod_t w_{t,I_t}∏t​wt,It​​. The algorithm is an argmax predicate on the weight function, never a choice function. Φt\Phi_tΦt​ is a real supremum over the simplex. Logarithms are natural, and real powers are Real.rpow with nonnegative bases.

The goal takes α∈(0,1)\alpha\in(0,1)α∈(0,1); the endpoints α∈{0,1}\alpha\in\{0,1\}α∈{0,1}, where the paper's learning rate and regularizer are limits, are not stated. The regime "stochastically constrained with a unique best arm" is replaced by the two consequences the proof uses: the self-bounding inequality Reg‾T≥E[∑t∑i≠i∗wt,iΔi]\overline{Reg}_T\ge\mathbb E[\sum_t\sum_{i\ne i^*}w_{t,i}\Delta_i]Reg​T​≥E[∑t​∑i=i∗​wt,i​Δi​] and iT∗=i∗i^*_T=i^*iT∗​=i∗. Every such regime satisfies both, so the formal statement is at least as strong as the printed one. The constant log⁡T+1\log T+1logT+1 in the first term is the one the proof reaches. A trivial formalization is ruled out: the expectation is a genuine probability law, the gaps are tied to the losses through the self-bounding hypothesis, and the weights are determined by the algorithm, so the bound cannot hold vacuously.

A complete development needs the explicit law of a bandit run with an adaptive randomized adversary, unbiasedness of the IW estimator, convex conjugates and Bregman divergences on the simplex, and elementary real analysis for Lemmas 14 and 16. The run-law and the stability–penalty decomposition are reusable for any mirror-descent bandit algorithm. Proofs of any milestone, and of the scalar Lemmas 14 and 16 in particular, are welcome independently.

Selected references

  • J. Zimmert and Y. Seldin, Tsallis-INF: An Optimal Algorithm for Stochastic and Adversarial Bandits, Journal of Machine Learning Research 22(28), 2021. https://arxiv.org/abs/1807.07623 (v6)
  • S. Bubeck and A. Slivkins, The best of both worlds: stochastic and adversarial bandits, COLT 2012. https://arxiv.org/abs/1202.4473
  • C.-Y. Wei and H. Luo, More adaptive algorithms for adversarial bandits, COLT 2018. https://arxiv.org/abs/1801.03265
  • J. Abernethy, C. Lee and A. Tewari, Fighting bandits with a new kind of smoothness, NeurIPS 2015. https://arxiv.org/abs/1512.04152
  • T. L. Lai and H. Robbins, Asymptotically efficient adaptive allocation rules, Advances in Applied Mathematics 6(1), 1985. https://doi.org/10.1016/0196-8858(85)90002-8
  • J.-Y. Audibert and S. Bubeck, Regret bounds and minimax policies under partial monitoring, Journal of Machine Learning Research 11, 2010. https://jmlr.org/papers/v11/audibert10a.html
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Formal VerificationMathematical LogicTheory of Computation·Captain: mikedeng1

Monitoring Metric First-Order Temporal Properties: The Monitor M_Φ Outputs Exactly the Violations (¬Φ)^(D̄,τ̄,i) of a Bounded MFOTL Formula Φ, as Regular Sets, at Every Time Point iResearch Paper

Motivation

Runtime monitoring checks a running system against a specification by inspecting its trace of events as it is produced. Policies on data, such as "every published report was approved within the last 10 days" or "each value stored in in reaches out within 5 time units", quantify over data values and constrain the time between events. Metric first-order temporal logic (MFOTL) expresses such policies: it extends first-order logic with past and future temporal operators that carry intervals of allowed time differences.

Basin, Klaedtke, Müller and Zălinescu (J. ACM 62(2), Article 15, 2015) give a monitor for MFOTL properties □Φ\square\Phi□Φ with Φ\PhiΦ bounded. It allows negation and quantification over the infinite domain N\mathbb NN without restriction, because every relation it manipulates is represented by a finite automaton: the input structures are automatic structures. The paper implements it in the prototype tool MonPoly-Reg (§6). Its correctness rests on Theorem 3.9: the monitor reports exactly the violations of Φ\PhiΦ, at every time point.

Setting

A signature S=(C,R,ι)S=(C,R,\iota)S=(C,R,ι) has finitely many constants and predicates with arities. Formulas are built from t≈t′t\approx t't≈t′ and r(t1,…,tι(r))r(t_1,\dots,t_{\iota(r)})r(t1​,…,tι(r)​) by ¬\neg¬, ∨\vee∨, ∃x\exists x∃x and the temporal operators ∙I\bullet_I∙I​ (previous), ∘I\circ_I∘I​ (next), SI\mathsf S_ISI​ (since) and UI\mathsf U_IUI​ (until), where I=[b,b′)I=[b,b')I=[b,b′) is a nonempty interval of N\mathbb NN with b′∈N∪{∞}b'\in\mathbb N\cup\{\infty\}b′∈N∪{∞}. A formula is bounded if every UI\mathsf U_IUI​ in it has b′<∞b'<\inftyb′<∞.

A temporal structure (Dˉ,τˉ)(\bar{\mathcal D},\bar\tau)(Dˉ,τˉ) assigns to each time point i∈Ni\in\mathbb Ni∈N relations rDi⊆Nι(r)r^{\mathcal D_i}\subseteq\mathbb N^{\iota(r)}rDi​⊆Nι(r) and a time stamp τi∈N\tau_i\in\mathbb Nτi​∈N; constants are rigid, τ0≤τ1≤⋯\tau_0\le\tau_1\le\cdotsτ0​≤τ1​≤⋯, and τˉ\bar\tauτˉ exceeds every bound. Satisfaction (Dˉ,τˉ,v,i)⊨φ(\bar{\mathcal D},\bar\tau,v,i)\models\varphi(Dˉ,τˉ,v,i)⊨φ is Definition 2.2; for example ψ UI ψ′\psi\,\mathsf U_I\,\psi'ψUI​ψ′ holds at iii if ψ′\psi'ψ′ holds at some j≥ij\ge ij≥i with τj−τi∈I\tau_j-\tau_i\in Iτj​−τi​∈I and ψ\psiψ holds at all k∈[i,j)k\in[i,j)k∈[i,j). For φ\varphiφ with free variables x1<⋯<xnx_1<\dots<x_nx1​<⋯<xn​, the satisfying set is

φ(Dˉ,τˉ,i)={dˉ∈Nn∣(Dˉ,τˉ,v[xˉ↦dˉ],i)⊨φ for some v}.\varphi^{(\bar{\mathcal D},\bar\tau,i)}=\{\bar d\in\mathbb N^n\mid(\bar{\mathcal D},\bar\tau,v[\bar x\mapsto\bar d],i)\models\varphi\ \text{for some }v\}.φ(Dˉ,τˉ,i)={dˉ∈Nn∣(Dˉ,τˉ,v[xˉ↦dˉ],i)⊨φ for some v}.

A domain representation is a regular language L\mathcal LL over a finite alphabet with a surjection ν:L→N\nu:\mathcal L\to\mathbb Nν:L→N whose equality relation is regular. A relation A⊆NkA\subseteq\mathbb N^kA⊆Nk is regular if the words u1⊗⋯⊗uku_1\otimes\cdots\otimes u_ku1​⊗⋯⊗uk​ (the letter-by-letter convolution, padded with #\##) with (ν(u1),…,ν(uk))∈A(\nu(u_1),\dots,\nu(u_k))\in A(ν(u1​),…,ν(uk​))∈A form a regular language.

The monitor MΦ\mathsf M_\PhiMΦ​ (Fig. 2) reads (D0,τ0),(D1,τ1),…(\mathcal D_0,\tau_0),(\mathcal D_1,\tau_1),\dots(D0​,τ0​),(D1​,τ1​),… one element per loop iteration. It extends each Dj\mathcal D_jDj​ to D^j\hat{\mathcal D}_jD^j​ with auxiliary relations pαp_\alphapα​ (and rαr_\alpharα​, sαs_\alphasα​ for since and until) for every temporal subformula α\alphaα, built incrementally by the constructions of §3.4 once a list QQQ of pending triples (α,j,S)(\alpha,j,S)(α,j,S) says that enough of the future has been read. When D^i\hat{\mathcal D}_iD^i​ is complete it outputs the set (¬Φ^)D^i(\neg\hat\Phi)^{\hat{\mathcal D}_i}(¬Φ^)D^i​ with τi\tau_iτi​, where Φ^\hat\PhiΦ^ is Φ\PhiΦ with each top-level temporal subformula α\alphaα replaced by the atom pα(xˉ)p_\alpha(\bar x)pα​(xˉ).

Formalization targets

Goal: Theorem 3.9

For every input satisfying the restrictions of §3.1 and every bounded Φ\PhiΦ:

(i)(n,O,t) output by line 9 ⟹ O=(¬Φ)(Dˉ,τˉ,n), O regular, t=τn;\text{(i)}\quad (n,O,t)\ \text{output by line 9}\ \Longrightarrow\ O=(\neg\Phi)^{(\bar{\mathcal D},\bar\tau,n)},\ O\ \text{regular},\ t=\tau_n;(i)(n,O,t) output by line 9 ⟹ O=(¬Φ)(Dˉ,τˉ,n), O regular, t=τn​; (ii)∀n∈N,n=0 or some output at index n−1 occurs,\text{(ii)}\quad \forall n\in\mathbb N,\quad n=0\ \text{or some output at index }n-1\text{ occurs},(ii)∀n∈N,n=0 or some output at index n−1 occurs,

where each output is followed by line 11 setting iii to the next index. This records counter values reached inside the while loop, including values that may never appear at a loop entry. Part (ii) excludes the vacuous reading of (i).

Milestones

  1. Lemma 3.4: φ^D^i=φ(Dˉ,τˉ,i)\hat\varphi^{\hat{\mathcal D}_i}=\varphi^{(\bar{\mathcal D},\bar\tau,i)}φ^​D^i​=φ(Dˉ,τˉ,i) once the auxiliary relations of tsub(φ)\mathit{tsub}(\varphi)tsub(φ) are correct, and regularity is preserved.
  2. Lemmas 3.5–3.8: the constructions for ∙I\bullet_I∙I​, ∘I\circ_I∘I​, SI\mathsf S_ISI​ and bounded UI\mathsf U_IUI​ produce regular relations equal to the satisfying sets, with the stated characterizations of rαr_\alpharα​ and sαs_\alphasα​.
  3. Observations (1)–(3) of the proof of Theorem 3.9 on the list QQQ and the counter iii.
  4. The claim that line 7 can always be executed, in the form: if (α,j,∅)∈Qk(\alpha,j,\emptyset)\in Q_k(α,j,∅)∈Qk​ then the build stores pαD^j=α(Dˉ,τˉ,j)p_\alpha^{\hat{\mathcal D}_j}=\alpha^{(\bar{\mathcal D},\bar\tau,j)}pαD^j​​=α(Dˉ,τˉ,j), which is regular.

Significance

Theorem 3.9 makes MΦ\mathsf M_\PhiMΦ​ a sound and complete monitor for the safety fragment □Φ\square\Phi□Φ, Φ\PhiΦ bounded: every violation at every time point is reported, nothing else is, and every output is a finitely represented (regular) set even though it may be infinite. It covers unrestricted negation and quantification, which finite-relation monitors (§4 of the paper) cannot handle. The incremental constructions of §3.4 are the template reused by later MFOTL monitors.

The paper gives a mathematical proof of its monitor's correctness. This mission asks for a Lean proof that checks the MFOTL semantics, automatic relations over N\mathbb NN, and the correctness of this particular monitor, including the until construction whose printed version is defective (see Formalization scope).

Difficulty

Two parts are hard. The regularity claims need the fundamental property of automatic structures: first-order definable relations are regular, which requires closure of padded convolution languages under Boolean operations, cylindrification, permutation of tracks and projection, the last with removal of trailing padding. The arithmetic constraints of the since and until constructions additionally need successor and offset relations definable from ≺\prec≺.

The scheduling argument is the other part. Correctness of a build at (α,j)(\alpha,j)(α,j) requires that every input relation, at time points up to j+ℓjj+\ell_jj+ℓj​ for until, was built before and not discarded since. Following only the syntax of α\alphaα does not settle this: a needed relation for a subformula at a later time point may be built in the same iteration as α\alphaα's.

Formalization scope

The domain is N\mathbb NN, as §3.1 assumes. Relations are sets of lists of natural numbers, ordered by the sorted free variables. Interval upper bounds are in N∞\mathbb N_\inftyN∞​; intervals carry the proof that they are nonempty. The representation (L,ν)(\mathcal L,\nu)(L,ν) is a single parameter shared by the hypothesis "every rDir^{\mathcal D_i}rDi​ is regular" and the regularity claims of the conclusions; it is never chosen existentially. The binary predicate ≺\prec≺ interpreted as <<< is a hypothesis.

Two hypotheses on Φ\PhiΦ besides boundedness are the paper's own "without loss of generality" assumptions: each temporal subformula occurs once in Φ\PhiΦ (§3.6), and the direct subformulas of each SI\mathsf S_ISI​, UI\mathsf U_IUI​ subformula have the same free variables (§3.4; achieved by padding with x≈xx\approx xx≈x, as in §3.5). No other restriction is placed on Φ\PhiΦ.

The printed until construction (§3.4.4) is repaired: the guard of UrU_rUr​ is "aˉ∈β^D^i+k\bar a\in\hat\beta^{\hat{\mathcal D}_{i+k}}aˉ∈β^​D^i+k​ for all ℓi−1≤k≤ℓi\ell_{i-1}\le k\le\ell_iℓi−1​≤k≤ℓi​", since the printed guard empties rαr_\alpharα​ in the paper's own example of §3.5; UsU_sUs​ keeps only tuples with j′≥1j'\ge1j′≥1, since otherwise a γ\gammaγ-witness at time point i−1i-1i−1 survives to time point iii when τi=τi−1\tau_i=\tau_{i-1}τi​=τi−1​; and time-stamp equations are encoded additively. Lemma 3.8(i) reads aˉ∈Nn\bar a\in\mathbb N^naˉ∈Nn and adds j≤ℓij\le\ell_ij≤ℓi​. "Effectively computable" in Theorem 3.9(i) is not formalized. Part (ii) uses the output at index n−1n-1n−1 as the record of the line-11 increment to nnn; for n=0n=0n=0, the counter is initialized by line 2. Loop-entry states alone can skip counter values reached within one iteration.

The monitor is a state machine whose builds and outputs are computed only from its store of relations; it never consults the satisfaction relation or satisfying sets. A formalization in which line 7 reads the semantics would turn Theorem 3.9(i) into a restatement of Lemma 3.4, and is ruled out. A build whose input is missing stores nothing, so a monitor that silently fails would violate (ii).

Contributions welcome: the theory of automatic relations (reusable beyond this mission), the semantic halves of Lemmas 3.4–3.8, and the scheduling invariants.

Selected references

  • D. Basin, F. Klaedtke, S. Müller, E. Zălinescu, Monitoring metric first-order temporal properties, J. ACM 62(2), Article 15, 2015. https://doi.org/10.1145/2699444
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Markov ChainMathematical PhysicsProbability·Captain: mikedeng1

The Endpoint Distribution of Directed Polymers 1: In the Low-Temperature Phase the Endpoint Distribution Is Asymptotically Purely Atomic, and at High Temperature It Is NotResearch Paper

Motivation

A directed polymer in a random environment is a random walk whose paths are weighted by the disorder they encounter. The walk favors paths with large accumulated weight, and its endpoint distribution can concentrate on a small number of sites even though the number of possible paths grows exponentially. Understanding how much probability remains spread across many small endpoint masses is a basic question about localization. The distinction matters especially beyond exactly solvable polymer models, where explicit formulas for the endpoint law are rarely available. Bates and Chatterjee study this question for independent disorder in every spatial dimension d≥1d\geq1d≥1 under a finite exponential-moment condition Bates and Chatterjee, 2021.

The paper separates two temperature regimes using the limiting free energy. Earlier localization statements detected persistent large atoms. The target here asks whether those atoms account for all endpoint probability in a time-averaged sense. It also specifies the complementary high-temperature behavior, where a suitable vanishing mass threshold captures asymptotically none of the probability. The result is Theorem 1.1 of the preprint, restated as Theorem 6.3 Bates and Chatterjee, 2021, pp. 16, 43.

Setting

Fix d≥1d\geq1d≥1. A path starts at the origin in Zd\mathbb Z^dZd and makes one of its 2d2d2d nearest-neighbor moves at each integer time. The environment (Xi,x)(X_{i,x})(Xi,x​) consists of independent, identically distributed real random variables with common law L\mathfrak LL. The disorder law is nondegenerate: it is not concentrated at one number. An inverse temperature β≥0\beta\geq0β≥0 determines the weight of a path γ\gammaγ of length nnn:

wβ(γ)=exp⁡ ⁣(β∑i=1nXi,γ(i)),Zn=(2d)−n∑γwβ(γ).w_\beta(\gamma)=\exp\!\left(\beta\sum_{i=1}^{n}X_{i,\gamma(i)}\right),\qquad Z_n=(2d)^{-n}\sum_{\gamma}w_\beta(\gamma).wβ​(γ)=exp(βi=1∑n​Xi,γ(i)​),Zn​=(2d)−nγ∑​wβ​(γ).

The endpoint mass function fn(x)f_n(x)fn​(x) is the sum of weights of paths ending at xxx, divided by the sum of all path weights. Thus fnf_nfn​ is a probability mass function on Zd\mathbb Z^dZd. For ε>0\varepsilon>0ε>0, the ε\varepsilonε-atoms are the sites Anε={x:fn(x)>ε}\mathcal A_n^\varepsilon=\{x:f_n(x)>\varepsilon\}Anε​={x:fn​(x)>ε}, and ρn(ωn∈Anε)\rho_n(\omega_n\in\mathcal A_n^\varepsilon)ρn​(ωn​∈Anε​) is their total mass. The strict inequality matters at a threshold equal to an atom mass.

Write Fn=log⁡Zn/nF_n=\log Z_n/nFn​=logZn​/n for n≥1n\geq1n≥1, with F0=0F_0=0F0​=0, and λ(α)=log⁡ELeαX\lambda(\alpha)=\log\mathbb E_{\mathfrak L}e^{\alpha X}λ(α)=logEL​eαX. The standing condition is that this exponential moment is finite for every α∈[−2β,2β]\alpha\in[-2\beta,2\beta]α∈[−2β,2β]. The paper's Theorem A characterizes the high-temperature phase by lim⁡nEFn=λ(β)\lim_n\mathbb E F_n=\lambda(\beta)limn​EFn​=λ(β) and the low-temperature phase by lim⁡nEFn<λ(β)\lim_n\mathbb E F_n<\lambda(\beta)limn​EFn​<λ(β) Bates and Chatterjee, 2021, pp. 4–5.

Formalization targets

Asymptotic pure atomicity

The goal is both clauses of Theorem 1.1. For every positive deterministic sequence εi→0\varepsilon_i\to0εi​→0, low temperature gives

1n∑i=0n−1ρi(ωi∈Aiεi)⟶1almost surely.\frac1n\sum_{i=0}^{n-1}\rho_i(\omega_i\in\mathcal A_i^{\varepsilon_i})\longrightarrow1 \quad\text{almost surely}.n1​i=0∑n−1​ρi​(ωi​∈Aiεi​​)⟶1almost surely.

At high temperature there exists a positive deterministic sequence εi→0\varepsilon_i\to0εi​→0 for which the same average converges almost surely to 000. The sequence in this second clause is selected independently of the realized environment. Together the clauses characterize the paper's stronger, almost-sure form of asymptotic pure atomicity Bates and Chatterjee, 2021, Theorems 1.1 and 6.3.

The milestones are fifteen statements of the paper, in the order the proof of the goal uses them:

  • the triangle inequality for the distance ddd on partitioned subprobability measures (Lemma 2.3) and sequential compactness of (S,d)(\mathcal S,d)(S,d) (Theorem 2.8);
  • continuity of the update law f↦Tff\mapsto\mathcal Tff↦Tf into (P(S),W)(\mathcal P(\mathcal S),\mathcal W)(P(S),W) and of the log moments f↦Elog⁡qF~f\mapsto\mathbb E\log^q\widetilde Ff↦ElogqF (Proposition 3.2);
  • convergence of the empirical endpoint measures μn=1n∑i<nδfi\mu_n=\frac1n\sum_{i<n}\delta_{f_i}μn​=n1​∑i<n​δfi​​ to the fixed-point set K\mathcal KK (Corollary 4.3); invariant laws charge only states of mass 000 or 111 (Proposition 4.4);
  • the variational formula for the free energy: ∣Fn−R(μn)∣→0|F_n-\mathcal R(\mu_n)|\to0∣Fn​−R(μn​)∣→0 (Proposition 4.5), the lower bound (Proposition 4.6), the key inequality ∑i<nR(Tiδf0)≥Elog⁡Zn\sum_{i<n}\mathcal R(\mathcal T^i\delta_{f_0})\ge\mathbb E\log Z_n∑i<n​R(Tiδf0​​)≥ElogZn​ (Lemma 4.8), and lim⁡Fn=inf⁡ν∈KR(ν)\lim F_n=\inf_{\nu\in\mathcal K}\mathcal R(\nu)limFn​=infν∈K​R(ν) (Theorem 4.7);
  • convergence of μn\mu_nμn​ to the minimizing set M\mathcal MM (Theorem 4.9), the extrema of RRR (Lemma 5.1) and the fixed-point characterization of the two phases (Theorem 5.2);
  • semicontinuity of the atom functionals (Lemma 6.1), a fixed-threshold criterion for pure atomicity (Lemma 6.2), and a Dini theorem for semicontinuous functions (Lemma 6.4).

