Abstract
The yield of the $^{60}\mathrm{Ni}$($^{18}\mathrm{O}$, $^{16}\mathrm{O}$)$^{62}\mathrm{Ni}_{\mathrm{g}.\mathrm{s}.}$ reaction at an incident energy of 65 MeV has been measured to forward angles using a QDDD spectrometer. Predicted, strong oscillations in the forward angle differential cross section are indeed observed. The detailed shape of this angular distribution can be reproduced by distorted-wave Born-approximation calculations employing an optical potential more strongly absorbing in the nuclear interior, and more weakly absorbing at the nuclear surface than previously used.NUCLEAR REACTIONS $^{60}\mathrm{Ni}$($^{18}\mathrm{O}$, $^{16}\mathrm{O}$); $E=65$ MeV measured $\ensuremath{\sigma}(\ensuremath{\theta})$; DWBA analysis.
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