Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole
We consider scalar and spinorial perturbations on a background described by a z = 3 three-dimensional Lifshitz black hole. We obtained the corresponding quasinormal modes which perfectly agree with the analytical result for the quasinormal frequency in the scalar case. The numerical results for the...
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todo:paper_17426588_v453_n1_p_CuadrosMelgar2023-10-03T16:30:50Z Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole Cuadros-Melgar, B. De Oliveira, J. Pellicer, C.E. Gravitation Analytical results Black holes Numerical results Quasinormal modes Thermodynamical Stars We consider scalar and spinorial perturbations on a background described by a z = 3 three-dimensional Lifshitz black hole. We obtained the corresponding quasinormal modes which perfectly agree with the analytical result for the quasinormal frequency in the scalar case. The numerical results for the spinorial perturbations reinforce our conclusion on the stability of the model under these perturbations. We also calculate the area spectrum, which prove to be equally spaced, as an application of our results. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17426588_v453_n1_p_CuadrosMelgar |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Gravitation Analytical results Black holes Numerical results Quasinormal modes Thermodynamical Stars |
spellingShingle |
Gravitation Analytical results Black holes Numerical results Quasinormal modes Thermodynamical Stars Cuadros-Melgar, B. De Oliveira, J. Pellicer, C.E. Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole |
topic_facet |
Gravitation Analytical results Black holes Numerical results Quasinormal modes Thermodynamical Stars |
description |
We consider scalar and spinorial perturbations on a background described by a z = 3 three-dimensional Lifshitz black hole. We obtained the corresponding quasinormal modes which perfectly agree with the analytical result for the quasinormal frequency in the scalar case. The numerical results for the spinorial perturbations reinforce our conclusion on the stability of the model under these perturbations. We also calculate the area spectrum, which prove to be equally spaced, as an application of our results. |
format |
CONF |
author |
Cuadros-Melgar, B. De Oliveira, J. Pellicer, C.E. |
author_facet |
Cuadros-Melgar, B. De Oliveira, J. Pellicer, C.E. |
author_sort |
Cuadros-Melgar, B. |
title |
Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole |
title_short |
Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole |
title_full |
Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole |
title_fullStr |
Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole |
title_full_unstemmed |
Quasinormal modes and thermodynamical aspects of the 3D Lifshitz black hole |
title_sort |
quasinormal modes and thermodynamical aspects of the 3d lifshitz black hole |
url |
http://hdl.handle.net/20.500.12110/paper_17426588_v453_n1_p_CuadrosMelgar |
work_keys_str_mv |
AT cuadrosmelgarb quasinormalmodesandthermodynamicalaspectsofthe3dlifshitzblackhole AT deoliveiraj quasinormalmodesandthermodynamicalaspectsofthe3dlifshitzblackhole AT pellicerce quasinormalmodesandthermodynamicalaspectsofthe3dlifshitzblackhole |
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1807317933306675200 |