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Gravitational collapse with tachyon field and barotropic fluid

dc.contributor.authorTavakoli, Yaser
dc.contributor.authorMarto, João
dc.contributor.authorZiaie, Amir Hadi
dc.contributor.authorMoniz, Paulo
dc.date.accessioned2018-11-26T15:34:30Z
dc.date.available2018-11-26T15:34:30Z
dc.date.issued2013
dc.description.abstractA particular class of space-time, with a tachyon field, ϕ, and a barotropic fluid constituting the matter content, is considered herein as a model for gravitational collapse. For simplicity, the tachyon potential is assumed to be of inverse square form i.e., V(ϕ)∼ϕ^(−2). Our purpose, by making use of the specific kinematical features of the tachyon, which are rather different from a standard scalar field, is to establish the several types of asymptotic behavior that our matter content induces. Employing a dynamical system analysis, complemented by a thorough numerical study, we find classical solutions corresponding to a naked singularity or a black hole formation. In particular, there is a subset where the fluid and tachyon participate in an interesting tracking behaviour, depending sensitively on the initial conditions for the energy densities of the tachyon field and barotropic fluid. Two other classes of solutions are present, corresponding respectively, to either a tachyon or a barotropic fluid regime. Which of these emerges as dominant, will depend on the choice of the barotropic parameter, γ. Furthermore, these collapsing scenarios both have as final state the formation of a black hole.pt_PT
dc.description.versioninfo:eu-repo/semantics/publishedVersionpt_PT
dc.identifier.citationTavakoli, Y., Marto, J., Ziaie, A.H. et al. Gen Relativ Gravit (2013) 45: 819pt_PT
dc.identifier.doi10.1007/s10714-013-1503-3pt_PT
dc.identifier.urihttp://hdl.handle.net/10400.6/6495
dc.language.isoengpt_PT
dc.peerreviewedyespt_PT
dc.publisherSpringerpt_PT
dc.relationSymmetries, gravitation and strings
dc.relationSymmetries, gravitation and strings
dc.relation.publisherversionhttps://doi.org/10.1007/s10714-013-1503-3pt_PT
dc.subjectGravitational collapsept_PT
dc.subjectSingularitiespt_PT
dc.titleGravitational collapse with tachyon field and barotropic fluidpt_PT
dc.typejournal article
dspace.entity.typePublication
oaire.awardTitleSymmetries, gravitation and strings
oaire.awardTitleSymmetries, gravitation and strings
oaire.awardURIinfo:eu-repo/grantAgreement/FCT/3599-PPCDT/CERN%2FFP%2F109351%2F2009/PT
oaire.awardURIinfo:eu-repo/grantAgreement/FCT/3599-PPCDT/CERN%2FFP%2F116373%2F2010/PT
oaire.citation.endPage844pt_PT
oaire.citation.issue4pt_PT
oaire.citation.startPage819pt_PT
oaire.citation.titleGeneral Relativity and Gravitationpt_PT
oaire.citation.volume45pt_PT
oaire.fundingStream3599-PPCDT
oaire.fundingStream3599-PPCDT
person.familyNameTavakoli
person.familyNamePedro de Jesus Marto
person.familyNameZiaie
person.familyNameMoniz
person.givenNameYaser
person.givenNameJoão
person.givenNameAmir Hadi
person.givenNamePaulo
person.identifierhttps://scholar.google.com/citations?user=kA-uFTYAAAAJ&hl=en
person.identifier277693
person.identifier.ciencia-id9812-C08C-3084
person.identifier.ciencia-id2F16-67B1-A930
person.identifier.ciencia-idB410-D0B7-55C1
person.identifier.orcid0000-0003-0099-5100
person.identifier.orcid0000-0003-3974-9177
person.identifier.orcid0000-0001-7029-134X
person.identifier.orcid0000-0001-7170-8952
person.identifier.ridM-9845-2013
person.identifier.scopus-author-id6701832578
project.funder.identifierhttp://doi.org/10.13039/501100001871
project.funder.identifierhttp://doi.org/10.13039/501100001871
project.funder.nameFundação para a Ciência e a Tecnologia
project.funder.nameFundação para a Ciência e a Tecnologia
rcaap.embargofctCopyright cedido à editora no momento da publicaçãopt_PT
rcaap.rightsclosedAccesspt_PT
rcaap.typearticlept_PT
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