Alphabeta Math
Pipeline-generated
How statement and proof provenance work

The first chip identifies the source of the statement or construction; the second identifies the source of its local proof or verification.

  • Literature-sourced: the exact statement appears in a cited source; only wording and notation differ.
  • AI-adapted: a semantically identical restatement of literature-sourced material, modulo indexing, notation, and boundary cases adopted by the library.
  • AI-generated: a genuinely novel statement formulated by AI, with no source for the claim itself.

These labels describe origin, not correctness: citations and verification chips remain separate evidence.

Finite regulated Newtonian gravitational canonical preparation — Examples

1 · Prerequisites

2 · Summary

The companion gives a finite softened two-body canonical instance, a point-particle collapse counterexample in a finite box, a confined Kepler energy with negative Gibbs-volume capacity and nonnegative canonical response under distinct preparations, and a constant-lapse gas normalization. These are exact examples within the stated models; none reports an observation or asserts that a physical system attains the model preparation.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

None yet.

5 · Examples, experiments and counterexamples

ExampleConstruction: AI-adaptedVerification: AI-adaptedprecheck passOpen item page →

Prepared finite softened two-body ensemble

Physical scope

One explicit finite box and positive softening instance of the adopted effective Newtonian preparation; establishes a normalized model probability, not observed equilibration or a claim about a real gravitating gas.

Example

Take B=(0,L)3 with L>0, N=2, equal mass m>0, Newton constant G>0, softening length a>0, action reference h∗>0, and β>0. Use the finite softened Newtonian preparation and its fixed Hamiltonian and measure.

Facts & Assumptions

Given: The cube has volume L3∈(0,∞), N=2, a>0, and all remaining physical parameters are positive as required by the adopted preparation.

[F1]

Under those hypotheses the finite regulated preparation has a positive finite partition function and normalized Gibbs density. (Constructed finite canonical gravitational equilibrium)

Verification

1.1givenF1

The box B=(0,L)3 is bounded and has positive finite volume, and N=2≥2 with a>0; therefore these data satisfy the hypotheses recorded in [F1].

2.1F1step 1.1∎

Apply [F1] to this instance. It gives 0<Z2(β)<∞ and pβ=Z2−1e−βH2,a as a normalized probability density relative to the stated phase reference. This is a constructed model ensemble and does not assert that the system dynamically reaches it.

CounterexampleConstruction: AI-adaptedVerification: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Point-particle preparation has no finite-box canonical law

Physical scope

Refutes finite-volume sufficiency for the exact unregulated two-point Newtonian canonical weight, for arbitrary positive masses. The collision limit is outside a controlled weak-field Newtonian regime and is not asserted to describe a real short-distance source.

Statement refuted

The claim refuted is that an outer finite box alone guarantees a normalizable canonical law for the unregulated two-point Newtonian gravity model. For any labelled positive masses m1,m2, bounded box B⊂R3 with nonempty interior, and β>0, define the collision-free phase domain Γ12cf:={(q1,q2,p1,p2)∈B2×R6:q1≠q2} and let ν12cf be the restriction of ν12 to this domain. The model in Distinct unregulated point-gravity attempted sampling has Z12(β)=∫Γ12cfe−βH12ptdν12cf=+∞. Thus the attempted weight cannot be normalized to a probability density.

Facts & Assumptions

Given: The labelled two-particle phase space, h∗−6 reference measure, off-diagonal Hamiltonian, and β>0 from the adopted unregulated model. The integral is taken on the collision-free phase domain, where the Hamiltonian is defined, with the restricted reference measure.

[A1]

The Postulate defines H12pt=∣p1∣2/(2m1)+∣p2∣2/(2m2)−Gm1m2/∣q1−q2∣ on Γ12cf, with dν12cf the restriction of h∗−6d3q1d3q2d3p1d3p2 to that domain. (Distinct unregulated point-gravity attempted sampling)

[F1]

For two equal positive masses in a bounded three-dimensional box with nonempty interior, the point Hamiltonian's canonical partition integral diverges for every β>0, relative to the identical-particle phase measure. (Point collapse and unscaled gravity nonextensivity)

Counterexample

1.1givenA1F1algebra

If m1=m2=m, the labelled-pair measure restricted to Γ12cf in [A1] is twice the identical-particle reference measure restricted to the same domain, dν2=dν12cf/2. The equal-mass divergence in [F1] therefore also holds for dν12cf, since multiplication of an infinite nonnegative integral by 2 leaves it infinite.

