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Title: Neutral currents, supernovae neutrinos, and nucleosynthesis

Conference ·
OSTI ID:6595216

The inelastic interactions of neutrinos during stellar collapse and neutron star cooling are discussed. The primary mechanism for dissipative neutrino reactions is nuclear excitation by neutral current scattering, a process not included in standard descriptions of supernovae. Charge-current and neutral current ''preheating'' of iron lying outside the shock front appears to be significant in the few milliseconds near shock breakout. This could help produce a more energetic shock. During the cooling phase, the neutral current interactions of muon and taon neutrinos appear to be responsible for some interesting nucleosynthesis. I discuss two examples the production of fluorine and neutrino-induced r-process nucleosynthesis. 26 refs., 1 fig., 3 tabs.

Research Organization:
Washington Univ., Seattle (USA). Inst. for Nuclear Theory
DOE Contract Number:
FG06-88ER40427
OSTI ID:
6595216
Report Number(s):
DOE/ER/40427-20-N8; CONF-880639-7; ON: DE89004565
Resource Relation:
Conference: International conference on contemporary topics in nuclear structure physics, Cocoyoc, Mexico, 9 Jun 1988; Other Information: Portions of this document are illegible in microfiche products
Country of Publication:
United States
Language:
English