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dc.contributor.authorValle, José W. F.-
dc.contributor.authorTórtola, María Amparo-
dc.contributor.authorRomao, J. C.-
dc.contributor.authorJoshipura, Anjan S.-
dc.contributor.authorJoaquim, F. R.-
dc.contributor.authorEsteves, J. N.-
dc.date.accessioned2010-11-16T12:01:20Z-
dc.date.available2010-11-16T12:01:20Z-
dc.date.issued2010-10-12-
dc.identifier.citationPhysical Review - Section D - Particles and Fields 82 (7): 073008 (2010)es_ES
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/10261/29117-
dc.description.abstractWe propose an A(4) flavor-symmetric SU(3) circle times SU(2) circle times U(1) seesaw model where lepton number is broken spontaneously. A consistent two-zero texture pattern of neutrino masses and mixing emerges from the interplay of type-I and type-II seesaw contributions, with important phenomenological predictions. We show that, if the Majoron becomes massive, such seesaw scenario provides a viable candidate for decaying dark matter, consistent with cosmic microwave background lifetime constraints that follow from current WMAP observations. We also calculate the subleading one-loop-induced decay into photons which leads to a monoenergetic emission line that may be observed in future x-ray missions such as Xenia.es_ES
dc.description.sponsorshipThis work was supported by the Spanish MICINN under grants FPA2008-00319/FPA and MULTIDARK CAD2009-00064 (Consolider-Ingenio 2010 Programme), by Prometeo/ 2009/091, by the EU Network grants UNILHC PITN-GA-2009-237920 and MRTNCT- 2006-035505 and by Fundaçao para a Ciência e a Tecnologia grants CFTP-FCT UNIT 777, POCI/81919/2007 and CERN/FP/83503/2008. M.A.T. acknowledges financial support from CSIC under the JAE-Doc program. The work of J. N. E. is supported by “Fundaçao para a Ciência e Tecnologia” under the grant SFRH/BD/29642/2006.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rightsopenAccesses_ES
dc.titleA(4)-based neutrino masses with Majoron decaying dark matteres_ES
dc.typeartículoes_ES
dc.identifier.doi10.1103/PhysRevD.82.073008-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1103/PhysRevD.82.073008es_ES
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairetypeartículo-
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.grantfulltextopen-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
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