Title

Study of the 18F (p,α) 15O Reaction at Astrophysical Energies Using a 18F Beam

Authors

K. E. Rehm, Argonne National Laboratory
M. Paul, Hebrew University of Jerusalem
Andrew D. Roberts, Minnesota State University - MankatoFollow
D. Blumenthal, Argonne National Laboratory
J. Gehring, Argonne National Laboratory
D. Henderson, Argonne National Laboratory
C. L. Jiang, 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

Article

Publication Date

8-1995

Abstract

For the first time the F18(p,α)15O reaction has been studied with a F18 beam at energies which are of interest to explosive nucleosynthesis. Utilizing the gas-filled magnet technique a clean identification of the reaction products was achieved. A resonance with spin 3/2+ at an equivalent c.m. energy of 660 keV dominates the yield.

Department

Physics and Astronomy

Publication Title

Physical Review C

Recommended Citation

K.E. Rehm, M. Paul, A.D. Roberts, D.J. Blumenthal, J. Gehring, D. Henderson, C.L. Jiang, R.J. Nickles, J. Nolen, R.C. Pardo, J.P. Schiffer, and R.E. Segel. (1995). Study of the 18F (p,α) 15O Reaction at Astrophysical Energies Using a 18F Beam. Physical Review C, 52(2), R460-R464.

DOI

10.1103/PhysRevC.52.R460

Link to Publisher Version (DOI)

https://doi.org/10.1103/PhysRevC.52.R460

Publisher's Copyright and Source

Copyright © 1995 The American Physical Society. Article published by the American Physical Society in Physical Review C, volume 52, issue number 2, August 1995, pages R460-R464. Available online:
https://doi.org/10.1103/PhysRevC.52.R460