[Submitted on 14 Jul 2016]
Radiative proton capture cross sections in the mass range
Dipti Chakraborty · Saumi Dutta · G. Gangopadhyay · Abhijit Bhattacharyya
Proton capture cross sections in the energy range of astrophysical interest for mass region 40-54 have been calculated in the Hauser-Feshbach formalism with reaction code TALYS1.6. The density dependent M3Y effective nucleon-nucleon interaction folded with target radial matter densities from relativistic mean field approach is used to obtain the semi-microscopic optical potential. A definite normalization of potential-well depths has been used over the entire mass region. The rates of some reactions, important in the astrophysical scenario, are calculated using the potential in the relevant mass region.
- Comments:
- 9 pages, 6 figures, accepted for publication in the journal Physical Review C
- Subjects:
- Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE); Solar and Stellar Astrophysics (astro-ph.SR)
- arXiv:
- 1607.03986 [pdf]