Microscopic Study of (p,$\gamma$) Reactions in Mass Region A=110-125

Abstract

Low energy proton capture reactions have been studied in statistical model using the semi-microscopic optical potential in the mass range A=110-125. Nuclear density obtained from relativistic mean field calculation has been folded with nucleon-nucleon interaction to obtain the optical potential. Theoretical results have been compared with experimental measurements to normalize the potential. Results have also been compared with a standard calculation available in the literature.

References in corpus (5)

• The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
• Neutron-Rich Nuclei in Heaven and Earth
• Folding model analysis of proton radioactivity of spherical proton emitters
• Low energy proton reactions of astrophysical interest in A$\sim 90-100$ region
• Correction to Relativistic Mean Field binding energy and $N_p{N}_n$ scheme

Cited by in corpus (2)

• Microscopic folding model analysis of the radiative $(n,\gamma )$ reactions near the $Z=28$ shell-closure and the weak s-process
• Radiative proton capture cross sections in the mass range $40-55$