Superfluid dynamics and energy dissipation in neutron stars

被引：0

作者：

Alper, MA ^{[1
]}

机构：

[1] Sabanci Univ, TR-81474 Istanbul, Turkey

来源：

NEUTRON STAR - BLACK HOLE CONNECTION | 2001年 / 567卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the basic properties of the neutron superfluid and the proton superconductor in the neutron star, and of the quantized neutron vortices and proton flux lines. Energy must be dissipated in the rotational dynamics of neutron stars, at rates that yield observable luminosities of dim thermal neutron stars.

引用

页码：57 / 70

页数：14

共 18 条

[1]

ALPAR A, 1987, ASTRON ASTROPHYS, V177, P101

[2]

Alpar MA, 1998, NATO ADV SCI I C-MAT, V515, P59

[3] VORTEX CREEP AND THE INTERNAL TEMPERATURE OF NEUTRON STARS - LINEAR AND NONLINEAR RESPONSE TO A GLITCH [J].