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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23154
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dc.contributor.authorRosenfeld, Rogério-
dc.date.accessioned2014-05-20T14:05:58Z-
dc.date.accessioned2016-10-25T17:11:16Z-
dc.date.available2014-05-20T14:05:58Z-
dc.date.available2016-10-25T17:11:16Z-
dc.date.issued2005-09-29-
dc.identifierhttp://dx.doi.org/10.1016/j.physletb.2005.08.049-
dc.identifier.citationPhysics Letters B. Amsterdam: Elsevier B.V., v. 624, n. 3-4, p. 158-161, 2005.-
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/11449/23154-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/23154-
dc.description.abstractIn models of coupled dark energy and dark matter the mass of the dark matter particle depends on the cosmological evolution of the dark energy field. In this Letter we exemplify in a simple model the effects of this mass variation on the relic abundance of cold dark matter. (c) 2005 Elsevier B.V. All rights reserved.en
dc.format.extent158-161-
dc.language.isoeng-
dc.publisherElsevier B.V.-
dc.sourceWeb of Science-
dc.titleRelic abundance of mass-varying cold dark matter particlesen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUnespUNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.doi10.1016/j.physletb.2005.08.049-
dc.identifier.wosWOS:000232169100004-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofPhysics Letters B-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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