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dc.contributor.authorDorame, Luis-
dc.contributor.authorMiranda, O. G.-
dc.contributor.authorValle, José W. F.-
dc.date.accessioned2017-07-14T12:33:05Z-
dc.date.available2017-07-14T12:33:05Z-
dc.date.issued2013-12-03-
dc.identifier.citationFront. Physics 1: 25 (2014)-
dc.identifier.issn2296-424X-
dc.identifier.urihttp://hdl.handle.net/10261/153160-
dc.description.abstractGamma-ray bursts (GRBs) are expected to provide a source of ultra high energy cosmic rays, accompanied with potentially detectable neutrinos at neutrino telescopes. Recently, IceCube has set an upper bound on this neutrino flux well below theoretical expectation. We investigate whether this mismatch between expectation and observation can be due to neutrino decay. We demonstrate the phenomenological consistency and theoretical plausibility of the neutrino decay hypothesis. A potential implication is the observability of majoron-emitting neutrinoless double beta decay.-
dc.description.sponsorshipWork supported by MINECO grants FPA2011-22975 and MULTIDARK Consolider CSD2009-00064, by Prometeo/2009/091 (Gen. Valenciana), and by EPLANET. L. D. is supported by JAE Predoctoral fellowship. O. G. M. was supported by CONACyT grant 132197.-
dc.publisherFrontiers Media-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleInvisible decays of ultra-high energy neutrinos-
dc.typeArtículo-
dc.identifier.doi10.3389/fphy.2013.00025-
dc.description.peerreviewedPeer reviewed-
dc.relation.publisherversionhttp://dx.doi.org/10.3389/fphy.2013.00025-
dc.date.updated2017-07-14T12:33:05Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066en-
dc.rights.holderCopyright © 2013 Dorame, Miranda and Valle.-
dc.rights.licensehttp://creativecommons.org/licenses/by/4.0/-
dc.contributor.funderGeneralitat Valenciana-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.contributor.funderConsejo Superior de Investigaciones Científicas (España)-
dc.contributor.funderComisión Nacional de Investigación Científica y Tecnológica (Chile)-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003359es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002848es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003339es_ES
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