Level structures of 56,58Ca cast doubt on a doubly magic 60Ca

S. Chen, F. Browne, P. Doornenbal,J. Lee,A. Obertelli, Y. Tsunoda, T. Otsuka,Y. Chazono, G. Hagen, J. D. Holt, G. R. Jansen,K. Ogata, N. Shimizu,Y. Utsuno, K. Yoshida,N. L. Achouri, H. Baba, D. Calvet, F. Chateau,N. Chiga, A. Corsi, M. L. Cortes, A. Delbart, J. -M. Gheller, A. Giganon, A. Gillibert, C. Hilaire, T. Isobe, T. Kobayashi, Y. Kubota, V. Lapoux, H. N. Liu, T. Motobayashi, I. Murray, H. Otsu, V. Panin,N. Paul, W. Rodriguez, H. Sakurai, M. Sasano, D. Steppenbeck, L. Stuhl, Y. L. Sun, Y. Togano, T. Uesaka, K. Wimmer, K. Yoneda, O. Aktas, T. Aumann, L. X. Chung, F. Flavigny, S. Franchoo, I. Gasparic, R. -B. Gerst, J. Gibelin, K. I. Hahn,D. Kim, T. Koiwai, Y. Kondo, P. Koseoglou, C. Lehr, B. D. Linh, T. Lokotko, M. MacCormick, K. Moschner, T. Nakamura, S. Y. Park, D. Rossi, E. Sahin, P. -A. Soderstrom, D. Sohler, S. Takeuchi, H. Tornqvist, V. Vaquero, V. Wagner,S. Wang, V. Werner, X. Xu, H. Yamada, D. Yan, Z. Yang, M. Yasuda, L. Zanetti

Physics Letters B(2023)

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摘要
Gamma decays were observed in Ca-56 and Ca-58 following quasi-free one-proton knockout reactions from Sc-57,Sc-59 beams at approximate to 200MeV/nucleon. For Ca-56, a gamma ray transition was measured to be 1456(12) keV, while for Ca-58 an indication for a transition was observed at 1115(34) keV. Both transitions were tentatively assigned as the 2(1)(+) -> 0(gs)(+) decays, and were compared to results from ab initioand conventional shell-model approaches. A shell-model calculation in a wide model space with a marginally modified effective nucleon-nucleon interaction depicts excellent agreement with experiment for 2(1)(+) level energies, two-neutron separation energies, and reaction cross sections, corroborating the formation of a new nuclear shell above the N= 34 shell. Its constituents, the 0f(5/2)and 0g(9/2) orbitals, are almost degenerate. This degeneracy precludes the possibility for a doubly magic Ca-60 and potentially drives the dripline of Ca isotopes to Ca-70 or even beyond. (c) 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3.
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Shell evolution,gamma Ray spectroscopy
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