Orbital ordering and fluctuations in a kagome superconductor CsV3Sb5

Recently, competing electronic instabilities, including superconductivity and density-wave-like order, have been discovered in vanadium-based kagome metals A V 3 Sb 5 ( A = K, Rb, Cs) with a nontrivial band topology. This finding stimulates considerable interest to study the interplay of these compe...

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Veröffentlicht in:Science China. Physics, mechanics & astronomy mechanics & astronomy, 2022-04, Vol.65 (4), p.247462, Article 247462
Hauptverfasser: Song, DianWu, Zheng, LiXuan, Yu, FangHang, Li, Jian, Nie, LinPeng, Shan, Min, Zhao, Dan, Li, ShunJiao, Kang, BaoLei, Wu, ZhiMian, Zhou, YanBing, Sun, KuangLv, Liu, Kai, Luo, XiGang, Wang, ZhenYu, Ying, JianJun, Wan, XianGang, Wu, Tao, Chen, XianHui
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Sprache:eng
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Zusammenfassung:Recently, competing electronic instabilities, including superconductivity and density-wave-like order, have been discovered in vanadium-based kagome metals A V 3 Sb 5 ( A = K, Rb, Cs) with a nontrivial band topology. This finding stimulates considerable interest to study the interplay of these competing electronic orders and possible exotic excitations in the superconducting state. Here, we performed 51 V and 133 Cs nuclear magnetic resonance (NMR) measurements on a CsV 3 Sb 5 single crystal to clarify the nature of density-wave-like transition in these kagome superconductors. A first-order structural transition is unambiguously revealed below T s ∼ 94 K by observing the sudden splitting of Knight shift in 51 V NMR spectrum. Moreover, combined with 133 Cs NMR spectrum, the present result confirms a three-dimensional structural modulation. By further analyzing the anisotropy of Knight shift and 1/ T 1 T at 51 V nuclei, we proposed that the orbital order is the primary electronic order induced by the first-order structural transition, which is supported by further analysis on electric field gradient at 51 V nuclei. In addition, the evidence for possible orbital fluctuations is also revealed above T s . The present work sheds light on a rich orbital physics in kagome superconductors A V 3 Sb 5 .
ISSN:1674-7348
1869-1927
DOI:10.1007/s11433-021-1826-1