Study of the (p, γ) and (α, γ) reactions for 96,98,104Ru and 112,114,116Sn at astrophysically relevant energies
- Authors: Bajpeyi A.1, Shukla A.1, Koning A.J.2, Åberg S.3
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Affiliations:
- Department of Physics
- Nuclear Research and Consultancy Group NRG
- Mathematical Physics
- Issue: Vol 80, No 3 (2017)
- Pages: 402-411
- Section: Nuclei Theory
- URL: https://journals.rcsi.science/1063-7788/article/view/191819
- DOI: https://doi.org/10.1134/S1063778817030024
- ID: 191819
Cite item
Abstract
Cross section and S factor of the proton- and alpha-induced reactions have been studied for the Ruthenium and tin isotopes in the effective energy range, i.e. Gamow window. These reactions are important for developing the understanding for nucleosynthesis, particularly for the synthesis of p nuclei (p process). In this work, cross sections and S factor have been calculated through TALYS in Hauser–Feshbach formalism using nuclear densities calculated in relativistic mean field (RMF) formalism. Calculated results of cross sections, S factor and nuclear structure have been compared with existing theoretical as well as experimental results available and are found to be in good agreement.
About the authors
Awanish Bajpeyi
Department of Physics
Email: amritanshu.shukla@gmail.com
India, Raebareli
A. Shukla
Department of Physics
Author for correspondence.
Email: amritanshu.shukla@gmail.com
India, Raebareli
A. J. Koning
Nuclear Research and Consultancy Group NRG
Email: amritanshu.shukla@gmail.com
Netherlands, Petten
Sven Åberg
Mathematical Physics
Email: amritanshu.shukla@gmail.com
Sweden, Lund
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