Phases of dense matter in neuron stars

被引：373

作者：

Heiselberg, H

Hjorth-Jensen, M

机构：

[1] NORDITA, DK-2100 Copenhagen O, Denmark

[2] Univ Oslo, Dept Phys, N-0316 Oslo, Norway

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2000年 / 328卷 / 5-6期

关键词：

neutron star properties; phase transitions; equation of state for dense neutron star matter;

D O I：

10.1016/S0370-1573(99)00110-6

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Recent equations of state for dense nuclear matter are discussed with possible phase transitions arising in neutron stars such as pion, kaon and hyperon condensation, superfluidity and quark matter. Specifically, we treat the nuclear to quark matter phase transition, the possible mixed phase and its structure. A number of numerical calculations of rotating neutron stars with and without phase transitions are given and compared to observed masses, radii, temperatures and glitches. (C) 2000 Elsevier Science B.V. All rights reserved.

引用

页码：237 / 327

页数：91

共 232 条

[1] EFFECTIVE INTERACTIONS AND SUPERFLUID ENERGY GAPS FOR LOW-DENSITY NEUTRON MATTER [J].