Evanescent gravitons in warped anti-de Sitter space

Besides black holes, the phase space of three-dimensional massive gravity about warped anti-de Sitter space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with nonvanishing effective mass, do not carry net...

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Autores principales: Giribet, G., Vásquez, Y.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_24700010_v93_n2_p_Giribet
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
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spelling todo:paper_24700010_v93_n2_p_Giribet2023-10-03T16:41:53Z Evanescent gravitons in warped anti-de Sitter space Giribet, G. Vásquez, Y. Besides black holes, the phase space of three-dimensional massive gravity about warped anti-de Sitter space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with nonvanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of topologically massive gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms. © 2016 American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_24700010_v93_n2_p_Giribet
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description Besides black holes, the phase space of three-dimensional massive gravity about warped anti-de Sitter space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with nonvanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of topologically massive gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms. © 2016 American Physical Society.
format JOUR
author Giribet, G.
Vásquez, Y.
spellingShingle Giribet, G.
Vásquez, Y.
Evanescent gravitons in warped anti-de Sitter space
author_facet Giribet, G.
Vásquez, Y.
author_sort Giribet, G.
title Evanescent gravitons in warped anti-de Sitter space
title_short Evanescent gravitons in warped anti-de Sitter space
title_full Evanescent gravitons in warped anti-de Sitter space
title_fullStr Evanescent gravitons in warped anti-de Sitter space
title_full_unstemmed Evanescent gravitons in warped anti-de Sitter space
title_sort evanescent gravitons in warped anti-de sitter space
url http://hdl.handle.net/20.500.12110/paper_24700010_v93_n2_p_Giribet
work_keys_str_mv AT giribetg evanescentgravitonsinwarpedantidesitterspace
AT vasquezy evanescentgravitonsinwarpedantidesitterspace
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