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New γ -ray transitions observed in Ne19 with implications for the O15(α,γ)Ne19 reaction rate

Journal Article · · Physical Review C
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  1. Univ. of Notre Dame, IN (United States). Dept. of Physics
  2. Rutgers Univ., New Brunswick, NJ (United States). Dept. of Physics and Astronomy
  3. Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Physics Division
  4. Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.
  5. Argonne National Lab. (ANL), Argonne, IL (United States). Physics Division
  6. Louisiana State Univ., Baton Rouge, LA (United States). Dept. of Physics and Astronomy
  7. Univ. of Tennessee, Knoxville, TN (United States). Dept. of Physics and Astronomy
  8. Sungkyunkwan Univ., Suwon (South Korea). Dept. of Physics
  9. Univ. of Notre Dame, IN (United States). Dept. of Physics; Univ. of Surrey, Guildford (United Kingdom). Dept. of Physics
  10. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States). Physics Division
  11. Sungkyunkwan Univ., Suwon (South Korea). Dept. of Physics; Univ. of Tennessee, Knoxville, TN (United States). Dept. of Physics and Astronomy
  12. Louisiana State Univ., Baton Rouge, LA (United States). Dept. of Physics and Astronomy; Univ. of Massachusetts, Lowell, MA (United States). Dept. of Physics and Applied Physics
The 15O(α,γ) 19Ne reaction is responsible for breakout from the hot CNO cycle in type I x-ray bursts. Understanding the properties of resonances between Ex=4 and 5 MeV in 19Ne is crucial in the calculation of this reaction rate. The spins and parities of these states are well known, with the exception of the 4.14- and 4.20-MeV states, which have adopted spin-parities of 9/2- and 7/2-, respectively. γ-ray transitions from these states were studied using triton-γ – γ coincidences from the 19F(3He,tγ) 19Ne reaction measured with the GODDESS (Gammasphere ORRUBA Dual Detectors for Experimental Structure Studies) at Argonne National Laboratory. The observed transitions from the 4.14- and 4.20-MeV states provide strong evidence that the Jπ values are actually 7/2- and 9/2-, respectively. These assignments are consistent with the values in the 19F mirror nucleus and in contrast to previously accepted assignments.
Research Organization:
Argonne National Lab. (ANL), Argonne, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
USDOE; USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC02-06CH11357; AC05-00OR22725; FG02-96ER40963; FG02-96ER40978
OSTI ID:
1506778
Alternate ID(s):
OSTI ID: 1504532
OSTI ID: 1514273
Journal Information:
Physical Review C, Journal Name: Physical Review C Journal Issue: 3 Vol. 99; ISSN PRVCAN; ISSN 2469-9985
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (1)

γ -ray spectroscopy of astrophysically important states in Ca 39 journal January 2020

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