Excitonic and magnetic phases in doped WTe$_2$ monolayers: a Hartree-Fock approach
Guillermo Parra-Martínez, Daniel Muñoz-Segovia, Héctor Ochoa, Jose Angel Silva-Guillén
TL;DR
This work employs zero-temperature Hartree-Fock calculations on a folded two-band k·p model with long-range Coulomb interactions to map the competition among broken-symmetry phases in doped 1T'-WTe2 monolayers. It reveals a rich neutrality phase diagram featuring a spin density wave, a quantum spin Hall insulator, a spin spiral, and an intermediate orbital–magnetic OM3 state, with a later transition to a trivial insulator at strong coupling. Upon electron doping, an easy-plane ferromagnet FM2 emerges via a Stoner-like instability and competes with the spin-spiral phase, suggesting a link between magnetic fluctuations and observed superconductivity. The results provide a framework for interpreting transport and spectroscopic data and guide future experiments probing magnetic and topological order near the QSHI gap.
Abstract
Transport and local spectroscopy measurements have revealed that monolayers of tungsten ditelluride ($1T'$-WTe$_2$) display a quantum spin Hall effect and an excitonic gap at neutrality, besides becoming superconducting at low electron concentrations. With the aim of studying the competition among different broken-symmetry phases upon electron doping, we have performed extensive Hartree-Fock calculations as a function of electron density and Coulomb interaction strength. At charge neutrality, we reproduce the emergence of a spin density wave and a spin spiral state surrounding a quantum spin Hall insulator at intermediate interaction strengths. For stronger interactions, the spin spiral is disrupted by a state breaking both inversion and time-reversal symmetries (but not their product) before the system becomes a trivial band insulator. With electron doping the quantum spin Hall insulator evolves into an easy-plane ferromagnet due to a Stoner-like instability of the conduction band. This phase competes energetically with the spin spiral state. We discuss how our results may help to interpret past and future measurements.
