Quasi-Normal Modes in Topologically Massive Gravity

We determine the black hole quasi-normal mode spectrum for tensor perturbations in topologically massive AdS-gravity. In the special case of chiral gravity quasi-normal modes are absent despite of the presence of a horizon. In the process we uncover a simple algebraic structure in the quasi normal m...

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Detalles Bibliográficos
Autores principales: Sachs, Ivo, Solodukhin, Sergey N.
Lenguaje:eng
Publicado: 2008
Materias:
Particle Physics - Theory
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2008/08/003
http://cds.cern.ch/record/1109452
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author Sachs, Ivo
Solodukhin, Sergey N.
author_facet Sachs, Ivo
Solodukhin, Sergey N.
author_sort Sachs, Ivo
collection CERN
description We determine the black hole quasi-normal mode spectrum for tensor perturbations in topologically massive AdS-gravity. In the special case of chiral gravity quasi-normal modes are absent despite of the presence of a horizon. In the process we uncover a simple algebraic structure in the quasi normal modes spectrum: the tower of QNM's consists of descendents of a "chiral highest weight'' QNM which in turn satisfies a first oder equation.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2008
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spelling cern-11094522023-03-12T04:55:02Zdoi:10.1088/1126-6708/2008/08/003http://cds.cern.ch/record/1109452engSachs, IvoSolodukhin, Sergey N.Quasi-Normal Modes in Topologically Massive GravityParticle Physics - TheoryWe determine the black hole quasi-normal mode spectrum for tensor perturbations in topologically massive AdS-gravity. In the special case of chiral gravity quasi-normal modes are absent despite of the presence of a horizon. In the process we uncover a simple algebraic structure in the quasi normal modes spectrum: the tower of QNM's consists of descendents of a "chiral highest weight'' QNM which in turn satisfies a first oder equation.We determine the black hole quasi-normal mode spectrum for tensor perturbations in topologically massive AdS-gravity. In the special case of chiral gravity quasi-normal modes are absent despite of the presence of a horizon. In the process we uncover a simple algebraic structure in the quasi normal modes spectrum: the tower of QNM's consists of descendents of a 'chiral highest weight'' QNM which in turn satisfies a first oder equation.arXiv:0806.1788LMU-ASC-35-08LMU-ASC 35-08oai:cds.cern.ch:11094522008-06-12
spellingShingle Particle Physics - Theory
Sachs, Ivo
Solodukhin, Sergey N.
Quasi-Normal Modes in Topologically Massive Gravity
title Quasi-Normal Modes in Topologically Massive Gravity
title_full Quasi-Normal Modes in Topologically Massive Gravity
title_fullStr Quasi-Normal Modes in Topologically Massive Gravity
title_full_unstemmed Quasi-Normal Modes in Topologically Massive Gravity
title_short Quasi-Normal Modes in Topologically Massive Gravity
title_sort quasi-normal modes in topologically massive gravity
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/1126-6708/2008/08/003
http://cds.cern.ch/record/1109452
work_keys_str_mv AT sachsivo quasinormalmodesintopologicallymassivegravity
AT solodukhinsergeyn quasinormalmodesintopologicallymassivegravity

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