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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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Investigation of Mg-22 levels via resonant scattering of Ne-18 + alpha

Author(s)
Cha, S. M.Chae, K. Y.Abe, K.Bae, S.Binh, D. N.Choi, S. H.Duy, N. N.Ge, Z.Hahn, K. I.Hayakawa, S.Hong, B.Iwasa, N.Kahl, D.Khiem, L. H.Kim, A.Kim, D.Kim, E. J.Kim, G. W.Kim, M. J.Kwak, KyujinKwag, M. S.Lee, E. J.Lim, S. I.Moon, B.Moon, J. Y.Park, S. Y.Phong, V. H.Shimizu, H.Yamaguchi, H.Yang, L.
Issued Date
2023-05
DOI
10.3389/fphy.2023.1163299
URI
https://scholarworks.unist.ac.kr/handle/201301/65202
Citation
FRONTIERS IN PHYSICS, v.11, pp.1163299
Abstract
The a resonant scattering on Ne-18 was measured in inverse kinematics to understand the a-clustering of proton-rich Mg-22 nucleus, performed at the CNS Radio-Isotope Beam Separator (CRIB) of Center for Nuclear Study, University of Tokyo, located at the RIBF of RIKEN Nishina Center. The excitation function of Mg-22 was obtained for the excitation energies of 10-16 MeV by adopting the thick-target method. Several resonances were evident in the present work, which implies the existence of energy levels with large a widths. Since energy levels were not clearly observed at the astrophysically important energy range, upper limits on the Ne-18 (a, a)Ne-18 cross section were set. The astrophysical impact was also investigated by estimating the Ne-18 (a, p)Na-21 cross section.
Publisher
FRONTIERS MEDIA SA
ISSN
2296-424X
Keyword (Author)
nuclear clusteralpha-cluster structureresonant scatteringenergy level propertiesthick-target method in inverse kinematicsRI beamexplosive stellar environmentsNe-18(a,p)Na-21
Keyword
CLUSTERSYSTEMSTATES

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