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Cosmic crystallography with a pullback

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dc.contributor.authorFagundes, Helio V. [UNESP]
dc.contributor.authorGausmann, Evelise [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-27T11:19:46Z
dc.date.available2014-05-27T11:19:46Z
dc.date.issued1999-10-18
dc.description.abstractWe present a modified version of the cosmic crystallography method, especially useful for testing closed models of negative spatial curvature. The images of clusters of galaxies in simulated catalogs are 'pulled back' to the fundamental domain before the set of distances is calculated. © 1999 Published by Elsevier Science B.V. All rights reserved.en
dc.description.affiliationInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona, 145, São Paulo, SP 01405-900
dc.description.affiliationUnespInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona, 145, São Paulo, SP 01405-900
dc.format.extent235-239
dc.identifierhttp://dx.doi.org/10.1016/S0375-9601(99)00647-7
dc.identifier.citationPhysics Letters, Section A: General, Atomic and Solid State Physics, v. 261, n. 5-6, p. 235-239, 1999.
dc.identifier.doi10.1016/S0375-9601(99)00647-7
dc.identifier.issn0375-9601
dc.identifier.scopus2-s2.0-0347875984
dc.identifier.urihttp://hdl.handle.net/11449/65863
dc.identifier.wosWOS:000083334400002
dc.language.isoeng
dc.relation.ispartofPhysics Letters, Section A: General, Atomic and Solid State Physics
dc.relation.ispartofjcr1.863
dc.relation.ispartofsjr0,595
dc.rights.accessRightsAcesso restrito
dc.sourceScopus
dc.titleCosmic crystallography with a pullbacken
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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