Reaction rates for neutron capture reactions to C, N, and O isotopes to the neutron rich side of stability

H. Herndl; R. Hofinger; J. Jank; H. Oberhummer; J. Görres; M. Wiescher; F.-K. Thielemann; B. A. Brown

doi:10.1103/PhysRevC.60.064614

Reaction rates for neutron capture reactions to C, N, and O isotopes to the neutron rich side of stability

H. Herndl, R. Hofinger, J. Jank, H. Oberhummer, J. Görres, M. Wiescher, F.-K. Thielemann, and B. A. Brown

Phys. Rev. C 60, 064614 – Published 16 November 1999

Abstract

The reaction rates of neutron capture reactions on light nuclei are important for reliably simulating nucleosynthesis in a variety of stellar scenarios. Neutron capture reaction rates on neutron-rich C, N, and O isotopes are calculated in the framework of a hybrid compound and direct capture model. The results are tabulated and compared with the results of previous calculations as well as with experimental results.