Microscopic magnetic dipole radiation in neutron stars

被引：2
作者：
Tong, Hao [1 ]
Peng, Qiu-He [1 ]
Bai, Hua [1 ]
机构：
[1] Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
来源：
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2008年 / 8卷 / 03期
关键词：
stars : neutron; pulsars : general; dense matter; magnetic fields;
D O I：
10.1088/1009-9271/8/3/04
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
There is a (3)P(2) neutron superfluid region in NS (neutron star) interior. For a rotating NS the (3)P(2) superfluid region is like a system of rotating magnetic dipoles. It will give out electromagnetic radiation, which may provide a new heating mechanism of NSs. This mechanism plus some cooling agent may give a sound explanation to NS glitches.
引用
收藏
页码：269 / 276
页数：8
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