The Origin of Glitches in Pulsars-Phase Oscillation between Anisotropic Superfluid and Normal State of Neutrons in Neutron Stars
文献类型：期刊论文
| 作者 | Qiuhe Peng1; Zhiquan Luo1; Chihkang Chou2 |
| 刊名 | Chinese Journal of Astronomy and Astrophysics
 |
| 出版日期 | 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 |
| 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. |
入库方式： OAI收割
来源：国家天文台
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