Significance

The low-temperature conclusion rules out a residual diffuse component in the time-averaged endpoint law. A vanishing threshold may still be used to collect almost all of the polymer's probability. The high-temperature clause shows that this property distinguishes the phases under the stated moment assumption. The result strengthens a statement that only asks for a positive amount of mass on large atoms, and gives an almost-sure conclusion for the Cesàro averages Bates and Chatterjee, 2021, §§1.2.3, 6.

A formal development would supply a reusable compactification of endpoint probability measures and a checked route from its invariant laws to localization observables. The milestones expose the pieces that need separate verification, and the compactification and variational formula are reusable for the companion mission on geometric localization. The paper proves the mathematical theorem; this mission asks for its Lean proof and the supporting definitions. A compiled statement with sorry is a proof obligation, not a completed machine-checked result.

Difficulty

The endpoint distribution may move through space as time grows, so ordinary pointwise convergence of mass functions does not capture concentration. The compact state space used by the paper permits separated clusters to live on different copies of Zd\mathbb Z^dZd. Its distance identifies translated representatives and loses information about remote mass. A direct application of weak convergence to the event f(x)>εf(x)>\varepsilonf(x)>ε also fails at a threshold, because the mass-above-threshold functional is not continuous. The proof must handle its one-sided semicontinuity and the limiting behavior of the update law Bates and Chatterjee, 2021, §§2–3, 6.

Formalization scope

Lean represents sites as Fin d → ℤ and paths as finite step sequences, so the starting point, the 2d2d2d choices per step, and the normalization of ZnZ_nZn​ are explicit. An environment is a measurable independent family on a probability space with common law L\mathfrak LL. The unused time-zero row comes from indexing cells by N\mathbb NN; only rows with index at least one enter the polymer. The moment condition includes the full interval [−2β,2β][-2\beta,2\beta][−2β,2β], and the disorder law must be nondegenerate. Both phase predicates refer to the canonical product environment, making the classification depend on L\mathfrak LL, ddd, and β\betaβ rather than on an arbitrary realization.

Partitioned subprobability measures are structures of nonnegative summable functions with mass at most one. Their topology is generated by the paper's distance balls. The Borel representation identifies states at distance zero, corresponding to the paper's separation quotient S\mathcal SS. Finite partial isometries carry the degree penalty 2−deg⁡φ2^{-\deg\varphi}2−degφ through an infimum over admissible degrees. The update uses an extended nonnegative sum before conversion to a real denominator. The intended probability law requires the almost-sure finiteness of that denominator and measurability of the update. The real-valued energy integrals require the stated moment condition; a default value for a nonintegrable integral cannot serve as the paper's expectation, and a non-measurable update would make the pushforward Tf\mathcal TfTf the zero measure, which is not the paper's object either. The infimum inf⁡ν∈KR(ν)\inf_{\nu\in\mathcal K}\mathcal R(\nu)infν∈K​R(ν) is taken over the set K\mathcal KK itself, never as a real infimum whose empty inner range defaults to 000. The intermediate results in §§3–4 and Lemma 5.1 use the standing β>0\beta>0β>0 range. Theorems 1.1 and 5.2 explicitly include β=0\beta=0β=0. Wasserstein cost imports the published RWPI.SqrtLasso.transportCost definition.

Solvers can contribute proofs of the compactness, continuity, variational-formula, invariant-law, and atom-functional milestones, or of reusable supporting results such as Lemma 2.11 (measurability of the update) and Corollary 2.5 (when d(f,g)=0d(f,g)=0d(f,g)=0). The strict positivity of thresholds, nondegenerate disorder, genuine probability laws, and full phase hypotheses are essential: removing any of them could make a formally easy statement unrelated to Theorem 1.1.

Selected references

  • Erik Bates and Sourav Chatterjee, The endpoint distribution of directed polymers, Annals of Probability 48 (2020); preprint arXiv:1612.03443v5 (2021). Preprint.
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Distribution-Free, Risk-Controlling Prediction Sets III: Thresholding the Conditional Expected Loss Gives the Smallest Sets Among Predictors of No Larger Risk (Theorem 8)Research Paper

Motivation

A set-valued predictor returns, for each input xxx, a set of plausible responses rather than a single guess. Such sets are used wherever a model's output feeds a decision with asymmetric costs: a medical classifier that lists every diagnosis it cannot rule out, a segmentation model that marks every pixel that may belong to a tumour, a protein-structure predictor that reports a range of distances. Bates, Angelopoulos, Lei, Malik and Jordan, Distribution-Free, Risk-Controlling Prediction Sets (J. ACM 68(6), 2021), calibrate a nested family of such predictors {Tλ}\{\mathcal T_\lambda\}{Tλ​} so that a chosen loss is controlled with high probability, without distributional assumptions.

Calibration says nothing about which family to calibrate. Any nested family can be made risk-controlling; families differ in how large their sets are, and large sets are uninformative. §4 of the paper asks which family is best in the population: which predictor achieves a given risk with the smallest expected set size. For a weighted miscoverage loss (Theorem 7, §4.2) the answer thresholds a weighted conditional density, in the spirit of the optimality results of Sadinle, Lei and Wasserman (2019) for classification. Theorem 8 (§4.3) extends the answer to every loss of integral form. This mission formalizes Theorem 8.

Setting

Let (X,Y)(X, Y)(X,Y) take values in X×Y\mathcal X \times \mathcal YX×Y with law PPP, marginal PXP_XPX​, and conditional law κ(x)\kappa(x)κ(x) of YYY given X=xX = xX=x. Prediction sets are subsets of a measurable space Z\mathcal ZZ (in the paper's examples Z=Y\mathcal Z = \mathcal YZ=Y). A set-valued predictor is a map T:X→2Z\mathcal T : \mathcal X \to 2^{\mathcal Z}T:X→2Z.

Fix a finite measure μ\muμ on Z\mathcal ZZ and a nonnegative cost ℓ:Y×Z→[0,∞)\ell : \mathcal Y \times \mathcal Z \to [0, \infty)ℓ:Y×Z→[0,∞); ℓ(y,z)\ell(y, z)ℓ(y,z) is the cost of leaving zzz out of the prediction set when the true response is yyy. The loss of a set S\mathcal SS is the total cost of what it leaves out,

L(y;S)=∫z∈Scℓ(y,z) dμ(z),L(y; \mathcal S) = \int_{z \in \mathcal S^c} \ell(y, z)\, d\mu(z),L(y;S)=∫z∈Sc​ℓ(y,z)dμ(z),

and the risk of a predictor is R(T)=E[L(Y;T(X))]R(\mathcal T) = \mathbb E[L(Y; \mathcal T(X))]R(T)=E[L(Y;T(X))] (§2.1). Larger sets have smaller loss. The conditional expected cost of omitting zzz at xxx is

E[ℓ(Y;z)∣X=x]=∫ℓ(y,z) dκ(x)(y),\mathbb E[\ell(Y; z) \mid X = x] = \int \ell(y, z)\, d\kappa(x)(y),E[ℓ(Y;z)∣X=x]=∫ℓ(y,z)dκ(x)(y),

and for λ<0\lambda < 0λ<0 the threshold predictor of display (11) is

Tλ(x)={z∈Z:E[ℓ(Y;z)∣X=x]≥−λ}.\mathcal T_\lambda(x) = \{z \in \mathcal Z : \mathbb E[\ell(Y; z) \mid X = x] \ge -\lambda\}.Tλ​(x)={z∈Z:E[ℓ(Y;z)∣X=x]≥−λ}.

It includes exactly the points whose omission is expected to cost at least −λ-\lambda−λ. The size of a set is its μ\muμ-measure, ∣S∣=μ(S)|\mathcal S| = \mu(\mathcal S)∣S∣=μ(S), and the expected size of a predictor is E[∣T(X)∣]=∫μ(T(x)) dPX(x)\mathbb E[|\mathcal T(X)|] = \int \mu(\mathcal T(x))\, dP_X(x)E[∣T(X)∣]=∫μ(T(x))dPX​(x).

In Lean: setLoss μ ℓ y S, risk P μ ℓ T, condLoss κ ℓ x z, thresholdSet κ ℓ lam x and expSize P μ T in the namespace RiskControl.Optimal.

Formalization targets

Goal: Theorem 8

For every λ<0\lambda < 0λ<0 and every set-valued predictor T′\mathcal T'T′ (with measurable graph),

R(T′)≤R(Tλ)  ⟹  E[∣Tλ(X)∣]≤E[∣T′(X)∣].R(\mathcal T') \le R(\mathcal T_\lambda) \implies \mathbb E\big[|\mathcal T_\lambda(X)|\big] \le \mathbb E\big[|\mathcal T'(X)|\big].R(T′)≤R(Tλ​)⟹E[∣Tλ​(X)∣]≤E[∣T′(X)∣].

No constant is involved; the statement is uniform over ℓ\ellℓ, μ\muμ, PPP and T′\mathcal T'T′.

Milestones: the steps of the proof (p. 27)

  1. Moving the conditional expectation inside the μ\muμ-integral: for a predictor A\mathcal AA with measurable graph, E[∫A(X)ℓ(Y;z) dμ(z)]=E[∫A(X)E[ℓ(Y;z)∣X] dμ(z)]\mathbb E[\int_{\mathcal A(X)} \ell(Y; z)\, d\mu(z)] = \mathbb E[\int_{\mathcal A(X)} \mathbb E[\ell(Y; z) \mid X]\, d\mu(z)]E[∫A(X)​ℓ(Y;z)dμ(z)]=E[∫A(X)​E[ℓ(Y;z)∣X]dμ(z)].
  2. From the risk comparison to the set differences:
E[∫T′(X)∖Tλ(X)E[ℓ(Y;z)∣X] dμ]≥E[∫Tλ(X)∖T′(X)E[ℓ(Y;z)∣X] dμ].\mathbb E\Big[\int_{\mathcal T'(X) \setminus \mathcal T_\lambda(X)} \mathbb E[\ell(Y; z) \mid X]\, d\mu\Big] \ge \mathbb E\Big[\int_{\mathcal T_\lambda(X) \setminus \mathcal T'(X)} \mathbb E[\ell(Y; z) \mid X]\, d\mu\Big].E[∫T′(X)∖Tλ​(X)​E[ℓ(Y;z)∣X]dμ]≥E[∫Tλ​(X)∖T′(X)​E[ℓ(Y;z)∣X]dμ].
  1. From costs to sizes: E∣T′(X)∖Tλ(X)∣≥E∣Tλ(X)∖T′(X)∣\mathbb E|\mathcal T'(X) \setminus \mathcal T_\lambda(X)| \ge \mathbb E|\mathcal T_\lambda(X) \setminus \mathcal T'(X)|E∣T′(X)∖Tλ​(X)∣≥E∣Tλ​(X)∖T′(X)∣.
  2. From set differences to sets: E∣A(X)∖B(X)∣≤E∣B(X)∖A(X)∣\mathbb E|\mathcal A(X) \setminus \mathcal B(X)| \le \mathbb E|\mathcal B(X) \setminus \mathcal A(X)|E∣A(X)∖B(X)∣≤E∣B(X)∖A(X)∣ implies E∣A(X)∣≤E∣B(X)∣\mathbb E|\mathcal A(X)| \le \mathbb E|\mathcal B(X)|E∣A(X)∣≤E∣B(X)∣.

Significance

The result. Theorem 8 identifies the population-optimal shape of a set-valued predictor for every loss that charges for omitted points through a nonnegative cost and a finite measure. It justifies building nested families by thresholding an estimate of the conditional expected cost: if the estimate were exact, no other predictor with the same or smaller risk could have smaller sets on average. It contains the weighted-miscoverage case (Theorem 7) when Y\mathcal YY is discrete and μ\muμ is counting measure, and it covers losses for which no such special case exists, such as costs that depend on the distance between zzz and yyy.

Formalizing it. The proof on p. 27 is a chain of eight displays. A machine-checked version settles the measure-theoretic points the chain passes over: the conditional expectation inside an integral over a random set, the cancellation of possibly infinite terms, and the range of λ\lambdaλ. To our knowledge no formal proof of Theorem 8 or of the Neyman–Pearson-type optimality results it generalizes for set predictors exists in Lean or Mathlib.

Difficulty

The natural reading of the proof subtracts the quantity E∫ZE[ℓ(Y;z)∣X] dμ(z)\mathbb E\int_{\mathcal Z} \mathbb E[\ell(Y; z) \mid X]\, d\mu(z)E∫Z​E[ℓ(Y;z)∣X]dμ(z) from both sides of the risk comparison to pass from complements to sets. Nothing in the setting makes this quantity finite, so that step is not valid as written, and a proof that follows the displays literally breaks there. The theorem itself does not need finiteness of ℓ\ellℓ, and no such hypothesis is in scope.

The other obstacle is measure-theoretic bookkeeping. The conditional expectation E[ℓ(Y;z)∣X]\mathbb E[\ell(Y; z) \mid X]E[ℓ(Y;z)∣X] is indexed by a point zzz of a second space, and must be a jointly measurable function of (x,z)(x, z)(x,z) before it can be integrated over the random set T(X)\mathcal T(X)T(X); here it is given by a regular conditional distribution, and every integral over T(x)\mathcal T(x)T(x) needs the measurability of the graph of T\mathcal TT.

Formalization scope

  • Spaces and measures. X,Y,Z\mathcal X, \mathcal Y, \mathcal ZX,Y,Z are arbitrary measurable spaces; PPP is a probability measure on X×Y\mathcal X \times \mathcal YX×Y; μ\muμ is a finite measure on Z\mathcal ZZ; ℓ\ellℓ takes values in [0,∞)[0, \infty)[0,∞) and is jointly measurable.
  • Conditional law. E[ℓ(Y;z)∣X=x]\mathbb E[\ell(Y; z) \mid X = x]E[ℓ(Y;z)∣X=x] is ∫ℓ(y,z) dκ(x)(y)\int \ell(y, z)\, d\kappa(x)(y)∫ℓ(y,z)dκ(x)(y) for a Markov kernel κ\kappaκ with P=PX⊗κP = P_X \otimes \kappaP=PX​⊗κ, which is exactly the statement that κ\kappaκ is a regular conditional distribution of YYY given XXX. Such a kernel exists, for instance, when Y\mathcal YY is standard Borel; the formalization does not assume this. The threshold predictor is built from the same κ\kappaκ and the same ℓ\ellℓ as the risk; neither is a free object.
  • Integrals. Every integral is a lower Lebesgue integral with values in [0,∞][0, \infty][0,∞]; no integrability hypothesis is made, and an infinite risk is +∞+\infty+∞.
  • Range of λ\lambdaλ (correction of the print). The paper states Theorem 8 for λ∈Λ⊂(−∞,0]\lambda \in \Lambda \subset (-\infty, 0]λ∈Λ⊂(−∞,0]. At λ=0\lambda = 0λ=0 it is false: with ℓ≡0\ell \equiv 0ℓ≡0 and μ(Z)>0\mu(\mathcal Z) > 0μ(Z)>0, T0(x)=Z\mathcal T_0(x) = \mathcal ZT0​(x)=Z and T′≡∅\mathcal T' \equiv \emptysetT′≡∅ both have risk 000, but E∣T′(X)∣=0<μ(Z)\mathbb E|\mathcal T'(X)| = 0 < \mu(\mathcal Z)E∣T′(X)∣=0<μ(Z). The proof divides by −λ-\lambda−λ. Theorem 8 and its milestones are posed for λ<0\lambda < 0λ<0.
  • Set size (correction of the print). p. 13 describes ∣⋅∣|\cdot|∣⋅∣ as Lebesgue or counting measure, a sentence written for Theorem 7. In Theorem 8 the proof measures sets with the measure μ\muμ of the loss, and ∣⋅∣=μ|\cdot| = \mu∣⋅∣=μ throughout.
  • Measurable graphs. The competing predictor T′\mathcal T'T′ is required to have a measurable graph {(x,z):z∈T′(x)}\{(x, z) : z \in \mathcal T'(x)\}{(x,z):z∈T′(x)}; otherwise its risk and expected size are not integrals of measurable functions. The page leaves this implicit. The graph of Tλ\mathcal T_\lambdaTλ​ is measurable by construction.
  • Not a trivialization. The goal is stated about the threshold sets (11) built from the given ℓ\ellℓ, μ\muμ and κ\kappaκ, for every competing predictor; it does not assume any of the intermediate inequalities, and its hypotheses are satisfiable (for instance ℓ≡1\ell \equiv 1ℓ≡1, λ=−1/2\lambda = -1/2λ=−1/2, where Tλ(x)=Z\mathcal T_\lambda(x) = \mathcal ZTλ​(x)=Z).

The development needs Mathlib's composition of a measure with a kernel, Tonelli's theorem for kernels and lower integrals over sections of a measurable set. Lemmas about expected μ\muμ-sizes of random sets (milestone 4) and about moving a kernel integral inside a set integral (milestone 1) are reusable beyond this mission. Proofs of the milestones, and of the goal by other routes, are welcome.

Selected references

  • S. Bates, A. Angelopoulos, L. Lei, J. Malik, M. I. Jordan, Distribution-Free, Risk-Controlling Prediction Sets, Journal of the ACM 68(6), 2021. arXiv:2101.02703v3. https://arxiv.org/abs/2101.02703 — Theorem 8, p. 13; proof p. 27.
  • M. Sadinle, J. Lei, L. Wasserman, Least Ambiguous Set-Valued Classifiers With Bounded Error Levels, Journal of the American Statistical Association 114(525), 2019. https://doi.org/10.1080/01621459.2017.1395341
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Machine LearningProbabilityStatistics·Captain: mikedeng1

Distribution-Free, Risk-Controlling Prediction Sets I: Upper Confidence Bound Calibration Selects a λ̂ Whose Risk Is at Most α with Probability at Least 1 − δ (Theorem 1)Research Paper

Motivation

A trained classifier or regressor returns a point prediction, but many uses of machine learning need a prediction set: a set of plausible labels together with a guarantee about how often, or how badly, it misses the truth. Medical imaging, protein structure prediction and multi-label classification are examples where a user wants a set whose expected loss is bounded, not just a best guess. Bates, Angelopoulos, Lei, Malik and Jordan (arXiv:2101.02703, J. ACM 68(6), 2021) give a procedure that wraps any black-box predictor and returns sets whose risk is controlled, with no assumption on the data distribution beyond i.i.d. calibration data.

The procedure generalizes split conformal prediction (Vovk, Gammerman and Shafer, 2005) and the tolerance regions of Wilks (1941), which control only the probability of missing the label, to an arbitrary monotone loss on sets (false-negative rate, coverage of a segmentation mask, a hierarchical loss). This mission formalizes its central guarantee, Theorem 1 (p. 5), together with the abstract form Theorem A.1 (p. 26) from which the paper derives it.

Setting

Let (X,Y)(X, Y)(X,Y) be a random pair in X×Y\mathcal X \times \mathcal YX×Y with law PPP, and let Z\mathcal ZZ be a set of labels. A set-valued predictor is a map T:X→2Z\mathcal T : \mathcal X \to 2^{\mathcal Z}T:X→2Z. The paper considers a family {Tλ}λ∈Λ\{\mathcal T_\lambda\}_{\lambda \in \Lambda}{Tλ​}λ∈Λ​ indexed by a closed set Λ⊆R∪{±∞}\Lambda \subseteq \mathbb R \cup \{\pm\infty\}Λ⊆R∪{±∞} that is nested:

λ1<λ2  ⟹  Tλ1(x)⊆Tλ2(x).(1)\lambda_1 < \lambda_2 \implies \mathcal T_{\lambda_1}(x) \subseteq \mathcal T_{\lambda_2}(x). \tag{1}λ1​<λ2​⟹Tλ1​​(x)⊆Tλ2​​(x).(1)

A loss on sets L(y,S)≥0L(y, S) \ge 0L(y,S)≥0 is required to decrease as the set grows:

S⊆S′  ⟹  L(y,S)≥L(y,S′).(2)S \subseteq S' \implies L(y, S) \ge L(y, S'). \tag{2}S⊆S′⟹L(y,S)≥L(y,S′).(2)

The risk of Tλ\mathcal T_\lambdaTλ​ is R(λ)=E[L(Y,Tλ(X))]R(\lambda) = \mathbb E[L(Y, \mathcal T_\lambda(X))]R(λ)=E[L(Y,Tλ​(X))], and the section assumes some λmax⁡∈Λ\lambda_{\max} \in \Lambdaλmax​∈Λ with R(λmax⁡)=0R(\lambda_{\max}) = 0R(λmax​)=0.

A risk-controlling prediction set at levels (α,δ)(\alpha, \delta)(α,δ) (Definition 1, p. 2) is a data-dependent predictor T\mathcal TT with R(T)≤αR(\mathcal T) \le \alphaR(T)≤α with probability at least 1−δ1 - \delta1−δ.

Given an i.i.d. calibration sample D=((X1,Y1),…,(Xn,Yn))D = ((X_1, Y_1), \dots, (X_n, Y_n))D=((X1​,Y1​),…,(Xn​,Yn​)), a pointwise upper confidence bound is a function R^+(λ)=R^+(D,λ)\widehat R^+(\lambda) = \widehat R^+(D, \lambda)R+(λ)=R+(D,λ) with

P(R(λ)≤R^+(λ))≥1−δfor each fixed λ.(3)P\big(R(\lambda) \le \widehat R^+(\lambda)\big) \ge 1 - \delta \quad \text{for each fixed } \lambda. \tag{3}P(R(λ)≤R+(λ))≥1−δfor each fixed λ.(3)

UCB calibration selects

λ^=inf⁡{λ∈Λ:R^+(λ′)<α  ∀λ′∈Λ, λ′≥λ}.(4)\hat\lambda = \inf\big\{\lambda \in \Lambda : \widehat R^+(\lambda') < \alpha \ \ \forall \lambda' \in \Lambda,\ \lambda' \ge \lambda\big\}. \tag{4}λ^=inf{λ∈Λ:R+(λ′)<α  ∀λ′∈Λ, λ′≥λ}.(4)

In Lean, the risk is RiskControl.UCB.risk P L T lam, the calibration set of (4) for one realization r of R^+\widehat R^+R+ is calSet Λ r α, and λ^\hat\lambdaλ^ is lambdaHat Λ r α.

