中子星的微观磁偶极辐射
Microscopic magnetic dipole radiation in neutron stars
摘要：
NS（中子星）内部存在${}^3P_2$中子超流区。对于旋转的NS，${}^3P_2$超流区就像一个旋转的磁偶极子系统。它会发出电磁辐射，这可能为纳米结构提供了一种新的加热机制。这种加热机制加上一些冷却剂可能会给NS毛刺的合理解释。
英文摘要：
There is ${}^3P_2$ neutron superfluid region in NS (neutron star) interior. For a rotating NS, the ${}^3P_2$ superfluid region is like a system of rotating magnetic dipoles. It will give out electromagnetic radiation, which may provides a new heating mechanism of NSs. This heating mechanism plus some cooling agent may give sound explanation to NS glitches.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
