Microscopic Magnetic Dipole Radiation in Neutron Stars |
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Authors: | Hao Tong Qiu-He Peng Hua Bai |
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Affiliation: | Department of Astronomy, Nanjing University, Nanjing 210093, China |
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Abstract: | There is a 3P2 neutron superfluid region in NS (neutron star) interior. For a rotating NS the 3P2 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. |
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Keywords: | stars: neutron-pulsars: general-dense matter-magnetic fields |
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