Formalization targets

Goal: Theorem 1 (p. 5)

In the setting above, if (3) holds for every λ∈Λ\lambda \in \Lambdaλ∈Λ and RRR is continuous on Λ\LambdaΛ, then

Pn(R(Tλ^)≤α)≥1−δ.P^n\big(R(\mathcal T_{\hat\lambda}) \le \alpha\big) \ge 1 - \delta .Pn(R(Tλ^​)≤α)≥1−δ.

Nothing is assumed of R^+\widehat R^+R+ beyond (3); α\alphaα and δ\deltaδ are arbitrary reals.

Milestones

  1. Monotone risk (§2.1, pp. 4–5): (1) and (2) make RRR nonincreasing on Λ\LambdaΛ.
  2. The failure point (proof of Theorem A.1, p. 26, corrected): λ†=sup⁡{λ∈Λ:R(λ)>α}\lambda^\dagger = \sup\{\lambda \in \Lambda : R(\lambda) > \alpha\}λ†=sup{λ∈Λ:R(λ)>α} lies in Λ\LambdaΛ and R(λ†)≥αR(\lambda^\dagger) \ge \alphaR(λ†)≥α.
  3. Failure implies a low bound at λ†\lambda^\daggerλ† (p. 26, corrected): deterministically, R(λ^)>αR(\hat\lambda) > \alphaR(λ^)>α implies R^+(λ†)<α\widehat R^+(\lambda^\dagger) < \alphaR+(λ†)<α.
  4. Theorem A.1 (p. 26): for any continuous nonincreasing R:Λ→RR : \Lambda \to \mathbb RR:Λ→R and any R^+\widehat R^+R+ satisfying (3) on an abstract probability space, P(R(λ^)≤α)≥1−δP(R(\hat\lambda) \le \alpha) \ge 1 - \deltaP(R(λ^)≤α)≥1−δ.

Significance

Theorem 1 turns a confidence bound for one fixed parameter into a guarantee for a parameter chosen from the data. No uniform convergence over Λ\LambdaΛ is needed, so any concentration inequality for a mean (Hoeffding, Bentkus, the betting bound of Waudby-Smith and Ramdas) yields a calibration procedure immediately; the paper's Theorems 2–5 and 9–10 are of exactly this form, and the later Learn-then-Test and conformal risk control frameworks build on the same template.

The result is proved in the paper; nothing here is open. What the mission adds is a machine-checked version of an argument whose printed form has a gap. The printed proof of Theorem A.1 introduces λ∗=inf⁡{λ∈Λ:R(λ)≤α}\lambda^* = \inf\{\lambda \in \Lambda : R(\lambda) \le \alpha\}λ∗=inf{λ∈Λ:R(λ)≤α} and asserts R(λ∗)=αR(\lambda^*) = \alphaR(λ∗)=α "by continuity", which is false when Λ\LambdaΛ is not an interval. Finite grids, the usual choice of Λ\LambdaΛ in practice, are not intervals. The theorem remains true, and milestones 2 and 3 state the corrected steps. No formalization of risk-controlling prediction sets or of conformal prediction is known to exist in Lean or on this platform.

Difficulty

The obvious argument applies the confidence bound at λ^\hat\lambdaλ^; that fails because λ^\hat\lambdaλ^ depends on the data, so (3) says nothing at λ=λ^\lambda = \hat\lambdaλ=λ^. The proof must find one deterministic point at which a failure of calibration forces a failure of (3). The paper's choice λ∗\lambda^*λ∗ works only when RRR attains the value α\alphaα on Λ\LambdaΛ; on Λ={0,1}\Lambda = \{0, 1\}Λ={0,1} with R(0)=1R(0) = 1R(0)=1, R(1)=0R(1) = 0R(1)=0, α=1/2\alpha = 1/2α=1/2 and the exact bound R^+=R\widehat R^+ = RR+=R, the event {R^+(λ∗)<α}\{\widehat R^+(\lambda^*) < \alpha\}{R+(λ∗)<α} has probability one, so the printed last step does not bound anything. The second difficulty is boundary behaviour: Λ\LambdaΛ may contain ±∞\pm\infty±∞, the infimum in (4) may be over an empty set, and the calibration set need not contain its own infimum.

Formalization scope

  • Λ\LambdaΛ is a closed subset of EReal (the extended reals with the order topology); λ\lambdaλ is only compared, never added. Continuity of RRR is in the subspace topology of Λ\LambdaΛ.
  • Set-valued predictions are Set 𝒵, i.e. Y′=2Z\mathcal Y' = 2^{\mathcal Z}Y′=2Z (the paper uses 2Y2^{\mathcal Y}2Y for most of its examples).
  • The risk is the published definition WassersteinDRO.Duality.nominalRisk, a Bochner integral. Because a non-integrable integrand integrates to 000 in Lean, Theorem 1 assumes (x,y)↦L(y,Tλ(x))(x, y) \mapsto L(y, \mathcal T_\lambda(x))(x,y)↦L(y,Tλ​(x)) is PPP-integrable for every λ∈Λ\lambda \in \Lambdaλ∈Λ.
  • The standing assumptions of §2.1 are hypotheses of Theorem 1: Λ\LambdaΛ closed, (1) on Λ\LambdaΛ, (2), L≥0L \ge 0L≥0, and R(λmax⁡)=0R(\lambda_{\max}) = 0R(λmax​)=0 for some λmax⁡∈Λ\lambda_{\max} \in \Lambdaλmax​∈Λ. The monotonicity of RRR is not assumed in Theorem 1; it is milestone 1. Theorem A.1 assumes it, as printed.
  • The i.i.d. sample is Fin n → 𝒳 × 𝒴 under the product measure PnP^nPn. R^+\widehat R^+R+ is an arbitrary real function of the sample and of λ\lambdaλ; an infinite bound is represented by any value ≥α\ge \alpha≥α.
  • "With probability at least 1−δ1 - \delta1−δ" is written as a failure probability at most δ\deltaδ, measured as an outer measure; no measurability of R^+\widehat R^+R+ or λ^\hat\lambdaλ^ is assumed. For a measurable event this is the page's statement.
  • λ^\hat\lambdaλ^ is an infimum in EReal, so inf⁡∅=+∞\inf \emptyset = +\inftyinf∅=+∞ as on the page. Since +∞+\infty+∞ need not belong to Λ\LambdaΛ, the failure event is "the set in (4) is nonempty and R(λ^)>αR(\hat\lambda) > \alphaR(λ^)>α"; when the set is nonempty, λ^∈Λ\hat\lambda \in \Lambdaλ^∈Λ. When it is empty the procedure certifies nothing, and the natural output is Tλmax⁡\mathcal T_{\lambda_{\max}}Tλmax​​, of risk 000.
  • Corrections of the print: Theorem A.1's conclusion reads P(R(λ)≤α)P(R(\lambda) \le \alpha)P(R(λ)≤α), stated here with λ^\hat\lambdaλ^; the proof's point λ∗\lambda^*λ∗ and the claim R(λ∗)=αR(\lambda^*) = \alphaR(λ∗)=α are replaced by λ†=sup⁡{λ∈Λ:R(λ)>α}\lambda^\dagger = \sup\{\lambda \in \Lambda : R(\lambda) > \alpha\}λ†=sup{λ∈Λ:R(λ)>α} and R(λ†)≥αR(\lambda^\dagger) \ge \alphaR(λ†)≥α, which coincide with the page for an interval Λ\LambdaΛ.
  • A formalization that assumes RRR monotone in Theorem 1, quantifies over R^+\widehat R^+R+ inside the event, takes a real-valued infimum (which is 000 on unbounded sets) or drops the integrability guard would state a different theorem; the statement here does none of these.

Needed infrastructure is small: closed subsets of EReal and their infima and suprema (IsClosed.sInf_mem, IsClosed.sSup_mem), continuity within a set, monotonicity of the Bochner integral, and monotonicity of outer measure. Proofs of the milestones are welcome individually; the deterministic milestones 2 and 3 are reusable for every UCB-calibration theorem of the paper.

Selected references

  • S. Bates, A. Angelopoulos, L. Lei, J. Malik, M. I. Jordan, Distribution-Free, Risk-Controlling Prediction Sets, J. ACM 68(6), 2021; arXiv:2101.02703v3. https://arxiv.org/abs/2101.02703
  • V. Vovk, A. Gammerman, G. Shafer, Algorithmic Learning in a Random World, Springer, 2005. https://doi.org/10.1007/b106715
  • S. S. Wilks, Determination of sample sizes for setting tolerance limits, Ann. Math. Statist. 12(1), 1941. https://doi.org/10.1214/aoms/1177731788
  • I. Waudby-Smith, A. Ramdas, Estimating means of bounded random variables by betting, arXiv:2010.09686, 2020. https://arxiv.org/abs/2010.09686
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CombinatoricsGraph Theory·Captain: mikedeng1

Turán Graphs with Bounded Matching Number 2: For Color-Critical H of Chromatic Number k+1 > 2, Large s and n ≫ s, H-Free Graphs with Matching Number at Most s Have at Most g(n,k,s) EdgesResearch Paper

Motivation

Two classical extremal results bound the number of edges of an nnn-vertex graph under a single restriction. Turán's theorem (1941) says that a graph with no clique on k+1k+1k+1 vertices has at most t(n,k)t(n,k)t(n,k) edges, the edge count of the balanced complete kkk-partite graph. The Erdős–Gallai theorem (1959) gives the maximum number of edges of an nnn-vertex graph whose largest matching has at most sss edges. N. Alon and P. Frankl, Turán graphs with bounded matching number (arXiv:2210.15076v1; J. Combin. Theory Ser. B, 2024, DOI 10.1016/j.jctb.2023.12.002), combine the two restrictions. Their Theorem 1.1 determines the maximum for the clique constraint and every n≥2s+1n\ge 2s+1n≥2s+1 (mission 1 of this series). Their Proposition 3.1, the goal here, treats a whole class of forbidden graphs, the color-critical ones, when sss is large in terms of the forbidden graph and nnn is large in terms of sss.

Color-critical graphs are the natural class for exact Turán results: by a theorem of M. Simonovits (1968), for a color-critical HHH of chromatic number k+1k+1k+1 the Turán graph T(N,k)T(N,k)T(N,k) is extremal for HHH-freeness once NNN is large. Proposition 3.1 is the analogue of Simonovits' theorem under a matching constraint.

Setting

All graphs are finite and simple. For a graph GGG, a matching is a set of pairwise disjoint edges, and the matching number ν(G)\nu(G)ν(G) is the largest size of a matching. For a graph HHH, GGG is HHH-free if it contains no subgraph (not necessarily induced) isomorphic to HHH. The chromatic number χ(H)\chi(H)χ(H) is the least number of colors in a proper vertex coloring. HHH is color-critical if it has an edge eee with χ(H−e)<χ(H)\chi(H-e)<\chi(H)χ(H−e)<χ(H); examples are complete graphs and odd cycles.

The Turán graph T(n,k)T(n,k)T(n,k) is the complete kkk-partite graph on nnn vertices with classes of sizes as equal as possible; t(n,k)t(n,k)t(n,k) is its number of edges. For k≥2k\ge 2k≥2 and 2s≤n2s\le n2s≤n, the graph G(n,k,s)G(n,k,s)G(n,k,s) is the complete kkk-partite graph on nnn vertices consisting of k−1k-1k−1 classes of sizes as equal as possible whose total size is sss, and one further class of size n−sn-sn−s. Its number of edges is g(n,k,s)g(n,k,s)g(n,k,s).

In the Lean development, vertices of GGG are Fin n; the shared objects of this series live in TuranMatching.Clique.Setting: ν\nuν is matchingNumber, t(n,k)t(n,k)t(n,k) is turanNum n k (Mathlib's turanGraph), G(n,k,s)G(n,k,s)G(n,k,s) is bigGraph n k s, g(n,k,s)g(n,k,s)g(n,k,s) is gNum n k s, color-criticality is IsColorCritical, and the set XXX of vertices of degree exceeding 2s2s2s is highDeg G s.

Formalization targets

Goal: Proposition 3.1 (p. 5)

There is n0:N→Nn_0:\mathbb N\to\mathbb Nn0​:N→N such that for every color-critical HHH with χ(H)=k+1>2\chi(H)=k+1>2χ(H)=k+1>2 there is s0(H)s_0(H)s0​(H) with: for all s>s0(H)s>s_0(H)s>s0​(H) and n>n0(s)n>n_0(s)n>n0​(s),

max⁡{∣E(G)∣:∣V(G)∣=n, G H-free, ν(G)≤s}=g(n,k,s).\max\{|E(G)| : |V(G)|=n,\ G\ H\text{-free},\ \nu(G)\le s\}=g(n,k,s).max{∣E(G)∣:∣V(G)∣=n, G H-free, ν(G)≤s}=g(n,k,s).

The maximum is stated as an upper bound for every admissible GGG together with an admissible graph attaining g(n,k,s)g(n,k,s)g(n,k,s). The thresholds s0s_0s0​ and n0n_0n0​ are left existential, as on the page.

Milestones (pp. 5–6)

  1. G(n,k,s)G(n,k,s)G(n,k,s) is kkk-colorable, HHH-free for every HHH with χ(H)=k+1\chi(H)=k+1χ(H)=k+1, and ν(G(n,k,s))=s\nu(G(n,k,s))=sν(G(n,k,s))=s (for 2s≤n2s\le n2s≤n).
  2. If ν(G)≤s\nu(G)\le sν(G)≤s then at most sss vertices have degree exceeding 2s2s2s: ∣X∣≤s|X|\le s∣X∣≤s.
  3. If every degree is at most 2s2s2s and ν(G)≤s\nu(G)\le sν(G)≤s, then ∣E(G)∣≤(2s+1)s|E(G)|\le(2s+1)s∣E(G)∣≤(2s+1)s.
  4. If ν(G)≤s\nu(G)\le sν(G)≤s and ∣X∣<s|X|<s∣X∣<s, then ∣E(G)∣<(s−1)n+2(s+1)s|E(G)|<(s-1)n+2(s+1)s∣E(G)∣<(s−1)n+2(s+1)s.
  5. (s−1)n+2(s+1)s<g(n,k,s)(s-1)n+2(s+1)s<g(n,k,s)(s−1)n+2(s+1)s<g(n,k,s) for n>3s2+2sn>3s^2+2sn>3s2+2s.
  6. If ν(G)≤s\nu(G)\le sν(G)≤s and ∣X∣=s|X|=s∣X∣=s, then V−XV-XV−X is independent.
  7. Simonovits' theorem: an HHH-free graph on N≥N0(H)N\ge N_0(H)N≥N0​(H) vertices has at most t(N,k)t(N,k)t(N,k) edges.
  8. If ∣X∣=s|X|=s∣X∣=s, V−XV-XV−X is independent, ZZZ is disjoint from XXX with ∣Z∣=⌊s/(k−1)⌋|Z|=\lfloor s/(k-1)\rfloor∣Z∣=⌊s/(k−1)⌋ and G[X∪Z]G[X\cup Z]G[X∪Z] has at most t(s+⌊s/(k−1)⌋,k)t(s+\lfloor s/(k-1)\rfloor,k)t(s+⌊s/(k−1)⌋,k) edges, then ∣E(G)∣≤g(n,k,s)|E(G)|\le g(n,k,s)∣E(G)∣≤g(n,k,s).

Significance

The proposition settles, for every color-critical HHH and large parameters, the Turán problem with a bounded matching number, and identifies the extremal graph G(n,k,s)G(n,k,s)G(n,k,s), which does not depend on HHH beyond its chromatic number. For H=Kk+1H=K_{k+1}H=Kk+1​ it agrees with the large-nnn case of Theorem 1.1 of the same paper. The structural steps (few high-degree vertices, the independence of the low-degree side) are reusable in other degree-based arguments under matching constraints.

The result is proved in the paper; none of it is formalized. The mission produces, besides the goal, two classical theorems absent from Mathlib in the forms needed here: the matching-number consequence of Vizing's theorem (milestone 3) and Simonovits' exact Turán theorem for color-critical graphs (milestone 7). Milestone 7 is a cited classical theorem, not a result of Alon and Frankl; it is posed because the proof rests on it. Mathlib currently has Turán's theorem for cliques and the Erdős–Stone–Simonovits density theorem, but not the exact result for color-critical graphs.

Difficulty

Milestones 1, 2, 4, 5, 6 and 8 are elementary counting arguments, though each requires building matchings or explicit counts in Lean. Milestone 8 contains the paper's "easy to see" isomorphism, which in Lean is an identity between two edge counts, t(s+m,k)+(n−s−m)s=g(n,k,s)t(s+m,k)+(n-s-m)s=g(n,k,s)t(s+m,k)+(n−s−m)s=g(n,k,s) with m=⌊s/(k−1)⌋m=\lfloor s/(k-1)\rfloorm=⌊s/(k−1)⌋.

Milestone 3 needs Vizing's edge-coloring theorem (a graph of maximum degree Δ\DeltaΔ is properly (Δ+1)(\Delta+1)(Δ+1)-edge-colorable). A naive greedy edge coloring gives only 2Δ−12\Delta-12Δ−1 colors, which bounds the edge count by about (4s−1)s(4s-1)s(4s−1)s and is too weak for the comparison in milestones 4 and 5.

Milestone 7 is the hardest item. The density version (Erdős–Stone–Simonovits) gives t(N,k)+o(N2)t(N,k)+o(N^2)t(N,k)+o(N2) edges only; the exact bound for color-critical HHH requires Simonovits' stability method, an argument that an almost-extremal HHH-free graph is close to T(N,k)T(N,k)T(N,k) followed by a cleaning step that uses the critical edge.

Formalization scope

Graphs are SimpleGraph (Fin n) with decidable adjacency; edges are counted by #G.edgeFinset. The matching number is the supremum, in N\mathbb NN, of the edge counts of matching subgraphs; the set is nonempty and bounded, so this is the true maximum and not a junk value. g(n,k,s)g(n,k,s)g(n,k,s) is defined as the edge count of the graph G(n,k,s)G(n,k,s)G(n,k,s), not by a closed formula. Chromatic numbers live in N∪{∞}\mathbb N\cup\{\infty\}N∪{∞} (Mathlib's chromaticNumber), both in the definition of color-critical and in the hypothesis χ(H)=k+1\chi(H)=k+1χ(H)=k+1. HHH-freeness is Mathlib's SimpleGraph.Free (no subgraph copy). The vertex type of HHH is any finite type in the lowest universe.

Conventions committed to:

  • k≥2k\ge 2k≥2 is the page's k+1>2k+1>2k+1>2; it is needed because G(n,k,s)G(n,k,s)G(n,k,s) has k−1k-1k−1 classes and the proof divides by k−1k-1k−1.
  • Quantifier order is the page's: n0n_0n0​ is a function of sss alone and is chosen before HHH; s0s_0s0​ depends on HHH only.
  • Milestone 1 states kkk-colorability for the page's "kkk chromatic", and carries 2s≤n2s\le n2s≤n, which the page leaves implicit.
  • Milestone 3 bounds edges where the page writes "the number of vertices"; the vertex count is not bounded.
  • Milestone 5 uses the threshold n>3s2+2sn>3s^2+2sn>3s2+2s. The page's "nnn exceeding, say, 3s23s^23s2" is too small: for k=2k=2k=2, s=2s=2s=2, n=13n=13n=13 one has (s−1)n+2(s+1)s=25>22=g(13,2,2)(s-1)n+2(s+1)s=25>22=g(13,2,2)(s−1)n+2(s+1)s=25>22=g(13,2,2). The goal is unaffected, since n0(s)n_0(s)n0​(s) is unspecified.
  • Milestone 4 carries s≥1s\ge 1s≥1 so that s−1s-1s−1 is honest natural-number subtraction.

A formalization that states only the upper bound, without an attaining graph, or that places the existential n0n_0n0​ after sss is fixed as a constant independent of sss, or that defines ν\nuν or ggg so that they take junk values, is a different and weaker statement and is ruled out.

Infrastructure that would be reusable beyond this mission: a matching-number API on Mathlib's Subgraph.IsMatching (in particular ν(G)≤ν(G′)\nu(G)\le\nu(G')ν(G)≤ν(G′) for G≤G′G\le G'G≤G′ and the behaviour under induced subgraphs); Vizing's theorem; and Simonovits' theorem. Contributions of any of these, and of partial results toward milestone 7 (for example the case H=C2ℓ+1H=C_{2\ell+1}H=C2ℓ+1​), are welcome.

Selected references

  • N. Alon and P. Frankl, Turán graphs with bounded matching number, arXiv:2210.15076v1, 2022; J. Combin. Theory Ser. B, 2024. https://arxiv.org/abs/2210.15076, https://doi.org/10.1016/j.jctb.2023.12.002
  • M. Simonovits, A method for solving extremal problems in graph theory, stability problems, in: Theory of Graphs (Proc. Colloq., Tihany, 1966), Academic Press, 1968, pp. 279–319.
  • P. Erdős and T. Gallai, On maximal paths and circuits of graphs, Acta Math. Acad. Sci. Hungar. 10 (1959), 337–356. https://doi.org/10.1007/BF02024498
  • P. Turán, On an extremal problem in graph theory (in Hungarian), Mat. Fiz. Lapok 48 (1941), 436–452.
  • V. G. Vizing, On an estimate of the chromatic class of a p-graph, Diskret. Analiz 3 (1964), 25–30.
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Algorithmic Game TheoryEconomics·Captain: mikedeng1

Competitive Equilibrium with Indivisible Goods and Generic Budgets 1: Two Additive Agents with Almost Equal but Unequal Budgets Have a Competitive Equilibrium Giving Each Agent Her Truncated ShareResearch Paper

Motivation

Many allocation problems divide indivisible goods among agents who are entitled to different shares but cannot pay with real money: course seats among students, shifts among workers, inherited items among heirs. A standard mechanism gives each agent a budget of artificial currency and lets a market run. When budgets are equal this is the competitive equilibrium from equal incomes (CEEI) of Varian (1974), the basis of the course-allocation mechanism of Budish (2011). With indivisible items, however, an equilibrium can fail to exist: one item and two agents with equal budgets already admit none, because whoever does not get the item could afford it at any price the owner can pay.

