The entropy of a hole in spacetime

A bstract We compute the gravitational entropy of “spherical Rindler space”, a timedependent, spherically symmetric generalization of ordinary Rindler space, defined with reference to a family of observers traveling along non-parallel, accelerated trajectories. All these observers are causally disco...

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Bibliographic Details
Published in:The journal of high energy physics Vol. 2013; no. 10; pp. 1 - 12
Main Authors: Balasubramanian, Vijay, Chowdhury, Borun D., Czech, Bartlomiej, de Boer, Jan
Format: Journal Article
Language:English
Published: Berlin/Heidelberg Springer Berlin Heidelberg 01-10-2013
Springer Nature B.V
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Summary:A bstract We compute the gravitational entropy of “spherical Rindler space”, a timedependent, spherically symmetric generalization of ordinary Rindler space, defined with reference to a family of observers traveling along non-parallel, accelerated trajectories. All these observers are causally disconnected from a spherical region H (a “hole”) located at the origin of Minkowski space. The entropy evaluates to S = / 4 G , where is the area of the spherical acceleration horizon, which coincides with the boundary of H . We propose that S is the entropy of entanglement between quantum gravitational degrees of freedom supporting the interior and the exterior of the sphere H .
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ISSN:1029-8479
1029-8479
DOI:10.1007/JHEP10(2013)220