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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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Spectroscopic study of the radionuclide Na-21 for the astrophysical F-17(alpha, p)Ne-20 reaction rate

Author(s)
Cha, S. M.Chae, K. Y.Ahn, S.Bardayan, D. W.Chipps, K. A.Cizewski, J. A.Howard, M. E.Kozub, R. L.Kwak, KyujinManning, B.Matos, M.O'Malley, P. D.Pain, S. D.Peters, W. A.Pittman, S. T.Ratkiewicz, A.Smith, M. S.Strauss, S.
Issued Date
2017-08
DOI
10.1103/PhysRevC.96.025810
URI
https://scholarworks.unist.ac.kr/handle/201301/22719
Fulltext
https://journals.aps.org/prc/abstract/10.1103/PhysRevC.96.025810
Citation
PHYSICAL REVIEW C, v.96, no.2, pp.025810
Abstract
The Mg-24(p,alpha)Na-21 reaction was measured at the Holifield Radioactive Ion Beam Facility of the Oak Ridge National Laboratory to study the spectroscopy of the radionuclide Na-21. A 31-MeV proton beam from the 25 MV tandem accelerator bombarded isotopically enriched Mg-24 targets. Recoiling He-4 particles were identified by an annular silicon strip detector array. Two energy levels at E-x = 6.594 and 7.132 MeV were observed for the first time. By comparing the experimentally obtained angular distributions and distorted wave Born approximation calculations, the spins and parities of Na-21 energy levels were constrained. The astrophysicallyi-mportant F-17(alpha, p)Ne-20 reaction rate was also calculated for the first time using resonance parameters for 12 energy levels.
Publisher
AMER PHYSICAL SOC
ISSN
2469-9985
Keyword
X-RAY-BURSTSTI-44SUPERNOVAEMODELSDECAY

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