Superfluidity in relativistic neutron stars

被引：0

作者：

Langlois, D ^{[1
]}

机构：

[1] Observ Paris, Dept Astrophys Relativiste & Cosmol, CNRS, F-92195 Meudon, France

来源：

VORTICES IN UNCONVENTIONAL SUPERCONDUCTORS AND SUPERFLUIDS | 2002年 / 132卷

关键词：

D O I：

暂无

中图分类号：

O469 [凝聚态物理学];

学科分类号：

070205 ;

摘要：

The purpose of this chapter is to give a brief review of superfluidity in neutron stars. After a short presentation explaining why and how superfluidity is expected in the crust and core of neutron stars, consequences on thermal evolution and rotational dynamics are discussed. The second part summarizes a formalism that has been recently developed to describe the hydrodynamics of superfluids or superconductors in the framework of general relativity. As an application, one call compute the oscillations of a two-component relativistic neutron star.

引用

页码：65 / 81

页数：17

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