Smallest universe of negative curvature

Detalhes bibliográficos
Autor(a) principal: Fagundes, Helio V. [UNESP]
Data de Publicação: 1993
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevLett.70.1579
http://hdl.handle.net/11449/225054
Resumo: The smallest known three-dimensional closed manifold of curvature k-1 was discovered a few years ago by Weeks. This kind of manifold is constructed from a hyperbolic polyhedron with faces pairwise identified. Here it is used as the comoving spatial section of a Friedmann cosmological model, in the spirit of Ellis and Schreibers idea of small universes. Its nontrivial global topology has the effect of producing multiple images of single cosmic sources, and this is the basis of an attempt to solve a famous controversy about the redshifts of quasars. © 1993 The American Physical Society.
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spelling Smallest universe of negative curvatureThe smallest known three-dimensional closed manifold of curvature k-1 was discovered a few years ago by Weeks. This kind of manifold is constructed from a hyperbolic polyhedron with faces pairwise identified. Here it is used as the comoving spatial section of a Friedmann cosmological model, in the spirit of Ellis and Schreibers idea of small universes. Its nontrivial global topology has the effect of producing multiple images of single cosmic sources, and this is the basis of an attempt to solve a famous controversy about the redshifts of quasars. © 1993 The American Physical Society.Instituto de Física Terica, Universidade Estadual Paulista, rua Pamplona, 145, Sao Paulo, Sao Paulo 01405-900Instituto de Física Terica, Universidade Estadual Paulista, rua Pamplona, 145, Sao Paulo, Sao Paulo 01405-900Universidade Estadual Paulista (UNESP)Fagundes, Helio V. [UNESP]2022-04-28T20:37:17Z2022-04-28T20:37:17Z1993-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1579-1582http://dx.doi.org/10.1103/PhysRevLett.70.1579Physical Review Letters, v. 70, n. 11, p. 1579-1582, 1993.0031-9007http://hdl.handle.net/11449/22505410.1103/PhysRevLett.70.15792-s2.0-3943114098Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Lettersinfo:eu-repo/semantics/openAccess2022-04-28T20:37:17Zoai:repositorio.unesp.br:11449/225054Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T17:53:12.176036Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Smallest universe of negative curvature
title Smallest universe of negative curvature
spellingShingle Smallest universe of negative curvature
Fagundes, Helio V. [UNESP]
title_short Smallest universe of negative curvature
title_full Smallest universe of negative curvature
title_fullStr Smallest universe of negative curvature
title_full_unstemmed Smallest universe of negative curvature
title_sort Smallest universe of negative curvature
author Fagundes, Helio V. [UNESP]
author_facet Fagundes, Helio V. [UNESP]
author_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Fagundes, Helio V. [UNESP]
description The smallest known three-dimensional closed manifold of curvature k-1 was discovered a few years ago by Weeks. This kind of manifold is constructed from a hyperbolic polyhedron with faces pairwise identified. Here it is used as the comoving spatial section of a Friedmann cosmological model, in the spirit of Ellis and Schreibers idea of small universes. Its nontrivial global topology has the effect of producing multiple images of single cosmic sources, and this is the basis of an attempt to solve a famous controversy about the redshifts of quasars. © 1993 The American Physical Society.
publishDate 1993
dc.date.none.fl_str_mv 1993-01-01
2022-04-28T20:37:17Z
2022-04-28T20:37:17Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevLett.70.1579
Physical Review Letters, v. 70, n. 11, p. 1579-1582, 1993.
0031-9007
http://hdl.handle.net/11449/225054
10.1103/PhysRevLett.70.1579
2-s2.0-3943114098
url http://dx.doi.org/10.1103/PhysRevLett.70.1579
http://hdl.handle.net/11449/225054
identifier_str_mv Physical Review Letters, v. 70, n. 11, p. 1579-1582, 1993.
0031-9007
10.1103/PhysRevLett.70.1579
2-s2.0-3943114098
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review Letters
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 1579-1582
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
_version_ 1808128871342538752

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