Abstract
Cross sections for the production of , , , and produced in the reaction have been measured over the energy range 60—160 MeV. Detailed angular distributions are presented for exit channels leading to , , and (g.s.), along with cross sections for the three-body exit channels leading to the production of and . The astrophysical significance of the reaction is discussed with particular emphasis on the production of in the interaction of galactic cosmic rays with the interstellar medium. In addition, two-nucleon-transfer distorted-wave Born approximation calculations are presented in an attempt to understand the reaction mechanism operating in the reaction.
NUCLEAR REACTIONS (,HI), HI=, , , and ; MeV; measured and ; astrophysical relevance discussed; DWBA calculations for (,).
- Received 13 July 1981
DOI:https://doi.org/10.1103/PhysRevC.25.34
©1982 American Physical Society