Statistical spectroscopy for neutron-rich sd-shell nuclei

被引：2

作者：

Kar, Kamales ^{[1
]}

机构：

[1] Saha Inst Nucl Phys, Kolkata 700064, India

来源：

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 2013年 / 40卷 / 01期

关键词：

BETA-DECAY RATES; SPECTRAL DISTRIBUTION; PRESUPERNOVA STARS; MODEL; DISTRIBUTIONS; DEPENDENCE; DENSITIES;

D O I：

10.1088/0954-3899/40/1/015105

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：

Statistical spectroscopic results using the spectral distribution theory are obtained for the structure of neutron-rich light nuclei going towards the drip line and compared to experimental values available. It is seen that the spectral distribution methods work reasonably well for light nuclei with large neutron excess. These methods are useful for problems in nuclear astrophysics where often averaged nuclear properties are adequate.

引用

页数：10

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