|Original language||English (US)|
|State||Published - 2020|
Bibliographical noteKAUST Repository Item: Exported on 2020-10-01
Acknowledged KAUST grant number(s): OSR-2017-CRG6-3427
Acknowledgements: Y.G., Y.P, and Z.R.Y. have contributed equally to this work. Financial support from the National Key Research and Development Program of China (Grants No. 2017YFA0206200), the National Natural Science Foundation of China (NSFC, Grants No. 11874409, 11804380, 51801087), Beijing Natural Science Foundation (Grant No. Z190009), the Strategic Priority Research Program (B) [Grant No. XDB07030200], the Key Research Program of Frontier Sciences (Grant No. QYZDJ-SSW-SLH016), the International Partnership Program (Grant No. 112111KYSB20170090) of the Chinese Academy of Sciences (CAS), K. C. Wong Education Foundation (GJTD-2019-14), and Fujian Innovation Academy, Chinese Academy of Sciences (Grant No. FJCXY18040302). J.Z. and X.Z. acknowledge the financial support from the King Abdullah University of Science and Technology (KAUST), Office of Sponsored Research (OSR) under the Award No. OSR-2017-CRG6-3427. S.L.Z. acknowledges the starting grant from ShanghaiTech University and the Eastern Scholar Scheme. T.H. gratefully acknowledges support from EPSRC (EP/N032128/1). We acknowledge beamtime on beamline I10 at Diamond Light Source (Didcot, UK) under proposals SI20183 and MM21868, and on the SEXTANTS beamline at the SOLEIL synchrotron (Gif-sur-Yvette, France) under proposal 20181882. Guoqiang Yu acknowledges helpful discussions with Haifeng Du and Junjie Li.