dc.creator | Gutiérrez Rodríguez, Alejandro | |
dc.creator | Hernández Ruíz, María de los Angeles | |
dc.date.accessioned | 2018-08-08T14:55:22Z | |
dc.date.accessioned | 2022-10-14T15:16:33Z | |
dc.date.available | 2018-08-08T14:55:22Z | |
dc.date.available | 2022-10-14T15:16:33Z | |
dc.date.created | 2018-08-08T14:55:22Z | |
dc.date.issued | 2017-08-01 | |
dc.identifier | 1742-6588 | |
dc.identifier | 1742-6596 | |
dc.identifier | http://hdl.handle.net/20.500.11845/609 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4248678 | |
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. | |
dc.language | eng | |
dc.publisher | IOP Publishing | |
dc.relation | generalPublic | |
dc.relation | doi :10.1088/1742-6596/888/1/012258 | |
dc.rights | http://creativecommons.org/licenses/by-nc-sa/3.0/us/ | |
dc.rights | Atribución-NoComercial-CompartirIgual 3.0 Estados Unidos de América | |
dc.source | Journal of Physics: Conf. Series 888 (2017) 012258 | |
dc.title | Emissivity of Neutrinos in Supernova via the pair-annihilation process beyond the Standard Model | |
dc.type | Artículos de revistas | |