On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework

On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework

In this paper we investigate scalar perturbations of black holes embedded in a five-dimensional bulk space. The quasinormal frequencies of such black holes are calculated using the third order of Wentzel, Kramers, and Brillouin (WKB) approximation for scalar perturbations. The high overtones of quas...

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Main Authors: Sergio C. Ulhoa, Ronni G. G. Amorim, Abraão J. S. Capistrano
Format: Article
Language:English
Published: Hindawi Limited 2017-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2017/9891231
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spelling doaj-7e7e860e75894da38a9dbd65394546f82020-11-25T00:39:18ZengHindawi LimitedAdvances in High Energy Physics1687-73571687-73652017-01-01201710.1155/2017/98912319891231On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding FrameworkSergio C. Ulhoa0Ronni G. G. Amorim1Abraão J. S. Capistrano2Instituto de Física, Universidade de Brasília, 70910-900 Brasília, DF, BrazilFaculdade Gama, Universidade de Brasília, Setor Leste (Gama), 72444-240 Brasília, DF, BrazilCasimiro Montenegro Filho Astronomy Center, Itaipu Technological Park, Federal University of Latin-American Integration, P.O. Box 2123, 85867-970 Foz do Iguaçu, PR, BrazilIn this paper we investigate scalar perturbations of black holes embedded in a five-dimensional bulk space. The quasinormal frequencies of such black holes are calculated using the third order of Wentzel, Kramers, and Brillouin (WKB) approximation for scalar perturbations. The high overtones of quasinormal modes indicate a resonant-like set of black holes suggesting a serious constraint of embedding models in five dimensions.http://dx.doi.org/10.1155/2017/9891231
collection DOAJ
language English
format Article
sources DOAJ
author Sergio C. Ulhoa
Ronni G. G. Amorim
Abraão J. S. Capistrano
spellingShingle Sergio C. Ulhoa
Ronni G. G. Amorim
Abraão J. S. Capistrano
On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework
Advances in High Energy Physics
author_facet Sergio C. Ulhoa
Ronni G. G. Amorim
Abraão J. S. Capistrano
author_sort Sergio C. Ulhoa
title On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework
title_short On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework
title_full On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework
title_fullStr On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework
title_full_unstemmed On Quasinormal Modes for Scalar Perturbations of Static Spherically Symmetric Black Holes in Nash Embedding Framework
title_sort on quasinormal modes for scalar perturbations of static spherically symmetric black holes in nash embedding framework
publisher Hindawi Limited
series Advances in High Energy Physics
issn 1687-7357
1687-7365
publishDate 2017-01-01
description In this paper we investigate scalar perturbations of black holes embedded in a five-dimensional bulk space. The quasinormal frequencies of such black holes are calculated using the third order of Wentzel, Kramers, and Brillouin (WKB) approximation for scalar perturbations. The high overtones of quasinormal modes indicate a resonant-like set of black holes suggesting a serious constraint of embedding models in five dimensions.
url http://dx.doi.org/10.1155/2017/9891231
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AT ronniggamorim onquasinormalmodesforscalarperturbationsofstaticsphericallysymmetricblackholesinnashembeddingframework
AT abraaojscapistrano onquasinormalmodesforscalarperturbationsofstaticsphericallysymmetricblackholesinnashembeddingframework
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