Babaioff, Nisan and Talgam-Cohen (arXiv 2017; Math. Oper. Res. 2021, doi:10.1287/moor.2020.1062) ask whether this failure is robust or a knife edge, and answer for two agents with additive preferences: an arbitrarily small, strict inequality between the budgets restores existence. Budish's approximate CEEI perturbs budgets randomly for the same reason; this mission formalizes the exact two-agent result.

Setting

A discrete Fisher market has a set MMM of mmm indivisible items and two agents. Agent iii has a valuation viv_ivi​ assigning a real value to every bundle S⊆MS\subseteq MS⊆M, and a budget bi>0b_i>0bi​>0. Valuations are additive (vi(S)=∑j∈Svi({j})v_i(S)=\sum_{j\in S}v_i(\{j\})vi​(S)=∑j∈S​vi​({j})), normalized (vi(M)=1v_i(M)=1vi​(M)=1), non-negative, monotone (vi(S)<vi(T)v_i(S)<v_i(T)vi​(S)<vi​(T) when S⊊TS\subsetneq TS⊊T) and strict (different bundles have different values). Budgets are normalized, b1+b2=1b_1+b_2=1b1​+b2​=1; money has no value to the agents.

An allocation S=(S1,S2)\mathcal S=(\mathcal S_1,\mathcal S_2)S=(S1​,S2​) is a partition of all items between the agents. Item prices pj≥0p_j\ge 0pj​≥0 give bundle prices p(S)=∑j∈Spjp(S)=\sum_{j\in S}p_jp(S)=∑j∈S​pj​. Agent iii demands SSS if p(S)≤bip(S)\le b_ip(S)≤bi​ and p(T)>bip(T)>b_ip(T)>bi​ for every bundle TTT with vi(T)>vi(S)v_i(T)>v_i(S)vi​(T)>vi​(S). A competitive equilibrium (CE) is a pair (S,p)(\mathcal S,p)(S,p) in which each agent demands her own bundle. An allocation is Pareto optimal (PO) if every other allocation is strictly worse for some agent.

Agent iii's budget-proportional share is bib_ibi​ (her budget times vi(M)=1v_i(M)=1vi​(M)=1). Her truncated share is the best value she gets in a PO allocation that gives her at most that share:

bi−=max⁡{vi(Si): S PO, vi(Si)≤bi}.b_i^-=\max\{v_i(\mathcal S_i):\ \mathcal S\ \text{PO},\ v_i(\mathcal S_i)\le b_i\}.bi−​=max{vi​(Si​): S PO, vi​(Si​)≤bi​}.

The Lean development uses the same names: bundle σ i for Si\mathcal S_iSi​, price, IsCE, IsPO, IsStandardValuation, GetsTruncatedShare.

Formalization targets

Goal: Theorem 7.1 (p. 17)

For every two-agent additive market there is ϵ>0\epsilon>0ϵ>0 such that every budget pair with

b2<b1≤b2+ϵb_2<b_1\le b_2+\epsilonb2​<b1​≤b2​+ϵ

admits a CE (S,p)(\mathcal S,p)(S,p) in which vj(Sj)≥bj−v_j(\mathcal S_j)\ge b_j^-vj​(Sj​)≥bj−​ for both agents. The goal fixes no value of ϵ\epsilonϵ; it asserts only that one exists for each market.

Milestones

  1. Proposition 4.1 (p. 10): for a PO allocation with non-empty bundles and budget-exhausting prices, CE is equivalent to a pairwise swap condition, Condition (1).
  2. Lemma 4.3 (p. 11): a budget-exhausting combination pricing pj=αv1({j})+βv2({j})p_j=\alpha v_1(\{j\})+\beta v_2(\{j\})pj​=αv1​({j})+βv2​({j}) (α,β≥0\alpha,\beta\ge0α,β≥0, max⁡{α,β}>0\max\{\alpha,\beta\}>0max{α,β}>0) at a PO allocation is a CE.
  3. Proposition 5.1 (p. 12): budget-proportional and anti-proportional PO allocations are supported in a CE.
  4. Lemma 5.5 (p. 14): without budget-proportional or PO anti-proportional allocations, agent iii's augmented-share minimizer is agent kkk's truncated-share maximizer.
  5. Lemma 6.3 (p. 15): if the budgets avoid the finite exceptional set RiR_iRi​ and the rectangle of allocations TiT_iTi​ is empty, a CE with truncated shares exists.
  6. Case 1 of the proof (p. 18): a CE at budgets (12,12)(\tfrac12,\tfrac12)(21​,21​) remains a CE, after rescaling prices, when agent 1's budget is raised slightly.
  7. RiR_iRi​ avoidance (p. 19): almost equal but unequal budgets lie outside RiR_iRi​.

Two companion statements are drafted without being milestones: Theorem 4.4 (second welfare theorem) and Theorem 5.2 (a budget-proportional allocation implies a CE).

Significance

The result. Theorem 7.1 shows that the non-existence of CEEI with indivisible goods is a measure-zero phenomenon for two additive agents: equal budgets are the only bad point near equality, and the equilibrium obtained is also fair in the truncated-share sense. It justifies tie-breaking by tiny budget differences in practice. It is the two-agent base case of the paper's main open question (§9.1, p. 20), whether generic almost-equal budgets guarantee a CE for more than two agents; the paper also leaves open two agents with arbitrary generic budgets and non-identical preferences (p. 21). For arbitrary, not almost-equal, budgets, Segal-Halevi (AAMAS 2018) shows that genericity does not guarantee existence for four additive agents.

Formalizing it. No machine-checked proof of any result of this paper is known. The paper's own argument for one case of the goal is incomplete: in Case 2(b) of the proof of Theorem 7.1 (p. 19) it asserts that the two candidate allocations are mirror images of each other and that the rectangles T1,T2T_1,T_2T1​,T2​ are empty. Both claims fail on an explicit three-item market. Theorem 7.1 itself held in every one of 6000 markets checked numerically during planning, including that one, where a CE with truncated shares exists at prices proportional to one agent's valuation. A formal proof therefore has to supply an argument the paper does not contain; the two false steps are not posed as milestones.

Difficulty

The milestones 1–5 are finite combinatorics on the Pareto frontier with sign bookkeeping. The difficulty sits in Case 2(b) of the goal: every allocation gives one agent more than 12\tfrac1221​ and the other less. The natural route, invoking Lemma 6.3, needs some TiT_iTi​ to be empty, and in that case both can be non-empty. Lemma 6.3 does not cover it, and the paper's symmetry argument cannot be repaired by choosing ϵ\epsilonϵ smaller, since in the counterexample the two candidate allocations stay the same for every small ϵ\epsilonϵ. A complete proof must show directly that one of the two "as fair as possible" allocations is supported by suitable prices.

Formalization scope

Items are Fin m and agents Fin 2; the paper's agents 1, 2 are indices 0, 1, so "b1>b2b_1>b_2b1​>b2​" reads b 1 < b 0. An allocation is a map σ : Fin m → Fin 2, which builds in that every item is allocated exactly once. All quantities are real numbers. Demand quantifies over every bundle, with strict inequality p(T)>bip(T)>b_ip(T)>bi​. Prices are non-negative by definition of a CE. The truncated share is a maximum over PO allocations only.

Two conventions are disclosed restrictions or additions:

  1. Strictness without identical items. The paper allows identical items as the single exception to strict preferences (p. 6). Here each valuation is injective on bundles, so markets with identical items are excluded.
  2. Rescaled prices in Case 1. The page says the perturbed CE uses unchanged prices; at normalized budgets the prices must be divided by 1+ϵ1+\epsilon1+ϵ, and the milestone says so.

In the goal ϵ\epsilonϵ is chosen after the valuations and before the budgets. A formalization in which ϵ\epsilonϵ depends on the budgets, demand ranges over a restricted family of bundles, allocations need not allocate every item, prices may be negative, or the truncated share is a maximum over all allocations, would be a different and in several cases trivial statement; all of these are ruled out.

The definitions file GenericBudgets.AlmostEqual.Setting holds the market, CE, PO, the fairness notions, combination pricing, Condition (1), TiT_iTi​ and RiR_iRi​, and is reusable for any two-agent indivisible-goods market with budgets. Proofs of the milestones, a repaired argument for Case 2(b), and general nnn-agent versions of the CE and PO infrastructure are welcome.

Selected references

  • M. Babaioff, N. Nisan, I. Talgam-Cohen, Competitive Equilibrium with Indivisible Goods and Generic Budgets, arXiv:1703.08150v2, 2018; Mathematics of Operations Research 46(1), 2021. https://arxiv.org/abs/1703.08150v2, https://doi.org/10.1287/moor.2020.1062
  • H. R. Varian, Equity, envy, and efficiency, Journal of Economic Theory 9(1), 1974. https://doi.org/10.1016/0022-0531(74)90075-1
  • E. Budish, The combinatorial assignment problem: approximate competitive equilibrium from equal incomes, Journal of Political Economy 119(6), 2011. https://doi.org/10.1086/664613
  • E. Segal-Halevi, Competitive equilibrium for almost all incomes, Proceedings of AAMAS 2018, pp. 1267–1275. https://arxiv.org/abs/1705.04212
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Linear OptimizationMachine LearningOperations Research+1·Captain: mikedeng1

Strong Mixed-Integer Programming Formulations for Trained Neural Networks 2: Under Strict Activity Every Inequality of the Exponential Family (6b) Is Facet-DefiningResearch Paper

Motivation

Trained neural networks are increasingly embedded inside optimization models: to verify that a classifier is robust to small input perturbations, to optimize over a learned surrogate of an expensive system, or to choose decisions whose outcome is predicted by a network. When the network uses rectified linear units (ReLU), each neuron y=max⁡{0, w⋅x+b}y=\max\{0,\,w\cdot x+b\}y=max{0,w⋅x+b} is piecewise linear, and the whole network can be written exactly as a mixed-integer program (MIP) with one binary variable per neuron. How fast a branch-and-bound solver closes such a model depends on how tight the linear-programming relaxation of each neuron's formulation is.

Anderson, Huchette, Tjandraatmadja and Vielma (arXiv:1811.08359v2, the IPCO 2019 extended abstract) gave a formulation (6) of a single ReLU neuron over a box that uses only the original variables and one binary variable, and is ideal: its LP relaxation has integral extreme points (Proposition 1, p. 6). The price is an exponential family of inequalities (6b), one for every subset III of the support of www. The present mission formalizes their Proposition 2: each of these inequalities is facet-defining, so no member of the family can be dropped without weakening the relaxation. A longer journal version of the work, with different numbering, appeared later (arXiv:1811.01988); this mission follows the extended abstract.

Setting

Fix η∈N\eta\in\mathbb Nη∈N, a weight vector w∈Rηw\in\mathbb R^\etaw∈Rη, a bias b∈Rb\in\mathbb Rb∈R, and bounds L,U∈RηL,U\in\mathbb R^\etaL,U∈Rη with Li<UiL_i<U_iLi​<Ui​ for every iii (§1.3, p. 4). Write f(x)=w⋅x+bf(x)=w\cdot x+bf(x)=w⋅x+b and [L,U]={x:L≤x≤U}[L,U]=\{x : L\le x\le U\}[L,U]={x:L≤x≤U}. The sign-adjusted bounds are

L˘i={Liwi≥0Uiwi<0,U˘i={Uiwi≥0Liwi<0,\breve L_i=\begin{cases}L_i & w_i\ge 0\\ U_i & w_i<0\end{cases},\qquad \breve U_i=\begin{cases}U_i & w_i\ge 0\\ L_i & w_i<0\end{cases},L˘i​={Li​Ui​​wi​≥0wi​<0​,U˘i​={Ui​Li​​wi​≥0wi​<0​,

so that M+(f)=w⋅U˘+bM^+(f)=w\cdot\breve U+bM+(f)=w⋅U˘+b and M−(f)=w⋅L˘+bM^-(f)=w\cdot\breve L+bM−(f)=w⋅L˘+b are the maximum and minimum of fff over [L,U][L,U][L,U]. The support is supp⁡(w)={i:wi≠0}\operatorname{supp}(w)=\{i : w_i\neq 0\}supp(w)={i:wi​=0}. Strict activity means M−(f)<0<M+(f)M^-(f)<0<M^+(f)M−(f)<0<M+(f): the neuron is neither always off nor always on over the box. The paper assumes it throughout (§1.3).

Formulation (6) (p. 6) consists of the points (x,y,z)(x,y,z)(x,y,z) with

y≥w⋅x+b,(6a)y≤∑i∈Iwi(xi−L˘i(1−z))+(b+∑i∉IwiU˘i)z∀I⊆supp⁡(w),(6b)(x,y,z)∈[L,U]×R≥0×{0,1}.(6c)\begin{aligned} &y\ge w\cdot x+b, &&\text{(6a)}\\ &y\le\sum_{i\in I}w_i\bigl(x_i-\breve L_i(1-z)\bigr)+\Bigl(b+\sum_{i\notin I}w_i\breve U_i\Bigr)z\quad\forall I\subseteq\operatorname{supp}(w), &&\text{(6b)}\\ &(x,y,z)\in[L,U]\times\mathbb R_{\ge0}\times\{0,1\}. &&\text{(6c)} \end{aligned}​y≥w⋅x+b,y≤i∈I∑​wi​(xi​−L˘i​(1−z))+(b+i∈/I∑​wi​U˘i​)z∀I⊆supp(w),(x,y,z)∈[L,U]×R≥0​×{0,1}.​​(6a)(6b)(6c)​

In Lean, form6 w b L U is this set, and relax6 w b L U is its LP relaxation (0≤z≤10\le z\le10≤z≤1 in place of z∈{0,1}z\in\{0,1\}z∈{0,1}). The right-hand side of (6b) for the subset III is rhs6b w b L U I x z.

An inequality g≤0g\le0g≤0 is facet-defining for a set PPP when it holds on PPP, its face F=P∩{g=0}F=P\cap\{g=0\}F=P∩{g=0} is nonempty, and dim⁡F=dim⁡P−1\dim F=\dim P-1dimF=dimP−1, the dimension of a set being that of its affine hull. The paper uses this standard notion without defining it.

Formalization targets

Goal: Proposition 2 (p. 6)

Under L<UL<UL<U and strict activity, for every I⊆supp⁡(w)I\subseteq\operatorname{supp}(w)I⊆supp(w), the inequality (6b) for III is facet-defining for

P=conv⁡{(x,y,z):(x,y,z) satisfies (6a)–(6c)}.P=\operatorname{conv}\{(x,y,z) : (x,y,z)\text{ satisfies (6a)–(6c)}\}.P=conv{(x,y,z):(x,y,z) satisfies (6a)–(6c)}.

The page states the result as "Each inequality in (6b) is facet-defining", and adds right after the proof line: "We require the assumption of strict activity above, as introduced in Section 1.3."

Milestones (App. A.2, p. 15)

  1. For some ε>0\varepsilon>0ε>0, the η+2\eta+2η+2 points p0=(L˘,0,0)p^0=(\breve L,0,0)p0=(L˘,0,0), p1=(U˘,f(U˘),1)p^1=(\breve U,f(\breve U),1)p1=(U˘,f(U˘),1), p~i=(L˘+εσiei,0,0)\tilde p^i=(\breve L+\varepsilon\sigma_ie^i,0,0)p~​i=(L˘+εσi​ei,0,0) for i∉Ii\notin Ii∈/I, and p~i=(U˘−εσiei,f(U˘−εσiei),1)\tilde p^i=(\breve U-\varepsilon\sigma_ie^i,f(\breve U-\varepsilon\sigma_ie^i),1)p~​i=(U˘−εσi​ei,f(U˘−εσi​ei),1) for i∈Ii\in Ii∈I are feasible with respect to (6) and satisfy (6b) for III at equality; here σi=±1\sigma_i=\pm1σi​=±1 is the sign of wiw_iwi​ (with σi=1\sigma_i=1σi​=1 when wi=0w_i=0wi​=0).
  2. For every ε>0\varepsilon>0ε>0 these η+2\eta+2η+2 points are affinely independent.

Significance

The result. Proposition 1 shows that (6) is ideal; Proposition 2 shows it cannot be made smaller: removing any single inequality (6b) produces a strictly weaker relaxation. Since the family has 2∣supp⁡(w)∣2^{|\operatorname{supp}(w)|}2∣supp(w)∣ members, this is what justifies the paper's practical recommendation to start from the big-MMM formulation and separate inequalities of (6b) on demand (Proposition 3, p. 7) rather than to search for a smaller ideal description in the same variables. The facet structure also gives the geometric picture the paper describes after Proposition 2: each facet is the convex combination of an (η−∣I∣)(\eta-|I|)(η−∣I∣)-dimensional face at z=0z=0z=0 and an ∣I∣|I|∣I∣-dimensional face at z=1z=1z=1.

Formalizing it. The result is proved in the paper, in a half-page appendix; it has not been machine-checked. The formalization adds two things. First, the proof is written for w≥0w\ge0w≥0 "without loss of generality by appropriately interchanging +++ and −-−"; the Lean statements are for every sign pattern, including zero weights. Second, the appendix exhibits η+2\eta+2η+2 affinely independent points on the face, which bounds the face dimension from below; the statement that the face has dimension exactly one less than the polyhedron also needs the polyhedron to be full-dimensional and the face to lie in a proper hyperplane, steps the extended abstract leaves implicit and a complete proof must supply.

Difficulty

The arithmetic in each step is elementary. The work lies in the bookkeeping: choosing a single ε\varepsilonε that keeps every perturbed point inside the box and on the correct side of f=0f=0f=0 (this is exactly where strict activity enters), checking the perturbed points against all 2∣supp⁡(w)∣2^{|\operatorname{supp}(w)|}2∣supp(w)∣ inequalities of (6b) and not only the one for III, and turning a row-reduction argument on an (η+1)×(η+2)(\eta+1)\times(\eta+2)(η+1)×(η+2) matrix into a statement about AffineIndependent and finrank of a vectorSpan in Lean. The natural shortcut, proving only that η+2\eta+2η+2 affinely independent tight points exist, is not Proposition 2: it says nothing about the dimension of the polyhedron itself.

Formalization scope

Inputs are Fin η → ℝ (indices 0,…,η−10,\dots,\eta-10,…,η−1 for the paper's 1,…,η1,\dots,\eta1,…,η); a point (x,y,z)(x,y,z)(x,y,z) is p : (Fin η → ℝ) × ℝ × ℝ with p.1 = x, p.2.1 = y, p.2.2 = z. M±(f)M^\pm(f)M±(f) are given by their closed forms w⋅U˘+bw\cdot\breve U+bw⋅U˘+b and w⋅L˘+bw\cdot\breve L+bw⋅L˘+b. In (6b), "i∉Ii\notin Ii∈/I" ranges over all indices outside III, zero weights included; III ranges over subsets of supp⁡(w)\operatorname{supp}(w)supp(w), as on the page.

Every goal and milestone keeps the standing assumptions of §1.3, Li<UiL_i<U_iLi​<Ui​ for all iii and strict activity, except the affine-independence milestone, which holds without them and is stated without them (a stronger statement). No other hypothesis is added. Strict activity excludes η=0\eta=0η=0, so no nonemptiness assumption on the index set is needed.

IsFacetDefining P g is the standard notion: validity, a nonempty face, and dim⁡F+1=dim⁡P\dim F+1=\dim PdimF+1=dimP with dimensions the finrank of the vectorSpan. The equation is written with +1+1+1 on the left so that no natural-number subtraction can make the empty set or a point a facet. The polyhedron is the convex hull of the points of (6), not the set form6 itself (which is not convex, since z∈{0,1}z\in\{0,1\}z∈{0,1}); by Proposition 1 it equals the LP relaxation relax6, but the statement does not depend on that.

The shared objects of this paper (the ReLU graph, L˘\breve LL˘, U˘\breve UU˘, M±M^\pmM±, support, strict activity, formulation (6), ideality) come from the shared definitions module ReluMIP.Ideal.Setting, common to the companion mission on Proposition 1; this mission's own definitions module adds form6, IsFacetDefining, the sign inward, and the indexed family facetPts of the η+2\eta+2η+2 points. The facet notion and the affine-independence argument are reusable for other facet proofs of polyhedra in product spaces. Proofs of the milestones, of the goal, and of the full-dimensionality step are all welcome.

Selected references

  • R. Anderson, J. Huchette, C. Tjandraatmadja, J. P. Vielma, Strong mixed-integer programming formulations for trained neural networks, IPCO 2019, LNCS 11480, pp. 27–42; preprint arXiv:1811.08359v2, 2019. https://arxiv.org/abs/1811.08359v2
  • R. Anderson, J. Huchette, W. Ma, C. Tjandraatmadja, J. P. Vielma, Strong mixed-integer programming formulations for trained neural networks, Mathematical Programming 183 (2020), 3–39. https://doi.org/10.1007/s10107-020-01474-5
  • G. L. Nemhauser, L. A. Wolsey, Integer and Combinatorial Optimization, Wiley, 1988. https://doi.org/10.1002/9781118627372
  • M. Conforti, G. Cornuéjols, G. Zambelli, Integer Programming, Springer, 2014. https://doi.org/10.1007/978-3-319-11008-0
  • J. P. Vielma, Mixed integer linear programming formulation techniques, SIAM Review 57 (2015), 3–57. https://doi.org/10.1137/130915303
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Differential GeometryFunctional AnalysisProbability·Captain: mikedeng1

Bakry–Émery Curvature-Dimension Condition and Riemannian Ricci Curvature Bounds 5: A Product of Riemannian Energy Measure Spaces with BE(K,N_X) and BE(K,N_Y) Satisfies BE(K,N_X+N_Y)Research Paper

Motivation

A lower bound KKK on the Ricci curvature of a Riemannian manifold and an upper bound NNN on its dimension can be expressed without coordinates in two ways. The Bakry–Émery condition BE(K,N)\mathrm{BE}(K,N)BE(K,N) is a property of the heat semigroup and its generator: the iterated carré du champ Γ2\Gamma_2Γ2​ dominates KΓ+1N(Δf)2K\Gamma+\frac1N(\Delta f)^2KΓ+N1​(Δf)2 (Bakry–Émery 1985). The Riemannian curvature-dimension conditions RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) and RCD∗(K,N)\mathrm{RCD}^*(K,N)RCD∗(K,N) are properties of a metric measure space, defined through optimal transport (Ambrosio–Gigli–Savaré 2014). A basic test for any notion of "Ricci curvature at least KKK, dimension at most NNN" is its behaviour under products: on a product of manifolds, Ricci curvature bounds combine and dimensions add.

