Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component

Detalhes bibliográficos
Autor(a) principal: Brito, Irene
Data de Publicação: 2017
Outros Autores: Silva, M. F. A. da, Mena, Filipe C., Santos, N. O.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/1822/46666
Resumo: We investigate a class of cylindrically symmetric inhomogeneous Λ-dust spacetimes which have a regular axis and some zero expansion component. For Λ \neq 0, we obtain new exact solutions to the Einstein equations and show that they are unique, within that class. For Λ = 0, we recover the Senovilla– Vera metric and show that it can be locally matched to an Einstein–Rosen type of exterior. Finally, we explore some consequences of the matching, such as trapped surface formation and gravitational radiation in the exterior.
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spelling Cylindrically symmetric inhomogeneous dust collapse with a zero expansion componentExact solutionsSpacetime matchingGravitational collapseGravitational radiationBlack hole formationScience & TechnologyWe investigate a class of cylindrically symmetric inhomogeneous Λ-dust spacetimes which have a regular axis and some zero expansion component. For Λ \neq 0, we obtain new exact solutions to the Einstein equations and show that they are unique, within that class. For Λ = 0, we recover the Senovilla– Vera metric and show that it can be locally matched to an Einstein–Rosen type of exterior. Finally, we explore some consequences of the matching, such as trapped surface formation and gravitational radiation in the exterior.We thank Jose Senovilla for suggesting solutions of the form (8) and (9) and for other very useful comments which led to substancial improvements in the paper. IB and FM are supported by Portuguese Funds through Fundacao para a Cincia e Tecnologia (FCT), within the Projects UID/MAT/00013/2013 and PTDC/MAT-ANA/1275/2014. FM and NOS acknowledge a grant received from UERJ and thank the warm hospitality from Instituto de Fisica, UERJ, Rio de Janeiro, where a great part of this work was completed. MFAdaSilva acknowledges the financial support from FAPERJ (no. E-26/171.754/2000, E-26/171.533.2002, E-26/170.951/2006, E-26/110.432/2009 and E-26/111.714/2010), Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq) Brazil (no. 450572/2009-9, 301973/2009-1 and 477268/2010-2) and Financiadora de Estudos e Projetos (FINEP) Brazil.info:eu-repo/semantics/publishedVersionIOP PublishingUniversidade do MinhoBrito, IreneSilva, M. F. A. daMena, Filipe C.Santos, N. O.2017-092017-09-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/1822/46666eng0264-93811361-638210.1088/1361-6382/aa8aa8The original publication is available at http://iopscience.iop.org/article/10.1088/1361-6382/aa8aa8# .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:RCAAP2023-07-21T12:21:13Zoai:repositorium.sdum.uminho.pt:1822/46666Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T19:14:26.250760Repositório 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 Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
title Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
spellingShingle Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
Brito, Irene
Exact solutions
Spacetime matching
Gravitational collapse
Gravitational radiation
Black hole formation
Science & Technology
title_short Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
title_full Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
title_fullStr Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
title_full_unstemmed Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
title_sort Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
author Brito, Irene
author_facet Brito, Irene
Silva, M. F. A. da
Mena, Filipe C.
Santos, N. O.
author_role author
author2 Silva, M. F. A. da
Mena, Filipe C.
Santos, N. O.
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidade do Minho
dc.contributor.author.fl_str_mv Brito, Irene
Silva, M. F. A. da
Mena, Filipe C.
Santos, N. O.
dc.subject.por.fl_str_mv Exact solutions
Spacetime matching
Gravitational collapse
Gravitational radiation
Black hole formation
Science & Technology
topic Exact solutions
Spacetime matching
Gravitational collapse
Gravitational radiation
Black hole formation
Science & Technology
description We investigate a class of cylindrically symmetric inhomogeneous Λ-dust spacetimes which have a regular axis and some zero expansion component. For Λ \neq 0, we obtain new exact solutions to the Einstein equations and show that they are unique, within that class. For Λ = 0, we recover the Senovilla– Vera metric and show that it can be locally matched to an Einstein–Rosen type of exterior. Finally, we explore some consequences of the matching, such as trapped surface formation and gravitational radiation in the exterior.
publishDate 2017
dc.date.none.fl_str_mv 2017-09
2017-09-01T00:00:00Z
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/1822/46666
url http://hdl.handle.net/1822/46666
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 0264-9381
1361-6382
10.1088/1361-6382/aa8aa8
The original publication is available at http://iopscience.iop.org/article/10.1088/1361-6382/aa8aa8# .
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