Please use this identifier to cite or link to this item: http://ricaxcan.uaz.edu.mx/jspui/handle/20.500.11845/609
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dc.contributor121130es_ES
dc.coverage.spatialGlobales_ES
dc.creatorGutiérrez Rodríguez, Alejandro-
dc.creatorHernández Ruíz, María de los Angeles-
dc.date.accessioned2018-08-08T14:55:22Z-
dc.date.available2018-08-08T14:55:22Z-
dc.date.issued2017-08-01-
dc.identifierinfo:eu-repo/semantics/publishedVersiones_ES
dc.identifier.issn1742-6588es_ES
dc.identifier.issn1742-6596es_ES
dc.identifier.urihttp://hdl.handle.net/20.500.11845/609-
dc.description.abstractWe calculate the emissivity due to neutrino-pair production in e+ e- annihilation in the context of a 331 model and a left-right symmetric model in a way that can be used intorealistic supernova model to evaluate the energy lost in the form of neutrinos.es_ES
dc.language.isoenges_ES
dc.publisherIOP Publishinges_ES
dc.relationdoi :10.1088/1742-6596/888/1/012258es_ES
dc.relation.urigeneralPublices_ES
dc.rightsAtribución-NoComercial-CompartirIgual 3.0 Estados Unidos de América*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.sourceJournal of Physics: Conf. Series 888 (2017) 012258es_ES
dc.subject.classificationCIENCIAS FISICO MATEMATICAS Y CIENCIAS DE LA TIERRA [1]es_ES
dc.subject.otherNeutrinoses_ES
dc.subject.othernuclear reactionses_ES
dc.titleEmissivity of Neutrinos in Supernova via the pair-annihilation process beyond the Standard Modeles_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
Appears in Collections:*Documentos Académicos*-- UA Ciencias Químicas

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