Compactification of Friedmann's hyperbolic model

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dc.contributor.authorFagundes, Helio V.
dc.contributor.institutionInstituto de Física Teórica
dc.date.accessioned2022-04-29T08:43:28Z
dc.date.available2022-04-29T08:43:28Z
dc.date.issued1983-01-01
dc.description.abstractA compact hyperbolic three-manifold is substituted for the infinite space H3, as space section of Friedmann's cosmological model of negative curvature. Some consequences are briefly analyzed. In particular it is shown that an apparent observational isotropy persists when the particle horizon intersects an anisotropic region of space. © 1983 The American Physical Society.en
dc.description.affiliationInstituto de Física Teórica, 01405 Sao Paulo, Sao Paulo
dc.format.extent517-518
dc.identifierhttp://dx.doi.org/10.1103/PhysRevLett.51.517
dc.identifier.citationPhysical Review Letters, v. 51, n. 6, p. 517-518, 1983.
dc.identifier.doi10.1103/PhysRevLett.51.517
dc.identifier.issn0031-9007
dc.identifier.scopus2-s2.0-4243260451
dc.identifier.urihttp://hdl.handle.net/11449/231088
dc.language.isoeng
dc.relation.ispartofPhysical Review Letters
dc.sourceScopus
dc.titleCompactification of Friedmann's hyperbolic modelen
dc.typeArtigo

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