Please use this identifier to cite or link to this item: http://ricaxcan.uaz.edu.mx/jspui/handle/20.500.11845/2139
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dc.contributor.other0000-0002-1478-7946es_ES
dc.contributor.other0000-0001-5324-1834es_ES
dc.coverage.spatialGlobales_ES
dc.creatorLlamas-Bugarin, Alejandra-
dc.creatorGutierrez-Rodriguez, Alejandro-
dc.creatorGonzalez-Sanchez, Alejandro-
dc.creatorHernandez-Ruiz, María de los Angeles-
dc.creatorEspinoza, Augusto-
dc.creatorChubykalo, Andrew-
dc.date.accessioned2020-10-27T17:28:58Z-
dc.date.available2020-10-27T17:28:58Z-
dc.date.issued2020-06-08-
dc.identifierinfo:eu-repo/semantics/publishedVersiones_ES
dc.identifier.issn2190-5444es_ES
dc.identifier.urihttp://ricaxcan.uaz.edu.mx/jspui/handle/20.500.11845/2139-
dc.description.abstractIt is known that the dipolemoments of the neutrino lead to important astrophysical and cosmological effects. In this regard, within the context of a U(1)B−L model, we develop and present novel analytical formulas to assess the effects of the anomalous magnetic moment and electric dipole moment of the neutrino on the stellar energy loss rates through some common physical process of pair-annihilation e+e− → (γ, Z, Z ) → ν¯ν. Our results show that the stellar energy loss rates strongly depend on the effective magnetic moment of the neutrino, but also on the parameters which characterize the adopted U(1)B−L modeles_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.relationhttps://rdcu.be/b4KgVes_ES
dc.relationhttps://doi.org/10.1140/epjp/s13360-020-00454-0es_ES
dc.relation.urigeneralPublices_ES
dc.subject.classificationCIENCIAS FISICO MATEMATICAS Y CIENCIAS DE LA TIERRA [1]es_ES
dc.subject.otherstandard modeles_ES
dc.subject.otherstellar energyes_ES
dc.titleStellar energy loss rates beyond the standard modeles_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
Appears in Collections:*Documentos Académicos*-- UA Cien. y Tec. de la Luz y la Mat. (LUMAT)

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