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Ensembles And Limits — Examples

1 · Prerequisites

2 · Summary

These examples calculate one countable partition sum and three finite probability models. Each example checks definitions and conditional results on the A page; no measurement or physical preparation is asserted.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

None yet.

5 · Examples, experiments and counterexamples

ExampleConstruction: AI-generatedVerification: AI-generatedverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

A lower energy bound does not ensure a countable partition function

Facts & Assumptions

Given: As stated in the item.

[F1]

Countable canonical model: Z is the extended nonnegative sum and a canonical probability law is defined only when 0<Z<∞.

[A1]

The state set is N and every state has zero energy and unit weight.

Example

Take I=N, En=0, and gn=1 for every n. The energy list is bounded below, but Z(β)=+∞ for every real β, so this model has no normalized canonical law.

Verification

Given: The countable model in [F1] with the data in [A1].

1.1F1A1algebra

Every summand is gne−βEn=1, so the first N terms sum to N for every N; their supremum is infinite.

2.1F1step 1.1∎

Thus Z(β)=+∞, which violates the finite-normalization condition in [F1]; no normalized canonical probabilities pn are defined.

ExampleConstruction: AI-generatedVerification: AI-generatedverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

Canonical mean and variance for a two-level system

Facts & Assumptions

Given: As stated in the item.

[F1]

Countable canonical model: the finite partition sum and normalized state weights are defined as stated there.

[F2]

Summable canonical differentiation: a finite energy list has the required local summable moment envelope on every compact parameter interval (each of finitely many terms is bounded there), so −∂βlog⁡Z is the mean and ∂β2log⁡Z is the variance.

[A1]

E0=0, E1=ε>0, g0=g1=1, and β>0.

Example

Let the state set be {0,1}, with energies E0=0, E1=ε>0, unit weights, and β>0. Writing q=e−βε, the excited-state probability is q/(1+q), the mean energy is εq/(1+q), and the energy variance is ε2q/(1+q)2>0.

Verification

Given: The finite canonical model [F1] with data [A1].

1.1F1A1algebra

Direct summation gives Z=1+e−βε=1+q, hence p1=q/(1+q) and p0=1/(1+q).

2.1F1F2A1step 1.1algebra∎

The finite weighted sum gives Eˉ=εp1=εq/(1+q). The second centered moment is p0(0−Eˉ)2+p1(ε−Eˉ)2=ε2q/(1+q)2, which is positive because q∈(0,1). The values also agree with the finite-list derivative identities of [F2].

ExampleConstruction: AI-generatedVerification: AI-generatedverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

A perfectly correlated uniform pair has zero conditional entropy

Facts & Assumptions

Given: As stated in the item.

[F1]

Mutual information of finite random variables: I(M;R)=H(M)+H(R)−H(M,R)=H(M)−H(M∣R).

[F2]

Conditional entropy of finite memory given side information: conditional entropy is computed from the conditional laws on positive-probability register values.

[A1]

The pair law assigns probability 1/2 to (0,0) and (1,1) and zero to the other two pairs.

Example

Let M,R∈{0,1} have joint probabilities p(0,0)=p(1,1)=1/2 and p(0,1)=p(1,0)=0. Then H(M)=H(R)=log⁡2, H(M,R)=log⁡2, H(M∣R)=0, and I(M;R)=log⁡2.

Verification

Given: The finite joint probability law in [A1].

1.1A1algebra

Both marginals are uniform, so their entropies are −2(1/2)log⁡(1/2)=log⁡2. The joint law has two positive entries of size 1/2, so H(M,R)=log⁡2.

2.1F1F2A1step 1.1∎

Conditional on either value of R, M is determined, so its conditional law has one probability 1 and one 0; therefore H(M∣R)=0. Substituting these values into [F1] gives I(M;R)=log⁡2.

ExampleConstruction: AI-generatedVerification: AI-generatedverified 2026-10-15 (gpt-6-luna, gpt-6.1-sol, and delegated Codex review/repair agents; see completed run evidence)Open item page →

A finite canonical law differs from a narrow-shell microcanonical law

Facts & Assumptions

Given: As stated in the item.

[F1]

Countable canonical model: finite canonical probabilities are normalized exponential weights.

[F2]

Summable canonical differentiation: if each compact interval K⊂J admits a summable nonnegative majorant ai with gi(1+∣Ei∣2)e−βEi≤ai for all i and β∈K, then Z is positive, finite and C2 on J, and the canonical law is normalized.

[F3]

The natural logarithm as the inverse of the exponential function identifies the exponential as a bijection from R onto (0,∞); The exponential function is strictly increasing supplies its monotonicity.

[A1]

The state set has energies 0 and ε>0, the weights are one, β>0, and 0<Δ<ε. The finite-shell convention is the uniform law on states with energies in [0,Δ) when the shell is nonempty.

Example

Let a two-state model have energies 0 and ε>0, with unit state weights and β>0. Adopt the finite-shell convention that the microcanonical law is uniform over states whose energy lies in [0,Δ) when the shell is nonempty. For 0<Δ<ε, that shell contains only the ground state, whereas the canonical law assigns the excited state probability e−βε/(1+e−βε)>0. Thus the two finite-ensemble laws differ.

Verification

Given: The finite model and shell convention in [A1].

1.1F1F2F3A1

Take J=(0,∞). For any nonempty compact interval K⊂J, set a0=1 and a1=(1+ε2)e−εmin⁡K. These two finite nonnegative numbers are summable and bound the ground and excited terms in [F2], by [F3]. Thus the hypotheses of [F2] hold on J. The canonical partition sum is 1+e−βε; its excited probability is e−βε/(1+e−βε), strictly positive because the exponential is positive.

2.1A1step 1.1∎

The shell condition 0≤Ei<Δ includes the state of energy zero and excludes the state of energy ε, since Δ<ε. Uniform weighting of this one-state shell gives excited probability zero, which differs from step 1.1.

Sources