Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole

Details Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole Radial geodesics as a microscopic origin of black hole entropy. II: Features of Reissner--Nordstrom black hole

2004-12-21

arxiv.org/abs/gr-qc/0412097v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, 6 eps-figures, iopart class, acknowledgement extended

Scientific paper

The entropy of charged black hole is calculated by using the partition
function evaluated at radial geodesics confined under horizons. We establish
two quantum phase states inside the black hole and a transition between them.

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