Thermodynamic Relations for the Entropy and Temperature of Multi-Horizon Black Holes

Publisher： MDPI

E-ISSN： 2075-4434|3|1|53-71

ISSN： 2075-4434

Source： Galaxies, Vol.3, Iss.1, 2015-02, pp. : 53-71

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Abstract

We present some entropy and temperature relations of multi-horizons, even including the “virtual” horizon. These relations are related to the product, division and sum of the entropy and temperature of multi-horizons. We obtain the additional thermodynamic relations of both static and rotating black holes in three- and four-dimensional (A)dS spacetime. Especially, a new dimensionless, charge-independence and T + S + = T - S - -like relation is presented. This relation does not depend on the mass, electric charge, angular momentum and cosmological constant, as it is always a constant. These relations lead us to obtaining some interesting thermodynamic bounds of entropy and temperature, including the Penrose inequality, which is the first geometrical inequality of black holes. Besides, based on these new relations, one can obtain the first law of thermodynamics and the Smarr relation for all horizons of a black hole.