Spin Modes, Neutrino-Induced Reactions and Nucleosynthesis in Stars

Journal Article · Tue Nov 11 00:00:00 EST 2008 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.3039812· OSTI ID:21254788

Suzuki, Toshio ^[1]; Otsuka, Takaharu ^[2]; Honma, Michio ^[3]; Higashiyama, Koji ^[4]

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1. Department of Physics, College of Humanities and Sciences, Nihon University, Sakurajosui 3-25-40, Setagaya-ku, Tokyo 156-8550 (Japan)
2. Department of Physics and Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)
3. Center for Mathematical Sciences, University of Aizu, Aizu-Wakamatsu, Fukushima (Japan)
4. Department of Physics, Chiba Institute of Technology, Narashino, Chiba 275-0023 (Japan)

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 {sup 56}Fe and {sup 56}Ni are studied, and implications on production yields of heavy elements in stars are discussed.

• OSTI ID: 21254788
• Journal Information: AIP Conference Proceedings, Vol. 1072, Issue 1; Conference: International conference on nuclear physics and astrophysics: From stable beams to exotic nuclei, Cappadocia (Turkey), 25-30 Jun 2008; Other Information: DOI: 10.1063/1.3039812; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
CARBON ISOTOPES
ENERGY-LEVEL TRANSITIONS
HAMILTONIANS
IRON 56
NEUTRINO REACTIONS
NEUTRINOS
NICKEL 56
NUCLEOSYNTHESIS
SHELL MODELS
SPIN
STAR EVOLUTION
STARS
TENSORS