Astrophysical S factor for {alpha}-capture on {sup 112}Sn in the p-process energy range
- Kocaeli University, Department of Physics, Umuttepe TR-41380, Kocaeli (Turkey)
The cross section of the reaction {sup 112}Sn({alpha},{gamma}){sup 116}Te has been measured in the energy range of astrophysical interest for the p-process. Highly enriched self-supporting {sup 112}Sn foils were bombarded with {alpha} beams in the effective center of mass energy range from 7.59 to 11.42 MeV at the Notre Dame FN Tandem Van de Graaff accelerator. The characteristic activity of {sup 116}Te was counted with a pair of large volume Ge clover detectors in close geometry to maximize the detection efficiency. The cross section of the concurrent ({alpha},p) reaction has also been measured. The results are compared with statistical model predictions for different global {alpha}-nucleus potentials.
- OSTI ID:
- 20991041
- Journal Information:
- Physical Review. C, Nuclear Physics, Vol. 75, Issue 2; Other Information: DOI: 10.1103/PhysRevC.75.025801; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2813
- Country of Publication:
- United States
- Language:
- English
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