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