Thermodynamics of scalar fields in Kerr's geometry

Details Thermodynamics of scalar fields in Kerr's geometry Thermodynamics of scalar fields in Kerr's geometry

1997-10-28

arxiv.org/abs/gr-qc/9710118v3

Phys.Rev. D57 (1998) 6292-6296

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, LaTex, (revised version-last section modified)

Scientific paper

10.1103/PhysRevD.57.6292

The one-loop contributions to the entropy for a massive scalar field in a
Kerr black hole are investigated using an approximation of the metric, which,
after a conformal transformation, permits to work in a Rindler-like spacetime.
Of course, as for the Schwarzschild case, the entropy is divergent in the
proximity of the event horizon.

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