On a possibility to determine the S-factor of the hep process in experiments with thermal (cold) neutrons

preprint2000arXivOpen access

Abstract

The problem of the magnitude of the S--factor of the hep process p+3He→4He+e++νep + {^3\mathrm{He}} \to {^4\mathrm{He}} + e^+ + ν_e is one of the most important unsolved problems in nuclear astrophysics. The magnitude of S(hep)S(hep) has also an important impact on the interpretation of the Super-Kamiokande solar neutrino results in terms of neutrino oscillations. We point out the possiblity to determine the major hadronic contribution to S(hep)S(hep) from the measurement of the total cross section of the process n+3H→4He+e−+νˉen + {^3\mathrm{H}} \to {^4\mathrm{He}} + e^- + \barν_e in experiments with high intensity beams of thermal or cold neutrons.

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