Abstract
In this work we perform ultrafast time-resolved reflectivity measurements to study the symmetry breaking in the charge-density wave (CDW) phase of CsV3Sb5. By extracting the coherent phonon spectrum in the CDW phase of CsV3Sb5, we discover close phonon pairs near 1.3 THz and 3.1 THz, as well as a new mode at 1.84 THz. The 1.3 THz phonon pair and the 1.84 THz mode are observed up to the CDW transition temperature. Combining density-functional theory calculations, we show that these phonon pairs arise from the coexistence of Star of David and inverse Star of David distortions combined with sixfold rotational symmetry breaking. An anisotropy in the magnitude of transient reflectivity change is also revealed at the onset of CDW order. Our results thus indicate broken sixfold rotational symmetry in the charge-density wave state of CsV3Sb5, along with the absence of nematic fluctuation above TCDW. Meanwhile, the measured coherent phonon spectrum in the CDW phase of CsV3Sb5−xSnx with x = 0.03–0.04 matches the staggered inverse Star of David with interlayer π phase shift. This CDW structure contrasts with undoped CsV3Sb5 and explains the evolution from a phonon pair to a single mode at 1.3 THz by x = 0.03–0.04 Sn doping.
| Original language | English |
|---|---|
| Article number | 125127 |
| Journal | Physical Review B |
| Volume | 112 |
| Issue number | 12 |
| DOIs | |
| State | Published - Sep 12 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 National Science Foundation EPM program under Grant no. DMR-2213891. S.D.W. and B.R.O. gratefully acknowledge support via the UC Santa Barbara National Science Foundation Quantum Foundry funded via the QAMASE-i program under award DMR-1906325. B.R.O. acknowledges 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 a research grant from the Estate of Gerald Alexander. L.W. acknowledges support from the Sloan Foundation under Award No. FG-2025-25036. 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 National Science Foundation EPM program under Grant no. DMR-2213891. S.D.W. and B.R.O. gratefully acknowledge support via the UC Santa Barbara National Science Foundation Quantum Foundry funded via the Q-AMASE-i program under award DMR-1906325. B.R.O. acknowledges 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 a research grant from the Estate of Gerald Alexander. L.W. acknowledges support from the Sloan Foundation under Award No. FG-2025-25036.