Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps

Detalhes bibliográficos
Autor(a) principal: Fagundes, H. V.
Data de Publicação: 1996
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1086/177847
http://hdl.handle.net/11449/36727
Resumo: On the possibility that the universe's matter density is low (Ohm(0) < 1), cosmologies can be considered with the metric of Friedmann's open universe but with closed hyperbolic manifolds as the physical three-space. These models have nontrivial spatial topology, with the property of producing multiple images of cosmic sources. Here a fit is attempted of 10 of these models to the physical cold and hot spots found by Cayon & Smoot in the COBE/DMR maps. These spots are interpreted as early, distant images of much nearer sources of inhomogeneity. The source for one of the cold spots is seen as the seed of a known supercluster.
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spelling Fitting hyperbolic universes to Cayon-Smoot spots in COBE mapscosmic microwave backgroundcosmology, theoryOn the possibility that the universe's matter density is low (Ohm(0) < 1), cosmologies can be considered with the metric of Friedmann's open universe but with closed hyperbolic manifolds as the physical three-space. These models have nontrivial spatial topology, with the property of producing multiple images of cosmic sources. Here a fit is attempted of 10 of these models to the physical cold and hot spots found by Cayon & Smoot in the COBE/DMR maps. These spots are interpreted as early, distant images of much nearer sources of inhomogeneity. The source for one of the cold spots is seen as the seed of a known supercluster.UNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405900 SAO PAULO,BRAZILUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405900 SAO PAULO,BRAZILUniv Chicago PressUniversidade Estadual Paulista (Unesp)Fagundes, H. V.2014-05-20T15:26:34Z2014-05-20T15:26:34Z1996-10-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article43-48application/pdfhttp://dx.doi.org/10.1086/177847Astrophysical Journal. Chicago: Univ Chicago Press, v. 470, n. 1, p. 43-48, 1996.0004-637Xhttp://hdl.handle.net/11449/3672710.1086/177847WOS:A1996VL72300003WOSA1996VL72300003.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstrophysical Journal5.551info:eu-repo/semantics/openAccess2023-12-14T06:17:24Zoai:repositorio.unesp.br:11449/36727Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-12-14T06:17:24Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
title Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
spellingShingle Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
Fagundes, H. V.
cosmic microwave background
cosmology, theory
title_short Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
title_full Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
title_fullStr Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
title_full_unstemmed Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
title_sort Fitting hyperbolic universes to Cayon-Smoot spots in COBE maps
author Fagundes, H. V.
author_facet Fagundes, H. V.
author_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Fagundes, H. V.
dc.subject.por.fl_str_mv cosmic microwave background
cosmology, theory
topic cosmic microwave background
cosmology, theory
description On the possibility that the universe's matter density is low (Ohm(0) < 1), cosmologies can be considered with the metric of Friedmann's open universe but with closed hyperbolic manifolds as the physical three-space. These models have nontrivial spatial topology, with the property of producing multiple images of cosmic sources. Here a fit is attempted of 10 of these models to the physical cold and hot spots found by Cayon & Smoot in the COBE/DMR maps. These spots are interpreted as early, distant images of much nearer sources of inhomogeneity. The source for one of the cold spots is seen as the seed of a known supercluster.
publishDate 1996
dc.date.none.fl_str_mv 1996-10-10
2014-05-20T15:26:34Z
2014-05-20T15:26:34Z
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/10.1086/177847
Astrophysical Journal. Chicago: Univ Chicago Press, v. 470, n. 1, p. 43-48, 1996.
0004-637X
http://hdl.handle.net/11449/36727
10.1086/177847
WOS:A1996VL72300003
WOSA1996VL72300003.pdf
url http://dx.doi.org/10.1086/177847
http://hdl.handle.net/11449/36727
identifier_str_mv Astrophysical Journal. Chicago: Univ Chicago Press, v. 470, n. 1, p. 43-48, 1996.
0004-637X
10.1086/177847
WOS:A1996VL72300003
WOSA1996VL72300003.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astrophysical Journal
5.551
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 43-48
application/pdf
dc.publisher.none.fl_str_mv Univ Chicago Press
publisher.none.fl_str_mv Univ Chicago Press
dc.source.none.fl_str_mv Web of Science
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_ 1799965277604020224

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