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The Landau level-superfluid modified factor and the overal soft X/gamma-ray efficiency coefficient of a magnetar
Gao, Z. F.1,2,3; Peng, Q. H.4,5; Wang, N.1,2; Chou, C. K.6; Huo, W. S.7,8
刊名ASTROPHYSICS AND SPACE SCIENCE
2011-12-01
卷号336期号:2页码:427-439
关键词Magnetar Landau levels Electron capture Neutron star Fermi energy
通讯作者Gao, Z. F.
英文摘要As soon as the energies of electrons near the Fermi surface exceed Q, the threshold energy of inverse beta-decay, electron capture (EC) dominates inside a neutron star. The high-energy neutrons released by EC will destroy anisotropic (3) P (2) neutron Cooper pairs in the degenerate superfluid. By colliding with the neutrons produced in the process n+(na dagger na dagger")-> n+n+n, the kinetic energies of the neutrons released by EC will be transformed into thermal energy. A portion of this thermal energy will be transported from the star interior to the star surface by conduction, then converted to a thermal spectrum of soft X-rays and gamma-rays. By introducing two important parameters: the Landau level-superfluid modified factor and the overal soft X/gamma-ray efficiency coefficient, we compute the theoretical luminosity L (X) of a magnetar under our model and plot a diagram of L (X) as a function of magnetic field strength B. Numerical calculations based on our model agree well with the observed properties of magnetar candidates.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]XMM-NEWTON OBSERVATIONS ; X-RAY ; NEUTRON-STARS ; PULSAR XTE-J1810-197 ; GAMMA-REPEATERS ; FIELD-DECAY ; SUPERNOVA MODELS ; RADIO-EMISSION ; XTE J1810-197 ; LIGHT-CURVE
收录类别SCI
语种英语
WOS记录号WOS:000297359900016
内容类型期刊论文
源URL[http://ir.xao.ac.cn/handle/45760611-7/839]  
专题脉冲星研究团组
新疆天文台_射电天文研究室
新疆天文台_其它
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi Xinjiang 830011, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
4.Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
5.Nanjing Univ, Minist Educ, Key Lab Astron & Astrophys, Nanjing 210093, Peoples R China
6.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
7.Xinjiang Univ, Sch Phys, Urumqi Xinjiang 830011, Peoples R China
8.Xinjiang Univ, Natl Astron Observ, Joint Ctr Astrophys, Urumqi Xinjiang 830011, Peoples R China
推荐引用方式
GB/T 7714
Gao, Z. F.,Peng, Q. H.,Wang, N.,et al. The Landau level-superfluid modified factor and the overal soft X/gamma-ray efficiency coefficient of a magnetar[J]. ASTROPHYSICS AND SPACE SCIENCE,2011,336(2):427-439.
APA Gao, Z. F.,Peng, Q. H.,Wang, N.,Chou, C. K.,&Huo, W. S..(2011).The Landau level-superfluid modified factor and the overal soft X/gamma-ray efficiency coefficient of a magnetar.ASTROPHYSICS AND SPACE SCIENCE,336(2),427-439.
MLA Gao, Z. F.,et al."The Landau level-superfluid modified factor and the overal soft X/gamma-ray efficiency coefficient of a magnetar".ASTROPHYSICS AND SPACE SCIENCE 336.2(2011):427-439.
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