Relativistic Mean Field in $A\approx$80 nuclei and low energy proton reactions

Abstract

Relativistic Mean Field calculations have been performed for a number of nuclei in mass $A\approx$80 region. Ground state binding energy, charge radius and charge density values have been compared with experiment. Optical potential have been generated folding the nuclear density with the microscopic nuclear interaction DDM3Y. S-factors for low energy ($p,\gamma$) and ($p,n$) reactions have been calculated and compared with experiment.

To appear in Physical Review C

References in corpus (10)

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Cited by in corpus (12)

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• Low energy proton reactions of astrophysical interest in A$\sim 90-100$ region
• Endpoint of $rp$ process using relativistic mean field approach and a new mass formula
• Low-energy proton capture reactions in the mass region 55-60
• Neutron Capture Reactions near N=82 Shell-Closure
• Neutron capture reactions relevant to s-process and p-process in the domain of the $N=50$ shell closure
• Microscopic Study of (p,$\gamma$) Reactions in Mass Region A=110-125
• Importance of Q-values in astrophysical rp-proces
• Novel feature of doubly bubble nuclei in 50$\le$Z(N)$\le$82 region along with magicity and weakly bound structure
• 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 $40-55$
• Importance of $\alpha$-induced reactions and the inverse $(\gamma ,\alpha )$ on $p$-nuclei