Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability

Detalhes bibliográficos
Autor(a) principal: Abdalla, E.
Data de Publicação: 2019
Outros Autores: Cuadros-Melgar, B., Oliveira, Jeferson de, Pavan, A. B., Oliveira, Carlos Eduardo Pellicer de
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRN
Texto Completo: https://repositorio.ufrn.br/handle/123456789/31225
Resumo: In this work, we have considered a model that includes the interaction of gravity and matter fields with Galilean invariance (the so-called derivative coupling) as well as some corresponding black hole type solutions. Quasinormal perturbations of two kinds of matter fields have been computed by different methods. The effect of the derivative coupling in the quasinormal spectrum has been analyzed and evaluated
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spelling Abdalla, E.Cuadros-Melgar, B.Oliveira, Jeferson dePavan, A. B.Oliveira, Carlos Eduardo Pellicer de2021-01-07T17:41:24Z2021-01-07T17:41:24Z2019-02-14ABDALLA, E.; CUADROS-MELGAR, B.; OLIVEIRA, Jeferson de; PAVAN, A. B.; PELLICER, C. E.. Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability. Physical Review D, [S.L.], v. 99, n. 4, p. 044023-044023, 14 fev. 2019. Disponível em: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.044023. Acesso em: 14 out. 2020. http://dx.doi.org/10.1103/physrevd.99.044023.2470-00292470-0010https://repositorio.ufrn.br/handle/123456789/3122510.1103/physrevd.99.044023American Physical SocietyAttribution 3.0 Brazilhttp://creativecommons.org/licenses/by/3.0/br/info:eu-repo/semantics/openAccessGalilean invarianceMatter fieldsVectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stabilityinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleIn this work, we have considered a model that includes the interaction of gravity and matter fields with Galilean invariance (the so-called derivative coupling) as well as some corresponding black hole type solutions. Quasinormal perturbations of two kinds of matter fields have been computed by different methods. The effect of the derivative coupling in the quasinormal spectrum has been analyzed and evaluatedengreponame:Repositório Institucional da UFRNinstname:Universidade Federal do Rio Grande do Norte (UFRN)instacron:UFRNORIGINALVectorialSpinorialPerturbations_OLIVEIRA_2019.pdfVectorialSpinorialPerturbations_OLIVEIRA_2019.pdfapplication/pdf1711047https://repositorio.ufrn.br/bitstream/123456789/31225/1/VectorialSpinorialPerturbations_OLIVEIRA_2019.pdfcd4f05e6a4f454358167ff787bce6d31MD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8914https://repositorio.ufrn.br/bitstream/123456789/31225/2/license_rdf4d2950bda3d176f570a9f8b328dfbbefMD52LICENSElicense.txtlicense.txttext/plain; charset=utf-81484https://repositorio.ufrn.br/bitstream/123456789/31225/3/license.txte9597aa2854d128fd968be5edc8a28d9MD53TEXTVectorialSpinorialPerturbations_OLIVEIRA_2019.pdf.txtVectorialSpinorialPerturbations_OLIVEIRA_2019.pdf.txtExtracted texttext/plain38547https://repositorio.ufrn.br/bitstream/123456789/31225/4/VectorialSpinorialPerturbations_OLIVEIRA_2019.pdf.txt8a02bfa10f1b308dc5fc53cf4cc44cddMD54THUMBNAILVectorialSpinorialPerturbations_OLIVEIRA_2019.pdf.jpgVectorialSpinorialPerturbations_OLIVEIRA_2019.pdf.jpgGenerated Thumbnailimage/jpeg1631https://repositorio.ufrn.br/bitstream/123456789/31225/5/VectorialSpinorialPerturbations_OLIVEIRA_2019.pdf.jpg29476c712beb2e83571273838caea2c7MD55123456789/312252021-01-10 04:54:13.787oai:https://repositorio.ufrn.br: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Repositório de PublicaçõesPUBhttp://repositorio.ufrn.br/oai/opendoar:2021-01-10T07:54:13Repositório Institucional da UFRN - Universidade Federal do Rio Grande do Norte (UFRN)false
dc.title.pt_BR.fl_str_mv Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
title Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
spellingShingle Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
Abdalla, E.
Galilean invariance
Matter fields
title_short Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
title_full Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
title_fullStr Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
title_full_unstemmed Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
title_sort Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability
author Abdalla, E.
author_facet Abdalla, E.
Cuadros-Melgar, B.
Oliveira, Jeferson de
Pavan, A. B.
Oliveira, Carlos Eduardo Pellicer de
author_role author
author2 Cuadros-Melgar, B.
Oliveira, Jeferson de
Pavan, A. B.
Oliveira, Carlos Eduardo Pellicer de
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Abdalla, E.
Cuadros-Melgar, B.
Oliveira, Jeferson de
Pavan, A. B.
Oliveira, Carlos Eduardo Pellicer de
dc.subject.por.fl_str_mv Galilean invariance
Matter fields
topic Galilean invariance
Matter fields
description In this work, we have considered a model that includes the interaction of gravity and matter fields with Galilean invariance (the so-called derivative coupling) as well as some corresponding black hole type solutions. Quasinormal perturbations of two kinds of matter fields have been computed by different methods. The effect of the derivative coupling in the quasinormal spectrum has been analyzed and evaluated
publishDate 2019
dc.date.issued.fl_str_mv 2019-02-14
dc.date.accessioned.fl_str_mv 2021-01-07T17:41:24Z
dc.date.available.fl_str_mv 2021-01-07T17:41:24Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.citation.fl_str_mv ABDALLA, E.; CUADROS-MELGAR, B.; OLIVEIRA, Jeferson de; PAVAN, A. B.; PELLICER, C. E.. Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability. Physical Review D, [S.L.], v. 99, n. 4, p. 044023-044023, 14 fev. 2019. Disponível em: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.044023. Acesso em: 14 out. 2020. http://dx.doi.org/10.1103/physrevd.99.044023.
dc.identifier.uri.fl_str_mv https://repositorio.ufrn.br/handle/123456789/31225
dc.identifier.issn.none.fl_str_mv 2470-0029
2470-0010
dc.identifier.doi.none.fl_str_mv 10.1103/physrevd.99.044023
identifier_str_mv ABDALLA, E.; CUADROS-MELGAR, B.; OLIVEIRA, Jeferson de; PAVAN, A. B.; PELLICER, C. E.. Vectorial and spinorial perturbations in Galileon black holes: quasinormal modes, quasiresonant modes, and stability. Physical Review D, [S.L.], v. 99, n. 4, p. 044023-044023, 14 fev. 2019. Disponível em: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.044023. Acesso em: 14 out. 2020. http://dx.doi.org/10.1103/physrevd.99.044023.
2470-0029
2470-0010
10.1103/physrevd.99.044023
url https://repositorio.ufrn.br/handle/123456789/31225
dc.language.iso.fl_str_mv eng
language eng
dc.rights.driver.fl_str_mv Attribution 3.0 Brazil
http://creativecommons.org/licenses/by/3.0/br/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution 3.0 Brazil
http://creativecommons.org/licenses/by/3.0/br/
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:Repositório Institucional da UFRN
instname:Universidade Federal do Rio Grande do Norte (UFRN)
instacron:UFRN
instname_str Universidade Federal do Rio Grande do Norte (UFRN)
instacron_str UFRN
institution UFRN
reponame_str Repositório Institucional da UFRN
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