Evidence of halo structure in 37Mg observed via reaction cross sections and intruder orbitals beyond the island of inversion

Evidence of halo structure in 37Mg observed via reaction cross sections and intruder orbitals beyond the island of inversion
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通过反应截面和反演岛之外的侵入轨道观察到 37Mg 中晕结构的证据

DOI:
10.1103/physrevc.90.061305
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发表时间:
2014
期刊:
影响因子:
3.1
通讯作者:
N. Inabe et al.
N. Inabe et al.
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
M. Takechi;S. Suzuki;D. Nishimura;M. Fukuda;T. Ohtsubo;M. Nagashima;T. Suzuki;T. Yamaguchi;A. Ozawa;T. Moriguchi;H. Ohishi;T. Sumikama;H. Geissel;N. Aoi;Rui-Jiu Chen;De-Qing Fang;N. Fukuda;S. Fukuoka;H. Furuki;N. Inabe et al.

文献摘要

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在日本化学研究所放射性同位素束流工厂中,测量了能量约为240 MeV/核子的C靶的精确反应截面。这是首次测量。与球形稳定核的系统学相比,我们观察到了一种增强,特别是在富中子区,这反映了这些同位素的形变。在滴水线附近,压力特别大。用最近发展起来的理论方法分析表明,这种显著的增强应来自于打破壳隙的轨道晕的形成。
Precise reaction cross sections () foron C targets at energies around 240 MeV/nucleon have been measured at the Radioactive Isotope Beam Factory at RIKEN. Theforhave been measured for the first time. An enhancement ofcompared to the systematics for spherical stable nuclei has been observed, especially in the neutron-rich region, which reflects the deformation of those isotopes. In the vicinity of the drip line theforis especially large. It is shown by analysis using a recently developed theoretical method that this prominent enhancement offorshould come from the-orbital halo formation breaking theshell gap.