Rindler horizon entropy from nonstationarity

Details Rindler horizon entropy from nonstationarity Rindler horizon entropy from nonstationarity

2010-11-15

arxiv.org/abs/1011.3343v2

Phys.Lett.B703:641-644,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, no figures, version published in PLB 703(5),(2011) pp. 641-644, DOI: 10.1016/j.physletb.2011.08.068

Scientific paper

10.1016/j.physletb.2011.08.068

Finite entropy and energy are obtained for the horizon of a Rindler observer on the grounds of the nonstatic character of the geometry beyond the horizon. Edery - Constantineau prescription is used to find the dynamical phase space of this particular spacetime. The number of microstates rooted from the ignorance of a Rindler observer of the parameter $t$ from the nonstationary region is calculated. We suggest that the gravitational energy density constructed by means of the horizon energy and using the Holographic Principle is proportional to $g^{2}$, similar with a result recently obtained by Padmanabhan and with the energy density of the electromagnetic field.

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