Document Type
Conference Proceeding
Publication Date
8-1-1996
Abstract
The contribution of the {sup 18}F(p,{gamma}) reaction to the production of {sup 19}Ne, which is an important isotope in connection with the breakout from the hot CNO cycle, has been investigated in experiments with {sup 18}F beams. Measurements of the cross sections for the {sup 18}F(p,{alpha}){sup 15}O and {sup 18}F(p,{gamma}){sup 19 }Ne reactions indicate that the contribution of the {sup 18}F(p, {gamma}) route to the formation or {sup 19}Ne is small.
Department
Physics and Astronomy
Recommended Citation
K. E. Rehm, M. Paul, A. D. Roberts, C. L. Jiang, D. Blumenthal, C. N. Davids, P. DeCrock, S. M. Fischer, O, J. Gehring, D. Henderson, C. J. Lister, R. J. Nickles, J. Nolen, R. C. Pardo, J. P. Sciffer, R. E. Segel and D. Seweryniak. The Influence of {sup 18}F Induced Reactions in the Hot CNO Cycle. Nuclei in the Cosmos Conference, South Bend, IN, 20-27 June 1996.
Publisher's Copyright and Source
Reprinted from SciTech Connect, Office of Scientific and Technical Information, available online: http://www.osti.gov/scitech/biblio/274176.
Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License
