The Astrophysical Reaction Rate for the 18F(p,α) 15O Reaction

Authors

K. E. Rehm, Argonne National Laboratory
M. Paul, Hebrew University of Jerusalem
Andrew D. Roberts, Minnesota State University - MankatoFollow
C. L. Jiang, Argonne National Laboratory
D. Blumenthal, Argonne National Laboratory
J. Gehring, Argonne National Laboratory
Robert J. Nickles, University of Wisconsin - Madison
J. Nolen, Argonne National Laboratory
R. C. Pardo, Argonne National Laboratory
J. P. Schiffer, Argonne National Laboratory
R. E. Segel, Northwestern University

Document Type

Technical Report

Publication Date

3-13-1996

Abstract

Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using the results of recent measurements of the 18F(p,α)15O reaction. This l p = 0 resonance dominates the astrophysical reaction rates at temperatures T9>0.5.

Department

Physics and Astronomy

Recommended Citation

K.E. Rehm, M. Paul, A.D. Roberts, C.L. Jiang, D.J. Blumenthal, J. Gehring, J. Nickles, J. Nolen, R.C. Pardo, J.P Schiffer, and R.E. Segel. (1996). The Astrophysical Reaction Rate for the 18F(p,α) 15O Reaction. Technical Report ANL/PHY/PP-86895 (TRN:96:012139), U.S. Department of Energy, Nuclear Physics Division (contract number W-31-109-ENG-38). OSTI Identifier: 212427. http://dx.doi.org/10.2172/212427

DOI

10.2172/212427

Link to Publisher Version (DOI)

http://dx.doi.org/10.2172/212427

Publisher's Copyright and Source

Reprinted from SciTech Connect, OSTI Identifier 212427. Retrieved from: http://dx.doi.org/10.2172/212427.

Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.