Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-02-02
Phys.Lett. B478 (2000) 208-214
Physics
High Energy Physics
High Energy Physics - Phenomenology
10 pages, no figures
Scientific paper
10.1016/S0370-2693(00)00287-2
We discuss the problem of solar hep neutrinos originating from the reaction p + 3He -> 4He + e+ + nu and obtain a relation between the astrophysical S-factor of the hep process and the cross section of the process e- + 4He -> 3H + n + nu near threshold. The relation is based on the isotopic invariance of strong interactions. The measurement of the latter cross section would allow to obtain experimental information on S(hep), the value of which, at the moment, is known only from theoretical calculations.
Alberico Wanda M.
Bernabeu Jose
Bilenky Samoil M.
Grimus Walter
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