期刊
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
卷 65, 期 6, 页码 -出版社
SCIENCE PRESS
DOI: 10.1007/s11433-022-1894-6
关键词
halo; relativistic model; Glauber model; reaction cross section; momentum distribution
资金
- National Natural Science Foundation of China [11375022, 11775014, 11975237, U2032141]
- Strategic Priority Research Program of the Chinese Academy of Sciences [XDB34010000]
- U.S. Department of Energy Office of Science, Office of Nuclear Physics [DE-AC05-00OR22725]
This study combines self-consistent structure and reaction theories to investigate the exotic deformed nucleus Ne-31. The results demonstrate that deformation and pairing correlations lead to a halo structure in Ne-31. By using the predicted wave functions and density distributions, the observables of neutron-rich neon isotopes were studied, showing good agreement with experimental data.
The exotic deformed nucleus Ne-31 is studied with an approach that combines self-consistent structure and reaction theories. The deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc) is utilized to demonstrate that deformation and pairing correlations give rise to a halo structure with a large-amplitude p-wave configuration in Ne-31. Then the valence nucleon wave functions and angle-averaged density distributions of Ne-30 from this theory are used as input for the Glauber reaction model to study the observables of neutron-rich neon isotopes to search halo signatures. With NL1 effective interaction, our predictions of the reaction cross sections for these exotic neon isotopes on a carbon target can better reproduce the experimental data than those from the relativistic mean field model for a spherical shape with resonances and pairing correlation contributions, and are roughly 3.3% (similar to 50 mb) larger than those with Gaussian function-fitted densities of the core nuclei. The calculated one-neutron removal cross section at 240 MeV/nucleon, and the inclusive longitudinal momentum distribution of the Ne-30 residues from the Ne-31 breakup reaction are largely improved over previous theoretical predictions and agree well with data. These reaction evaluations indicate a dilute density distribution in coordinate space and are a canonical signature of a halo structure. Moreover, our predictions with the NL3 and PK1 effective interactions give slightly better descriptions of reaction observables for exotic neon isotopes.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据