1. E1 strength of the subthreshold 3/2+ state in 15O studied by Coulomb excitation
- Author
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H. Akiyoshi, Tomoko Gomi, Susumu Shimoura, H. Kobayashi, Masakazu Ishihara, Shuichi Ozawa, Satoshi Takeuchi, Koichi Yoshida, Yoshiyuki Yanagisawa, K. Yamada, Toshiharu Teranishi, N. Imai, Yoshihide Higurashi, Zs. Fülöp, Toshiyuki Minemura, Nori Aoi, Hiroyoshi Sakurai, T. Motobayashi, H. Iwasaki, Naohito Iwasa, Yoshiyuki Iwata, Zhiqiang Liu, M. Serata, and Meiko Kurokawa
- Subjects
Physics ,CNO cycle ,Nuclear and High Energy Physics ,Hydrogen ,Subthreshold conduction ,Coulomb excitation ,Electric potential energy ,Radiative width ,chemistry.chemical_element ,State (functional analysis) ,Stars ,chemistry ,Radiative transfer ,Radioactive beam ,Atomic physics - Abstract
The radiative width of the 3/2+ state at 6.793 MeV in 15O has been experimentally determined to be Γγ=0.95+0.60−0.95 eV by intermediate-energy Coulomb excitation. Our result independently supports the recent studies which point to a minor contribution of this state to the astrophysical rate of the 14N(p,γ)15O reaction in the CNO-cycle hydrogen burning in massive stars.
- Published
- 2004
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