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Relic abundance of mass-varying cold dark matter particles

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dc.contributor.authorRosenfeld, Rogério [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:05:58Z
dc.date.available2014-05-20T14:05:58Z
dc.date.issued2005-09-29
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.description.affiliationUNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.description.affiliationUnespUNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.format.extent158-161
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.doi10.1016/j.physletb.2005.08.049
dc.identifier.issn0370-2693
dc.identifier.urihttp://hdl.handle.net/11449/23154
dc.identifier.wosWOS:000232169100004
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofPhysics Letters B
dc.relation.ispartofjcr4.254
dc.relation.ispartofsjr2,336
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.titleRelic abundance of mass-varying cold dark matter particlesen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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São Paulo - IFT - Instituto de Física Teórica