Neutron Stars—Cooling and Transport

被引：0
|
作者：
Alexander Y. Potekhin
José A. Pons
Dany Page
机构：
[1] Ioffe Institute,Departament de Física Aplicada
[2] Central Astronomical Observatory at Pulkovo,Instituto de Astronomía
[3] St. Petersburg State Polytechnical University,undefined
[4] Universitat d’Alacant,undefined
[5] Universidad Nacional Autónoma de México,undefined
来源：
Space Science Reviews | 2015年 / 191卷
关键词：
Neutron stars; Magnetic fields; Dense matter; Thermal emission; Heat transport;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Observations of thermal radiation from neutron stars can potentially provide information about the states of supranuclear matter in the interiors of these stars with the aid of the theory of neutron-star thermal evolution. We review the basics of this theory for isolated neutron stars with strong magnetic fields, including most relevant thermodynamic and kinetic properties in the stellar core, crust, and blanketing envelopes.
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页码：239 / 291
页数：52
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