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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/113059
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dc.contributor.authorBernal, Nicolas-
dc.contributor.authorColucci, Stefano-
dc.contributor.authorJosse-Michaux, Francois-Xavier-
dc.contributor.authorRacker, J.-
dc.contributor.authorUbaldi, Lorenzo-
dc.date.accessioned2014-12-03T13:11:22Z-
dc.date.accessioned2016-10-25T20:14:00Z-
dc.date.available2014-12-03T13:11:22Z-
dc.date.available2016-10-25T20:14:00Z-
dc.date.issued2013-10-01-
dc.identifierhttp://dx.doi.org/10.1088/1475-7516/2013/10/035-
dc.identifier.citationJournal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 10, 30 p., 2013.-
dc.identifier.issn1475-7516-
dc.identifier.urihttp://hdl.handle.net/11449/113059-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/113059-
dc.description.abstractWe study in detail the conditions to generate the baryon asymmetry of the universe from the annihilation of dark matter. This scenario requires a low energy mechanism for thermal baryogenesis, hence we first discuss some of these mechanisms together with the specific constraints due to the connection with the dark matter sector. Then we show that, contrary to what stated in previous studies, it is possible to generate the cosmological asymmetry without adding a light sterile dark sector, both in models with violation and with conservation of B - L. In addition, one of the models we propose yields some connection to neutrino masses.en
dc.description.sponsorshipDFG-
dc.description.sponsorshipPortuguese national funds through FCT - Fundacao para a Ciencia e Tecnologia-
dc.description.sponsorshipSpanish MINECO Subprogramme Juan de la Cierva-
dc.description.sponsorshipSpanish MINECO-
dc.description.sponsorshipConsolider-Ingenio CUP-
dc.description.sponsorshipEuropean Union-
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.format.extent30-
dc.language.isoeng-
dc.publisherIop Publishing Ltd-
dc.sourceWeb of Science-
dc.subjectdark matter theoryen
dc.subjectbaryon asymmetryen
dc.subjectleptogenesisen
dc.titleOn baryogenesis from dark matter annihilationen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniv Bonn-
dc.contributor.institutionUniv Turin-
dc.contributor.institutionUniv Tecn Lisboa-
dc.contributor.institutionUniv Valencia-
dc.description.affiliationUniv Estadual Paulista, ICTP South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, Brazil-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil-
dc.description.affiliationUniv Bonn, Bethe Ctr Theoret Phys, D-53115 Bonn, Germany-
dc.description.affiliationUniv Bonn, Inst Phys, D-53115 Bonn, Germany-
dc.description.affiliationUniv Turin, Dept Phys, I-10125 Turin, Italy-
dc.description.affiliationUniv Tecn Lisboa, CFTP, Inst Super Tecn, P-1049001 Lisbon, Portugal-
dc.description.affiliationUniv Valencia, CSIC, Inst Fis Corpuscular IFIC, Valencia 46071, Spain-
dc.description.affiliationUnespUniv Estadual Paulista, ICTP South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil-
dc.description.sponsorshipIdDFGTRR33-
dc.description.sponsorshipIdPortuguese national funds through FCT - Fundacao para a Ciencia e TecnologiaPEst-OE/FIS/UI0777/2011-
dc.description.sponsorshipIdSpanish MINECOFPA2011-29678-C02-01-
dc.description.sponsorshipIdConsolider-Ingenio CUPC5D2008-00037-
dc.description.sponsorshipIdEuropean UnionPITN-GA-2011-289442-
dc.description.sponsorshipIdFAPESP: 13/01792-8-
dc.description.sponsorshipIdPTDC/FIS-NUC/0548/2012-
dc.description.sponsorshipIdCERN/FP/123580/2011-
dc.identifier.doi10.1088/1475-7516/2013/10/035-
dc.identifier.wosWOS:000326979500035-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofJournal of Cosmology and Astroparticle Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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