Atomistic Origin of Diverse Charge Density Wave States in CsV3Sb5

Binhua Zhang, Hengxin Tan, Binghai Yan, Changsong Xu, Hongjun Xiang

Research output: Contribution to journalArticlepeer-review

Abstract

Kagome metals AV3Sb5 (A=K, Rb, or Cs) exhibit intriguing charge density wave (CDW) instabilities, which interplay with superconductivity and band topology. However, despite firm observations, the atomistic origins of the CDW phases, as well as hidden instabilities, remain elusive. Here, we adopt our newly developed symmetry-adapted cluster expansion method to construct a first-principles-based effective Hamiltonian of CsV3Sb5, which not only reproduces the established inverse star of David (ISD) phase, but also predict a series of D3h-n states under mild tensile strains. With such atomistic Hamiltonians, the microscopic origins of different CDW states are revealed as the competition of the second-nearest neighbor V-V pairs versus the first-nearest neighbor V-V and V-Sb couplings. Interestingly, the effective Hamiltonians also reveal the existence of ionic Dzyaloshinskii-Moriya interaction in the high-symmetry phase of CsV3Sb5 and drives the formation of noncollinear CDW patterns. Our work thus not only deepens the understanding of the CDW formation in AV3Sb5, but also demonstrates that the effective Hamiltonian is a suitable approach for investigating CDW mechanisms, which can be extended to various CDW systems.

Original languageEnglish
Article number096101
JournalPhysical review letters
Volume132
Issue number9
DOIs
Publication statusPublished - 1 Mar 2024

Bibliographical note

We thank Professor Tao Wu for useful discussions on strain effects. H. T. acknowledges Shangfei Wu for helpful discussions. We acknowledge financial support from the National Key R&D Program of China (No. 2022YFA1402901), NSFC (Grants No. 11825403, No. 11991061, No. 12188101, No. 12174060, and No. 12274082), the Guangdong Major Project of the Basic and Applied basic Research (Future functional materials under extreme conditions–2021B0301030005), Shanghai Pilot Program for Basic Research–FuDan University 21TQ1400100 (23TQ017), and Shanghai Science and Technology Program (23JC1400900). C. X. also acknowledges support from the Shanghai Science and Technology Committee (Grant No. 23ZR1406600). B. Y. acknowledges the financial support by the European Research Council (ERC Consolidator Grant “NonlinearTopo,” No. 815869) and the ISF—Personal Research Grant (No. 2932/21).B. Z. also acknowledges the support from the China Postdoctoral Science Foundation (Grant No. 2022M720816).

Publisher Copyright:
© 2024 American Physical Society.

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

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