Recent progress in neutron star theory

被引：156
作者：
Heiselberg, H
Pandharipande, V
机构：
[1] NORDITA, DK-2100 Copenhagen O, Denmark
[2] Univ Illinois, Dept Phys, Urbana, IL 61801 USA
来源：
ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE | 2000年 / 50卷
关键词：
dense nuclear matter; hyperonic matter; quark matter; neutron star structure; radii; mass limits;
D O I：
10.1146/annurev.nucl.50.1.481
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 review recent progress in the theory of neutron stars and compare its predictions with the observational data on masses, radii, and temperatures. The theory of neutron stars made up of neutrons, protons, and leptons is discussed in detail along with recent models of nuclear forces and modern many-body techniques. The possibilities of pion and kaon condensation in dense neutron star matter are considered, as is the possible occurrence of strange hyperons and quark-matter drops in the stellar core. The structure of mixed-phase matter in neutron stars, as well as the probable effect of phase transitions on the spin down of pulsars, is also discussed.
引用
收藏
页码：481 / 524
页数：44
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