Spin Modes, Neutrino-Induced Reactions and Nucleosynthesis in Stars

Details Spin Modes, Neutrino-Induced Reactions and Nucleosynthesis in Stars Spin Modes, Neutrino-Induced Reactions and Nucleosynthesis in Stars

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1072..112s&link_type=abstract

NUCLEAR PHYSICS AND ASTROPHYSICS: Nuclear Physics and Astrophysics: From Stable Beams to Exotic Nuclei. AIP Conference Proceedi

Physics

Nuclear Physics

Shell Model, Weak Interaction And Neutrino Induced Processes, Galactic Radioactivity, Neutrino Scattering

Scientific paper

Recent advances in shell model calculations of spin modes in nuclei with the use of new shell model Hamiltonians are discussed. Important roles of tensor interaction in shell evolutions toward drip-lines are pointed out. Electromagnetic transitions in exotic carbon isotopes are investigated. Anomalous supressions of transition strengths in the isotopes are found to be rather well explained. Neutrino-induced reactions on 56Fe and 56Ni are studied, and implications on production yields of heavy elements in stars are discussed.

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