The paper of Ambrosio, Gigli and Savaré (arXiv:1209.5786) proves that BE(K,∞)\mathrm{BE}(K,\infty)BE(K,∞) and RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) coincide on a natural class of Dirichlet-form spaces, and draws from it, in its §5.1, two tensorization results. The first (Theorem 5.1) is the stability of RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) under products. This had been proved in Ambrosio–Gigli–Savaré 2014 only under a nonbranching assumption on the factors; the equivalence removes that assumption. The second (Theorem 5.2) is the dimensional statement: the product of two Riemannian Energy measure spaces satisfying BE(K,NX)\mathrm{BE}(K,N_X)BE(K,NX​) and BE(K,NY)\mathrm{BE}(K,N_Y)BE(K,NY​) satisfies BE(K,NX+NY)\mathrm{BE}(K,N_X+N_Y)BE(K,NX​+NY​), the bound on the dimension of the product that the smooth case predicts.

Setting

Let XXX be a complete separable metric space with a Borel measure m\mathfrak mm. A Dirichlet form is a quadratic, L2L^2L2-lower semicontinuous, Markovian functional E:L2(X,m)→[0,∞]\mathcal E:L^2(X,\mathfrak m)\to[0,\infty]E:L2(X,m)→[0,∞] with dense domain V\mathbb VV. Its generator ΔE\Delta_{\mathcal E}ΔE​ is defined by E(f,g)=−∫g ΔEf dm\mathcal E(f,g)=-\int g\,\Delta_{\mathcal E}f\,d\mathfrak mE(f,g)=−∫gΔE​fdm for all g∈Vg\in\mathbb Vg∈V, and its heat flow Pt\mathsf P_tPt​ solves ddtPtf=ΔEPtf\frac{d}{dt}\mathsf P_tf=\Delta_{\mathcal E}\mathsf P_tfdtd​Pt​f=ΔE​Pt​f. The carré du champ Γ(f)\Gamma(f)Γ(f) is the density of φ↦E(f,fφ)−12E(f2,φ)\varphi\mapsto\mathcal E(f,f\varphi)-\frac12\mathcal E(f^2,\varphi)φ↦E(f,fφ)−21​E(f2,φ). For ν=1/N≥0\nu=1/N\ge0ν=1/N≥0, BE(K,N)\mathrm{BE}(K,N)BE(K,N) is the weak form (2.33) of Γ2≥KΓ+ν(Δf)2\Gamma_2\ge K\Gamma+\nu(\Delta f)^2Γ2​≥KΓ+ν(Δf)2, written through the functional At[f;φ](s)=12∫(Pt−sf)2Psφ dm\mathsf A_t[f;\varphi](s)=\frac12\int(\mathsf P_{t-s}f)^2\mathsf P_s\varphi\,d\mathfrak mAt​[f;φ](s)=21​∫(Pt−s​f)2Ps​φdm.

The intrinsic distance is dE(x,y)=sup⁡{∣ψ(y)−ψ(x)∣:ψ continuous, Γ(ψ)≤1}\mathsf d_{\mathcal E}(x,y)=\sup\{|\psi(y)-\psi(x)|:\psi\text{ continuous},\ \Gamma(\psi)\le1\}dE​(x,y)=sup{∣ψ(y)−ψ(x)∣:ψ continuous, Γ(ψ)≤1}. An Energy measure space (Definition 3.6) is a strongly local Dirichlet form on a space whose metric is dE\mathsf d_{\mathcal E}dE​, with full-support measure and an exhausting function; a Riemannian Energy measure space (Definition 3.16) is in addition upper regular, and every ψ\psiψ with Γ(ψ)≤1\Gamma(\psi)\le1Γ(ψ)≤1 has a continuous version. An RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) space (Definition 3.1) is a length metric measure space with the growth bounds (MD.b) and (MD.exp) on which the relative entropy has an EVIK\mathrm{EVI}_KEVIK​ gradient flow in (P2(X),W2)(\mathscr P_2(X),W_2)(P2​(X),W2​).

The product (5.1) of (X,dX,mX)(X,\mathsf d_X,\mathfrak m_X)(X,dX​,mX​) and (Y,dY,mY)(Y,\mathsf d_Y,\mathfrak m_Y)(Y,dY​,mY​) is Z=X×YZ=X\times YZ=X×Y with

d((x,y),(x′,y′))=dX2(x,x′)+dY2(y,y′),m=mX×mY,\mathsf d((x,y),(x',y'))=\sqrt{\mathsf d_X^2(x,x')+\mathsf d_Y^2(y,y')},\qquad\mathfrak m=\mathfrak m_X\times\mathfrak m_Y,d((x,y),(x′,y′))=dX2​(x,x′)+dY2​(y,y′)​,m=mX​×mY​,

and the Cartesian Dirichlet form (5.2) is

E(f)=∫YEX(fy) dmY(y)+∫XEY(fx) dmX(x),\mathcal E(f)=\int_Y\mathcal E^X(f^y)\,d\mathfrak m_Y(y)+\int_X\mathcal E^Y(f^x)\,d\mathfrak m_X(x),E(f)=∫Y​EX(fy)dmY​(y)+∫X​EY(fx)dmX​(x),

where fy=f(⋅,y)f^y=f(\cdot,y)fy=f(⋅,y) and fx=f(x,⋅)f^x=f(x,\cdot)fx=f(x,⋅).

Formalization targets

Goal: Theorem 5.2

If (X,EX,mX)(X,\mathcal E^X,\mathfrak m_X)(X,EX,mX​) and (Y,EY,mY)(Y,\mathcal E^Y,\mathfrak m_Y)(Y,EY,mY​) are Riemannian Energy measure spaces satisfying (MD.exp), BE(K,NX)\mathrm{BE}(K,N_X)BE(K,NX​) and BE(K,NY)\mathrm{BE}(K,N_Y)BE(K,NY​), then

(Z,E,m) is a Riemannian Energy measure space with dE=d and BE(K,NX+NY).(Z,\mathcal E,\mathfrak m)\ \text{is a Riemannian Energy measure space with}\ \mathsf d_{\mathcal E}=\mathsf d\ \text{and}\ \mathrm{BE}(K,N_X+N_Y).(Z,E,m) is a Riemannian Energy measure space with dE​=d and BE(K,NX​+NY​).

In the parametrization ν=1/N\nu=1/Nν=1/N the product satisfies BE\mathrm{BE}BE with νZ=νXνY/(νX+νY)\nu_Z=\nu_X\nu_Y/(\nu_X+\nu_Y)νZ​=νX​νY​/(νX​+νY​).

Milestones

  1. Corollary 4.18 (i), p. 58: under (MD+exp) and a quadratic Cheeger energy, the length property together with the gradient bound
∣DPtf∣2≤e−2KtPt(∣Df∣w2)(4.30)|\mathrm D\mathsf P_tf|^2\le e^{-2Kt}\mathsf P_t(|\mathrm Df|_w^2)\tag{4.30}∣DPt​f∣2≤e−2KtPt​(∣Df∣w2​)(4.30)

implies RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞). 2. Theorem 5.1, p. 60: the product of two RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) spaces is RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞). 3. The elementary inequality of p. 62: νXa2+νYb2≥νXνYνX+νY(a+b)2\nu_Xa^2+\nu_Yb^2\ge\frac{\nu_X\nu_Y}{\nu_X+\nu_Y}(a+b)^2νX​a2+νY​b2≥νX​+νY​νX​νY​​(a+b)2 for positive νX,νY\nu_X,\nu_YνX​,νY​ and nonnegative a,ba,ba,b. 4. Lemma 5.3, p. 62: ΔZf(x,y)=ΔXfy(x)+ΔYfx(y)\Delta_Zf(x,y)=\Delta_Xf^y(x)+\Delta_Yf^x(y)ΔZ​f(x,y)=ΔX​fy(x)+ΔY​fx(y) under the fibrewise regularity (5.9), for the RCD factors and their Cheeger forms fixed in §5.1.

Significance

Theorem 5.1 shows that RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) is closed under products with no nonbranching condition on the factors, the hypothesis under which Ambrosio–Gigli–Savaré 2014 had obtained it. Theorem 5.2 gives the dimensional version for Dirichlet-form spaces, BE(K,NX)×BE(K,NY)⇒BE(K,NX+NY)\mathrm{BE}(K,N_X)\times\mathrm{BE}(K,N_Y)\Rightarrow\mathrm{BE}(K,N_X+N_Y)BE(K,NX​)×BE(K,NY​)⇒BE(K,NX​+NY​): a product of spaces of finite dimension has finite dimension, with the bound NX+NYN_X+N_YNX​+NY​ of the smooth case, while the condition BE(K,∞)\mathrm{BE}(K,\infty)BE(K,∞) alone loses all dimensional information.

Both results are proved in the paper; none of them, nor the objects they are stated for, has a machine-checked proof. The mission produces a Lean statement of the Cartesian Dirichlet form and of the product structure, the statements of the two tensorization theorems, and the characterization of RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞) that drives Theorem 5.1. A formal proof would also check the measure-theoretic steps that the paper takes for granted: the measurability of y↦EX(fy)y\mapsto\mathcal E^X(f^y)y↦EX(fy), the Fubini arguments of Lemma 5.3, and the identification of the domain of the Cartesian form (cited from [Ambrosio–Gigli–Savaré 2014], Theorem 6.18).

Difficulty

The obvious argument works fibre by fibre: apply BE(K,NX)\mathrm{BE}(K,N_X)BE(K,NX​) to each section fyf^yfy and BE(K,NY)\mathrm{BE}(K,N_Y)BE(K,NY​) to each fxf^xfx, and add. This fails as stated, because Pt\mathsf P_tPt​ on ZZZ does not act on the sections separately: (Ptf)y(\mathsf P_tf)^y(Pt​f)y is an average over y′y'y′ of the semigroup of XXX applied to fy′f^{y'}fy′, weighted by the heat kernel of YYY, so fibrewise gradient and Laplacian bounds have to be transported through this average. For Theorem 5.2 a second step is not fibrewise at all: before any dimensional estimate, the product has to be shown to be a Riemannian Energy measure space whose intrinsic distance is the product distance, which in the paper goes through Theorem 5.1 and hence through the equivalence BE(K,∞)⇔RCD(K,∞)\mathrm{BE}(K,\infty)\Leftrightarrow\mathrm{RCD}(K,\infty)BE(K,∞)⇔RCD(K,∞) of Theorem 4.17.

Formalization scope

Functions on XXX are X → ℝ, and L2L^2L2 membership is MemLp f 2 m; every object is invariant under m\mathfrak mm-a.e. equality. Dirichlet forms take values in [0,∞][0,\infty][0,∞] and are +∞+\infty+∞ off L2L^2L2. Heat flows are passed as functions pinned by the predicate IsHeatSemigroup. Γ(f)\Gamma(f)Γ(f) is a predicate on a density. BE(K,N)\mathrm{BE}(K,N)BE(K,N) is parametrized by ν=1/N≥0\nu=1/N\ge0ν=1/N≥0; νZ=νXνY/(νX+νY)\nu_Z=\nu_X\nu_Y/(\nu_X+\nu_Y)νZ​=νX​νY​/(νX​+νY​) is 000 when either factor has N=∞N=\inftyN=∞. The product ZZZ is WithLp 2 (X × Y), whose metric is the ℓ2\ell^2ℓ2 distance (5.1); the plain type X × Y would carry the max-metric. The second term of (5.2) uses EY\mathcal E^YEY, correcting the printed EX(fx)\mathcal E^X(f^x)EX(fx). Factors are σ-finite.

Theorem 5.2 assumes (MD.exp) for both factors: its proof invokes Theorem 5.1, whose factors must be RCD(K,∞)\mathrm{RCD}(K,\infty)RCD(K,∞), which a Riemannian Energy measure space with BE(K,∞)\mathrm{BE}(K,\infty)BE(K,∞) is only under (MD.exp). In Corollary 4.18, the minimal weak gradient is written as ∣Df∣w2=Γ(f)|\mathrm Df|_w^2=\Gamma(f)∣Df∣w2​=Γ(f), the identity that (QCh) asserts. Lemma 5.3 carries the RCD and Cheeger-form assumptions established at the opening of §5.1. The elementary inequality retains the printed a,b≥0a,b\ge0a,b≥0; applying it to signed Laplacians requires its all-real extension.

The goal is not met by stating BE\mathrm{BE}BE on the product with νZ=0\nu_Z=0νZ​=0: that is BE(K,∞)\mathrm{BE}(K,\infty)BE(K,∞), a strictly weaker claim; nor by defining the product form through the Cheeger energy of ZZZ instead of (5.2).

A complete development needs the Cartesian form's domain theorem, a pointwise version of the heat semigroups, Theorem 4.17 of the paper and the converse RCD(K,∞)⇒BE(K,∞)\mathrm{RCD}(K,\infty)\Rightarrow\mathrm{BE}(K,\infty)RCD(K,∞)⇒BE(K,∞) from [Ambrosio–Gigli–Savaré 2014]. The product layer (sections, Cartesian form, Lemma 5.3) is reusable for any tensorization argument on Dirichlet forms. Proofs of the elementary inequality and of Lemma 5.3 are the natural first contributions.

Selected references

  • L. Ambrosio, N. Gigli, G. Savaré, Bakry–Émery curvature-dimension condition and Riemannian Ricci curvature bounds, Ann. Probab. 43(1), 339–404, 2015. arXiv:1209.5786v4
  • L. Ambrosio, N. Gigli, G. Savaré, Metric measure spaces with Riemannian Ricci curvature bounded from below, Duke Math. J. 163(7), 1405–1490, 2014. arXiv:1109.0222
  • D. Bakry, M. Émery, Diffusions hypercontractives, Séminaire de Probabilités XIX, Lecture Notes in Math. 1123, 177–206, 1985. doi:10.1007/BFb0075847
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Algorithmic Game TheoryOperations ResearchOptimization·Captain: mikedeng1

Supplier Centrality and Auditing Priority in Socially Responsible Supply Chains II: A Stable Joint-Auditing Coalition Audits the Common Supplier and Shares Costs FairlyResearch Paper

Motivation

Brands that sell consumer goods are held responsible by the public for the labour and safety practices of their suppliers. After the 2013 Rana Plaza collapse in Bangladesh, about 200 clothing brands and retailers signed the Accord on Fire and Building Safety and inspect roughly 1,600 factories jointly; pharmaceutical companies such as Pfizer and GSK audit their suppliers jointly through the Pharmaceutical Supply Chain Initiative (both examples from the paper, pp. 4 and 14). Two features of such supply bases matter for auditing. Competing brands often share a common supplier, so a scandal at that supplier hurts both of them. And brands compete downstream, so a scandal that hurts only a rival can help a brand.

Chen, Qi and Dawande (MSOM 2020; accepted manuscript SSRN 2889889) model two competing buyers with one common and two independent suppliers. Their Proposition 2 shows that, when each buyer audits on his own, competition drives the buyers away from the common supplier: in every equilibrium it is left unaudited. This mission formalizes their Proposition 3. It shows that a coalition that audits jointly, and splits the cost by a Shapley-value rule, does audit the common supplier and is stable. A companion mission (Supplier Centrality … I) covers Proposition 2.

Setting

Two buyers B1,B2B_1, B_2B1​,B2​ source from three suppliers: BiB_iBi​ from its independent supplier SiS_iSi​, and both from the common supplier ScS_cSc​. Each supplier is compliant with probability e∈(0,1)e\in(0,1)e∈(0,1). A non-compliant supplier that passes an audit of effort x∈[0,1]x\in[0,1]x∈[0,1] (probability 1−x1-x1−x) is exposed in public with probability r∈(0,1]r\in(0,1]r∈(0,1]. An independent supplier audited with effort xxx therefore causes damage with probability λI(x)=r(1−e)(1−x)\lambda_I(x)=r(1-e)(1-x)λI​(x)=r(1−e)(1−x). The three suppliers offend independently.

If buyer BiB_iBi​ has ni∈{0,1,2}n_i\in\{0,1,2\}ni​∈{0,1,2} exposed suppliers, its demand intercept falls from α\alphaα to α−dM\alpha-d_Mα−dM​ (by dM>0d_M>0dM​>0 once, however many offend). Each exposed supplier also raises its unit input cost from www to w^≥w\hat w\ge ww^≥w. The buyers then play a Cournot game with differentiated products (substitution β∈(0,1]\beta\in(0,1]β∈(0,1]). Buyer B1B_1B1​'s equilibrium profit is π1b(n1,n2)=(q1∗)2\pi^b_1(n_1,n_2)=(q^*_1)^2π1b​(n1​,n2​)=(q1∗​)2, where

q1∗=2(A1−c1)−β(A2−c2)4−β2,Ai=α−dM1{ni≥1},ci=(2−ni)w+niw^.q^*_1=\frac{2(A_1-c_1)-\beta(A_2-c_2)}{4-\beta^2},\qquad A_i=\alpha-d_M\mathbf 1\{n_i\ge1\},\quad c_i=(2-n_i)w+n_i\hat w.q1∗​=4−β22(A1​−c1​)−β(A2​−c2​)​,Ai​=α−dM​1{ni​≥1},ci​=(2−ni​)w+ni​w^.

The aggregate ex post profit is πb(i dM,j dM)=π1b(i,j)+π2b(i,j)\pi^b(i\,d_M,j\,d_M)=\pi^b_1(i,j)+\pi^b_2(i,j)πb(idM​,jdM​)=π1b​(i,j)+π2b​(i,j). Auditing a supplier with effort xxx costs K1{x>0}+a2x2K\mathbf 1\{x>0\}+\tfrac a2x^2K1{x>0}+2a​x2.

Unilateral auditing. Each buyer audits at most one of his two suppliers. Πib\Pi^b_iΠib​ is buyer BiB_iBi​'s expected profit net of his own audit costs. An equilibrium is a pair of mutual best responses in which, by the paper's tie-breaking rule, a buyer who audits strictly prefers it to not auditing. The effort e^I\hat e_Ie^I​ of eq. (2) is a buyer's optimal effort on his own supplier when the rival does not audit.

Joint auditing. The coalition chooses efforts x=(ec1,ecc,ec2)∈[0,1]3x=(e_{c1},e_{cc},e_{c2})\in[0,1]^3x=(ec1​,ecc​,ec2​)∈[0,1]3 on S1,Sc,S2S_1,S_c,S_2S1​,Sc​,S2​, auditing at most two suppliers, and pays each audited supplier's cost once. The buyers still compete downstream. With Rib(x)R^b_i(x)Rib​(x) the buyers' expected profits excluding audit costs, the coalition's profit is

Πb(x)=R1b(x)+R2b(x)−∑j∈{1,c,2}[K1{ecj>0}+a2ecj2].\Pi^b(x)=R^b_1(x)+R^b_2(x)-\sum_{j\in\{1,c,2\}}\Big[K\mathbf 1\{e_{cj}>0\}+\tfrac a2e_{cj}^2\Big].Πb(x)=R1b​(x)+R2b​(x)−j∈{1,c,2}∑​[K1{ecj​>0}+2a​ecj2​].

The difference of the buyers' profits is ΔΠ=R1b−R2b\Delta\Pi=R^b_1-R^b_2ΔΠ=R1b​−R2b​. The cost shares are Γ1,2=12[total cost±ΔΠ]\Gamma_{1,2}=\tfrac12[\text{total cost}\pm\Delta\Pi]Γ1,2​=21​[total cost±ΔΠ] (eq. (3)). The analysis assumes the scenario

πb(0,0)≥πb(dM,0)≥πb(dM,dM)≥πb(2dM,dM)≥πb(2dM,2dM).\pi^b(0,0)\ge\pi^b(d_M,0)\ge\pi^b(d_M,d_M)\ge\pi^b(2d_M,d_M)\ge\pi^b(2d_M,2d_M).πb(0,0)≥πb(dM​,0)≥πb(dM​,dM​)≥πb(2dM​,dM​)≥πb(2dM​,2dM​).

Formalization targets

Goal: Proposition 3

There are thresholds KcL≤KcHK^L_c\le K^H_cKcL​≤KcH​ such that, for every K≥0K\ge0K≥0, an optimal joint plan

{audits S1 and Sc, ΔΠ>0,K<KcL,audits only Sc, ΔΠ=0,KcL≤K<KcH,audits nothing,K≥KcH.\begin{cases}\text{audits } S_1 \text{ and } S_c,\ \Delta\Pi>0, & K<K^L_c,\\ \text{audits only } S_c,\ \Delta\Pi=0, & K^L_c\le K<K^H_c,\\ \text{audits nothing}, & K\ge K^H_c.\end{cases}⎩⎨⎧​audits S1​ and Sc​, ΔΠ>0,audits only Sc​, ΔΠ=0,audits nothing,​K<KcL​,KcL​≤K<KcH​,K≥KcH​.​

The coalition is also stable. At an optimal plan its aggregate profit is at least the buyers' aggregate profit in any unilateral equilibrium. After paying Γi\Gamma_iΓi​, each buyer earns at least his profit in a symmetric unilateral equilibrium.

