Direct visualization of an incommensurate unidirectional charge density wave in
Phys. Rev. B 112, 045132 – Published 18 July, 2025
DOI: https://doi.org/10.1103/2p56-xl41
Abstract
Superconductivity emerges in both and under high pressure by suppressing their density-wave (DW) transitions, but critical temperature () differs significantly between these two compounds. To gain deeper insights into the distinct superconducting states, it is essential to unravel the nature of the DW states at ambient pressure, a topic that remains largely unexplored. Here, using scanning tunneling microscopy/spectroscopy, we report the direct visualization of an incommensurate unidirectional charge DW (CDW) in in real space. The density of states (DOS) is strongly depleted near , indicating the opening of a CDW gap of 2Δ ≈ 71 meV, which is unfavorable for the formation of superconductivity at ambient pressure. We propose that the CDW arises from Fermi surface nesting and is likely a subsidiary phase of a spin-DW. Compared with , the weaker electronic correlation in is likely one reason for the lower .