The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars

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	The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars
	Qiuhe Peng 1; Zhiquan Luo 1; Chihkang Chou 2
刊名	Chinese Journal of Astronomy and Astrophysics
	2006
卷号	6 期号:3 页码:297
ISSN号	1009-9271
英文摘要	Considering neutron star heating by magnetic dipole radiation from (PF2)-P-3 superfluid neutron vortices inside the star, we propose a neutron phase oscillation model between the normal neutron Fermi fluid and the (PF2)-P-3 superfluid neutron vortices at the transition temperature of T-trans = (2 - 3) x 10(8) K. With this model we can qualitatively explain most of the observations on pulsar glitches up to date.
语种	英语
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/49016]
专题	中国科学院国家天文台
作者单位	1.西华师范大学 2.中国科学院国家天文台
推荐引用方式 GB/T 7714	Qiuhe Peng,Zhiquan Luo,Chihkang Chou. The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars[J]. Chinese Journal of Astronomy and Astrophysics,2006,6(3):297.
APA	Qiuhe Peng,Zhiquan Luo,&Chihkang Chou.(2006).The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars.Chinese Journal of Astronomy and Astrophysics,6(3),297.
MLA	Qiuhe Peng,et al."The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars".Chinese Journal of Astronomy and Astrophysics 6.3(2006):297.