A relativistic acoustic metric for planar black holes

We demonstrate here that the metric of a planar black hole in asymptotic anti-de Sitter space can, on a slice of dimension 3+1, be reproduced as a relativistic acoustic metric. This completes an earlier calculation in which the non-relativistic limit was used, and also serves to obtain a concrete fo...

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Main Author: Sabine Hossenfelder
Format: Article
Language:English
Published: Elsevier 2016-01-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269315008746
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spelling doaj-ba4427c1efaf4063b7fd93f50e4506412020-11-25T00:12:10ZengElsevierPhysics Letters B0370-26931873-24452016-01-01752C131710.1016/j.physletb.2015.11.026A relativistic acoustic metric for planar black holesSabine HossenfelderWe demonstrate here that the metric of a planar black hole in asymptotic anti-de Sitter space can, on a slice of dimension 3+1, be reproduced as a relativistic acoustic metric. This completes an earlier calculation in which the non-relativistic limit was used, and also serves to obtain a concrete form of the Lagrangian.http://www.sciencedirect.com/science/article/pii/S0370269315008746
collection DOAJ
language English
format Article
sources DOAJ
author Sabine Hossenfelder
spellingShingle Sabine Hossenfelder
A relativistic acoustic metric for planar black holes
Physics Letters B
author_facet Sabine Hossenfelder
author_sort Sabine Hossenfelder
title A relativistic acoustic metric for planar black holes
title_short A relativistic acoustic metric for planar black holes
title_full A relativistic acoustic metric for planar black holes
title_fullStr A relativistic acoustic metric for planar black holes
title_full_unstemmed A relativistic acoustic metric for planar black holes
title_sort relativistic acoustic metric for planar black holes
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2016-01-01
description We demonstrate here that the metric of a planar black hole in asymptotic anti-de Sitter space can, on a slice of dimension 3+1, be reproduced as a relativistic acoustic metric. This completes an earlier calculation in which the non-relativistic limit was used, and also serves to obtain a concrete form of the Lagrangian.
url http://www.sciencedirect.com/science/article/pii/S0370269315008746
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AT sabinehossenfelder relativisticacousticmetricforplanarblackholes
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