The structure of charge density wave states in AVSb (A = K, Rb, Cs) kagome superconductors remains elusive, with three possible candidates: tri-hexagonal, star-of-David, and their mixture. In this study, we conducted a systematic first-principles investigation of the nuclear quadrupole resonance (NQR) and nuclear magnetic resonance (NMR) spectra for the CsVSb structures. By comparing our simulations with experimental data, we have concluded that the NQR spectrum indicates the tri-hexagonal structure as the proper structure for CsVSb after its charge density wave phase transition. The NMR calculation results obtained from the tri-hexagonal structure are also consistent with the experimental data.

生成讲解博客的中文版本

生成AI智能校验的中文版本