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Propagation of Scalar Fields in a Plane Symmetric Spacetime

dc.contributor.authorCelestino, Juliana
dc.contributor.authorAlves, Márcio E. S. [UNESP]
dc.contributor.authorBarone, F. A.
dc.contributor.institutionRio de Janeiro State University
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniversity Federal of Itajubá
dc.date.accessioned2018-12-11T16:44:31Z
dc.date.available2018-12-11T16:44:31Z
dc.date.issued2016-12-01
dc.description.abstractThe present article deals with solutions for a minimally coupled scalar field propagating in a static plane symmetric spacetime. The considered metric describes the curvature outside a massive infinity plate and exhibits an intrinsic naked singularity (a singular plane) that makes the accessible universe finite in extension. This solution can be interpreted as describing the spacetime of static domain walls. In this context, a first solution is given in terms of zero order Bessel functions of the first and second kind and presents a stationary pattern which is interpreted as a result of the reflection of the scalar waves at the singular plane. This is an evidence, at least for the massless scalar field, of an old interpretation given by Amundsen and Grøn regarding the behaviour of test particles near the singularity. A second solution is obtained in the limit of a weak gravitational field which is valid only far from the singularity. In this limit, it was possible to find out an analytic solution for the scalar field in terms of the Kummer and Tricomi confluent hypergeometric functions.en
dc.description.affiliationDepartmnt of Physics Rio de Janeiro State University, R. São Francisco Xavier, 524 - Maracanã
dc.description.affiliationInstituto de Ciência e Tecnologia UNESP - Univ Estadual Paulista
dc.description.affiliationIFQ University Federal of Itajubá, Av. BPS 1303
dc.description.affiliationUnespInstituto de Ciência e Tecnologia UNESP - Univ Estadual Paulista
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipIdFAPESP: 13/26258-4
dc.description.sponsorshipIdCNPq: 311514/2015-4
dc.description.sponsorshipIdCNPq: 484736/2012-4
dc.format.extent784-792
dc.identifierhttp://dx.doi.org/10.1007/s13538-016-0458-8
dc.identifier.citationBrazilian Journal of Physics, v. 46, n. 6, p. 784-792, 2016.
dc.identifier.doi10.1007/s13538-016-0458-8
dc.identifier.file2-s2.0-84994493493.pdf
dc.identifier.issn1678-4448
dc.identifier.issn0103-9733
dc.identifier.scopus2-s2.0-84994493493
dc.identifier.urihttp://hdl.handle.net/11449/169108
dc.language.isoeng
dc.relation.ispartofBrazilian Journal of Physics
dc.relation.ispartofsjr0,276
dc.rights.accessRightsAcesso aberto
dc.sourceScopus
dc.subjectGravitational waves
dc.subjectScalar field
dc.subjectTaub metric
dc.titlePropagation of Scalar Fields in a Plane Symmetric Spacetimeen
dc.typeArtigo
dspace.entity.typePublication

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