Rindler horizon entropy from nonstationarity
Abstract
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 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 , similar with a result recently obtained by Padmanabhan and with the energy density of the electromagnetic field.
Keywords
Cite
@article{arxiv.1011.3343,
title = {Rindler horizon entropy from nonstationarity},
author = {Hristu Culetu},
journal= {arXiv preprint arXiv:1011.3343},
year = {2011}
}
Comments
8 pages, no figures, version published in PLB 703(5),(2011) pp. 641-644, DOI: 10.1016/j.physletb.2011.08.068