Spectroscopic factors and asymptotic normalization coefficients (ANCs) have been determined for bound states in O-15 using the N-14(He-3,d)O-15 reaction. These results are used to calculate the astrophysical S factor for direct capture in the N-14(p,gamma)O-15 reaction. We also discuss how uncertainties in optical-model parameters influence both the spectroscopic factors and the ANCs, and the effect that this has on the predicted direct-capture reaction rate.
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