Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2000-11-07
Phys.Rev. D63 (2001) 064005
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
6 pages, references added and corrected, approved for publication in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.63.064005
We show that essentially pure classical thermodynamics is sufficient to determine Bekenstein's formula for the black hole's entropy, $S=\eta A$. We base our reasoning on the minimal assumption that since black body radiation is describable by classical thermodynamics, so is the complete black hole-Hawking radiation system. Furthermore, we argue that any non-linear correction to the black hole entropy must be quantum mechanical in nature. The proportionality coefficient, $\eta=1/4\ell_P^2$, must be calculated within a semi-classical or full-fledged quantum mechanical framework.
Gour Gilad
Mayo Avraham E.
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