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Relic density of neutrinos with primordial asymmetries

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Relic density of neutrinos with primordial asymmetries

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dc.contributor.author Pastor Carpi, Sergio
dc.contributor.author Pinto, Teguayco
dc.contributor.author Raffelt, Georg G.
dc.date.accessioned 2014-07-31T11:43:08Z
dc.date.available 2014-07-31T11:43:08Z
dc.date.issued 2009
dc.identifier.citation Pastor Carpi, Sergio Pinto, Teguayco Raffelt, Georg G. 2009 Relic density of neutrinos with primordial asymmetries Physical Review Letters 102 24 241302-1 241302-4
dc.identifier.uri http://hdl.handle.net/10550/37349
dc.description.abstract We study flavor oscillations in the early universe, assuming primordial neutrino-antineutrino asymmetries. Including collisions and pair processes in the kinetic equations, we not only estimate the degree of flavor equilibration, but for the first time also kinetic equilibration among neutrinos and with the ambient plasma. Typically the restrictive BBN bound on the nue-antinue asymmetry indeed applies to all flavors as claimed in the previous literature, but fine-tuned initial asymmetries always allow for a large surviving neutrino excess radiation that may show up in precision cosmological data.
dc.language.iso eng
dc.relation.ispartof Physical Review Letters, 2009, vol. 102, num. 24, p. 241302-1-241302-4
dc.subject Física
dc.title Relic density of neutrinos with primordial asymmetries
dc.type journal article es_ES
dc.date.updated 2014-07-31T11:43:08Z
dc.identifier.doi 10.1103/PhysRevLett.102.241302
dc.identifier.idgrec 060092
dc.rights.accessRights open access es_ES

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