Milestones

The coalition's profit as a sum of unilateral profits (proof of Lemma OA9). Lemma OA9: ScS_cSc​ beats one independent supplier, and beats no audit for K<K^K<\hat KK<K^. Lemma OA10: ScS_cSc​ with S1S_1S1​ beats S1S_1S1​ with S2S_2S2​. Lemma OA11: S1S_1S1​ with ScS_cSc​ beats ScS_cSc​ alone for K<K~K<\tilde KK<K~. The fair shares (3). The case analysis with KcL=min⁡{K^+K~2,K~}K^L_c=\min\{\frac{\hat K+\tilde K}2,\tilde K\}KcL​=min{2K^+K~​,K~} and KcH=max⁡{K^+K~2,K^}K^H_c=\max\{\frac{\hat K+\tilde K}2,\hat K\}KcH​=max{2K^+K~​,K^}. Stability.

Significance

The result separates two effects of downstream competition on responsible sourcing. Under unilateral auditing, a buyer gains nothing private from auditing the shared supplier: the reduction in risk accrues equally to his rival. The joint coalition removes this free-riding. The common supplier is audited whenever anything is, and the Shapley-type split (3) charges the buyer who also has his own supplier audited for the competitive advantage this gives him (Γ1>Γ2\Gamma_1>\Gamma_2Γ1​>Γ2​ exactly when ΔΠ>0\Delta\Pi>0ΔΠ>0). The paper's welfare comparison (Proposition 4) builds on this proposition and on Proposition 2.

The proof in the e-companion argues through four comparisons of candidate plans and short cost-sharing algebra. None of it is machine-checked. A formal proof fixes the model (in particular which costs the coalition pays and what "at most two suppliers" excludes) and checks each comparison. In one place it also corrects the printed claim: the per-firm stability argument is given only for the symmetric unilateral equilibrium, and it does not extend to the asymmetric one (see Formalization scope).

Difficulty

All objects are explicit polynomials in the efforts. The difficulty is in the comparisons. Lemmas OA9 and OA10 compare different audit plans through the scenario ordering of aggregate ex post profits, an assumption on the stage-2 closed form that is not implied by the standing conditions. The obvious attempt, comparing first-order conditions, fails because the coalition's profit is discontinuous at zero effort (the fixed cost) and the feasible set is not convex: "at most two of three" is a union of faces of the cube. The thresholds K^\hat KK^, K~\tilde KK~ are differences of maxima, so the case analysis has to handle ties and the boundary K=KcHK=K^H_cK=KcH​ with weak inequalities. Stability needs the unilateral equilibria of Proposition 2, so the full goal reaches into the companion mission's game.

Formalization scope

  • Model. Params holds α,β,w,w^,dM,e,r,a\alpha,\beta,w,\hat w,d_M,e,r,aα,β,w,w^,dM​,e,r,a with β∈[0,1]\beta\in[0,1]β∈[0,1], w≤w^w\le\hat ww≤w^, dM>0d_M>0dM​>0, e∈(0,1)e\in(0,1)e∈(0,1), r∈(0,1]r\in(0,1]r∈(0,1], a>0a>0a>0 and the three positivity conditions of p. 8. Every statement adds β>0\beta>0β>0 (Sec. 4.3 continues the competing case) and the p. 13 scenario as five inequalities between piAgg values. Their arguments count exposed suppliers: πb(2dM,dM)\pi^b(2d_M,d_M)πb(2dM​,dM​) is a label, not a damage of 2dM2d_M2dM​.
  • Expected profits are 8-outcome expectations of the closed-form stage-2 profit. The coalition's profit charges each audited supplier once, and the common supplier's damage probability under a joint audit is r(1−e)(1−ecc)r(1-e)(1-e_{cc})r(1−e)(1−ecc​).
  • Thresholds K^,K~\hat K,\tilde KK^,K~ are the maxima at K=0K=0K=0 written as sSup over [0,1][0,1][0,1] and [0,1]2[0,1]^2[0,1]2. At K=0K=0K=0 the profit is a polynomial, so these suprema are attained.
  • "Yields the highest aggregate profit" is read as "some maximizer over the feasible plans has this pattern"; uniqueness is not claimed. ΔΠ\Delta\PiΔΠ is evaluated at that maximizer (its mirror image, which audits S2S_2S2​, has ΔΠ<0\Delta\Pi<0ΔΠ<0).
  • Cost shares use the total cost of the plan. For plans with ec2=0e_{c2}=0ec2​=0 they are the printed formulas (3).
  • Unilateral benchmark. The equilibrium includes the tie-breaking rule of p. 10, and the interior-effort assumption of p. 10 is encoded as e^I<1\hat e_I<1e^I​<1, with e^I\hat e_Ie^I​ given by eq. (2).
  • Stability, corrected. Condition (b) of Sec. 4.3 (each firm earns more) is stated against symmetric unilateral equilibria only, the case the paper's proof treats. Against the asymmetric equilibrium, where one buyer audits with e^I\hat e_Ie^I​ and the other audits nothing, it fails. Take α=10\alpha=10α=10, β=1\beta=1β=1, w=1w=1w=1, w^=3\hat w=3w^=3, dM=12d_M=\tfrac12dM​=21​, e=110e=\tfrac1{10}e=101​, r=1r=1r=1, a=50a=50a=50, K=0.2K=0.2K=0.2: the coalition optimally audits nothing, yet the auditing buyer earns more unilaterally than half of the coalition's profit. Condition (a) is stated against every equilibrium. "Higher" is stated as ≥\ge≥.
  • The goal's thresholds are existential and come before ∀K\forall K∀K. Choosing KcL=KcHK^L_c=K^H_cKcL​=KcH​ does not trivialize it, because the three cases must cover every K≥0K\ge0K≥0. The milestone on part (2) fixes the thresholds explicitly.
  • The source is the authors' SSRN accepted manuscript. Main-text page numbers equal PDF pages, and e-companion page eckkk is PDF page 28+k28+k28+k.

Contributions welcome: proofs of Lemmas OA9–OA11, which are self-contained polynomial inequalities; existence of maximizers on the non-convex feasible set (upper semicontinuity); and the link to the unilateral equilibria needed for stability.

Selected references

  • F. Chen, A. Qi, M. Dawande, Supplier Centrality and Auditing Priority in Socially-Responsible Supply Chains, Manufacturing & Service Operations Management, 2020; accepted manuscript, SSRN 2889889. https://ssrn.com/abstract=2889889
  • E. L. Plambeck, T. A. Taylor, Supplier evasion of a buyer's audit: Implications for motivating supplier social and environmental responsibility, Manufacturing & Service Operations Management 18(2):184–197, 2016. https://doi.org/10.1287/msom.2015.0550
  • N. Singh, X. Vives, Price and quantity competition in a differentiated duopoly, RAND Journal of Economics 15(4):546–554, 1984. https://doi.org/10.2307/2555525
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Mathematical Physics·Captain: Lucas

Giunti–Studenikin 2015: Neutrino Oscillations, Majorana Form Factors and Spin PrecessionResearch Paper

Motivation

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

Timeline of the results formalized here:

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

Setting

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

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

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

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

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

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

Formalization targets

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

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

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

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

Selected references

  • C. Giunti and A. Studenikin, Neutrino electromagnetic interactions: A window to new physics, Rev. Mod. Phys. 87, 531 (2015). https://doi.org/10.1103/RevModPhys.87.531
  • C. Giunti and C. W. Kim, Fundamentals of Neutrino Physics and Astrophysics, Oxford University Press (2007).
  • L. Wolfenstein, Neutrino oscillations in matter, Phys. Rev. D 17, 2369 (1978). https://doi.org/10.1103/PhysRevD.17.2369
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Linear algebraMathematical Physics·Captain: Lucas

Baumgarten 2018: How to (Un-) Quantum Mechanics — Phase-Space AlgebraResearch Paper

Motivation

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

Setting

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

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

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

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

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

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

Target

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

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

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

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

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

Selected references

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

Motivation

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

Timeline (as recounted in the source article):

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

Setting

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

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

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

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

Formalization targets

Goal: the virial theorem

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

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

Milestones

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

Significance

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

Difficulty

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

Formalization scope

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

Selected references

  • Wikipedia, Virial theorem. https://en.wikipedia.org/wiki/Virial_theorem
  • R. Clausius, On a mechanical theorem applicable to heat, Philosophical Magazine, Series 4, 40 (1870), 122–127.
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Methanol Limit on a Drifting Proton-to-Electron Mass Ratio (Bagdonaite et al. 2013)Research Paper

Motivation

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

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

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

Setting

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

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

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

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

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

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

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

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

Formalization targets

Goal: the headline limit

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

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

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

Selected references

  • J. Bagdonaite, P. Jansen, C. Henkel, H. L. Bethlem, K. M. Menten, W. Ubachs, A Stringent Limit on a Drifting Proton-to-Electron Mass Ratio from Alcohol in the Early Universe, Science, 2013. https://doi.org/10.1126/science.1224898
  • P. Jansen, L.-H. Xu, I. Kleiner, W. Ubachs, H. L. Bethlem, Methanol as a sensitive probe for spatial and temporal variations of the proton-to-electron mass ratio, Phys. Rev. Lett. 106, 100801, 2011. https://doi.org/10.1103/PhysRevLett.106.100801
  • S. P. Ellingsen, M. A. Voronkov, S. L. Breen, J. E. J. Lovell, First cosmological constraints on the proton-to-electron mass ratio from observations of rotational transitions of methanol, Astrophys. J. Lett. 747, L7, 2012. https://doi.org/10.1088/2041-8205/747/1/L7
  • Ph. R. Bevington, D. K. Robinson, Data Reduction and Error Analysis for the Physical Sciences, 3rd ed., McGraw-Hill, 2003.
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Maldacena 1999 II: near-horizon geometries of M5-, M2- and D1-D5-branesResearch Paper

Motivation

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

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

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

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

Setting

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

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

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

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

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

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

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

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

Formalization targets

Explicit limit metrics (milestones)

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

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

for M5-branes; to

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

for M2-branes; and to

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

for the D1–D5 system.

Goal: identification with AdS × sphere

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

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

Significance

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

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

Difficulty

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

Formalization scope

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

Selected references

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

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

Motivation

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

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

Setting

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

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

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

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

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

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

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

Formalization targets

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

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

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

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

Selected references

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

Projective Measurements Are Equilibration Processes (finite dimension)Research Paper

Motivation

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

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

Setting

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

X=∑xx Px,X=\sum_{x}x\,P_x ,X=x∑​xPx​,

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

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

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

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

Formalization targets

Goal: Theorem 1 (finite-dimensional form)

For every Hermitian XXX and every map Φ\PhiΦ,

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

Selected references

  • G. Carcassi (Assumptions of Physics collaboration), Projective measurements are equilibration processes, AoP Technical Brief 017. https://assumptionsofphysics.org/resources/briefs
  • G. Lindblad, On the generators of quantum dynamical semigroups, Comm. Math. Phys. 48 (1976) 119–130. https://doi.org/10.1007/BF01608499
  • H. Umegaki, Conditional expectation in an operator algebra. IV. Entropy and information, Kodai Math. Sem. Rep. 14 (1962) 59–85. https://doi.org/10.2996/kmj/1138844604
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Feynman 1948: The Path-Integral Wave Function Satisfies Schrödinger's EquationResearch Paper

Motivation

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

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

Timeline:

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

Setting

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

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

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

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

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

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

Formalization targets

Goal — Eq. (30)

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

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

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

Milestones

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

Significance

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

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

Difficulty

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

Formalization scope

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

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

Selected references

  • R. P. Feynman, Space-Time Approach to Non-Relativistic Quantum Mechanics, Rev. Mod. Phys. 20, 367 (1948). https://doi.org/10.1103/RevModPhys.20.367
  • P. A. M. Dirac, On the Analogy Between Classical and Quantum Mechanics, Rev. Mod. Phys. 17, 195 (1945). https://doi.org/10.1103/RevModPhys.17.195
  • M. Kac, On distributions of certain Wiener functionals, Trans. Amer. Math. Soc. 65, 1 (1949).
  • E. Nelson, Feynman integrals and the Schrödinger equation, J. Math. Phys. 5, 332 (1964).
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Sen 1998: Tachyon condensation on the brane–antibrane systemResearch Paper

Motivation

A coincident pair of a D-brane and an anti-D-brane in type II string theory carries an open-string tachyon, a mode of negative mass squared. In Sen, hep-th/9805019 it was conjectured that at the minimum of the tachyon potential the negative potential energy exactly cancels the sum of the tensions of the brane and the anti-brane, so that the system decays to a configuration of zero energy density, i.e. the supersymmetric vacuum. The paper formalized here, A. Sen, Tachyon condensation on the brane antibrane system, JHEP 08 (1998) 012, gives a short argument for this, and the author says explicitly that it is not a rigorous mathematical proof. The argument follows Gava–Narain–Sarmadi, hep-th/9704006 and belongs to the programme of tachyon condensation. Later work, starting with open string field theory computations, tested the same conjecture numerically.

Setting

Work in string units (α′=1\alpha'=1α′=1). Wrap a D2-brane and an anti-D2-brane on a torus T2=S1×S1T^2=S^1\times S^1T2=S1×S1 with radii R1,R2R_1,R_2R1​,R2​ and area V=4π2R1R2V=4\pi^2R_1R_2V=4π2R1​R2​. Each brane carries one unit of magnetic flux, F12=2π/VF_{12}=2\pi/VF12​=2π/V, with signs chosen so that each carries +1+1+1 unit of D0-brane charge. T-duality on both circles gives a dual torus with radii R~i=1/Ri\tilde R_i=1/R_iR~i​=1/Ri​ and coupling g~=g/(R1R2)\tilde g=g/(R_1R_2)g~​=g/(R1​R2​). On the dual torus the system is described by a U(2)U(2)U(2) gauge theory: a gauge field is a pair A=(A1,A2)A=(A_1,A_2)A=(A1​,A2​) of 2×22\times22×2 complex-matrix-valued functions of x=(x1,x2)x=(x^1,x^2)x=(x1,x2), with field strength F12=∂1A2−∂2A1−i[A1,A2]F_{12}=\partial_1A_2-\partial_2A_1-i[A_1,A_2]F12​=∂1​A2​−∂2​A1​−i[A1​,A2​]. The gauge transform by a matrix-valued Ω\OmegaΩ is (Ω∘A)μ=ΩAμΩ−1−i(∂μΩ)Ω−1(\Omega\circ A)_\mu=\Omega A_\mu\Omega^{-1}-i(\partial_\mu\Omega)\Omega^{-1}(Ω∘A)μ​=ΩAμ​Ω−1−i(∂μ​Ω)Ω−1. The background configuration is

A1=0,A2=2πx1σ3V~,V~=4π2R~1R~2,A_1=0,\qquad A_2=\frac{2\pi x^1\sigma_3}{\tilde V},\qquad \tilde V=4\pi^2\tilde R_1\tilde R_2,A1​=0,A2​=V~2πx1σ3​​,V~=4π2R~1​R~2​,

subject to twisted boundary conditions with transition functions Ω1=exp⁡(ix2σ3/R~2)\Omega_1=\exp(ix^2\sigma_3/\tilde R_2)Ω1​=exp(ix2σ3​/R~2​) and Ω2=1\Omega_2=1Ω2​=1. A D-brane with coupling ggg has tension 1/(4π2g)1/(4\pi^2g)1/(4π2g).

Formalization targets

Goal

With M(R1,R2,g)M(R_1,R_2,g)M(R1​,R2​,g) the mass at the classical minimum (two D2-branes with zero field strength on the dual torus, re-expressed through R1,R2,gR_1,R_2,gR1​,R2​,g), for each fixed g>0g>0g>0:

lim⁡R1,R2→∞M(R1,R2,g)4π2R1R2=0.\lim_{R_1,R_2\to\infty}\frac{M(R_1,R_2,g)}{4\pi^2R_1R_2}=0 .R1​,R2​→∞lim​4π2R1​R2​M(R1​,R2​,g)​=0.

Milestones (in the paper's order)

  1. Eq. (1): 2π/(4π2R1R2)→02\pi/(4\pi^2R_1R_2)\to02π/(4π2R1​R2​)→0 as R1,R2→∞R_1,R_2\to\inftyR1​,R2​→∞.
  2. The background (4) is traceless Hermitian (no U(1)U(1)U(1) part).
  3. Eqs. (5)–(6): the background satisfies the twisted boundary conditions.
  4. Eq. (7): Ω2(2πR~1)Ω1(0)=Ω1(2πR~2)Ω2(0)\Omega_2(2\pi\tilde R_1)\Omega_1(0)=\Omega_1(2\pi\tilde R_2)\Omega_2(0)Ω2​(2πR~1​)Ω1​(0)=Ω1​(2πR~2​)Ω2​(0).
  5. The background has field strength F12=(2π/V~)σ3≠0F_{12}=(2\pi/\tilde V)\sigma_3\neq0F12​=(2π/V~)σ3​=0.
  6. Eq. (8): there is a smooth SU(2)SU(2)SU(2)-valued ggg with the boundary behaviour (8).
  7. Gauge transformations preserve F12≡0F_{12}\equiv0F12​≡0.
  8. Eq. (9): M=2R~1R~2/g~M=2\tilde R_1\tilde R_2/\tilde gM=2R~1​R~2​/g~​.
  9. Eq. (10): M=2/gM=2/gM=2/g.
  10. Eq. (11): M/(4π2R1R2)=1/(2π2R1R2g)M/(4\pi^2R_1R_2)=1/(2\pi^2R_1R_2g)M/(4π2R1​R2​)=1/(2π2R1​R2​g).

Significance

The vanishing of the energy at the tachyon minimum is the basis for identifying stable non-BPS D-branes as tachyonic solitons on brane–antibrane pairs, as discussed at the end of the paper, and it was a starting point for later work on tachyon condensation. The paper's argument is heuristic. This mission makes explicit which steps are mathematics (the gauge-theoretic facts (4)–(8), the gauge covariance used on p. 3, and the algebra (9)–(11) and its limit) and machine-checks them. The physical inputs (the BPS argument that the mass (9) persists as parameters vary, and the identification of the minimum-energy configuration) are recorded as modelling assumptions in the definitions, not proved.

Difficulty

The algebraic milestones (9)–(11) and the limits are elementary. The substantive formal work is in the gauge-theory milestones: computing derivatives of the matrix exponential in (5), the smooth homotopy with flat ends required by (8) (existence rests on the simple connectivity of SU(2)SU(2)SU(2), but the statement asks for an explicit smooth SU(2)SU(2)SU(2)-valued map with prescribed boundary values and vanishing normal derivative), and the covariance computation of the field strength under a non-unitary, merely invertible Ω\OmegaΩ.

Formalization scope

Coordinates are x=(x1,x2)∈R×Rx=(x^1,x^2)\in\mathbb R\times\mathbb Rx=(x1,x2)∈R×R; the paper's index μ∈{1,2}\mu\in\{1,2\}μ∈{1,2} is Fin 2 (1↦01\mapsto01↦0, 2↦12\mapsto12↦1). Matrices are Matrix (Fin 2) (Fin 2) ℂ; partial derivatives are taken entrywise; the inverse is the Mathlib matrix inverse; the exponential is NormedSpace.exp. Radii and couplings are real, with positivity assumed wherever the paper's quantities are physical. The goal cannot be trivialized by division by zero, because it is a statement about the limit of large positive radii. All definitions live in a single definition file under the namespace SenTachyon.

Selected references

  • A. Sen, Tachyon condensation on the brane antibrane system, JHEP 08 (1998) 012. https://doi.org/10.1088/1126-6708/1998/08/012 (arXiv: https://arxiv.org/abs/hep-th/9805170)
  • A. Sen, Stable non-BPS bound states of BPS D-branes, JHEP 08 (1998) 010. https://arxiv.org/abs/hep-th/9805019
  • E. Gava, K. S. Narain, M. H. Sarmadi, On the bound states of p- and (p+2)-branes, Nucl. Phys. B 504 (1997) 214. https://arxiv.org/abs/hep-th/9704006
  • G. 't Hooft, Some twisted self-dual solutions for the Yang–Mills equations on a hypertorus, Comm. Math. Phys. 81 (1981) 267. https://doi.org/10.1007/BF01208900
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CombinatoricsMathematical Physics·Captain: Lucas

't Hooft 1993: Dimensional Reduction in Quantum GravityResearch Paper

Motivation

In the 1993 essay Dimensional Reduction in Quantum Gravity (arXiv:gr-qc/9310026), G. 't Hooft argued that, once gravitational collapse is taken into account, the number of quantum states available to a region of space grows with the area of its boundary rather than with its volume. The essay is the origin of what is now called the holographic principle (developed further by Susskind, arXiv:hep-th/9409089). Besides the physical counting argument, the essay contains a small, fully precise mathematical model: a cellular automaton on the cubic lattice Z3\mathbb Z^3Z3 whose data on a one-dimensional line determine the data everywhere. This mission formalizes the quantitative estimates and the automaton statements of the essay.

Setting

Entropy estimates (eqs. (4)–(11)). In natural units, a region bounded by a sphere of radius RRR has volume V=43πR3V=\tfrac43\pi R^3V=34​πR3 and area A=4πR2A=4\pi R^2A=4πR2. A thermal gas of ZZZ particle species at temperature TTT has energy E=C1ZVT4E=C_1 Z V T^4E=C1​ZVT4 and entropy S=C2ZVT3S=C_2 Z V T^3S=C2​ZVT3 with positive constants C1,C2C_1,C_2C1​,C2​. It stays outside its own Schwarzschild radius if 2E<R2E<R2E<R. A black hole of mass MMM has entropy 4πM24\pi M^24πM2 (eq. (1), additive constant dropped).

