The Landau level-superfluid modified factor and the overal soft X/gamma-ray efficiency coefficient of a magnetar | |
Gao, Z. F.1,2,3![]() ![]() | |
刊名 | ASTROPHYSICS AND SPACE SCIENCE
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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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