Abstract
In order to test the reliability of reaction rate calculations in the
framework of the Hauser-Feshbach statistical model, the cross sections
of Cd-106(alpha,gamma)Sn-110 radiative capture reaction were determined
in the energy range close to the Gamow window for the astrophysical
p-process scenario. In addition, to reduce the errors in the predictions
of the statistical model calculations, the relevant optical potential
parameters are to be determined from the angular distribution
measurement of the Cd-106(alpha, alpha) Cd-106 elastic scattering
reaction at low energies.
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