Radial geodesics as a microscopic origin of black hole entropy. I: Confined under the Schwarzschild horizon

Details Radial geodesics as a microscopic origin of black hole entropy. I: Confined under the Schwarzschild horizon Radial geodesics as a microscopic origin of black hole entropy. I: Confined under the Schwarzschild horizon

2004-12-19

arxiv.org/abs/gr-qc/0412090v3

Phys.Rev. D72 (2005) 124011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages, 12 eps-figures, iopart class, tought experiment (p.7) added

Scientific paper

Causal radial geodesics with a positive interval in the Schwarzschild metric include a subset of trajectories completely confined under a horizon, which compose a thermal statistical ensemble with the Hawking-Gibbons temperature. The Bekenstein--Hawking entropy is given by an action at corresponding geodesics of particles with a summed mass equal to that of black hole in the limit of large mass.

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