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Explaining high braking indices of magnetars SGR 0501+4516 and 1E 2259+586 using the double magnetic-dipole model 期刊论文  OAI收割
ASTRONOMISCHE NACHRICHTEN, 2021, 卷号: 342, 期号: 1-2, 页码: 7
作者:  
Yan, Fang-Zhou;  Gao, Zhi-Fu;  Yang, Wen-Shen;  Dong, Ai-Jun
  |  收藏  |  浏览/下载:25/0  |  提交时间:2021/04/01
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition 期刊论文  OAI收割
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:  
HXMT
  |  收藏  |  浏览/下载:66/0  |  提交时间:2022/02/08
stars: magnetic field  stars: neutron  pulsars: general  Astrophysics  - High Energy Astrophysical Phenomena  Abstract: In 2011 December, PSR B054-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\ \rm per\ cent}}$. About 1000 d after the SRT, the X-ray luminosity of the associated pulsar wind nebula (PWN) was found to brighten by $32\pm 8{{\ \rm per\ cent}}$. After the SRT, the braking index n of PSR B0540-69 changes from n = 2.12 to 0.03 and then keeps this value for about five years before rising to n = 0.9 in the following years. We find that most of the current models have difficulties in explaining the measured braking index. One exceptive model of the braking index evolution is the increasing dipole magnetic field of PSR B0540-69. We suggest that the field increase may result from some instabilities within the pulsar core that enhance the poloidal component at the price of toroidal component of the magnetic field. The increasing dipole magnetic field will result in the X-ray brightening of the PWN. We fit the PWN X-ray light curve by two models: one assumes a constant magnetic field within the PWN during the brightening and the other assumes an enhanced magnetic field proportional to the energy density of the PWN. It appears that the two models fit the data well, though the later model seems to fit the data a bit better. This provides marginal observational evidence that magnetic field in the PWN is generated by the termination shock. Future high-quality and high-cadence data are required to draw a solid conclusion.  
Electroweak measurements in electron positron collisions at W-boson-pair energies at LEP 期刊论文  OAI收割
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2013, 卷号: 532, 期号: 4, 页码: 119-244
作者:  
ALEPH Collaboration;  DELPHI Collaboration;  OPAL Collaboration;  LEP Electroweak Working Grp
收藏  |  浏览/下载:23/0  |  提交时间:2015/12/02
Microwave absorption properties of Ni/(C, silicides) nanocapsules 期刊论文  OAI收割
Nanoscale Research Letters, 2012, 卷号: 7, 页码: 41281
J. J. Jiang; H. Wang; H. H. Guo; T. Yang; W. S. Tang; D. Li; S. Ma; D. Y. Geng; W. Liu; Z. D. Zhang
收藏  |  浏览/下载:30/0  |  提交时间:2013/02/05
A Practicable Method for Ferromagnetic Object Moving Direction Identification 期刊论文  OAI收割
IEEE TRANSACTIONS ON MAGNETICS, 2012, 卷号: 48, 期号: 8, 页码: 2340-2345
Zhou, QW; Tong, GJ; Li, BQ; Yuan, XB
收藏  |  浏览/下载:62/0  |  提交时间:2013/04/25
The gyrosynchrotron radiation spectrum in a nonuniform source 期刊论文  OAI收割
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS  , 2006, 卷号: 6, 期号: 2, 页码: 260-264
Zhou AH
收藏  |  浏览/下载:29/0  |  提交时间:2012/02/07
Effects of gyroresonance absorption and self absorption on the gyrosynchrotron radiation spectrum 期刊论文  OAI收割
CHINESE PHYSICS LETTERS, 2004, 卷号: 21, 期号: 10, 页码: 2067-2070
作者:  
Zhou, AH;  Su, YN;  Huang, GL
收藏  |  浏览/下载:20/0  |  提交时间:2012/12/22
Non-universal gaugino masses in supersymmetric SO(10) 期刊论文  OAI收割
NUCLEAR PHYSICS B, 2002, 卷号: 624, 期号: 40910, 页码: 81-94
作者:  
Chamoun, N;  Huang, CS;  Liu, C;  Wu, XH;  Wu, XH , Chinese Acad Sci, Inst Theoret Phys, POB 2735, Beijing 100080, Peoples R China.
  |  收藏  |  浏览/下载:19/0  |  提交时间:2012/08/29