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Investigation of Mg-22 levels via resonant scattering of Ne-18 + alpha
- Title
- Investigation of Mg-22 levels via resonant scattering of Ne-18 + alpha
- Authors
- 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, K.; Kwag, 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.
- Ewha Authors
- 한인식
- SCOPUS Author ID
- 한인식
- Issue Date
- 2023
- Journal Title
- FRONTIERS IN PHYSICS
- ISSN
- 2296-424X
- Citation
- FRONTIERS IN PHYSICS vol. 11
- Keywords
- nuclear cluster; alpha-cluster structure; resonant scattering; energy level properties; thick-target method in inverse kinematics; RI beam; explosive stellar environments; Ne-18(a,p)Na-21
- Publisher
- FRONTIERS MEDIA SA
- Indexed
- SCIE; SCOPUS
- Document Type
- Article
- 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.
- DOI
- 10.3389/fphy.2023.1163299|http://dx.doi.org/10.3389/fphy.2023.1163299
- Appears in Collections:
- 사범대학 > 과학교육과 > Journal papers
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