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Insulating moir\'e homobilayers lack a threefold symmetric second harmonic generation

Materials Science 2024-11-18 v1 Mesoscale and Nanoscale Physics

Abstract

Atoms within moir\'e bilayers relax in-plane to minimize elastic energy [e.g., Cazeaux et al., J. Elast. 154, 443 (2023)]; such relaxation brings their space group symmetries down to P1. Here, the ab initio second harmonic generation (SHG) of twisted and atomistically optimized hBN bilayers was determined at four twist angles (θ=38.21\theta=38.21^{\circ}, 60.0060.00^{\circ}, 73.1773.17^{\circ}, and 98.2198.21^{\circ}) and for three displacements τ\boldsymbol{\tau} measured away from the ground state AAAA^{\prime} configuration. All moir\'e bilayers have a P1 space symmetry after structural optimization. This situation is quite different to monolayers with hexagonal lattices, which retain a three-fold symmetry. We point out that the actual symmetries of the SHG reported for hBN bilayers on two experimental works do not coincide with the sixfold symmetric theoretical profiles they provide [either sin2(3ϕ)\sin^2(3\phi) or cos2(3ϕ)\cos^2(3\phi)], and show that the intrinsic low structural symmetry of (atomically optimized) hBN bilayer moir\'es can in fact be read out from experimental SHG intensity profiles--which are tunable by θ\theta and by the frequency of light ω\omega: The SHG is most definitely not sixfold-symmetric because moir\'es do not retain a three-fold symmetry. Furthermore, an extrinsic twofold symmetry of the SHG emission is realized by tilting the pump by an angle α\alpha away from the 2D material's normal, regardless of θ\theta and ω\omega. The design of in-plane and ultrathin sources of SHG with low symmetry could be useful for the eventual creation of entanglement sources from 2D materials.

Keywords

Cite

@article{arxiv.2410.22188,
  title  = {Insulating moir\'e homobilayers lack a threefold symmetric second harmonic generation},
  author = {Luis Enrique Rosas-Hernandez and Jose Luis Cabellos and Angiolo Huamán and Bernardo Mendoza and Salvador Barraza-Lopez},
  journal= {arXiv preprint arXiv:2410.22188},
  year   = {2024}
}

Comments

Accepted at Physical Review Materials on October 29, 2024

R2 v1 2026-06-28T19:39:51.632Z