ELLIPTICAL

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Progress on elliptical magnetic skyrmions被引量：2
《Rare Metals》2023年第2期359-367,共9页Bao-Shan Cui Yong-Qiang Yang Xiao-Bin Guo Shi-Heng Liang Hao Wu Guo-Qiang Yu 
financially supported by Guangdong Basic and Applied Basic Research Foundation(No.2020A1515110553);Science Center of the National Science Foundation of China(No.52088101);Beijing Natural Science Foundation(No.Z190009);the National Natural Science Foundation of China(NSFC,Nos.11874409 and 11904056);K.C.Wong Education Foundation(No.GJTD-2019-14);China Postdoctoral Science Foundation(No.2020M670499);Guangzhou basic and applied basic research project(No.202102020053);the startup funding from Songshan Lake Materials Laboratory(No.Y1D1071S511)。
Magnetic skyrmions,the topological spin textures firstly observed in chiral magnets,have aroused huge interest due to their emergent electromagnetism and potential applications in spintronics.Over the last decade,sign...
关键词：Dzyaloshinskii-Moriya interaction(DMI) Elliptical magnetic skyrmion Magnetic anisotropy(K_(u)) Skyrmion Hall effect 
Systematic Errors Induced by the Elliptical Power-law model in Galaxy–Galaxy Strong Lens Modeling被引量：1
《Research in Astronomy and Astrophysics》2022年第2期143-172,共30页Xiaoyue Cao Ran Li J.W.Nightingale Richard Massey Andrew Robertson Carlos SFrenk Aristeidis Amvrosiadis Nicola CAmorisco Qiuhan He Amy Etherington Shaun Cole Kai Zhu 
the support of the National Natural Science Foundation of China(Nos.11988101,11773032,12022306);the science research grants from the China Manned Space Project(Nos.CMS-CSST-2021-B01,CMS-CSST-2021-A01);the support from K.C.Wong Education Foundation;funding from the UK Space Agency through award ST/W002612/1;from STFC through award ST/T002565/1;support by the European Research Council(ERC)through Advanced Investigator grant to CSF,DMIDAS(GA 786910);supported by the European Research Council Horizon 2020 grant“EWC”(award AMD-776247-6);supported by an STFC/UKRI Ernest Rutherford Fellowship,Project Reference:ST/S004998/1。
The elliptical power-law model of the mass in a galaxy is widely used in strong gravitational lensing analyses.However,the distribution of mass in real galaxies is more complex.We quantify the biases due to this model...
关键词：galaxies:structure galaxies:halos gravitational lensing:strong 
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