Stellar energy loss rates beyond the standard model

dc.contributor0000-0002-1478-7946
dc.contributor0000-0001-5324-1834
dc.contributorhttps://orcid.org/0000-0001-5324-1834
dc.contributorhttps://orcid.org/0000-0002-1478-7946
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.created2020-10-27T17:28:58Z
dc.date.issued2020-06-08
dc.identifier2190-5444
dc.identifierhttp://ricaxcan.uaz.edu.mx/jspui/handle/20.500.11845/2139
dc.identifierhttps://doi.org/10.48779/25r6-r368
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 model
dc.languageeng
dc.publisherSpringer
dc.relationgeneralPublic
dc.relationhttps://rdcu.be/b4KgV
dc.relationhttps://doi.org/10.1140/epjp/s13360-020-00454-0
dc.titleStellar energy loss rates beyond the standard model
dc.typeinfo:eu-repo/semantics/article


Este ítem pertenece a la siguiente institución