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The $\alpha$-optical potential is one of the key input parameters used tomeasure the reaction rate of the ($\gamma,\alpha$)-process using theHauser-Feshbach(HF) statistical model and the principle of detailed balance.$\alpha$-elastic scattering experiment on $^{113}$In $p$-nucleus was carriedout in the energy range E$_{lab}$=26$-$32 MeV. The vacuum evaporation techniquewas used to prepare the $^{113}$In target~($\sim$86 $\mu$g/cm$^2$). Anenergy-dependent local optical potential parameters set was obtained byanalysing the experimental elastic scattering angular distribution data. Thelocal potential parameters are extrapolated for lower energies and are used tomeasure the $^{113}$In($\alpha,\gamma$) reaction cross-section.

Study of $^{113}$In($\alpha,\alpha$) elastic scattering to determine $\alpha$-optical potential relevant for astrophysical $\gamma$-process