中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Modified Fermi energy of electrons in a superhigh magnetic field

文献类型:期刊论文

作者Zhu, Cui1,2,3; Gao, Zhi Fu1,2; Li, Xiang Dong4,5; Wang, Na1; Yuan, Jian Ping1; Peng, Qiu He4
刊名MODERN PHYSICS LETTERS A
出版日期2016-04-10
卷号31期号:11
关键词Neutron star equation of state Fermi energy
英文摘要In this paper, we investigate the electron Landau level stability and its influence on the electron Fermi energy, E-F(e), in the circumstance of magnetars, which are powered by magnetic field energy. In a magnetar, the Landau levels of degenerate and relativistic electrons are strongly quantized. A new quantity g(n), the electron Landau level stability coefficient is introduced. According to the requirement that g(n) decreases with increasing the magnetic field intensity B, the magnetic field index beta in the expression of E-F(e) must be positive. By introducing the Dirac-delta function, we deduce a general formulae for the Fermi energy of degenerate and relativistic electrons, and obtain a particular solution to E-F(e) in a superhigh magnetic field (SMF). This solution has a low magnetic field index of beta = 1/6, compared with the previous one, and works when rho >= 10(7) g cm(-3) and B-cr << B <= 10(17) Gauss. By modifying the phase space of relativistic electrons, a SMF can enhance the electron number density n(e), and decrease the maximum of electron Landau level number, which results in a redistribution of electrons. According to Pauli exclusion principle, the degenerate electrons will fill quantum states from the lowest Landau level to the highest Landau level. As B increases, more and more electrons will occupy higher Landau levels, though g(n) decreases with the Landau level number n. The enhanced n(e) in a SMF means an increase in the electron Fermi energy and an increase in the electron degeneracy pressure. The results are expected to facilitate the study ofthe weak-interaction processes inside neutron stars and the magnetic-thermal evolution mechanism for magnetars.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields ; Physics, Mathematical
研究领域[WOS]Physics
关键词[WOS]NEUTRON-STARS ; NUCLEAR-MATTER ; X-RAY ; EMISSION ; STATE ; REPEATERS ; EQUATION ; PHYSICS ; DECAY
收录类别SCI
语种英语
WOS记录号WOS:000374542200006
源URL[http://libir.pmo.ac.cn/handle/332002/16210]  
专题紫金山天文台_宇宙伽马暴、中子星及相关物理研究团组
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi, Xinjiang, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China
3.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
4.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210008, Jiangsu, Peoples R China
5.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210008, Jiangsu, Peoples R China
推荐引用方式
GB/T 7714
Zhu, Cui,Gao, Zhi Fu,Li, Xiang Dong,et al. Modified Fermi energy of electrons in a superhigh magnetic field[J]. MODERN PHYSICS LETTERS A,2016,31(11).
APA Zhu, Cui,Gao, Zhi Fu,Li, Xiang Dong,Wang, Na,Yuan, Jian Ping,&Peng, Qiu He.(2016).Modified Fermi energy of electrons in a superhigh magnetic field.MODERN PHYSICS LETTERS A,31(11).
MLA Zhu, Cui,et al."Modified Fermi energy of electrons in a superhigh magnetic field".MODERN PHYSICS LETTERS A 31.11(2016).

入库方式: OAI收割

来源:紫金山天文台

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