Solar neutrinos (almost) without standard solar models

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dc.creatorFiorentini, G.
dc.creatorRicci, B.
dc.date1995-09-30
dc.date.accessioned2026-07-07T03:58:16Z
dc.date.available2026-07-07T03:58:16Z
dc.descriptionWe extract information on the fluxes of Be and CNO neutrinos directly from solar neutrino experiments, with minimal assumptions about solar models. Next we compare these results with solar models, both standard and non standard ones. Finally we discuss the expectations for Borexino, both in the case of standard and non standard neutrinos.
dc.descriptionBased on invited talks to Workshop on Double Beta Decay and Related Topics, Trento Italy, April 1995 and to TAUP95, Toledo Spain, September 1995. 11 pages with included figures, uuencoded postscript file
dc.identifierhttps://arxiv.org/abs/hep-ph/9509429
dc.identifierhttp://arxiv.org/abs/hep-ph/9509429
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45740
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSolar neutrinos (almost) without standard solar models
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