Neutrino Nucleosynthesis in Supernovae

Details Neutrino Nucleosynthesis in Supernovae Neutrino Nucleosynthesis in Supernovae

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1120..165y&link_type=abstract

PERSPECTIVE IN NUCLEAR PHYSICS: Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics. AIP Conference Proceedings,

Other

Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Neutrino Mass And Mixing, Cosmic Rays

Scientific paper

Neutrino nucleosynthesis is an important synthesis process for light elements in supernovae. One important physics input of neutrino nucleosynthesis is cross sections of neutrino-nucleus reactions. The cross sections of neutrino-12C and 4He reactions are derived using new shell model Hamiltonians. With the new cross sections, light element synthesis of a supernova is investigated. The appropriate range of the neutrino temperature for supernovae is constrained to be between 4.3 MeV and 6.5 MeV from the 11B abundance in Galactic chemical evolution. Effects by neutrino oscillations are also discussed.

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