Nuclear weak processes and astrophysical applications - INSPIRE

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Nuclear weak processes and astrophysical applications

Toshio Suzuki
(
- Nihon U., Tokyo and
- Tokyo U., CNS, Saitama
)
,
Michio Honma
(
- Aizu U.
)

2012

6 pages

Part of Proceedings, Rutherford Centennial Conference on Nuclear Physics : Manchester, UK, August 8-12,2011

Published in:

J.Phys.Conf.Ser. 381 (2012) 012118

Contribution to:

Rutherford Centennial Conference on Nuclear Physics

DOI:

10.1088/1742-6596/381/1/012118

View in:

Nuclear Science References

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Abstract: (IOP)

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 -(12)C reactions are discussed. Spin-dipole transitions and -induced reactions on (16)O are studied by using a new Hamiltonian with proper tensor components, and compared with conventional calculations and previous CRPA results. Gamow-Teller transition strength in (40)Ar and -induced reactions on (40)Ar by solar neutrinos are studied based on monopole-based-universal interaction (VMU). We finally discuss electron capture reactions on Ni isotopes in stellar environments.

neutrino: supernova
electron: capture
neutrino: solar
weak interaction
nucleus
Hamiltonian
Gamow-Teller transition
shell model
spin

References(21)

Figures(0)

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Toshio Suzuki
(
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,
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(
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)
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(
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)

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Toshio Suzuki
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)
,
Michio Honma
(
- Aizu U.
)
,
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)
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