Astrophysical S-factor for α-Capture of 113In in the p-Process Energy Range

Details Astrophysical S-factor for α-Capture of 113In in the p-Process Energy Range Astrophysical S-factor for α-Capture of 113In in the p-Process Energy Range

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1090..631y&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS: Proceedings of the 13th International Symposium on Capture Gamma-Ray Spectros

Other

Radiative Capture, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, X- And Gamma-Ray Spectroscopy

Scientific paper

The cross sections of 113In(α,γ)117Sb and 113In(α,n)116Sb reactions have been measured using the activation method. The experiments were carried out at the ATOMKI cyclotron accelerator in the center of mass energy range from 8.7 to 13.7 MeV. Astrophysical S-factors have been calculated, and preliminary results are compared with statistical model predictions.

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