Entropy of a Kerr-de Sitter black hole due to arbitrary spin fields

Details Entropy of a Kerr-de Sitter black hole due to arbitrary spin fields Entropy of a Kerr-de Sitter black hole due to arbitrary spin fields

2003-03-20

arxiv.org/abs/gr-qc/0303076v6

Phys.Rev. D69 (2004) 044019; Erratum-ibid. D73 (2006) 089902

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

28 pages, two figures, Revtex4.0. Final revised version to appear in PRD

Scientific paper

10.1103/PhysRevD.69.044019

The Newman-Penrose formalism is used to derive the Teukolsky master equations controlling massless scalar, neutrino, electromagnetic, gravitino, and gravitational field perturbations of the Kerr-de Sitter spacetime. Then the quantum entropy of a non-extreme Kerr-de Sitter black hole due to arbitrary spin fields is calculated by the improved thin-layer brick wall model. It is shown that the subleading order contribution to the entropy is dependent on the square of the spins of particles and that of the specific angular momentum of black holes as well as the cosmological constant. The logarithmic correction of the spins of particles to the entropy relies on the rotation of the black hole and the effect of the cosmological constant.

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