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arXiv · 1011.3343

Rindler horizon entropy from nonstationarity

Hristu Culetu
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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 $t$ 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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Hristu Culetu. 2011-09-23. Rindler horizon entropy from nonstationarity. https://doi.org/10.1016/j.physletb.2011.08.068

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