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AstrophysicalSfactor forαcapture onSn117

Physical Review C2008Vol. 78(3)

Citations Over TimeTop 10% of 2008 papers

I. Căta-Danil, D. Filipescu, M. Ivaşcu, D. Bucurescu, N. V. Zamfir, T. Glodariu, L. Stroe, G. Căta-Danil, D. G. Ghit ̧ă, C. Mihai, G. Suliman, T. Sava

Abstract

The cross sections of the $^{117}\mathrm{Sn}$($\ensuremath{\alpha},\ensuremath{\gamma}$) $^{121}\mathrm{Te}$ and $^{117}\mathrm{Sn}$($\ensuremath{\alpha},p$) $^{120}\mathrm{Sb}$ reactions have been measured in the effective center of mass energy from 11.5 to 14.6 MeV. Highly enriched self-supporting $^{117}\mathrm{Sn}$ (90%) foils were bombarded with an $\ensuremath{\alpha}$ beam delivered by the Bucharest IFIN-HH tandem accelerator. The induced activity of $^{121}\mathrm{Te}$ and $^{120}\mathrm{Sb}$ was measured with two large-volume high-purity Ge detectors in close geometry to maximize the detector efficiency. The experimental cross section and astrophysical $S$ factor are compared with statistical model predictions for different global $\ensuremath{\alpha}$-nucleus optical potentials.

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