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Ideal active-area half-mass cutoff interval

Physical scope

Conditional fixed-asymptotic-reference ideal emitter calculation with eta=1 and a positive half-mass cutoff. The effective area is not a material null-horizon surface, the exported entropy is coarse Gibbs/ray entropy, and the example is not an observation or a duration prediction for an actual evaporating black hole.

Statement

Assume ACω and the conditional model conclusion of Conditional ideal Planck emission and entropy accounting. Choose η=1 and Mmin⁡=M0/2 for M0>0, with GN,c,ℏ,kB as in that theorem. Define the model's algebraic zero-mass time scale

t∗:=M033α=5120πGN2M03ℏc4.

The stipulated model stops earlier, at

τ=78t∗=4480πGN2M03ℏc4,

when its mass parameter first reaches M0/2>0. It exports energy c2M0/2 joules. Its stationary-family entropy drop, coarse photon entropy export, and total coarse entropy gain are respectively

ΔSH=3πkBGNM02ℏc,Srad(τ)=4πkBGNM02ℏc,Δ(SH+Srad)=πkBGNM02ℏc.

For any ϵ0>0, if M02≥ℏc/(1920πGNϵ0), then the model's maximum diagnostic on the closed interval [0,τ], including its positive cutoff endpoint, satisfies ϵqs≤ϵ0. This is an exact ideal-model calculation, not a measured evaporation time or an error estimate for a gravitational backreaction solution.

Facts & Assumptions

Given: ACω, the conditional model conclusion of Conditional ideal Planck emission and entropy accounting, M0>0, and the choices η=1, Mmin⁡=M0/2.

[F1]

Conditional ideal Planck emission and entropy accounting: for the fixed-reference model, M(t∞)=(M03−3αt∞)1/3, τ=(M03−Mmin⁡3)/(3α), energy export is c2(M0−Mmin⁡), Srad=(4/3)ΔSH, and ϵqs=2GNα/(c3M2). These are conditional on the theorem's stated model and ACω.

[A1]

The thought experiment selects η=1 and Mmin⁡=M0/2; M0 remains an arbitrary positive mass parameter, not a measured value.

[A2]

The Axiom of Countable Choice (ACω): ACω is the exact countable-choice principle; no full Axiom of Choice is used.

Proof

Given: The model formulas of [F1] and the exact parameter choices [A1].

1.1givenF1A1A2algebra

With η=1, [F1] gives α=ℏc4/(15360πGN2). Hence t∗=M03/(3α)=5120πGN2M03/(ℏc4), and

τ=M03−(M0/2)33α=(1−18)t∗=78t∗.

The cutoff remains positive, M(τ)=M0/2, so the model does not reach its algebraic zero-mass time.

1.2F1A1A2algebra

The energy export in [F1] is c2(M0−Mmin⁡). Substituting [A1] gives c2M0/2 joules.

1.3givenF1A1A2algebra

By [F1], SH(M)=4πkBGNM2/(ℏc)+s∗ on the selected branch, with an unfixed constant s∗. Subtracting its values at M0 and M0/2 cancels s∗ and gives ΔSH=4πkBGN(3M02/4)/(ℏc)=3πkBGNM02/(ℏc). The entropy export is 4ΔSH/3=4πkBGNM02/(ℏc), and the total gain is ΔSH/3=πkBGNM02/(ℏc).

2.1F1A1A2algebra∎

The maximum diagnostic occurs at M=Mmin⁡=M0/2, so [F1] gives

ϵqs,max=2GNαc3(M0/2)2=8GNαc3M02=ℏc1920πGNM02.

The displayed lower bound on M02 is equivalent, after multiplication by the positive 1920πGNM02ϵ0/(ℏc), to ϵqs,max≤ϵ0. This remains an internal diagnostic for the stipulated ODE, not a comparison with a coupled spacetime solution.

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