Revealing rotational symmetry breaking charge density wave order in the kagome superconductor (Rb, K) V3Sb5 by ultrafast pump-probe experiments

  • Qinwen Deng
  • , Hengxin Tan
  • , Brenden R. Ortiz
  • , Stephen D. Wilson
  • , Binghai Yan
  • , Liang Wu

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

The recently discovered Kagome superconductor AV3Sb5 (where A refers to K, Rb, Cs) has stimulated widespread research interest due to its interplay of nontrivial topology and unconventional correlated physics including charge-density waves (CDW) and superconductivity. The essential prerequisite to understanding the microscopic mechanisms of this complex electronic landscape is to unveil the configuration and symmetry of the charge-density wave order. As to now, little consensus has been made on what symmetry is broken. Herein, we clarify the microscopic structure and symmetry breaking of the CDW phase in RbV3Sb5 and KV3Sb5 by ultrafast time-resolved reflectivity. Our approach is based on extracting coherent phonon spectra induced by three-dimensional CDW and comparing them to calculated phonon frequencies via density-functional theory. The combination of these experimental results and calculations provides compelling evidence that the CDW structure of both compounds prevailing up to TCDW is the 2×2×2 staggered inverse Star-of-David pattern with interlayer π phase shift, in which the sixfold rotational symmetry is broken. These observations thus corroborate sixfold rotational symmetry breaking throughout the CDW phase of RbV3Sb5 and KV3Sb5.

Original languageEnglish
Article number165134
JournalPhysical Review B
Volume111
Issue number16
DOIs
StatePublished - Apr 15 2025

Funding

The construction of the pump-probe setup was supported by the Air Force Office of Scientific Research under Award No. FA9550-22-1-0410. Q.D. was mainly supported by the Vagelos Institute of Energy Science and Technology graduate fellowship and also partly supported by the Air Force Office of Scientific Research under Award No. FA9550-22-1-0410 and the NSF EPM program under Grant No. DMR-2213891. S.D.W. and B.R.O. gratefully acknowledge support via the UC Santa Barbara NSF Quantum Foundry funded via the Q-AMASE-i program under Award DMR-1906325. B.R.O. thanks support from the U.S. Department of Energy (DOE), Office of Science, Basic Energy Sciences (BES), Materials Sciences and Engineering Division. B.Y. acknowledges the financial support by the Israel Science Foundation (ISF: 2932/21, 2974/23), German Research Foundation (DFG, CRC-183, A02), and by a research grant from the Estate of Gerald Alexander.

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