Plaquette automaton (eqs. (12)–(19)). Data f:Z3→Z/pf:\mathbb Z^3\to\mathbb Z/pf:Z3→Z/p live on lattice sites. An elementary plaquette has lowest corner xxx and is spanned by two of the unit vectors e1,e2,e3e^1,e^2,e^3e1,e2,e3; its corners in cyclic order are x,  x+u,  x+u+v,  x+vx,\;x+u,\;x+u+v,\;x+vx,x+u,x+u+v,x+v. On every plaquette a relation g(f1,f2,f3,f4)=0g(f_1,f_2,f_3,f_4)=0g(f1​,f2​,f3​,f4​)=0 is imposed such that any three entries determine the fourth uniquely. The relations may differ from plaquette to plaquette. On the unit cube with corners A=0A=0A=0, B=e1B=e^1B=e1, D=e2D=e^2D=e2, E=e3E=e^3E=e3, C=e1+e2C=e^1+e^2C=e1+e2, F=e1+e3F=e^1+e^3F=e1+e3, H=e2+e3H=e^2+e^3H=e2+e3, G=e1+e2+e3G=e^1+e^2+e^3G=e1+e2+e3, the six face relations are (12a–f). The staircase (eq. (14)) is the sequence

x(3n+1)=x(3n)+e1,x(3n+2)=x(3n+1)−e2,x(3n+3)=x(3n+2)+e3,n∈Z.x(3n+1)=x(3n)+e^1,\qquad x(3n+2)=x(3n+1)-e^2,\qquad x(3n+3)=x(3n+2)+e^3,\qquad n\in\mathbb Z .x(3n+1)=x(3n)+e1,x(3n+2)=x(3n+1)−e2,x(3n+3)=x(3n+2)+e3,n∈Z.

A family of face relations is consistent (eq. (16)) if every choice of f(A),f(B),f(D),f(E)f(A),f(B),f(D),f(E)f(A),f(B),f(D),f(E) extends to data on the cube satisfying all six relations; equivalently, the three values of f(G)f(G)f(G) produced by (12b), (12d), (12f) agree. Linear relations (eq. (17)) have the form ∑jajfj+b≡0(modp)\sum_j a_j f_j+b \equiv 0 \pmod p∑j​aj​fj​+b≡0(modp), with every aja_jaj​ invertible mod ppp.

Formalization targets

Goal: the staircase determines everything

For any family of plaquette relations with the three-determine-the-fourth property, two solutions on Z3\mathbb Z^3Z3 that agree on the staircase agree everywhere:

(∀n∈Z: f(x(n))=f′(x(n))) ⟹ f=f′.\Big(\forall n\in\mathbb Z:\ f(x(n))=f'(x(n))\Big)\ \Longrightarrow\ f=f' .(∀n∈Z: f(x(n))=f′(x(n))) ⟹ f=f′.

Milestones

  1. Eqs. (4)–(8): T<C3Z−1/4V−1/6T<C_3Z^{-1/4}V^{-1/6}T<C3​Z−1/4V−1/6 and S<C4Z1/4V1/2=C5Z1/4A3/4S<C_4Z^{1/4}V^{1/2}=C_5Z^{1/4}A^{3/4}S<C4​Z1/4V1/2=C5​Z1/4A3/4 for the thermal gas.
  2. Eqs. (9)–(11): black holes that fit inside the sphere have total entropy <A/4<A/4<A/4, and A/4A/4A/4 is the supremum.
  3. Discussion of Fig. 1: on one cube, the data at D,H,E,FD,H,E,FD,H,E,F determine all eight corners.
  4. Eqs. (17)–(19): consistent linear relations with invertible coefficients exist for every modulus p≥2p\ge 2p≥2.
  5. Eqs. (14), (17): for the linear relation f1−f2+f3−f4≡0f_1-f_2+f_3-f_4\equiv0f1​−f2​+f3​−f4​≡0, any data on the staircase extend uniquely to a global solution. The staircase data are then exactly the free degrees of freedom.

Significance

The goal is the essay's concrete mathematical example of dimensional reduction: in a 2+12+12+1-dimensional lattice model, a one-dimensional set of data carries all the information. Milestone 5 shows that the reduction is sharp in the linear case: no data beyond the staircase are needed, and none of the staircase data are constrained. Milestones 1–2 are the scaling estimates behind the area law Smax⁡=A/4S_{\max}=A/4Smax​=A/4. The physical argument around them (black-hole thermodynamics, the Schwarzschild criterion) is taken as modelling input, not formalized. The results are stated in the essay but, as far as is known, have not been machine-checked.

Difficulty

The local step (one cube, Milestone 3) is elementary. The goal needs a global propagation argument. The staircase is a thin zig-zag line, and each application of a plaquette relation fixes only one new site. So the proof has to show that repeated local determination starting from the line eventually reaches every site of Z3\mathbb Z^3Z3, in both directions along the line and in both transverse directions. Layer-by-layer propagation in t=x1+x2+x3t=x_1+x_2+x_3t=x1​+x2​+x3​ does not apply directly, because the staircase is not a full layer.

Formalization scope

Sites are ℤ × ℤ × ℤ. Data take values in ZMod p for an arbitrary natural number ppp; the uniqueness statements hold for every ppp. The three-determine-the-fourth property is stated with unique existence (∃!\exists!∃!) for each slot, which matches "uniquely determined" in the essay. Relations may depend on the plaquette, so no translation invariance is assumed. Consistency (16) is encoded as extendability of the four free values on the unit cube. In Milestones 1–2 the region is a round sphere of radius RRR, so VVV and AAA are expressions in RRR, and the constants are existentially quantified before all physical variables. Contributions welcome: proofs of each milestone, and further faithful statements from the triangular-lattice model (eqs. (20a–f)).

Selected references

  • G. 't Hooft, Dimensional Reduction in Quantum Gravity, essay in honour of A. Salam, 1993. https://arxiv.org/abs/gr-qc/9310026
  • L. Susskind, The World as a Hologram, J. Math. Phys. 36 (1995) 6377. https://arxiv.org/abs/hep-th/9409089
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Mathematical Physics·Captain: Lucas

Akhmedov Neutrino Physics I: MSW Oscillations at Constant DensityTextbook

Motivation

Neutrinos produced by weak interactions are created in flavour eigenstates (νe\nu_eνe​, νμ\nu_\muνμ​, ντ\nu_\tauντ​), while they propagate as mass eigenstates. When the two bases differ, the flavour content of a neutrino beam oscillates with distance. In ordinary matter this picture is modified: electron neutrinos scatter coherently forward on electrons via the charged current, which adds an extra potential energy VCC=2 GFNeV_{CC}=\sqrt2\,G_F N_eVCC​=2​GF​Ne​ to the νe\nu_eνe​ component only (Wolfenstein 1978). Mikheyev and Smirnov observed that this potential can resonantly enhance the mixing, so that an almost complete flavour conversion is possible even for a tiny vacuum mixing angle — the MSW effect. It is the accepted explanation of the energy dependence of the solar νe\nu_eνe​ deficit and is relevant for neutrinos crossing the Earth and for supernova neutrinos.

This mission formalizes the constant-density result of Section 8.2 of E. Kh. Akhmedov's lecture notes Neutrino physics (hep-ph/0001264): the two-flavour transition probability in matter of constant density, eq. (95), together with the statements that lead to it and follow from it, eqs. (91)–(98).

Setting

Fix the vacuum parameters: the mass-squared difference Δm2=m22−m12∈R\Delta m^2 = m_2^2-m_1^2\in\mathbb RΔm2=m22​−m12​∈R, the neutrino energy E>0E>0E>0, and the vacuum mixing angle θ0∈R\theta_0\in\mathbb Rθ0​∈R. The matter is described by the Fermi constant GFG_FGF​ and the electron number density NeN_eNe​, through the charged-current potential (eq. (87))

VCC=2 GFNe.V_{CC}=\sqrt2\,G_F N_e .VCC​=2​GF​Ne​.

Write a=Δm2/(2E)a=\Delta m^2/(2E)a=Δm2/(2E). After discarding all terms proportional to the identity (common phases), the vector ν(t)=(νe(t),νμ(t))∈C2\nu(t)=(\nu_e(t),\nu_\mu(t))\in\mathbb C^2ν(t)=(νe​(t),νμ​(t))∈C2 of flavour amplitudes evolves by the Schrödinger equation i ν˙=Hνi\,\dot\nu = H\nuiν˙=Hν with the real symmetric MSW Hamiltonian (eq. (91))

H=(−a2cos⁡2θ0+VCCa2sin⁡2θ0a2sin⁡2θ0a2cos⁡2θ0).H=\begin{pmatrix}-\tfrac a2\cos2\theta_0+V_{CC} & \tfrac a2\sin2\theta_0\\[2pt] \tfrac a2\sin2\theta_0 & \tfrac a2\cos2\theta_0\end{pmatrix}.H=(−2a​cos2θ0​+VCC​2a​sin2θ0​​2a​sin2θ0​2a​cos2θ0​​).

The derived quantities are the energy gap in matter (eq. (94)), the oscillation length in matter (eq. (96)) and the oscillation amplitude in matter (eq. (97)):

Δm=(acos⁡2θ0−VCC)2+a2sin⁡22θ0,lm=2πΔm,sin⁡22θ=a2sin⁡22θ0(acos⁡2θ0−VCC)2+a2sin⁡22θ0.\Delta_m=\sqrt{(a\cos2\theta_0-V_{CC})^2+a^2\sin^22\theta_0},\qquad l_m=\frac{2\pi}{\Delta_m},\qquad \sin^22\theta=\frac{a^2\sin^22\theta_0}{(a\cos2\theta_0-V_{CC})^2+a^2\sin^22\theta_0}.Δm​=(acos2θ0​−VCC​)2+a2sin22θ0​​,lm​=Δm​2π​,sin22θ=(acos2θ0​−VCC​)2+a2sin22θ0​a2sin22θ0​​.

The vacuum oscillation length is losc=4πE/Δm2l_{osc}=4\pi E/\Delta m^2losc​=4πE/Δm2 (eq. (61)). Distance and time are identified (L≃tL\simeq tL≃t, units with c=1c=1c=1).

Formalization targets

Goal — transition probability at constant density (eq. (95))

If ν\nuν solves iν˙=Hνi\dot\nu=H\nuiν˙=Hν for all ttt with ν(0)=(1,0)\nu(0)=(1,0)ν(0)=(1,0) (a pure νe\nu_eνe​ is produced at t=0t=0t=0), then for every LLL

∣νμ(L)∣2=sin⁡22θ  sin⁡2 ⁣(πLlm).|\nu_\mu(L)|^2=\sin^22\theta\;\sin^2\!\Big(\frac{\pi L}{l_m}\Big).∣νμ​(L)∣2=sin22θsin2(lm​πL​).

Milestones

  1. Common phases are unobservable (Sec. 8.1, below eq. (89)). Adding c 1c\,\mathbf 1c1 (c∈Rc\in\mathbb Rc∈R) to a Hamiltonian changes a solution only by a phase; multiplying back by eicte^{ict}eict gives a solution for the reduced Hamiltonian with the same component moduli.
  2. Mixing angle in matter (eq. (93)). There is an angle θ\thetaθ with Δmcos⁡2θ=acos⁡2θ0−VCC\Delta_m\cos2\theta=a\cos2\theta_0-V_{CC}Δm​cos2θ=acos2θ0​−VCC​ and Δmsin⁡2θ=asin⁡2θ0\Delta_m\sin2\theta=a\sin2\theta_0Δm​sin2θ=asin2θ0​; in particular tan⁡2θ=asin⁡2θ0/(acos⁡2θ0−VCC)\tan2\theta=a\sin2\theta_0/(a\cos2\theta_0-V_{CC})tan2θ=asin2θ0​/(acos2θ0​−VCC​) whenever the denominator is non-zero.
  3. Matter eigenstates and eigenenergy difference (eqs. (92), (94)). For such θ\thetaθ, (cos⁡θ,−sin⁡θ)(\cos\theta,-\sin\theta)(cosθ,−sinθ) and (sin⁡θ,cos⁡θ)(\sin\theta,\cos\theta)(sinθ,cosθ) are eigenvectors of HHH with eigenvalues (VCC∓Δm)/2(V_{CC}\mp\Delta_m)/2(VCC​∓Δm​)/2, whose difference is Δm\Delta_mΔm​.
  4. Oscillation amplitude (eq. (97)). For such θ\thetaθ and Δm≠0\Delta_m\neq0Δm​=0, sin⁡22θ\sin^2 2\thetasin22θ equals the explicit resonance expression above.
  5. MSW resonance (eq. (98)). The amplitude never exceeds 111, and when asin⁡2θ0≠0a\sin2\theta_0\ne0asin2θ0​=0 it equals 111 exactly when 2 GFNe=Δm22Ecos⁡2θ0\sqrt2\,G_FN_e=\frac{\Delta m^2}{2E}\cos2\theta_02​GF​Ne​=2EΔm2​cos2θ0​.
  6. Vacuum limit (text below eq. (96)). For Ne=0N_e=0Ne​=0 and Δm2≠0\Delta m^2\ne0Δm2=0: sin⁡22θ=sin⁡22θ0\sin^22\theta=\sin^22\theta_0sin22θ=sin22θ0​ and lm=∣losc∣l_m=|l_{osc}|lm​=∣losc​∣.

Significance

Eq. (95) shows that at constant density the flavour transition has exactly the vacuum form with θ0,losc\theta_0,l_{osc}θ0​,losc​ replaced by θ,lm\theta,l_mθ,lm​; together with the resonance condition (98) it underlies quantitative discussions of matter effects, from the solar neutrino problem to long-baseline experiments crossing the Earth. The milestones separate the linear-algebra content (diagonalizing a real symmetric 2×22\times22×2 matrix) from the analytic content (solving a linear constant-coefficient ODE and the uniqueness of its solution).

The result is textbook material and is proved in the source. This mission adds a machine-checked derivation from the Schrödinger equation itself — including uniqueness of the solution of the initial-value problem, which the source leaves implicit — and reusable Lean definitions for later missions on the adiabatic (variable-density) regime of Section 8.3.

Difficulty

The algebra of eqs. (93)–(97) is elementary. The substantive step for a formal proof is the passage from "the Hamiltonian is diagonalized by a rotation" to "every solution of the ODE with the given initial datum has the stated νμ\nu_\muνμ​ component": this needs a uniqueness theorem for linear ODEs on C2\mathbb C^2C2 (or an equivalent argument). Degenerate parameter values (Δm=0\Delta_m=0Δm​=0, asin⁡2θ0=0a\sin2\theta_0=0asin2θ0​=0) must be handled, since the Lean statements do not exclude them.

Formalization scope

All parameters are real numbers; the state is a function ν:R→C2\nu:\mathbb R\to\mathbb C^{2}ν:R→C2 (index 0=νe0=\nu_e0=νe​, 1=νμ1=\nu_\mu1=νμ​) assumed differentiable everywhere with derivative −i Hν(t)-i\,H\nu(t)−iHν(t), where HHH is the real matrix above viewed as a complex matrix. The probability is the squared modulus ∣νμ(L)∣2|\nu_\mu(L)|^2∣νμ​(L)∣2. E>0E>0E>0 is assumed throughout; the sign of Δm2\Delta m^2Δm2, the value of θ0\theta_0θ0​ and the density are unrestricted. Lean's division convention (x/0=0x/0=0x/0=0) applies to lml_mlm​ and sin⁡22θ\sin^22\thetasin22θ when Δm=0\Delta_m=0Δm​=0; in that degenerate case HHH is a multiple of the identity and both sides of the goal are 000.

A statement that assumed the closed-form solution, or assumed the probability formula as a hypothesis, would be trivial; the goal instead quantifies over every solution of the initial-value problem. Proofs of any milestone, and reusable lemmas on uniqueness for linear constant-coefficient ODEs, are welcome.

Selected references

  • E. Kh. Akhmedov, Neutrino physics, Trieste Summer School lectures, 1999. https://arxiv.org/abs/hep-ph/0001264
  • L. Wolfenstein, Neutrino oscillations in matter, Phys. Rev. D 17 (1978) 2369. https://doi.org/10.1103/PhysRevD.17.2369
  • S. P. Mikheyev, A. Yu. Smirnov, Resonance enhancement of oscillations in matter and solar neutrino spectroscopy, Sov. J. Nucl. Phys. 42 (1985) 913.
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Linear algebraMathematical Physics·Captain: Lucas

Davidson–Nardi–Nir 2008 (Leptogenesis), Eq. (5.10): upper bound on the flavoured CP asymmetry in N1 decaysResearch Paper

Motivation

Leptogenesis is a class of scenarios in which the baryon asymmetry of the Universe is produced from a lepton asymmetry generated in the out-of-equilibrium decays of heavy singlet neutrinos NkN_kNk​, which also give the light neutrinos their small masses through the type I seesaw (Fukugita–Yanagida 1986). The review of Davidson, Nardi and Nir (Phys. Rep. 466 (2008) 105) collects the standard results of the field. One of its central quantitative facts is an upper bound on the CP asymmetry in the decays of the lightest singlet N1N_1N1​, in terms of M1M_1M1​ and the light-neutrino masses. This bound is the origin of the familiar lower bound M1≳109 M_1\gtrsim10^9\,M1​≳109GeV for thermal leptogenesis with hierarchical singlets (Eq. (5.12) of the review).

Timeline. Casas and Ibarra introduced the orthogonal-matrix parametrization of the seesaw in 2001 (hep-ph/0103065). Davidson and Ibarra derived the bound ∣ε∣≤3M1(m3−m1)/(16πv2)|\varepsilon|\le 3M_1(m_3-m_1)/(16\pi v^2)∣ε∣≤3M1​(m3​−m1​)/(16πv2) on the total asymmetry in 2002 (hep-ph/0202239); Hamaguchi, Murayama and Yanagida gave a related bound (hep-ph/0109030). Once flavour effects were recognised (around 2006), attention moved to the flavoured asymmetries εαα\varepsilon_{\alpha\alpha}εαα​, whose bound (Eq. (5.10) of the review) is the goal of this mission.

Setting

There are three lepton flavours α\alphaα and three singlets NkN_kNk​ with Majorana masses Mk>0M_k>0Mk​>0. We work in the mass basis of the charged leptons and of the NkN_kNk​. The Yukawa matrix λ\lambdaλ is an arbitrary complex 3×33\times33×3 matrix, and v=vu>0v=v_u>0v=vu​>0 is the Higgs vev. The light-neutrino mass matrix (Eq. (2.5)) is

[m]αβ=∑kλαkMk−1λβkv2,[m]_{\alpha\beta}=\sum_k\lambda_{\alpha k}M_k^{-1}\lambda_{\beta k}v^2 ,[m]αβ​=k∑​λαk​Mk−1​λβk​v2,

a complex symmetric matrix. It is diagonalized as m=U∗DmU†m=U^*D_mU^\daggerm=U∗Dm​U† with UUU unitary and Dm=diag⁡(m1,m2,m3)D_m=\operatorname{diag}(m_1,m_2,m_3)Dm​=diag(m1​,m2​,m3​), mi≥0m_i\ge0mi​≥0 (Eq. (2.6)). The largest and smallest light masses are mmax⁡m_{\max}mmax​ and mmin⁡m_{\min}mmin​. The Casas–Ibarra matrix is R=Dm−1/2UTλDM−1/2vR=D_m^{-1/2}U^T\lambda D_M^{-1/2}vR=Dm−1/2​UTλDM−1/2​v (Eq. (2.11)).

At tree level N1N_1N1​ decays into ϕℓα\phi\ell_\alphaϕℓα​ and ϕˉℓˉα\bar\phi\bar\ell_\alphaϕˉ​ℓˉα​ with partial rate Γαα=∣λα1∣2M1/(8π)\Gamma_{\alpha\alpha}=|\lambda_{\alpha1}|^2M_1/(8\pi)Γαα​=∣λα1​∣2M1​/(8π) and total rate ΓD=[λ†λ]11M1/(8π)\Gamma_D=[\lambda^\dagger\lambda]_{11}M_1/(8\pi)ΓD​=[λ†λ]11​M1​/(8π) (Eq. (4.5)). So the branching fractions satisfy Bϕℓα+Bϕˉℓˉα=Γαα/ΓDB_{\phi\ell_\alpha}+B_{\bar\phi\bar\ell_\alpha}=\Gamma_{\alpha\alpha}/\Gamma_DBϕℓα​​+Bϕˉ​ℓˉα​​=Γαα​/ΓD​. For hierarchical singlets the flavoured CP asymmetry is (Eq. (5.9))

εαα=3M116πv2[λ†λ]11Im⁡{[λ]α1[m∗λ]α1}.\varepsilon_{\alpha\alpha}=\frac{3M_1}{16\pi v^2[\lambda^\dagger\lambda]_{11}}\operatorname{Im}\{[\lambda]_{\alpha1}[m^*\lambda]_{\alpha1}\}.εαα​=16πv2[λ†λ]11​3M1​​Im{[λ]α1​[m∗λ]α1​}.

Formalization targets

Goal — Eq. (5.10)

∣εαα∣≤3M1mmax⁡16πv2Bϕℓα+Bϕˉℓˉαfor every flavour α.|\varepsilon_{\alpha\alpha}|\le\frac{3M_1m_{\max}}{16\pi v^2}\sqrt{B_{\phi\ell_\alpha}+B_{\bar\phi\bar\ell_\alpha}}\qquad\text{for every flavour }\alpha.∣εαα​∣≤16πv23M1​mmax​​Bϕℓα​​+Bϕˉ​ℓˉα​​​for every flavour α.

