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arXiv 2302.08382nucl-exnucl-th
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$^{15}$C中的跨壳态:对p-sd相互作用的检验

Cross-shell states in $^{15}$C: a test for p-sd interactions

J. Lois-Fuentes, B. Fernández-Domínguez, X. Pereira-López, F. Delaunay, W. N. Catford, A. Matta, N. A. Orr, T. Duguet, T. Otsuka, V. Somà, O. Sorlin, T. Suzuki,… 展开作者

J. Lois-Fuentes, B. Fernández-Domínguez, X. Pereira-López, F. Delaunay, W. N. Catford, A. Matta, N. A. Orr, T. Duguet, T. Otsuka, V. Somà, O. Sorlin, T. Suzuki, N. L. Achouri, M. Assié, S. Bailey, B. Bastin, Y. Blumenfeld, R. Borcea, M. Caamaño, L. Caceres, E. Clément, A. Corsi, N. Curtis, Q. Deshayes, F. Farget, M. Fisichella, G. de France, S. Franchoo, M. Freer, J. Gibelin, A. Gillibert, G. F. Grinyer, F. Hammache, O. Kamalou, A. Knapton, Tz. Kokalova, V. Lapoux, B. Le Crom, S. Leblond, F. M. Marqués, P. Morfouace, J. Pancin, L. Perrot, J. Piot, E. Pollacco, D. Ramos, D. Regueira-Castro, C. Rodríguez-Tajes, T. Roger, F. Rotaru, M. Sénoville, N. de Séréville, R. Smith, M. Stanoiu, I. Stefan, C. Stodel, D. Suzuki, J. C. Thomas, N. Timofeyuk, M. Vandebrouck, J. Walshe, C. Wheldon

AI总结:

通过$^{16}$C$(d,t)$反应研究$^{15}$C的跨壳态,检验p-sd相互作用,结果与SFO-tls壳模型计算一致,并揭示了理论截断方案的不足。

摘要:

通过中子移除反应$^{16}$C$(d,t)$研究了$^{15}$C的低激发结构。除了束缚的中子sd壳层空穴态之外,非束缚的p壳层空穴态也被明确确认。这些跨壳态的激发能以及推导出的谱因子是衡量$^{15}$C中$[(p)^{-1}(sd)^{2}]$中子组态的重要指标。我们的结果与使用SFO-tls相互作用的壳模型计算对$^{15}$C的描述符合得很好。然而,为了重现$N=9$同中子异位素$^{17}$O,对$p$-$sd$和$sd$-$sd$单极项进行了修正。此外,还将激发能和谱因子与采用NNLO$_{sat}$相互作用的从头算自洽格林函数方法对$^{15}$C的首次计算进行了比较。结果表明了对$N=8$壳隙大小的敏感性,并强调了在理论中超越当前截断方案的必要性。

英文摘要:

The low-lying structure of $^{15}$C has been investigated via the neutron-removal $^{16}$C$(d,t)$ reaction. Along with bound neutron sd-shell hole states, unbound p-shell hole states have been firmly confirmed. The excitation energies and the deduced spectroscopic factors of the cross-shell states are an important measure of the $[(p)^{-1}(sd)^{2}]$ neutron configurations in $^{15}$C. Our results show a very good agreement with shell-model calculations using the SFO-tls interaction for $^{15}$C. However, a modification of the $p$-$sd$ and $sd$-$sd$ monopole terms was applied in order to reproduce the $N=9$ isotone $^{17}$O. In addition, the excitation energies and spectroscopic factors have been compared to the first calculations of $^{15}$C with the $ab~ initio$ self-consistent Green's function method employing the NNLO$_{sat}$ interaction. The results show the sensitivity to the size of the $N=8$ shell gap and highlight the need of going beyond the current truncation scheme in the theory.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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