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Microscopic Magnetic Dipole Radiation in Neutron Stars

Microscopic Magnetic Dipole Radiation in Neutron Stars
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摘要 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. 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.
出处 《Chinese Journal of Astronomy and Astrophysics》 CSCD 2008年第3期269-276,共8页 中国天文和天体物理学报(英文版)
基金 National Natural Science Foundation of China.
关键词 STARS neutron -- pulsars general -- dense matter -- magnetic fields stars neutron -- pulsars general -- dense matter -- magnetic fields
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