EPJ Web of Conferences (Jan 2023)

Astrophysical S factor and reaction rate of 92,94Mo(p, γ) relevant to the p-process

  • Hingu Akash,
  • Prajapati P.M.,
  • Mukherjee S.,
  • Pizzone R.G.,
  • Katovsky K.

DOI
https://doi.org/10.1051/epjconf/202327502006
Journal volume & issue
Vol. 275
p. 02006

Abstract

Read online

Abstract. Low energy proton capture cross sections on heavy isotopes are necessary for a better understanding of the astrophysical p-process. There are around 35 proton-rich stable isotopes between 74S e and 196Hg which are bypassed by the s- and r- processes. These are commonly referred as p-nuclei whose origin is still not completely understood. In the present study, proton capture reactions are studied on Mo isotopes at astrophysically relevant energies using nuclear modular code TALYS. Astrophysical S factor and reaction rates are also calculated inside a core-collapse supernova. The obtained results are compared with the literature data taken from EXFOR data library. In addition, the effect of different combinations of the nuclear input parameters entering the stellar reaction rate have been investigated.