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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:57/0  |  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.  
Probing the structural, electronic and magnetic properties of multicenter Fe2S2 (0/-), Fe3S4 (0/-) and Fe4S4 (0/-) clusters 期刊论文  OAI收割
Journal of Molecular Modeling, 2013, 卷号: 19, 期号: 4, 页码: 1527-1536
L. P. Ding; X. Y. Kuang; P. Shao; M. M. Zhong
收藏  |  浏览/下载:15/0  |  提交时间:2013/12/24
Surface properties of 3d transition metals 期刊论文  OAI收割
Philosophical Magazine, 2011, 卷号: 91, 期号: 27, 页码: 3627-3640
M. P. J. Punkkinen; Q. M. Hu; S. K. Kwon; B. Johansson; J. Kollar; L. Vitos
收藏  |  浏览/下载:18/0  |  提交时间:2012/04/13
Quantitative Analysis of CME Deflections in the Corona 期刊论文  OAI收割
SOLAR PHYSICS, 2011, 卷号: 271, 期号: 1-2, 页码: 111-139
作者:  
Gui, Bin;  Shen, Chenglong;  Wang, Yuming;  Ye, Pinzhong;  Liu, Jiajia
收藏  |  浏览/下载:24/0  |  提交时间:2014/12/15
Static equation of state of bcc iron 期刊论文  OAI收割
Physical Review B, 2010, 卷号: 82, 期号: 13
H. L. Zhang; S. Lu; M. P. J. Punkkinen; Q. M. Hu; B. Johansson; L. Vitos
收藏  |  浏览/下载:19/0  |  提交时间:2012/04/13
Electronic and magnetic properties of graphene absorbed with S atom: A first-principles study 期刊论文  OAI收割
Journal of Applied Physics, 2009, 卷号: 105, 期号: 10
Y. G. Zhou; X. T. Zu; F. Gao; H. Y. Xiao; H. F. Lv
收藏  |  浏览/下载:17/0  |  提交时间:2012/04/13
Effect of doping with Co and/or Cu on electronic structure and optical properties of ZnO 期刊论文  OAI收割
Journal of Applied Physics, 2009, 卷号: 105, 期号: 4
M. Xu; H. Zhao; K. Ostrikov; M. Y. Duan; L. X. Xu
收藏  |  浏览/下载:27/0  |  提交时间:2012/04/13
First-principles study of CoO films on MnO (111): Stability and interfacial structure 期刊论文  OAI收割
Physica B-Condensed Matter, 2008, 卷号: 403, 期号: 18, 页码: 3191-3194
K. L. Yao; H. M. Huang; Z. L. Liu
收藏  |  浏览/下载:24/0  |  提交时间:2012/04/13
The ground state of quantum rings in a magnetic field 期刊论文  OAI收割
MODERN PHYSICS LETTERS B, 2006, 卷号: 20, 期号: 23, 页码: 1443-1451
作者:  
Liu, Yi-Min;  Huang, Gang-Ming;  Shi, Ting-Yun
收藏  |  浏览/下载:21/0  |  提交时间:2015/07/17
Evidence of d-wave pairing in MTG-YBa2Cu2.99Li0.01Ox crystals determined from the low-temperature specific heat 期刊论文  OAI收割
SUPERCONDUCTOR SCIENCE & TECHNOLOGY, 2006, 卷号: 19, 期号: 6, 页码: 503-507
Bai, Z; Wang, ZH; Li, PJ; Qiu, L; Zhang, H; Gao, J
收藏  |  浏览/下载:23/0  |  提交时间:2012/03/24