Neutron star cooling: theoretical aspects and observational constraints

被引：51
|
作者：
Yakovlev, DG
Gnedin, OY
Kaminker, AD
Levenfish, KP
Potekhin, AY
机构：
[1] AF Ioffe Phys Tech Inst, St Petersburg 194021, Russia
[2] Space Telescope Sci Inst, Baltimore, MD 21218 USA
来源：
HIGH-ENERGY STUDIES OF SUPERNOVA REMNANTS AND NEUTRON STARS | 2004年 / 33卷 / 04期
基金：
俄罗斯基础研究基金会;
关键词：
neutron stars; neutron star cooling; Urca process;
D O I：
10.1016/j.asr.2003.07.020
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
The cooling theory of isolated neutron stars is reviewed. The main cooling regulators are discussed, first of all, operation of direct Urca process (or similar processes in exotic phases of dense matter) and superfluidity in stellar interiors. The prospects to constrain gross parameters of supranuclear matter in neutron star interiors by confronting cooling theory with observations of isolated neutron stars are outlined. A related problem of thermal states of transiently accreting neutron stars with deep crustal heating of accreted matter is discussed in application to soft X-ray transients. (C) 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：523 / 530
页数：8
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