New -ray transitions observed in with implications for the reaction rate
Journal Article
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· Physical Review C
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- Univ. of Notre Dame, IN (United States). Dept. of Physics
- Rutgers Univ., New Brunswick, NJ (United States). Dept. of Physics and Astronomy
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Physics Division
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.
- Argonne National Lab. (ANL), Argonne, IL (United States). Physics Division
- Louisiana State Univ., Baton Rouge, LA (United States). Dept. of Physics and Astronomy
- Univ. of Tennessee, Knoxville, TN (United States). Dept. of Physics and Astronomy
- Sungkyunkwan Univ., Suwon (South Korea). Dept. of Physics
- Univ. of Notre Dame, IN (United States). Dept. of Physics; Univ. of Surrey, Guildford (United Kingdom). Dept. of Physics
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States). Physics Division
- Sungkyunkwan Univ., Suwon (South Korea). Dept. of Physics; Univ. of Tennessee, Knoxville, TN (United States). Dept. of Physics and Astronomy
- 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
γ -ray spectroscopy of astrophysically important states in Ca 39
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journal | January 2020 |
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