Tests of transfer reaction determinations of astrophysicalSfactors
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The [Formula Presented] reaction has been used to determine asymptotic normalization coefficients for transitions to the ground and first excited states of [Formula Presented] The coefficients provide the normalization for the tails of the overlap functions for [Formula Presented] and allow us to calculate the S factors for [Formula Presented] at astrophysical energies. The calculated S factors are compared to measurements and found to be in very good agreement. This provides a test of this indirect method to determine astrophysical direct capture rates using transfer reactions. In addition, our results yield [Formula Presented] for capture to the ground and first excited states in [Formula Presented] without the uncertainty associated with extrapolation from higher energies. 1999 The American Physical Society.
author list (cited authors)
Gagliardi, C. A., Tribble, R. E., Azhari, A., Clark, H. L., Lui, Y., Mukhamedzhanov, A. M., ... Vincour, J.
complete list of authors
Gagliardi, CA||Tribble, RE||Azhari, A||Clark, HL||Lui, Y-W||Mukhamedzhanov, AM||Sattarov, A||Trache, L||Burjan, V||Cejpek, J||Kroha, V||Piskoř, Š||Vincour, J