Cross section measurements of alpha-induced reactions on (92,94)Mo and (112)Sn for p-process studies
The (92)Mo(alpha, n)(95)Ru, (94)Mo(alpha, n)(97)Ru, and (112)Sn(alpha, gamma)(116)Te cross sections were measured at the upper end of the p-process Gamow window between 8.2 and 11.1 MeV. Our results are slightly lower than global Hauser-Feshbach calculations from the code NON-SMOKER, but still within the uncertainty of the prediction. The (112)Sn(alpha, gamma)(116)T, cross section agrees well with a recently measured thick-target cross section in the same energy range. For the (92,94)Mo(alpha, n) reactions the present data close to the reaction thresholds could eliminate previous uncertainties within a factor of 20, and we can present now useful comparisons to statistical model calculations with different optical potentials.
Item Type | Article |
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Keywords | nuclear, statistical-model calculations, energies, process nucleosynthesis, massive stars, particles, elastic-scattering, astrophysical reaction-rates, rp-process, excitation-functions |
Date Deposited | 15 May 2025 12:35 |
Last Modified | 30 May 2025 23:54 |
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picture_as_pdf - 0809.0234v1.pdf
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subject - Submitted Version