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浏览/检索结果: 共65条,第1-10条 帮助

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Pure spin current generation with photogalvanic effect in graphene interconnect junctions 期刊论文  OAI收割
NANOPHOTONICS, 2021, 卷号: 10
作者:  
Zhou, Yan-Hong;  Yu, Shaohui;  Li, Yuejun;  Luo, Xin;  Zheng, Xiaohong
  |  收藏  |  浏览/下载:15/0  |  提交时间:2021/06/15
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:40/0  |  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.  
Reactivity descriptors of diverse copper-oxo species on ZSM-5 zeolite towards methane activation 期刊论文  OAI收割
CATALYSIS TODAY, 2019, 卷号: 338, 页码: 108-116
作者:  
Wang, Guiru;  Chen, Wei;  Huang, Ling;  Liu, Zhiqiang;  Sun, Xianyong
  |  收藏  |  浏览/下载:65/0  |  提交时间:2019/12/06
Difference in physical properties of MAX-phase compounds Cr2GaC and Cr2GaN induced by an anomalous structure change in Cr2GaN 期刊论文  OAI收割
INTERMETALLICS, 2019, 卷号: 105, 期号: 无, 页码: 39-43
作者:  
Tong, Haiyun;  Lin, Shuai;  Huang, Yanan;  Tong, Peng;  Song, Wenhai
  |  收藏  |  浏览/下载:8/0  |  提交时间:2020/03/31
Stretch/Compress-Modulated Spin Splitting in One-Dimensional Melem Chain with a Helical Structure 期刊论文  OAI收割
Physica Status Solidi-Rapid Research Letters, 2019, 卷号: 13, 期号: 10, 页码: 5
作者:  
D.Han;  X.J.Chen;  H.Xu;  C.Jiao;  J.L.Xu
  |  收藏  |  浏览/下载:12/0  |  提交时间:2020/08/24
Nucleon effective masses in neutron-rich matter 期刊论文  OAI收割
PROGRESS IN PARTICLE AND NUCLEAR PHYSICS, 2018, 卷号: 99, 页码: 29-119
作者:  
Li, BA;  Cai, BJ;  Chen, LW;  Xu, J
  |  收藏  |  浏览/下载:32/0  |  提交时间:2018/09/06
ESR study of free radicals in polysilazane irradiated by gamma rays 期刊论文  OAI收割
RADIATION PHYSICS AND CHEMISTRY, 2018, 卷号: 151, 期号: -, 页码: 108-113
作者:  
  |  收藏  |  浏览/下载:52/0  |  提交时间:2019/12/17
Atomic scale electronic structure of the ferromagnetic semiconductor Cr2Ge2Te6 期刊论文  OAI收割
SCIENCE BULLETIN, 2018, 卷号: 63
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  |  收藏  |  浏览/下载:9/0  |  提交时间:2020/10/26