Astrophysical Reaction Rate for the F18 (p,α) O15 Reaction
Document Type
Article
Publication Date
4-1996
Abstract
An excitation function for the 18F~p,a!15O reaction has been measured in the energy range Ec.m.5600–800 keV using a radioactive 18F beam. A resonant state with a spin value of 3/21 has been found at an energy of 652 keV above threshold. This l p50 resonance is found to dominate the astrophysical reaction rate at temperatures T9.0.5.
Department
Physics and Astronomy
Publication Title
Physical Review C
Recommended Citation
K. E. Rehm, M. Paul, A. D. Roberts, C. L. Jiang, D. J. Blumenthal, S. M. Fischer, J. Gehring, D. Henderson, J. Nickles, J. Nolen, R. C. Pardo, J. P. Schiffer, and R. E. Segel. (1996). Astrophysical Reaction Rate for the F18 (p,α) O15 Reaction. Physical Review C, 53 (4), 1950-1954.
DOI
10.1103/PhysRevC.53.1950
Link to Publisher Version (DOI)
Publisher's Copyright and Source
Copyright © 1996 The American Physical Society. Article published by The American Physical Society in Physical Review C, volume 53, issue number 4, April 1996, pages 1950-1954. Available online:
https://doi.org/10.1103/PhysRevC.53.1950
