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Dynamic black-hole entropy

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

We consider two non-statistical definitions of entropy for dynamic (non-stationary) black holes in spherical symmetry. The first is analogous to the original Clausius definition of thermodynamic entropy: there is a first law containing an energy-supply term which equals surface gravity times a total differential. The second is Wald's Noether-charge method, adapted to dynamic black holes by using the Kodama flow. Both definitions give the same answer for Einstein gravity: one-quarter the area of the trapping horizon.

fields

gr-qc 3

years

2026 3

verdicts

UNVERDICTED 3

representative citing papers

Modified Entropy from Action Principle

gr-qc · 2026-05-28 · unverdicted · novelty 5.0

Authors add f(R, K) to the Einstein-Hilbert action, obtain higher-derivative-free modified Friedmann equations for flat FRW, and derive a general apparent-horizon entropy expression usable for multiple entropy models.

Generalized Mass-to-Horizon Entropy and Horizon Thermodynamics

gr-qc · 2026-05-12 · unverdicted · novelty 3.0

A two-parameter extension of Bekenstein entropy is applied to derive the Friedmann equations and confirm thermodynamic consistency for an accelerating universe via entropy balance and maximization.

citing papers explorer

Showing 3 of 3 citing papers.

  • Modified Entropy from Action Principle gr-qc · 2026-05-28 · unverdicted · none · ref 16 · internal anchor

    Authors add f(R, K) to the Einstein-Hilbert action, obtain higher-derivative-free modified Friedmann equations for flat FRW, and derive a general apparent-horizon entropy expression usable for multiple entropy models.

  • Modified Cosmology from Mass-to-Horizon Relation: Background Evolution gr-qc · 2026-06-30 · unverdicted · none · ref 78 · internal anchor

    Viable generalized horizon entropies from the mass-to-horizon relation are restricted to a narrow neighborhood around the Bekenstein-Hawking law, yielding only Lambda-CDM-like background evolution.

  • Generalized Mass-to-Horizon Entropy and Horizon Thermodynamics gr-qc · 2026-05-12 · unverdicted · none · ref 40 · internal anchor

    A two-parameter extension of Bekenstein entropy is applied to derive the Friedmann equations and confirm thermodynamic consistency for an accelerating universe via entropy balance and maximization.