Emissivity of Neutrinos in Supernova via the pair-annihilation process beyond the Standard Model

dc.creatorGutiérrez Rodríguez, Alejandro
dc.creatorHernández Ruíz, María de los Angeles
dc.date.accessioned2018-08-08T14:55:22Z
dc.date.accessioned2022-10-14T15:16:33Z
dc.date.available2018-08-08T14:55:22Z
dc.date.available2022-10-14T15:16:33Z
dc.date.created2018-08-08T14:55:22Z
dc.date.issued2017-08-01
dc.identifier1742-6588
dc.identifier1742-6596
dc.identifierhttp://hdl.handle.net/20.500.11845/609
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4248678
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.
dc.languageeng
dc.publisherIOP Publishing
dc.relationgeneralPublic
dc.relationdoi :10.1088/1742-6596/888/1/012258
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/3.0/us/
dc.rightsAtribución-NoComercial-CompartirIgual 3.0 Estados Unidos de América
dc.sourceJournal of Physics: Conf. Series 888 (2017) 012258
dc.titleEmissivity of Neutrinos in Supernova via the pair-annihilation process beyond the Standard Model
dc.typeArtículos de revistas


Este ítem pertenece a la siguiente institución