Entropy in the NUT-Kerr-Newman Black Holes Due to an Arbitrary Spin Field

Details Entropy in the NUT-Kerr-Newman Black Holes Due to an Arbitrary Spin Field Entropy in the NUT-Kerr-Newman Black Holes Due to an Arbitrary Spin Field

2004-10-09

arxiv.org/abs/gr-qc/0410045v1

Class.Quant.Grav.20:3593-3602,2003

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

10.1088/0264-9381/20/16/305

Membrane method is used to compute the entropy of the NUT-Kerr-Newman black
holes. It is found that even though the Euler characteristic is greater than
two, the Bekenstein-Hawking area law is still satisfied. The formula $S=\chi
A/8$ relating the entropy and the Euler characteristic becomes inapplicable for
non-extreme four dimensional NUT-Kerr-Newman black holes.

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