| The Origin of Glitches in Pulsars—Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars |
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| 作者姓名： | Qiu-He Peng Zhi-Quan Luo and Chih-Kang Chou School of Physics and Electronic Information China West Normal University Nanchong |
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| 作者单位： | Qiu-He Peng，Zhi-Quan Luo and Chih-Kang Chou School of Physics and Electronic Information，China West Normal University，Nanchong 637002 Department of Astronomy，Nanjing University，Nanjing 210093; Department of Physics，Sichuan University，Chengdu 610065National Astronomical Observatories，Chinese Academy of Sciences，Beijing 100012 |
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| 基金项目： | Supported by the National Natural Science Foundation of China. |
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| 摘 要： | Considering neutron star heating by magnetic dipole radiation from 3PF2 super-fluid neutron vortices inside the star, we propose a neutron phase oscillation model between the normal neutron Fermi fluid and the 3PF2 superfluid neutron vortices at the transition temperature of T_(trans) = (2-3)×108 K. With this model we can qualitatively explain most of the observations on pulsar glitches up to date.
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| 关 键 词： | stars: neutron—pulsars: general |
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