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Spectroscopic study of Ne20+p reactions using the JENSA gas-jet target to constrain the astrophysical F18
Author(s) -
D. W. Bardayan,
K. A. Chipps,
SungHoon Ahn,
J. C. Blackmon,
Stephen W. Carmichael,
U. Greife,
K. L. Jones,
J. José,
A. Kontos,
R. L. Kozub,
L. E. Linhardt,
B. Manning,
M. Matoš,
P. D. O’Malley,
S. Ota,
S. D. Pain,
William A. Peters,
S. T. Pittman,
A. Sachs,
K. T. Schmitt,
M. S. Smith,
P. Thompson
Publication year - 2017
Publication title -
physical review. c
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.679
H-Index - 235
eISSN - 2469-9993
pISSN - 2469-9985
DOI - 10.1103/physrevc.96.055806
Subject(s) - physics , spins , atomic physics , crystallography , condensed matter physics , chemistry
The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target was used to perform spectroscopic studies of 20Ne+p reactions. Levels in 19Ne were probed via the 20Ne(p,d)19Ne reaction to constrain the astrophysical rate of the 18F(p,a)15O reaction. Additionally, the first spectroscopic study of the 20Ne(p,3He)18F reaction was performed. Angular distribution data were used to determine or confirm the spins of several previously observed levels, and the existence of a strong subthreshold 18F(p,a)15O resonance was verified.Peer ReviewedPostprint (author's final draft

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