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

dc.contributor	121130	es_ES
dc.coverage.spatial	Global	es_ES
dc.creator	Gutiérrez Rodríguez, Alejandro
dc.creator	Hernández Ruíz, María de los Angeles
dc.date.accessioned	2018-08-08T14:55:22Z
dc.date.available	2018-08-08T14:55:22Z
dc.date.issued	2017-08-01
dc.identifier	info:eu-repo/semantics/publishedVersion	es_ES
dc.identifier.issn	1742-6588	es_ES
dc.identifier.issn	1742-6596	es_ES
dc.identifier.uri	http://hdl.handle.net/20.500.11845/609
dc.description.abstract	We 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.iso	eng	es_ES
dc.publisher	IOP Publishing	es_ES
dc.relation	doi :10.1088/1742-6596/888/1/012258	es_ES
dc.relation.uri	generalPublic	es_ES
dc.rights	Atribución-NoComercial-CompartirIgual 3.0 Estados Unidos de América	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-sa/3.0/us/	*
dc.source	Journal of Physics: Conf. Series 888 (2017) 012258	es_ES
dc.subject.classification	CIENCIAS FISICO MATEMATICAS Y CIENCIAS DE LA TIERRA [1]	es_ES
dc.subject.other	Neutrinos	es_ES
dc.subject.other	nuclear reactions	es_ES
dc.title	Emissivity of Neutrinos in Supernova via the pair-annihilation process beyond the Standard Model	es_ES
dc.type	info:eu-repo/semantics/article	es_ES