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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/65863
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dc.contributor.authorFagundes, Helio V.-
dc.contributor.authorGausmann, Evelise-
dc.date.accessioned2014-05-27T11:19:46Z-
dc.date.accessioned2016-10-25T18:15:51Z-
dc.date.available2014-05-27T11:19:46Z-
dc.date.available2016-10-25T18:15:51Z-
dc.date.issued1999-10-18-
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.issn0375-9601-
dc.identifier.urihttp://hdl.handle.net/11449/65863-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/65863-
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.format.extent235-239-
dc.language.isoeng-
dc.sourceScopus-
dc.titleCosmic crystallography with a pullbacken
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
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.identifier.doi10.1016/S0375-9601(99)00647-7-
dc.identifier.wosWOS:000083334400002-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofPhysics Letters, Section A: General, Atomic and Solid State Physics-
dc.identifier.scopus2-s2.0-0347875984-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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