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arXiv · 0801.0489

Microscopic magnetic dipole radiation in neutron stars

Hao Tong·Qiu-he Peng·Hua Bai
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Abstract

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.

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Hao Tong, Qiu-he Peng, Hua Bai. 2008-01-03. Microscopic magnetic dipole radiation in neutron stars. https://doi.org/10.1088/1009-9271%2F8%2F3%2F04

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