Abstract

Janus single-layer transition metal dichalcogenides, in which the two chalcogen layers have a different chemical nature, push chemical composition control beyond what is usually achievable with van der Waals heterostructures. Here, we report such a Janus compound, SPtSe, which is predicted to exhibit strong Rashba spin–orbit coupling. We synthetized it by conversion of a single-layer of PtSe2 on Pt(111) via sulfurization under H2S atmosphere. Our in situ and operando structural analysis with grazing incidence synchrotron X-ray diffraction reveals the process by which the Janus alloy forms. The crystalline long-range order of the as-grown PtSe2 monolayer is first lost due to thermal annealing. A subsequent recrystallization in presence of a source of sulfur yields a highly ordered SPtSe alloy, which is isostructural to the pristine PtSe2. The chemical composition is resolved, layer-by-layer, using angle-resolved X-ray photoelectron spectroscopy, demonstrating that Se-by-S substitution occurs selectively in the topmost chalcogen layer.

Highlights

  • Most electronic properties of crystals are inherited from their symmetries

  • For monolayer transition metal dichalcogenides (TMDCs) in the 1H phase like MX2 (M=Mo,W and X=S, Se), the mirror symmetry with respect to the transition metal atoms plane leads to zero internal out-of-plane electric field and suppresses any Rashba spin–orbit coupling (SOC)

  • Before we address the formation and structure of the Janus alloy, we discuss about its parent compound, the pristine single layer (SL) PtSe2

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Summary

Introduction

Most electronic properties of crystals are inherited from their symmetries. For monolayer transition metal dichalcogenides (TMDCs) in the 1H phase like MX2 (M=Mo,W and X=S, Se), the mirror symmetry with respect to the transition metal atoms plane leads to zero internal out-of-plane electric field and suppresses any Rashba spin–orbit coupling (SOC). Most superstructure peaks (except those of PtSe2 with h and k multiple of 3), are located close to integer values of l (see e.g., (50l) rod in UHV a few tens of degrees above the growth temperature (between 370 °C and 400 ° C), in order to create Se vacancies in the topmost chalcogen layer, which will be eventually filled with S atoms.

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