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Relativistic mean field calculations have been performed to obtain nucleardensity pro- file. Microscopic interactions have been folded with thecalculated densities of finite nuclei to obtain a semi-microscopic potential.Life time values for the emission of proton, alpha particles and complexclusters have been calculated in the WKB approach assum- ing a tunnelingprocess through the potential barrier. Elastic scattering cross sections havebeen estimated for proton-nucleus scattering in light neutron rich nuclei. Lowen- ergy proton reactions have been studied and their astrophysicalimplications have been discussed. The success of the semi-microscopicpotentials obtained in the folding model with RMF densities in explainingnuclear decays and reactions has been emphasized.

Study of reaction and decay using densities from relativistic mean field theory