Be7(p,gamma)B8 and the high-energy solar neutrino flux

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dc.creatorCsoto, Attila
dc.date1997-04-23
dc.date.accessioned2026-07-07T05:41:58Z
dc.date.available2026-07-07T05:41:58Z
dc.descriptionThe importance of the Be7(p,gamma)B8 reaction in predicting the high-energy solar neutrino flux is discussed. I present a microscopic eight-body model and a potential model for the calculation of the Be7(p,gamma)B8 cross section.
dc.description4 pages with 3 figures. To appear in the proceedings of the "Exotic Nuclear Shapes" Conference
dc.identifierhttps://arxiv.org/abs/nucl-th/9704053
dc.identifierhttp://arxiv.org/abs/nucl-th/9704053
dc.identifierHeavy Ion Physics 6 (1997) 103
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82769
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleBe7(p,gamma)B8 and the high-energy solar neutrino flux
dc.typetext

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