Intermediate Energy Solar Neutrinos
High Energy Physics - Phenomenology
2011-01-04 v1 Astrophysics
Abstract
We 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.
Keywords
Cite
@article{arxiv.hep-ph/9511286,
title = {Intermediate Energy Solar Neutrinos},
author = {E. Calabresu and G. Fiorentini and M. Lissia and B. Ricci},
journal= {arXiv preprint arXiv:hep-ph/9511286},
year = {2011}
}
Comments
8 pages, LaTeX, plus 4 figures included via epsfig added as uuencoded compressed postscript files. Based on an invited talk given at TAUP 95, Toledo, Spain, September 1995. To appear in Nucl. Phys. B Proc. Supl