1.2givenA1constructalgebra

Suppose m1≠m2. Choose an interior point q0∈B and a length ℓ>0 metres small enough that, for all sufficiently large integers n, the disjoint cubes Q1,n=q0+(0,ℓ/n)3 and Q2,n=q0+(2ℓ/n,0,0)+(0,ℓ/n)3 lie in B. For q1∈Q1,n and q2∈Q2,n, their separation satisfies ℓ/n<∣q1−q2∣≤11ℓ/n. Fix a momentum scale p0>0 in kg m s−1 and restrict both momenta to [−p0,p0]3; there the kinetic energy is at most K0=3p02/(2m1)+3p02/(2m2). Hence on this positive-volume phase subset, H12pt≤K0−Gm1m2n/(11ℓ) and the Boltzmann weight is at least e−βK0eβGm1m2n/(11ℓ).

2.1A1step 1.1step 1.2algebra∎

The restricted subset in step 1.2 lies in Γ12cf, so its restricted reference measure is h∗−6(ℓ/n)6(2p0)6. Thus Z12(β)≥h∗−6(ℓ/n)6(2p0)6e−βK0eβGm1m2n/(11ℓ) for every sufficiently large n. The right-hand side tends to +∞ because exponential growth dominates n6; therefore the full collision-free nonnegative integral is infinite for m1≠m2. The equal-mass case was established in step 1.1, so no normalized canonical law exists for any positive mass pair in this model.

ExampleConstruction: AI-adaptedVerification: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Confined negative-capacity Kepler preparation

Physical scope

One energy and shell-radius instance of the finite regulated relative Kepler model under its declared Gibbs-volume convention and weak-field restriction; the canonical comparison remains a distinct preparation with unbounded momenta.

Example

Choose m1,m2>0, A=Gm1m2, reduced mass μ=m1m2/(m1+m2), inner radius r0>0, and outer radius R>32r0. Set E=−A/(32r0) and assume 2A/(μr0c2)≤δNR≪1. Use the two preparations and response conventions of the A-page comparison theorem.

Facts & Assumptions

Given: R>32r0, E=−A/(32r0), A,μ,r0>0, and the stated weak-field slow-motion condition.

[F1]

Under these hypotheses, the microcanonical Gibbs-volume response is strictly negative, and the separate canonical response for the same relative Hamiltonian is nonnegative. (Regulated gravitational preparations have different responses)

Verification

1.1givenF1algebra

The selected energy has e=−E=A/(32r0), so A/R<e<A/(16r0) and δ=er0/A=1/32. The weak-field restriction is the condition required in [F1].

2.1F1step 1.1∎

Apply [F1] to this branch point. It gives CG<0 for the declared Gibbs-volume microcanonical preparation and CK≥0 for the separate canonical preparation. These are model deductions about distinct finite ensembles, not measurements or evidence that either preparation is realized.

ExampleConstruction: AI-adaptedVerification: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Fixed lapse two gas normalization

Physical scope

Grand-canonical classical ideal gas on a prescribed flat finite box with constant dimensionless lapse two and a stated Killing-generator normalization; the local temperature parameter is T_K/2 and is not a reported measurement.

Example

Let B=(0,L)3 with L>0, Ix0⊂R open, hij=δij, and constant dimensionless lapse N=2 on the prescribed static metric g=−4(dx0)2+δijdxidxj, with x0=ct. Choose positive particle mass m>0 in kilograms, c>0 in metres per second, action reference h∗>0 in joule-seconds, inverse Killing-energy parameter βK>0 in inverse joules, and dimensionless fugacity z>0. Select the grand-canonical branch, in which particle number is summed rather than fixed. Since the metric coefficients are independent of x0, choose the Killing generator ξ=∂x0 to define TK=(kBβK)−1. This fixes a normalization convention for the generator; TK is not identified with the proper temperature at the wall.

Facts & Assumptions

Given: The spatial box is bounded with positive finite volume, the static metric is prescribed, its lapse is the constant N=2, the Killing generator has the stated normalization, m,c,h∗,βK,z>0, and the grand-canonical branch is selected.

[F1]

On a prescribed bounded-lapse static background, the selected grand-canonical classical gas has 0<Z1<∞, Ξ=ezZ1∈(0,∞), and Tloc=TK/N. (Constructed static gas redshift and hydrostatics)

Verification

1.1givenF1

The constant lapse satisfies 0<N0≤N≤N1<∞ with N0=N1=2, the flat spatial box has positive finite volume, the classical parameters are positive, and the grand-canonical branch is selected; thus [F1] applies.

2.1F1step 1.1algebra∎

Apply [F1] to the selected branch: Z1 is finite and positive and Ξ=ezZ1 is finite and positive. Substituting N=2 gives Tloc=TK/2. These are normalization and parameter identities in the selected model and report no observed temperature.

Sources