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Ideal photon reservoir and active-area mass-balance model
An adopted zero-mode-excluded ideal photon reservoir and isotropic ray model attached to the positive-mass Schwarzschild stationary family with one fixed asymptotic time and energy normalization. The emitter area is the phenomenological far-field value eta A_H, incoming flux is zero, and the model stops at a strictly positive mass cutoff. The statement is not a time-dependent Einstein solution, a Hawking collapse derivation, a material null-horizon emitter, a measured flux, or a generalized second law.
Postulate
Use SI constants in , in , in , and in . In Exact ideal emitter mass ODE and entropy accounting, the mathematical constant is identified with this same .
For each fixed mass in kilograms, take the zero-angular-momentum, zero-charge member of the selected Kerr–Newman stationary family Physical KN family work and constancy, with geometric mass length in metres. In the Schwarzschild exterior use coordinates , in metres, , and metric
where is the unit-sphere metric. The asymptotic generator is , with at infinity. The selected stationary-family radius, area, and geometric surface gravity are
Thus is in metres, in , and in , using the length-normalized generator convention of Thermodynamics-GR fields, currents, reference normalization and units.
Adopt the selected reduced-model reference temperature from Restricted reversible horizon entropy identification on this Schwarzschild subfamily:
This is an adopted model identification for one fixed asymptotic reference. It is not a local proper-temperature field and does not assert a general Hawking state. The reversible entropy state is the value of the stationary-family state function on each Schwarzschild member; evaluating that family function along a changing parameter is bookkeeping in this model, not a claim that the changing family is an exact spacetime solution.
Adopt the zero-mode-excluded, zero-point-subtracted, two-polarization photon Gibbs model and isotropic freely streaming ray convention of Actual photon box trace and Planck energy/entropy flux, under from The Axiom of Countable Choice (). Its energy density , coarse diagonal-mode entropy density , and one-sided fluxes are those of that theorem. This identification is an ideal reservoir assumption; no photon-wall equilibration theorem or physical preparation is asserted.
Fix , a constant dimensionless active-area fraction, an initial mass , and a positive cutoff . Let be on an interval containing its first cutoff time , with , and let be measured in seconds by the fixed asymptotic time parameter. Define in joules and the effective far-field emitting area
Adopt zero incoming flux, the power law in watts, the balance equation
and the coarse exported entropy rate , with . Here is the entropy carried by the ideal Gibbs/ray model, not an outside von Neumann entropy. The effective area is not a material patch of the null horizon and is not a frequency-independent greybody factor applied separately to entropy.
The model holds only for the fixed normalization . Under , , the model conventions scale , , , and leave unchanged. The Stefan closure above is therefore not stipulated as a reference-independent luminosity law. No experiment, coupled backreaction solution, physical extinction event, or universal generalized second law is adopted.
Depends on
Dependency tree · 2 levels
Sources
- Robert M. Wald, The Thermodynamics of Black Holes, Living Reviews in Relativity 4 (2001), 6
- Pietro Benetti Genolini, Introduction to black hole thermodynamics, lecture notes for the Roberto Salmeron School in Mathematical Physics (2025), arXiv:2512.24929v1
- Mehran Kardar, MIT OpenCourseWare 8.333 Statistical Mechanics I, Lecture 20
- University of Mississippi PHY 727 course notes, Lecture 18: The Photon Gas