Abstract
The 18O(p, α) 15N reaction has been studied at a proton energy of 40.9 MeV with an overall energy resolution of about 100keV. Differential cross sections for levels with excitation energies up to about 12 MeV were measured. Finite-range DWBA calculations were performed using cluster form factors, and the deduced spectroscopic factors compared with the shell-model calculations of Millener. Numerous states show considerably greater strength than predicted by the shell model.
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