Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators?
Autor(a) principal: | |
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Data de Publicação: | 2011 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
Texto Completo: | http://hdl.handle.net/10773/7090 |
Resumo: | We study the geometry inside the event horizon of perturbed D dimensional Reissner-Nordstrom-(anti) de Sitter type black holes showing that, similarly to the four dimensional case, mass inflation also occurs for D > 4. First, using the homogeneous approximation, we show that an increase of the number of spatial dimensions contributes to a steeper variation of the metric coefficients with the areal radius and that the phenomenon is insensitive to the cosmological constant in leading order. Then, using the code reported in [P. P. Avelino, A. J. S. Hamilton, and C. A. R. Herdeiro, Phys. Rev. D 79, 124045 (2009).] adapted to D dimensions, we perform fully nonlinear numerical simulations. We perturb the black hole with a compact pulse adapting the pulse amplitude such that the relative variation of the black hole mass is the same in all dimensions and determine how the black hole interior evolves under the perturbation. We qualitatively confirm that the phenomenon is similar to four dimensions as well as the behavior observed in the homogeneous approximation. We speculate about the formation of black holes inside black holes triggered by mass inflation, and about possible consequences of this scenario. |
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7160 |
spelling |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators?We study the geometry inside the event horizon of perturbed D dimensional Reissner-Nordstrom-(anti) de Sitter type black holes showing that, similarly to the four dimensional case, mass inflation also occurs for D > 4. First, using the homogeneous approximation, we show that an increase of the number of spatial dimensions contributes to a steeper variation of the metric coefficients with the areal radius and that the phenomenon is insensitive to the cosmological constant in leading order. Then, using the code reported in [P. P. Avelino, A. J. S. Hamilton, and C. A. R. Herdeiro, Phys. Rev. D 79, 124045 (2009).] adapted to D dimensions, we perform fully nonlinear numerical simulations. We perturb the black hole with a compact pulse adapting the pulse amplitude such that the relative variation of the black hole mass is the same in all dimensions and determine how the black hole interior evolves under the perturbation. We qualitatively confirm that the phenomenon is similar to four dimensions as well as the behavior observed in the homogeneous approximation. We speculate about the formation of black holes inside black holes triggered by mass inflation, and about possible consequences of this scenario.American Physical Society2012-02-29T15:47:42Z2011-01-01T00:00:00Z2011info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/7090eng1550-799810.1103/PhysRevD.84.024019Avelino, P. P.Hamilton, A. J. S.Herdeiro, C. A. R.Zilhão, M.info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2024-05-06T03:39:20Zoai:ria.ua.pt:10773/7090Portal AgregadorONGhttps://www.rcaap.pt/oai/openairemluisa.alvim@gmail.comopendoar:71602024-05-06T03:39:20Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse |
dc.title.none.fl_str_mv |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
title |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
spellingShingle |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? Avelino, P. P. |
title_short |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
title_full |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
title_fullStr |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
title_full_unstemmed |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
title_sort |
Mass inflation in a D-dimensional Reissner-Nordstrom black hole: A hierarchy of particle accelerators? |
author |
Avelino, P. P. |
author_facet |
Avelino, P. P. Hamilton, A. J. S. Herdeiro, C. A. R. Zilhão, M. |
author_role |
author |
author2 |
Hamilton, A. J. S. Herdeiro, C. A. R. Zilhão, M. |
author2_role |
author author author |
dc.contributor.author.fl_str_mv |
Avelino, P. P. Hamilton, A. J. S. Herdeiro, C. A. R. Zilhão, M. |
description |
We study the geometry inside the event horizon of perturbed D dimensional Reissner-Nordstrom-(anti) de Sitter type black holes showing that, similarly to the four dimensional case, mass inflation also occurs for D > 4. First, using the homogeneous approximation, we show that an increase of the number of spatial dimensions contributes to a steeper variation of the metric coefficients with the areal radius and that the phenomenon is insensitive to the cosmological constant in leading order. Then, using the code reported in [P. P. Avelino, A. J. S. Hamilton, and C. A. R. Herdeiro, Phys. Rev. D 79, 124045 (2009).] adapted to D dimensions, we perform fully nonlinear numerical simulations. We perturb the black hole with a compact pulse adapting the pulse amplitude such that the relative variation of the black hole mass is the same in all dimensions and determine how the black hole interior evolves under the perturbation. We qualitatively confirm that the phenomenon is similar to four dimensions as well as the behavior observed in the homogeneous approximation. We speculate about the formation of black holes inside black holes triggered by mass inflation, and about possible consequences of this scenario. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-01-01T00:00:00Z 2011 2012-02-29T15:47:42Z |
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.uri.fl_str_mv |
http://hdl.handle.net/10773/7090 |
url |
http://hdl.handle.net/10773/7090 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
1550-7998 10.1103/PhysRevD.84.024019 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
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 Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação instacron:RCAAP |
instname_str |
Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
instacron_str |
RCAAP |
institution |
RCAAP |
reponame_str |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
collection |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
repository.name.fl_str_mv |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
repository.mail.fl_str_mv |
mluisa.alvim@gmail.com |
_version_ |
1817543449099894784 |