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Thermodynamics of scalar fields in Kerr's geometry

Guido Cognola
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Abstract

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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Guido Cognola. 1998-01-22. Thermodynamics of scalar fields in Kerr's geometry. https://doi.org/10.1103/physrevd.57.6292

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