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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23514
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dc.contributor.authorMuller, D.-
dc.contributor.authorFagundes, H. V.-
dc.date.accessioned2014-05-20T14:06:57Z-
dc.date.accessioned2016-10-25T17:12:16Z-
dc.date.available2014-05-20T14:06:57Z-
dc.date.available2016-10-25T17:12:16Z-
dc.date.issued2002-11-20-
dc.identifierhttp://dx.doi.org/10.1142/S0217751X02013459-
dc.identifier.citationInternational Journal of Modern Physics A. Singapore: World Scientific Publ Co Pte Ltd, v. 17, n. 29, p. 4385-4392, 2002.-
dc.identifier.issn0217-751X-
dc.identifier.urihttp://hdl.handle.net/11449/23514-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/23514-
dc.description.abstractThe original Casimir effect results from the difference in the vacuum energies of the electromagnetic field, between that in a region of space with boundary conditions and that in the same region without boundary conditions. In this paper we develop the theory of a similar situation, involving a scalar field in spacetimes with closed spatial sections of negative curvature.en
dc.format.extent4385-4392-
dc.language.isoeng-
dc.publisherWorld Scientific Publ Co Pte Ltd-
dc.sourceWeb of Science-
dc.subjectCasimir effectpt
dc.subjectcosmologypt
dc.titleCasimir energy density in closed hyperbolic universesen
dc.typeoutro-
dc.contributor.institutionUniversidade de Brasília (UnB)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Brasilia, Inst Fis, BR-70919970 Brasilia, DF, Brazil-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, SP, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, SP, Brazil-
dc.identifier.doi10.1142/S0217751X02013459-
dc.identifier.wosWOS:000179333300031-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofInternational Journal of Modern Physics A-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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