Impacts of in-plane strain on commensurate graphene/hexagonal boron nitride superlattices
Due to atomically thin structure, graphene/hexagonal boron nitride (G/hBN) heterostructures are intensively sensitive to the external mechanical forces and deformations being applied to their lattice structure. In particular, strain can lead to the modification of the electronic properties of G/hBN....
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Veröffentlicht in: | Physica. B, Condensed matter Condensed matter, 2019-07, Vol.565, p.33-39 |
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Sprache: | eng |
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Zusammenfassung: | Due to atomically thin structure, graphene/hexagonal boron nitride (G/hBN) heterostructures are intensively sensitive to the external mechanical forces and deformations being applied to their lattice structure. In particular, strain can lead to the modification of the electronic properties of G/hBN. Furthermore, moiré structures driven by misalignment of graphene and hBN layers introduce new features to the electronic behavior of G/hBN. Utilizing ab initio calculation, we study the strain-induced modification of the electronic properties of diverse stacking faults of G/hBN when applying in-plane strain on both layers, simultaneously. We observe that the interplay of few percent magnitude in-plane strain and moiré pattern in the experimentally applicable systems leads to considerable valley drifts, band gap modulation and enhancement of the substrate-induced Fermi velocity renormalization. Furthermore, we find that regardless of the strain alignment, the zigzag direction becomes more efficient for electronic transport, when applying in-plane non-equibiaxial strains.
•Giant strain-induced valley drifts and band gap modulation for non-equibiaxial strain.•Largely tunable band gaps at low strain costs (1-3%) compared to monolayer graphene (>20%).•Substrate-induced Fermi velocity renormalization is enhanced for in-plane biaxial strain.•For non-equibiaxial strains, regardless of the strain alignment, zigzag direction is more efficient for electronic transport. |
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ISSN: | 0921-4526 1873-2135 |
DOI: | 10.1016/j.physb.2018.11.029 |