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

Abstract

The problem of the magnitude of the S--factor of the hep process p + 3He 4He + e+ + e is one of the most important unsolved problems in nuclear astrophysics. The magnitude of 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) from the measurement of the total cross section of the process n + 3H 4He + e- + e in experiments with high intensity beams of thermal or cold neutrons.

0

Turn this paper into a full lesson

ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.

Discussion (0)

Sign in to join the discussion.

Loading comments…