Astrophysical S-factor for alpha-Capture of (113)In in the p-Process Energy Range
Yalcin, C., Gueray, R. T., Oezkan, N., Kutlu, S., Gyuerky, Gy., Farkas, J., Kiss, G. G., Fueloep, Zs., Rauscher, T. and Somorjai, E.
(2009)
Astrophysical S-factor for alpha-Capture of (113)In in the p-Process Energy Range.
American Institute of Physics (AIP).
The cross sections of (113)In(alpha, gamma)(117)Sb and (113)In(alpha,n)(116)Sb 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.
Item Type | Other |
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Keywords | p-process; (113)In; nucleosynthesis; reaction cross section |
Date Deposited | 29 May 2025 09:03 |
Last Modified | 29 May 2025 09:03 |