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APS » Journals » Phys. Rev. C » Volume 60 » Issue 6
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Phys. Rev. C 60, 064614 (1999) [12 pages]

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

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H. Herndl, R. Hofinger, J. Jank, and H. Oberhummer
Institut für Kernphysik, Technische Universität Wien, Wiedner Hauptstraße 8-10, A-1040 Wien, Austria

J. Görres and M. Wiescher
Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556

F.-K. Thielemann
Department für Physik und Astronomie, Universität Basel, Klingelbergstrasse 82, CH-4056 Basel, Switzerland

B. A. Brown
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan

Received 25 June 1999; published 16 November 1999

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.

© 1999 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.60.064614
DOI:
10.1103/PhysRevC.60.064614
PACS:
24.50.+g, 25.40.Lw, 26.20.+f, 97.10.Cv
 
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