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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23350
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dc.contributor.authorMuller, D.-
dc.contributor.authorFagundes, H. V.-
dc.contributor.authorOpher, R.-
dc.date.accessioned2014-05-20T14:06:32Z-
dc.date.available2014-05-20T14:06:32Z-
dc.date.issued2001-06-15-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.63.123508-
dc.identifier.citationPhysical Review D. College Pk: American Physical Soc, v. 63, n. 12, 5 p., 2001.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/23350-
dc.description.abstractA few years ago, Cornish, Spergel and Starkman (CSS) suggested that a multiply connected small universe could allow for classical chaotic mixing as a preinflationary homogenization process. The smaller the volume, the more important the process. Also, a smaller universe has a greater probability of being spontaneously created. Previously DeWitt, Hart and Isham (DHI) calculated the Casimir energy for static multiply connected fat space-times. Because of the interest in small volume hyperbolic universes (e.g., CSS), we generalize the DHI calculation by making a numerical investigation of the Casimir energy for a conformally coupled, massive scalar field in a static universe, whose spatial sections are the Weeks manifold, the smallest universe of negative curvature known. In spite of being a numerical calculation, our result is in fact exact. It is shown that there is spontaneous vacuum excitation of low multipolar components.en
dc.format.extent5-
dc.language.isoeng-
dc.publisherAmerican Physical Soc-
dc.sourceWeb of Science-
dc.titleCasimir energy in a small volume multiply connected static hyperbolic preinflationary universeen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUSP, Inst Astron & Geofis, BR-04301904 São Paulo, Brazil-
dc.description.affiliationUNESP, Inst Fis Teor, BR-01405000 São Paulo, Brazil-
dc.description.affiliationUnespUNESP, Inst Fis Teor, BR-01405000 São Paulo, Brazil-
dc.identifier.doi10.1103/PhysRevD.63.123508-
dc.identifier.wosWOS:000169288400014-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOS000169288400014.pdf-
dc.relation.ispartofPhysical Review D-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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