出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：Coupled Reaction Channel Calculations have been performed for transitions to ground and rst
excited states of 17F and 17O at deuteron incident energies from Ed=2.279 MeV up to 3.186 MeV.
The n+16O and p+16O astrophysical direct capture cross sections have been calculated using the
spectroscopic factors obtained from 16O(d,p)17O and 16O(d,n)17F transfer reactions. The astrophysical
S-factors are compared to recent experimental data. The Maxwellian-averaged neutron
capture cross section at kT=30 keV is obtained as 22(3)m barn.
