Black-hole entropy and horizon area.

Physics

Scientific paper

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Black Holes: Thermodynamics

Scientific paper

Employing the relationship between the black-hole thermodynamic functions and the Euclidean path-integral approach to quantum gravity, the author proves, in the framework of four-dimensional Einstein gravity, that the entropy of a stationary black-hole with a bifurcating Killing horizon surrounded by arbitrary classical matter fields is one quarter of the area of the event horizon independent of the matter fields involved.

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