The N-14(Be-7,B-8)C-13 reaction and the Be-7(p,gamma)B-8 S factor
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abstract
The [Formula Presented] reaction was studied using an 85 MeV [Formula Presented] radioactive beam. The asymptotic normalization coefficients for the virtual transitions [Formula Presented] were determined from the measured cross section. These coefficients specify the amplitude of the tail of the [Formula Presented] overlap function in the [Formula Presented] channel, and were used to calculate the astrophysical S factor for the direct capture reaction [Formula Presented] at solar energies [Formula Presented] We find that [Formula Presented] eV b. 1999 The American Physical Society.