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Study of the (p, γ) and (α, γ) reactions for 96,98,104Ru and 112,114,116Sn at astrophysically relevant energies

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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.

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Authors and Affiliations

  1. Department of Physics, Rajiv Gandhi Institute of Petroleum Technology, Raebareli, India

    Awanish Bajpeyi & A. Shukla

  2. Nuclear Research and Consultancy Group NRG, Petten, The Netherlands

    A. J. Koning

  3. Mathematical Physics, Lund University, Lund, Sweden

    Sven Åberg

Authors
  1. Awanish Bajpeyi
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  2. A. Shukla
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  3. A. J. Koning
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  4. Sven Åberg
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Corresponding author

Correspondence to A. Shukla.

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The text was submitted by the authors in English.

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Bajpeyi, A., Shukla, A., Koning, A.J. et al. Study of the (p, γ) and (α, γ) reactions for 96,98,104Ru and 112,114,116Sn at astrophysically relevant energies. Phys. Atom. Nuclei 80, 402–411 (2017). https://doi.org/10.1134/S1063778817030024

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