Three-state nematicity and magneto-optical Kerr effect in the charge density waves in kagome superconductors

Yishuai Xu, Zhuoliang Ni, Yizhou Liu, Brenden R. Ortiz, Qinwen Deng, Stephen D. Wilson, Binghai Yan, Leon Balents, Liang Wu

Research output: Contribution to journalArticlepeer-review

108 Scopus citations

Abstract

The kagome lattice provides a fascinating playground to study geometrical frustration, topology and strong correlations. The newly discovered kagome metals AV3Sb5 (where A can refer to K, Rb or Cs) exhibit phenomena including topological band structure, symmetry-breaking charge-density waves and superconductivity. Nevertheless, the nature of the symmetry breaking in the charge-density wave phase is not yet clear, despite the fact that it is crucial in order to understand whether the superconductivity is unconventional. In this work, we perform scanning birefringence microscopy on all three members of this family and find that six-fold rotation symmetry is broken at the onset of the charge-density wave transition in all these compounds. We show that the three nematic domains are oriented at 120° to each other and propose that staggered charge-density wave orders with a relative π phase shift between layers is a possibility that can explain these observations. We also perform magneto-optical Kerr effect and circular dichroism measurements. The onset of both signals is at the transition temperature, indicating broken time-reversal symmetry and the existence of the long-sought loop currents in that phase.

Original languageEnglish
Pages (from-to)1470-1475
Number of pages6
JournalNature Physics
Volume18
Issue number12
DOIs
StatePublished - Dec 2022
Externally publishedYes

Funding

We thank C. Varma, Z. Wang and I. Zeljkovic for helpful discussions. This project is mainly supported by L.W.’s startup package at the University of Pennsylvania. The development of the imaging systems was sponsored by the Army Research Office and was accomplished under grants no. W911NF-21-1-0131, W911NF-20-2-0166 and W911NF-19-1-0342, and the Vice Provost for Research University Research Foundation. Y.X. is also partially supported by the NSF EAGER grant via the CMMT programme (DMR-2132591), a seed grant from NSF-funded Penn MRSEC (DMR-1720530) and the Gordon and Betty Moore Foundation’s EPiQS Initiative, and grant GBMF9212 to L.W.. Z.N. acknowledges support from the Vagelos Institute of Energy Science and Technology graduate fellowship and the Dissertation Completion Fellowship at the University of Pennsylvania. B.R.O. and S.D.W. acknowledge support via the UC Santa Barbara NSF Quantum Foundry funded via the Q-AMASE-i program under award DMR-1906325. Q.D. is partially supported by the NSF EPM program under grant no. DMR-2213891. B.Y. acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (ERC Consolidator Grant ‘NonlinearTopo’, no. 815869). L.B. is supported by the NSF CMMT program under grant no. DMR-2116515. L.W. acknowledges the support by the Air Force Office of Scientific Research under award no. FA9550-22-1-0410.

FundersFunder number
NSF-funded Penn MRSECDMR-1720530
UC Santa Barbara NSFDMR-2213891, DMR-1906325
Vice Provost for Research University Research Foundation
National Science FoundationDMR-2132591
Air Force Office of Scientific ResearchFA9550-22-1-0410
Army Research OfficeW911NF-20-2-0166, W911NF-21-1-0131, W911NF-19-1-0342
Gordon and Betty Moore FoundationGBMF9212
University of Pennsylvania
Horizon 2020 Framework Programme815869, DMR-2116515
Vagelos Institute for Energy Science and Technology, University of Pennsylvania
European Research Council

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