dc.creatorSamana, Arturo Rodolfo
dc.creatorBarbero, César Alberto
dc.creatorDuarte, S. B.
dc.creatorDimarco, A. J.
dc.creatorKrmpotić, Francisco
dc.date2008
dc.date2019-10-10T14:26:20Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/83039
dc.identifierissn:1367-2630
dc.descriptionThe nuclear gross theory, originally formulated by Takahashi and Yamada (1969 Prog. Theor. Phys. 41 1470) for the β-decay, is applied to the electronic-neutrino nucleus reactions, employing a more realistic description of the energetics of the Gamow-Teller resonances. The model parameters are gauged from the most recent experimental data, both for βand electron capture, separately for even-even, even-odd, odd-odd and odd-even nuclei. The numerical estimates for neutrino-nucleus cross-sections agree fairly well with previous evaluations done within the framework of microscopic models. The formalism presented here can be extended to the heavy nuclei mass region, where weak processes are quite relevant, which is of astrophysical interest because of its applications in supernova explosive nucleosynthesis.
dc.descriptionFacultad de Ciencias Exactas
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto de Física La Plata
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/3.0/
dc.rightsCreative Commons Attribution 3.0 Unported (CC BY 3.0)
dc.subjectFísica
dc.subjectnuclear neutrino capture
dc.subjectnuclear β-decay
dc.titleThe gross theory model for neutrino-nucleus cross-section
dc.typeArticulo
dc.typeArticulo


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