Relativistic Mean-Field and Beyond Approaches for Deformed Hypernuclei

被引:2
|
作者
Yao, J. M. [1 ]
Mei, H. [2 ,3 ]
Hagino, K. [2 ,4 ]
Motoba, T. [5 ,6 ]
机构
[1] Michigan State Univ, FRIB NSCL, E Lansing, MI 48824 USA
[2] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan
[3] Southwest Univ, Sch Phys Sci & Technol, Chongqing 400715, Peoples R China
[4] Tohoku Univ, Res Ctr Electron Photon Sci, 1-2-1 Mikamine, Sendai, Miyagi 9820826, Japan
[5] Osaka Electrocommun Univ, Phys Lab, Neyagawa, Osaka 5728530, Japan
[6] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
基金
中国国家自然科学基金; 美国国家科学基金会;
关键词
LAMBDA; SPECTROSCOPY; HYPERON;
D O I
10.1063/1.5118376
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We report the recent progress in relativistic mean-field (RMF) and beyond approaches for the low-energy structure of deformed hypernuclei. We show that the Lambda hyperon with orbital angular momentum l = 0 (or l > 1) generally reduces (enhances) nuclear quadrupole collectivity. The beyond mean-field studies of hypernuclear low-lying states demonstrate that there is generally a large configuration mixing between the two components [(A-1)Z(I+) circle times Lambda p(1/2)](J) and [(A-1)Z(I +/- 2(+)) circle times Lambda p(3/2)](J) in the hypernuclear 1/2(1)(-) ; 3/2(1)(-) states. The mixing weight increases as the collective correlation of nuclear core becomes stronger. Finally, we show how the energies of hypernuclear low-lying states are sensitive to parameters in the effective N Lambda interaction, the uncertainty of which has a large impact on the predicted maximum mass of neutron stars.
引用
收藏
页数:12
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