New γ -ray transitions observed in Ne 19 with implications for the O 15 (α,γ) Ne 19 reaction rate

  • M. R. Hall
  • , D. W. Bardayan
  • , T. Baugher
  • , A. Lepailleur
  • , S. D. Pain
  • , A. Ratkiewicz
  • , S. Ahn
  • , J. M. Allen
  • , J. T. Anderson
  • , A. D. Ayangeakaa
  • , J. C. Blackmon
  • , S. Burcher
  • , M. P. Carpenter
  • , S. M. Cha
  • , K. Y. Chae
  • , K. A. Chipps
  • , J. A. Cizewski
  • , M. Febbraro
  • , O. Hall
  • , J. Hu
  • C. L. Jiang, K. L. Jones, E. J. Lee, P. D. O'Malley, S. Ota, B. C. Rasco, D. Santiago-Gonzalez, D. Seweryniak, H. Sims, K. Smith, W. P. Tan, P. Thompson, C. Thornsberry, R. L. Varner, D. Walter, G. L. Wilson, S. Zhu

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

The O15(α,γ)Ne19 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 Ne19 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 F19(He3,tγ)Ne19 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 F19 mirror nucleus and in contrast to previously accepted assignments.

Original languageEnglish
Article number035805
JournalPhysical Review C
Volume99
Issue number3
DOIs
StatePublished - Mar 29 2019

Funding

This research was supported in part by the National Science Foundation Grants No. PHY-1419765 (Notre Dame) and No. PHY-1404218 (Rutgers), the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Cooperative Agreement No. DE-NA002132, and by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2016R1A5A1013277 and No. NRF-2013M7A1A1075764). The authors also acknowledge support from the DOE Office of Science, Office of Nuclear Physics, under Contracts No. DE-AC05-00OR22725, No. DE-FG02-96ER40963, No. DE-FG02-96ER40978, and No. DE-AC02-06CH11357. This research used resources of Argonne National Laboratory's ATLAS facility, which is a DOE Office of Science User Facility.

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