Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..227y&link_type=abstract
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From
Physics
Cosmic Ray Nucleosynthesis, Cluster Models, Electromagnetic Transitions, Neutron Capture Gamma-Rays
Scientific paper
For the key reactions 16O(n,γ)17O and 17O(n,γ)18O on nucleosyntheses in stellar interior, the theoretical estimate for the cross section and reaction rate have been made. The careful description of the nuclear structure is important in very low energy regions. The Cluster Orbital Shell Model is adopted for reproducing the structure of the nuclei. Our results for the cross section of the 16O(n,γ)17O reaction are consistent with that of the microscopic two cluster model. The straightforward application becames possible to the case of the 17O(n,γ)18O reaction with a substantial reliance.
Kato Kazuhiro
Masui Hiroki
Ohta Masayuki
Wada Takehiko
Yamamoto Kaichi
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