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The interplay of field-tunable strongly correlated states in a multi-orbital moiré system (2303.05347v1)

Published 9 Mar 2023 in cond-mat.mes-hall, cond-mat.mtrl-sci, and cond-mat.str-el

Abstract: The interplay of charge, spin, lattice, and orbital degrees of freedom leads to a wide range of emergent phenomena in strongly correlated systems. In heterobilayer transition metal dichalcogenide moir\'e systems, recent observations of Mott insulators and generalized Wigner crystals are well described by triangular lattice single-orbital Hubbard models based on K-valley derived moir\'e bands. Richer phase diagrams, mapped onto multi-orbital Hubbard models, are possible with hexagonal lattices in $\Gamma$-valley derived moir\'e bands and additional layer degrees of freedom. Here we report the tunable interaction between strongly correlated hole states hosted by $\Gamma$- and K-derived moir\'e bands in a monolayer MoSe$2$ / natural WSe$_2$ bilayer device. To precisely probe the nature of the correlated states, we optically characterise the behaviour of exciton-polarons and distinguish the layer and valley degrees of freedom. We find that the honeycomb $\Gamma$-band gives rise to a charge-transfer insulator described by a two-orbital Hubbard model with inequivalent $\Gamma\mathrm{A}$ and $\Gamma_\mathrm{B}$ orbitals. With an out-of-plane electric field, we re-order the $\Gamma_\mathrm{B}$- and K-derived bands energetically, driving an abrupt redistribution of carriers to the layer-polarized K orbital where new correlated states are observed. Finally, by fine-tuning the band-alignment, we obtain degeneracy of the $\Gamma_\mathrm{B}$ and K orbitals at the Fermi level. In this critical condition, stable Wigner crystals with carriers distributed across the two orbitals are observed until the Fermi-level reaches one hole per lattice site, whereupon the system collapses into a filled $\Gamma_\mathrm{B}$ orbital. Our results establish a platform to investigate the interplay of charge, spin, lattice, and layer geometry in multi-orbital Hubbard model Hamiltonians.

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