Casimir energy density in closed hyperbolic universes

dc.contributorUniversidade de Brasília (UnB)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:06:57Z
dc.date.accessioned2022-10-05T15:00:57Z
dc.date.available2014-05-20T14:06:57Z
dc.date.available2022-10-05T15:00:57Z
dc.date.created2014-05-20T14:06:57Z
dc.date.issued2002-11-20
dc.identifierInternational Journal of Modern Physics A. Singapore: World Scientific Publ Co Pte Ltd, v. 17, n. 29, p. 4385-4392, 2002.
dc.identifier0217-751X
dc.identifierhttp://hdl.handle.net/11449/23514
dc.identifier10.1142/S0217751X02013459
dc.identifierWOS:000179333300031
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3896862
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.
dc.languageeng
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relationInternational Journal of Modern Physics A
dc.relation1.291
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectCasimir effect
dc.subjectcosmology
dc.titleCasimir energy density in closed hyperbolic universes
dc.typeArtigo


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