Statistical Origin of Gravity

Published 11 Mar 2010 in gr-qc and hep-th | (1003.2312v3)

Abstract: Starting from the definition of entropy used in statistical mechanics we show that it is proportional to the gravity action. For a stationary black hole this entropy is expressed as $S = E/ 2T$, where $T$ is the Hawking temperature and $E$ is shown to be the Komar energy. This relation is also compatible with the generalised Smarr formula for mass.

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