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Constraints for solar neutrinos fluxes

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DOI: 10.1016/S0375-9474(97)00269-8
OAI: oai:inspirehep.net:419210
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INSPIRE-HEP
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Abstract

Constraints on the neutrino fluxes Φ p , Φ B , Φ CNO and Φ Be are derived from the available experimental results. Physical implications are discussed by means of non-extensive statistics which takes into account many-body effects and long-range interactions. The different reduction factors for 7 Be and 8 B fluxes with respect to their standard solar model values are physically understood, with proper shapes of the shape of the electron and proton distribution functions.

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