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Microscopic optical potentials obtained by folding the DDM3Y interaction withthe densities from Relativistic Mean Field approach have been utilized toevaluate S-factors of low-energy $(p,\gamma)$ reactions in mass 60-80 regionand to compare with experiments. The Lagrangian density FSU Gold has beenemployed. Astrophysical rates for important proton capture reactions have beencalculated to study the behaviour of rapid proton nucleosynthesis for waitingpoint nuclei with mass less than A=80.

Microscopic calculation of proton capture reactions in mass 60-80 region and its astrophysical implications