Entropy in Kerr-Newman-Kasuya spacetime

Details Entropy in Kerr-Newman-Kasuya spacetime Entropy in Kerr-Newman-Kasuya spacetime

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19.4933g&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 19, pp. 4933-4941 (2002).

Physics

2

Scientific paper

The entropy of a rotating Kerr-Newman-Kasuya black hole due to massive charged fields (bosons and fermions) is calculated using an improved brick-wall model. The result shows that the entropy depends not on the mass and charge but the spin of the fields. Considering statistical physics, we do not propose to consider the superradiant modes for bosons (fermion fields do not display superradiance). In fact, the non-superradiant mode contributes exactly the area entropy for both bosons and fermions.

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