Scalar field perturbations in asymptotically Lifshitz black holes

We consider scalar field perturbations about asymptotically Lifshitz black holes with dynamical exponent z in D dimensions. We show that, for suitable boundary conditions, these Lifshitz black holes are stable under scalar field perturbations. For z≥2, we explicitly compute the quasinormal mode freq...

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Autores principales: Giacomini, A., Giribet, G., Leston, M., Oliva, J., Ray, S.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_15507998_v85_n12_p_Giacomini
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spelling todo:paper_15507998_v85_n12_p_Giacomini2023-10-03T16:24:34Z Scalar field perturbations in asymptotically Lifshitz black holes Giacomini, A. Giribet, G. Leston, M. Oliva, J. Ray, S. We consider scalar field perturbations about asymptotically Lifshitz black holes with dynamical exponent z in D dimensions. We show that, for suitable boundary conditions, these Lifshitz black holes are stable under scalar field perturbations. For z≥2, we explicitly compute the quasinormal mode frequencies, which result to be purely imaginary, and then obtain the damping-off of the scalar field perturbation in these backgrounds. The general analysis includes, in particular, the z≥3 black hole solution of three-dimensional massive gravity. © 2012 American Physical Society. Fil:Giribet, G. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Leston, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_15507998_v85_n12_p_Giacomini
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description We consider scalar field perturbations about asymptotically Lifshitz black holes with dynamical exponent z in D dimensions. We show that, for suitable boundary conditions, these Lifshitz black holes are stable under scalar field perturbations. For z≥2, we explicitly compute the quasinormal mode frequencies, which result to be purely imaginary, and then obtain the damping-off of the scalar field perturbation in these backgrounds. The general analysis includes, in particular, the z≥3 black hole solution of three-dimensional massive gravity. © 2012 American Physical Society.
format JOUR
author Giacomini, A.
Giribet, G.
Leston, M.
Oliva, J.
Ray, S.
spellingShingle Giacomini, A.
Giribet, G.
Leston, M.
Oliva, J.
Ray, S.
Scalar field perturbations in asymptotically Lifshitz black holes
author_facet Giacomini, A.
Giribet, G.
Leston, M.
Oliva, J.
Ray, S.
author_sort Giacomini, A.
title Scalar field perturbations in asymptotically Lifshitz black holes
title_short Scalar field perturbations in asymptotically Lifshitz black holes
title_full Scalar field perturbations in asymptotically Lifshitz black holes
title_fullStr Scalar field perturbations in asymptotically Lifshitz black holes
title_full_unstemmed Scalar field perturbations in asymptotically Lifshitz black holes
title_sort scalar field perturbations in asymptotically lifshitz black holes
url http://hdl.handle.net/20.500.12110/paper_15507998_v85_n12_p_Giacomini
work_keys_str_mv AT giacominia scalarfieldperturbationsinasymptoticallylifshitzblackholes
AT giribetg scalarfieldperturbationsinasymptoticallylifshitzblackholes
AT lestonm scalarfieldperturbationsinasymptoticallylifshitzblackholes
AT olivaj scalarfieldperturbationsinasymptoticallylifshitzblackholes
AT rays scalarfieldperturbationsinasymptoticallylifshitzblackholes
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