Low energy ($p,\gamma$) reactions in Ni and Cu nuclei using microscopic optical model

Abstract

Radiative capture reactions for low energy protons have been theoretically studied for Ni and Cu isotopes using the microscopic optical model. The optical potential has been obtained in the folding model using different microscopic interactions with the nuclear densities from Relativistic Mean Field calculations. The calculated total cross sections as well as the cross sections for individually low lying levels have been compared with measurements involving stable nuclear targets. Rates for the rapid proton capture process have been evaluated for astrophysically important reactions.

To appear in Physical Review C

References in corpus (4)

• Neutron-Rich Nuclei in Heaven and Earth
• Simple parametrization of $\alpha$-decay spectroscopic factor in $150\le A\le 200$ region
• Correction to Relativistic Mean Field binding energy and $N_p{N}_n$ scheme
• Role of pairing interaction in neutron rich odd and even Zr nuclei

Cited by in corpus (9)

• Effects of $NN$ potentials on $p$ nuclides in the A$\sim$100-120 region
• Microscopic calculation of proton capture reactions in mass 60-80 region and its astrophysical implications
• Relativistic Mean Field in $A\approx$80 nuclei and low energy proton reactions
• Low energy proton reactions of astrophysical interest in A$\sim 90-100$ region
• Neutron Capture Reactions near N=82 Shell-Closure
• Low-energy proton capture reactions in the mass region 55-60
• Proton dripline in a new formula for nuclear binding energy
• Microscopic Study of (p,$\gamma$) Reactions in Mass Region A=110-125
• Radiative proton capture cross sections in the mass range $40-55$