Microscopic magnetic dipole radiation in neutron stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To be published by ChJAA

Scientific paper

10.1088/1009-9271/8/3/04

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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