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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Published in: | The journal of high energy physics Vol. 2013; no. 10; pp. 1 - 12 |
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Main Authors: | , , , |
Format: | Journal Article |
Language: | English |
Published: |
Berlin/Heidelberg
Springer Berlin Heidelberg
01-10-2013
Springer Nature B.V |
Subjects: | |
Online Access: | Get full text |
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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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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 1029-8479 1029-8479 |
DOI: | 10.1007/JHEP10(2013)220 |