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Nuclear Weak Processes and Astrophysical Applications
2012
Journal of Physics, Conference Series
Nuclear weak processes are investigated based on new shell model Hamiltonians, which give successful description of spin responses in nuclei, and applied to astrophysical problems. Neutrino-induced reactions on 12 C and synthesis of light elements by supernova neutrinos, and effects of contamination of 13 C, whose natural isotopic abundance is 1.1%, on inclusive ν-12 C reactions are discussed. Spin-dipole transitions and ν-induced reactions on 16 O are studied by using a new Hamiltonian with
doi:10.1088/1742-6596/381/1/012118
fatcat:6tqjw5d7nrg4hkd37eapvgnl3e