Milestones

  1. Eq. (2.6): the matrix mmm admits a diagonalization m=U∗DmU†m=U^*D_mU^\daggerm=U∗Dm​U† with UUU unitary and mi≥0m_i\ge0mi​≥0.
  2. Eq. (2.11): for mi>0m_i>0mi​>0, RRR is complex orthogonal, RTR=RRT=1R^TR=RR^T=1RTR=RRT=1.
  3. Sec. 5.2: ∣m⋅x∗∣≤mmax⁡∣x∣|m\cdot x^*|\le m_{\max}|x|∣m⋅x∗∣≤mmax​∣x∣ for all x∈C3x\in\mathbb C^3x∈C3.
  4. Sec. 5.2 / Eq. (5.17): the total asymmetry bound ∣∑αεαα∣≤3M1(mmax⁡−mmin⁡)/(16πv2)|\sum_\alpha\varepsilon_{\alpha\alpha}|\le 3M_1(m_{\max}-m_{\min})/(16\pi v^2)∣∑α​εαα​∣≤3M1​(mmax​−mmin​)/(16πv2).

Significance

Eq. (5.10) is the input to the lower bounds on M1M_1M1​ and on the reheat temperature for hierarchical thermal leptogenesis (Eq. (5.12), Sec. 9.4.3), and it shows that flavoured asymmetries are not suppressed for degenerate light neutrinos, unlike the total one (Eq. (5.17)). These are established results. The work here is to formalize them: to state the seesaw quantities precisely and machine-check the linear-algebra steps (Takagi factorization, complex orthogonality, operator-norm bounds) that the physics literature takes for granted. To the captain's knowledge none of these statements has a machine-checked proof.

Difficulty

The goal reduces to an operator-norm estimate for the complex symmetric matrix mmm. That estimate needs the diagonalization m=U∗DmU†m=U^*D_mU^\daggerm=U∗Dm​U†, which is a Takagi (Autonne–Takagi) factorization, not a unitary eigen-decomposition: mmm is symmetric, not Hermitian. The obvious move, applying the spectral theorem to mmm, fails because mmm is in general not normal. The milestone-1 existence statement therefore needs its own argument, for example through the Hermitian matrix m†mm^\dagger mm†m. The total-asymmetry bound (milestone 4) needs a finer argument than the triangle inequality to produce the difference mmax⁡−mmin⁡m_{\max}-m_{\min}mmax​−mmin​ rather than mmax⁡m_{\max}mmax​.

Formalization scope

  • Everything is 3×33\times33×3 over C\mathbb CC with index set {0,1,2}\{0,1,2\}{0,1,2} (Fin 3); the singlet "N1N_1N1​" is index 000.
  • mmax⁡m_{\max}mmax​ and mmin⁡m_{\min}mmin​ are ⨆ i, masses i and ⨅ i, masses i over the three diagonal entries. No ordering of the mim_imi​ is imposed.
  • The diagonalization is a hypothesis IsLightMassDiagonalization m U masses (unitary UUU, mi≥0m_i\ge0mi​≥0, m=U‾ diag(mi) U†m=\overline U\,\mathrm{diag}(m_i)\,U^\daggerm=Udiag(mi​)U†). It is always satisfiable by milestone 1, so it is not vacuous.
  • εαα\varepsilon_{\alpha\alpha}εαα​ is the explicit hierarchical-limit expression (5.9), with [λ†λ]11[\lambda^\dagger\lambda]_{11}[λ†λ]11​ written as ∑β∣λβ1∣2\sum_\beta|\lambda_{\beta1}|^2∑β​∣λβ1​∣2. The physical approximation M2,3≫M1M_{2,3}\gg M_1M2,3​≫M1​ is built into this formula and is not a hypothesis. The branching sum is the tree-level ratio Γαα/ΓD\Gamma_{\alpha\alpha}/\Gamma_DΓαα​/ΓD​.
  • Division by zero returns 000 in Lean. This only matters when the first column of λ\lambdaλ vanishes, where both sides of the goal are 000.
  • Needed infrastructure: Takagi factorization of complex symmetric matrices (reusable beyond this mission), and elementary Euclidean-norm estimates on C3\mathbb C^3C3.

Selected references

  • S. Davidson, E. Nardi, Y. Nir, Leptogenesis, Physics Reports 466 (2008) 105–177. https://doi.org/10.1016/j.physrep.2008.06.002 · https://arxiv.org/abs/0802.2962
  • J. A. Casas, A. Ibarra, Oscillating neutrinos and μ → e γ, Nucl. Phys. B 618 (2001) 171. https://arxiv.org/abs/hep-ph/0103065
  • S. Davidson, A. Ibarra, A lower bound on the right-handed neutrino mass from leptogenesis, Phys. Lett. B 535 (2002) 25. https://arxiv.org/abs/hep-ph/0202239
  • M. Fukugita, T. Yanagida, Baryogenesis without grand unification, Phys. Lett. B 174 (1986) 45. https://doi.org/10.1016/0370-2693(86)91126-3
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Mathematical Physics·Captain: Lucas

Thorn 1991: String Bits and the 1/N Expansion — Discretized-String SpectrumResearch Paper

Motivation

In the note Reformulating String Theory with the 1/N Expansion (arXiv:hep-th/9405069), C. B. Thorn argues that stability and causality, which are manifest in quantum field theory but obscure in string theory, would become evident if strings were composite objects built from point-like constituents ("string bits"). The proposal combines the light-cone parametrization of the string with 't Hooft's 1/N1/N1/N expansion (G. 't Hooft, Nucl. Phys. B72 (1974) 461): bits are created by the entries of an N×NN\times NN×N matrix field aˉ(x)\bar a(x)aˉ(x), closed strings by the singlet traces tr{aˉ(x1)⋯aˉ(xM)}\mathrm{tr}\{\bar a(x_1)\cdots\bar a(x_M)\}tr{aˉ(x1​)⋯aˉ(xM​)}, and 1/N1/N1/N plays the role of the string coupling.

A load-bearing step of the proposal is that a long closed chain of MMM bits behaves like a continuous string: in the continuum limit M→∞M\to\inftyM→∞ with P+=MϵT0P^+=M\epsilon T_0P+=MϵT0​ fixed, the finite-energy excitations must be string excitations. Thorn justifies this with the remark (p. 5) that "the low energy excitations of an MMM particle discretized string are O(1/M)×O(1/M)\timesO(1/M)× the two-body level spacing". This mission formalizes that remark for the harmonic Hamiltonian written in the paper, together with the cyclic symmetry that ties the matrix traces to closed strings.

Setting

A discretized light-cone string with MMM bits is described by transverse positions x1,…,xMx_1,\dots,x_Mx1​,…,xM​ with cyclic identification xM+1=x1x_{M+1}=x_1xM+1​=x1​ and Hamiltonian (p. 4)

P−=1ϵ∑i=1M12T0(−∇i2+T02 (xi+1−xi)2).P^- = \frac1\epsilon\sum_{i=1}^{M}\frac{1}{2T_0}\Bigl(-\nabla_i^2 + T_0^2\,(x_{i+1}-x_i)^2\Bigr).P−=ϵ1​i=1∑M​2T0​1​(−∇i2​+T02​(xi+1​−xi​)2).

The potential term is the quadratic form of the cyclic Laplacian LML_MLM​, (LMx)i=2xi−xi+1−xi−1(L_Mx)_i=2x_i-x_{i+1}-x_{i-1}(LM​x)i​=2xi​−xi+1​−xi−1​ (indices mod MMM), and the equations of motion are x¨=−ϵ−2LMx\ddot x=-\epsilon^{-2}L_Mxx¨=−ϵ−2LM​x. A normal-mode frequency is an ω>0\omega>0ω>0 with ϵ2ω2\epsilon^2\omega^2ϵ2ω2 an eigenvalue of LML_MLM​; write ΩM,ϵ\Omega_{M,\epsilon}ΩM,ϵ​ for the set of them. With ℏ=1\hbar=1ℏ=1 these are the excitation-level spacings of the chain.

The singlet creation operators are Aˉ(x1,…,xM)=(1/N)M/2tr{aˉ(x1)⋯aˉ(xM)}\bar A(x_1,\dots,x_M)=(1/N)^{M/2}\mathrm{tr}\{\bar a(x_1)\cdots\bar a(x_M)\}Aˉ(x1​,…,xM​)=(1/N)M/2tr{aˉ(x1​)⋯aˉ(xM​)}; since the aˉkℓ\bar a_{k\ell}aˉkℓ​ commute with each other, cyclic invariance of the trace gives the cyclic symmetry ψM(x1,…,xM)=ψM(x2,…,xM,x1)\psi_M(x_1,\dots,x_M)=\psi_M(x_2,\dots,x_M,x_1)ψM​(x1​,…,xM​)=ψM​(x2​,…,xM​,x1​) of the string wave function.

Formalization targets

Goal

For all M≥2M\ge2M≥2 and ϵ>0\epsilon>0ϵ>0,

min⁡ΩM,ϵ=2ϵsin⁡πM,min⁡Ω2,ϵ=2ϵ,min⁡ΩM,ϵ≤πM min⁡Ω2,ϵ.\min\Omega_{M,\epsilon}=\frac2\epsilon\sin\frac\pi M,\qquad \min\Omega_{2,\epsilon}=\frac2\epsilon,\qquad \min\Omega_{M,\epsilon}\le\frac\pi M\,\min\Omega_{2,\epsilon}.minΩM,ϵ​=ϵ2​sinMπ​,minΩ2,ϵ​=ϵ2​,minΩM,ϵ​≤Mπ​minΩ2,ϵ​.

Milestones

  1. Cyclic symmetry: tr(a0a1⋯aM)=tr(a1⋯aMa0)\mathrm{tr}(a_0a_1\cdots a_M)=\mathrm{tr}(a_1\cdots a_Ma_0)tr(a0​a1​⋯aM​)=tr(a1​⋯aM​a0​) for matrices over a commutative ring.
  2. The bond potential is a quadratic form: ∑i(xi+1−xi)2=xTLMx\sum_i(x_{i+1}-x_i)^2=x^{\mathsf T}L_Mx∑i​(xi+1​−xi​)2=xTLM​x.
  3. Each 4sin⁡2(πk/M)4\sin^2(\pi k/M)4sin2(πk/M) is an eigenvalue of LML_MLM​ (M≥1M\ge1M≥1).
  4. Every eigenvalue of LML_MLM​ is 4sin⁡2(πk/M)4\sin^2(\pi k/M)4sin2(πk/M) for some 0≤k<M0\le k<M0≤k<M.

Significance

The goal is the quantitative content of the paper's continuum-limit argument in the harmonic case: the gap of an MMM-bit chain closes like 1/M1/M1/M relative to the two-body scale, so at fixed P+P^+P+ the low-lying spectrum approaches the equally spaced string spectrum. The same spectral facts about the cyclic Laplacian (the spectrum of the cycle graph) are used in lattice field theory and spectral graph theory, so the milestones are reusable outside this mission. The results are classical; the work here is their machine-checked formalization in a form tied to the string-bit Hamiltonian.

Difficulty

The trace and quadratic-form statements are finite algebra. The substance lies in the spectrum: exhibiting real eigenvectors for every kkk needs trigonometric sum identities, and the completeness statement needs an argument that no other eigenvalues exist, which must handle the degenerate pairs k↔M−kk\leftrightarrow M-kk↔M−k. Identifying the least positive value then requires the symmetry sin⁡(πk/M)=sin⁡(π(M−k)/M)\sin(\pi k/M)=\sin(\pi(M-k)/M)sin(πk/M)=sin(π(M−k)/M) and monotonicity of sin⁡\sinsin on [0,π/2][0,\pi/2][0,π/2].

Formalization scope

  • LML_MLM​ is a real matrix indexed by Fin M\mathrm{Fin}\,MFinM; eigenvalues are those of the real linear map x↦LMxx\mapsto L_Mxx↦LM​x (nonzero real eigenvector).
  • One transverse dimension is used; with d−2d-2d−2 transverse dimensions the modes decouple and the frequency set is the same. The tension T0T_0T0​ drops out of the frequencies.
  • "Two-body level spacing" is formalized as the lowest frequency of the M=2M=2M=2 member of the same cyclic family. The paper's claim for a general attractive potential VVV (and the quantum field theory, the 1/N1/N1/N expansion itself, and the postscript remarks) is outside the scope.
  • Edge cases: the goal assumes M≥2M\ge2M≥2 and ϵ>0\epsilon>0ϵ>0, so ΩM,ϵ\Omega_{M,\epsilon}ΩM,ϵ​ is nonempty and its minimum is attained; the definition of Ω\OmegaΩ requires ω>0\omega>0ω>0, which excludes the zero mode.

Selected references

  • C. B. Thorn, Reformulating String Theory with the 1/N Expansion, invited talk, First Int. A. D. Sakharov Conference (1991); arXiv:hep-th/9405069 (1994). https://arxiv.org/abs/hep-th/9405069
  • G. 't Hooft, A planar diagram theory for strong interactions, Nucl. Phys. B72 (1974) 461.
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Mathematical PhysicsProbability·Captain: Lucas

Douglas 2003: Statistics of String Vacua — Flux Counting and Gaussian EnsemblesResearch Paper

Motivation

String/M theory appears to admit a very large number of four-dimensional vacua, and M. R. Douglas's 2003 paper The statistics of string/M theory vacua proposes to study them statistically: instead of constructing vacua one at a time, one places a measure on a space of effective theories and computes expected numbers and distributions of vacua. Two concrete mathematical ingredients of that programme are the subject of this mission.

The first is the Bousso–Polchinski counting of flux vacua (Section 3.6 of the paper, following Bousso–Polchinski 2000). Quantized fluxes form an integer vector N∈ZJN\in\mathbb Z^JN∈ZJ, and the flux energy is a positive quadratic form in NNN. The number of flux choices with energy below VVV controls whether a small cosmological constant can be realised; the paper evaluates the number distribution (3.13) by replacing the lattice sum with an integral, obtaining a density proportional to VJ/2−1 dVV^{J/2-1}\,dVVJ/2−1dV.

The second is the Gaussian ensemble of superpotentials (Section 4 and 4.1): a random polynomial superpotential whose coefficients are independent complex Gaussians, with an explicit normalising constant and an explicit count of coefficients.

Setting

Fix an integer J≥0J\ge 0J≥0 (the number of independent flux quanta, J=bp+1J=b_{p+1}J=bp+1​ in the paper) and a constant c>0c>0c>0 (in the paper c=Mpl2/(M2pVp+12)c=M_{pl}^2/(M^{2p}V_{p+1}^2)c=Mpl2​/(M2pVp+12​)). For a flux vector N=(N1,…,NJ)∈ZJN=(N_1,\dots,N_J)\in\mathbb Z^JN=(N1​,…,NJ​)∈ZJ the flux potential is

V(N)=c∑i=1JNi2,V(N)=c\sum_{i=1}^J N_i^2 ,V(N)=ci=1∑J​Ni2​,

and the flux vacua count below level VVV is

NJ(c,V)=#{N∈ZJ:V(N)≤V}.\mathcal N_J(c,V)=\#\{N\in\mathbb Z^J : V(N)\le V\}.NJ​(c,V)=#{N∈ZJ:V(N)≤V}.

This is the cumulative distribution function of the measure dμ(V)=∑Nδ(V−V(N))d\mu(V)=\sum_N\delta(V-V(N))dμ(V)=∑N​δ(V−V(N)) of eq. (3.13). The unit ball in RJ\mathbb R^JRJ has volume ωJ=πJ/2/Γ(J/2+1)\omega_J=\pi^{J/2}/\Gamma(J/2+1)ωJ​=πJ/2/Γ(J/2+1), and the unit sphere has area Vol(SJ−1)=2πJ/2/Γ(J/2)=JωJ\mathrm{Vol}(S^{J-1})=2\pi^{J/2}/\Gamma(J/2)=J\omega_JVol(SJ−1)=2πJ/2/Γ(J/2)=JωJ​.

For the superpotential ensemble, a polynomial in nnn variables of degree at most ddd has one coefficient per monomial zI=z1I1⋯znInz^{I}=z_1^{I_1}\cdots z_n^{I_n}zI=z1I1​​⋯znIn​​ with ∣I∣≤d|I|\le d∣I∣≤d; the paper states there are c(d,n)=(d+n)!/(d! n!)c(d,n)=(d+n)!/(d!\,n!)c(d,n)=(d+n)!/(d!n!) of them. The coefficients wI∈Cw_I\in\mathbb CwI​∈C are given the weight (α/π)c(d,n)∏Id2wI e−α∣wI∣2(\alpha/\pi)^{c(d,n)}\prod_I d^2w_I\,e^{-\alpha|w_I|^2}(α/π)c(d,n)∏I​d2wI​e−α∣wI​∣2, α>0\alpha>0α>0, which the paper says is unit normalised.

Formalization targets

Goal: asymptotic count of flux vacua

lim⁡V→∞NJ(c,V)(V/c)J/2=πJ/2Γ(J/2+1).\lim_{V\to\infty}\frac{\mathcal N_J(c,V)}{(V/c)^{J/2}}=\frac{\pi^{J/2}}{\Gamma(J/2+1)} .V→∞lim​(V/c)J/2NJ​(c,V)​=Γ(J/2+1)πJ/2​.

This is the precise, integrated form of the approximation in (3.13): integrating 12Vol(SJ−1) c−J/2vJ/2−1\tfrac12\mathrm{Vol}(S^{J-1})\,c^{-J/2}v^{J/2-1}21​Vol(SJ−1)c−J/2vJ/2−1 from 000 to VVV gives exactly ωJ(V/c)J/2\omega_J (V/c)^{J/2}ωJ​(V/c)J/2.

Milestones

  1. Finiteness: for every VVV, only finitely many N∈ZJN\in\mathbb Z^JN∈ZJ satisfy V(N)≤VV(N)\le VV(N)≤V (so NJ\mathcal N_JNJ​ is a genuine count).
  2. Continuum volume: the Lebesgue volume of {x∈RJ:c∑xi2≤V}\{x\in\mathbb R^J : c\sum x_i^2\le V\}{x∈RJ:c∑xi2​≤V} equals ωJ(V/c)J/2\omega_J (V/c)^{J/2}ωJ​(V/c)J/2 for V≥0V\ge 0V≥0.
  3. Continuum density (3.13): for 0≤V1≤V20\le V_1\le V_20≤V1​≤V2​ and J≥1J\ge1J≥1, the volume of the shell {V1<c∑xi2≤V2}\{V_1<c\sum x_i^2\le V_2\}{V1​<c∑xi2​≤V2​} equals ∫V1V212Vol(SJ−1) c−J/2 vJ/2−1 dv\int_{V_1}^{V_2}\tfrac12\mathrm{Vol}(S^{J-1})\,c^{-J/2}\,v^{J/2-1}\,dv∫V1​V2​​21​Vol(SJ−1)c−J/2vJ/2−1dv.
  4. Coefficient count: #{I∈Nn:∣I∣≤d}=#{I∈Nn+1:∣I∣=d}=(d+n)!/(d! n!)\#\{I\in\mathbb N^n : |I|\le d\}=\#\{I\in\mathbb N^{n+1} : |I|=d\}=(d+n)!/(d!\,n!)#{I∈Nn:∣I∣≤d}=#{I∈Nn+1:∣I∣=d}=(d+n)!/(d!n!).
  5. Normalisation of the complex Gaussian ensemble: ∫Cm(α/π)me−α∑I∣wI∣2 d2mw=1\int_{\mathbb C^m}(\alpha/\pi)^m e^{-\alpha\sum_I|w_I|^2}\,d^{2m}w=1∫Cm​(α/π)me−α∑I​∣wI​∣2d2mw=1 for every mmm and α>0\alpha>0α>0.

Significance

The goal makes rigorous the step "replace the sum with an integral" that underlies the Bousso–Polchinski estimate of how many flux vacua lie below a given energy, with the exact constant appearing in (3.13). Milestones 4 and 5 certify the combinatorial and analytic constants of the Gaussian ensemble (4.6) on which the paper's densities (4.7)–(4.10) are built. None of these results is new mathematics: the goal is the JJJ-dimensional analogue of the Gauss circle problem at leading order, and the milestones are classical. What the mission adds is a machine-checked version of the precise constants used in the paper.

Difficulty

The goal requires comparing a lattice-point count with a volume. The naive bound, counting unit cubes centred at lattice points, must be controlled uniformly: cubes meeting the boundary of the ball contribute an error of order RJ−1R^{J-1}RJ−1 with R=V/cR=\sqrt{V/c}R=V/c​, and one has to show that this is o(RJ)o(R^J)o(RJ). The volume formula for Euclidean balls expressed through the Gamma function, and its transport to the product space RJ\mathbb R^JRJ with the sum-of-squares form, is further required infrastructure.

Formalization scope

  • Flux vectors are functions Fin J → ℤ; the count uses Set.ncard, whose value on an infinite set would be 000 — milestone 1 rules out that degenerate reading.
  • Continuum statements use the product Lebesgue measure on Fin J → ℝ (not EuclideanSpace), with the quadratic form c∑xi2c\sum x_i^2c∑xi2​ written out explicitly.
  • The Gaussian ensemble is formalised only for complex coefficients (the "GUE" case). For real coefficients the paper's constant (α/π)c(d,n)(\alpha/\pi)^{c(d,n)}(α/π)c(d,n) would not normalise the measure (the correct constant is (α/π)c(d,n)/2(\alpha/\pi)^{c(d,n)/2}(α/π)c(d,n)/2), so the real case is deliberately omitted.
  • The paper's finiteness conjecture (3.16) for full string compactifications, and the densities (4.7)–(4.10), are not formalised; they are not stated precisely enough in the source.
  • Definitions: DouglasVacua.fluxPotential, DouglasVacua.fluxVacuaCount.

Selected references

  • M. R. Douglas, The statistics of string/M theory vacua, JHEP 05 (2003) 046. https://doi.org/10.1088/1126-6708/2003/05/046 — arXiv:hep-th/0303194
  • R. Bousso, J. Polchinski, Quantization of four-form fluxes and dynamical neutralization of the cosmological constant, JHEP 06 (2000) 006. https://arxiv.org/abs/hep-th/0004134
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