Abstract
Broken time-reversal symmetry in the absence of spin order indicates the presence of unusual phases such as orbital magnetism and loop currents1–4. The recently discovered kagome superconductors AV3Sb5 (where A is K, Rb or Cs)5,6 display an exotic charge-density-wave (CDW) state and have emerged as a strong candidate for materials hosting a loop current phase. The idea that the CDW breaks time-reversal symmetry7–14 is, however, being intensely debated due to conflicting experimental data15–17. Here we use laser-coupled scanning tunnelling microscopy to study RbV3Sb5. By applying linearly polarized light along high-symmetry directions, we show that the relative intensities of the CDW peaks can be reversibly switched, implying a substantial electro-striction response, indicative of strong nonlinear electron–phonon coupling. A similar CDW intensity switching is observed with perpendicular magnetic fields, which implies an unusual piezo-magnetic response that, in turn, requires time-reversal symmetry breaking. We show that the simplest CDW that satisfies these constraints is an out-of-phase combination of bond charge order and loop currents that we dub a congruent CDW flux phase. Our laser scanning tunnelling microscopy data open the door to the possibility of dynamic optical control of complex quantum phenomenon in correlated materials.
Original language | English |
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Pages (from-to) | 60-66 |
Number of pages | 7 |
Journal | Nature |
Volume | 631 |
Issue number | 8019 |
DOIs | |
State | Published - Jul 4 2024 |
Funding
This material is based on work supported by the US Department of Energy Office of Science National Quantum Information Science Research Centers as part of the Q-NEXT centre, which supported the laser-STM work of S.B. and provided partial support for laser-STM development. V.M. acknowledges support from the Gordon and Betty Moore Foundation\u2019s EPiQS initiative through grant number GBMF9465 for magnetic-field STM studies and the laser-STM instrument development. Funding for sample growth was provided via the UC Santa Barbara NSF Quantum Foundry funded via the Q-AMASE-i programme under award DMR-1906325. A.N.C.S. acknowledges support from the Eddlemam Center for Quantum Innovation at UC Santa Barbara. E.R., F.Y. and T.B. were supported by NSF CAREER grant DMR-2046020. R.M.F. was supported by the Air Force Office of Scientific Research under award number FA9550-21-1-0423. Z.W. is supported by the US Department of Energy, Basic Energy Sciences (grant number DE-FG02-99ER45747) and by Research Corporation for Science Advancement (Cottrell SEED award number 27856). B.R.O. gratefully acknowledges support from the US Department of Energy (DOE), Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division.