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The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars
Qiuhe Peng1; Zhiquan Luo1; Chihkang Chou2
2006
Source PublicationChinese Journal of Astronomy and Astrophysics
ISSN1009-9271
Volume6Issue:3Pages:297
AbstractConsidering 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.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/49017
Collection中国科学院国家天文台
Affiliation1.西华师范大学
2.中国科学院国家天文台
Recommended Citation
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.
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