The first science result with the JENSA gas-jet target: Confirmation and study of a strong subthreshold F18(p,α)O15 resonance

D.W. Bardayan (Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN, 37831, USA; Dept. of Physics, University of Notre Dame, Notre Dame, IN, 46556, USA) ; K.A. Chipps (Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN, 37831, USA; Dept. of Physics and Astronomy, University of Tennessee, Knoxville, TN, 37996, USA; Physics Dept., Colorado School of Mines, Golden, CO, 80401, USA) ; S. Ahn (Dept. of Physics and Astronomy, University of Tennessee, Knoxville, TN, 37996, USA; National Superconducting Cyclotron Laboratory, East Lansing, MI, 48824, USA) ; J.C. Blackmon (Dept. of Physics and Astronomy, Louisiana State University, Baton Rouge, LA, 70803, USA) ; R.J. deBoer (Dept. of Physics, University of Notre Dame, Notre Dame, IN, 46556, USA) ; et al. - Show all 21 authors

The astrophysical F18(p,α)O15 rate determines, in large part, the extent to which the observable radioisotope 18 F is produced in novae. This rate, however, has been extremely uncertain owing to the unknown properties of a strong subthreshold resonance and its possible interference with higher-lying resonances. The new Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target has been used for the first time to determine the spin of this important resonance and significantly reduce uncertainties in the F18(p,α)O15 rate.

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      "value": "The astrophysical F18(p,\u03b1)O15 rate determines, in large part, the extent to which the observable radioisotope 18 F is produced in novae. This rate, however, has been extremely uncertain owing to the unknown properties of a strong subthreshold resonance and its possible interference with higher-lying resonances. The new Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas-jet target has been used for the first time to determine the spin of this important resonance and significantly reduce uncertainties in the F18(p,\u03b1)O15 rate."
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Published on:
30 October 2015
Publisher:
Elsevier
Published in:
Physics Letters B (2015)

DOI:
https://doi.org/10.1016/j.physletb.2015.10.073
Copyrights:
The Authors
Licence:
CC-BY-3.0

Fulltext files: