Microscopic magnetic dipole radiation in neutron stars
Astrophysics
2009-11-13 v1
Abstract
There is neutron superfluid region in NS (neutron star) interior. For a rotating NS, the 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.
Keywords
Cite
@article{arxiv.0801.0489,
title = {Microscopic magnetic dipole radiation in neutron stars},
author = {Hao Tong and Qiu-he Peng and Hua Bai},
journal= {arXiv preprint arXiv:0801.0489},
year = {2009}
}
Comments
To be published by ChJAA