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      Strong Coupling Phases of Partially Filled Twisted Bilayer Graphene Narrow Bands

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      Physical Review Letters
      American Physical Society (APS)

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          Is Open Access

          Failure of Nielsen-Ninomiya Theorem and Fragile Topology in Two-Dimensional Systems with Space-Time Inversion Symmetry: Application to Twisted Bilayer Graphene at Magic Angle

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            Strength of effective Coulomb interactions in graphene and graphite.

            To obtain an effective many-body model of graphene and related materials from first principles we calculate the partially screened frequency dependent Coulomb interaction. In graphene, the effective on-site (Hubbard) interaction is U(00)=9.3  eV in close vicinity to the critical value separating conducting graphene from an insulating phase emphasizing the importance of nonlocal Coulomb terms. The nearest-neighbor Coulomb interaction strength is computed to U(01)=5.5  eV. In the long-wavelength limit, we find the effective background dielectric constant of graphite to be ϵ=2.5 in very good agreement with experiment.
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              Electrostatic effects, band distortions, and superconductivity in twisted graphene bilayers

              Significance For small twist angles, bilayer graphene forms long-wavelength Moiré patterns. For specific, so-called magic, angles of the order of 1 degree, very narrow bands have been seen that lead to superconductivity. The underlying mechanisms have since been discussed in a variety of theoretical approaches. We show that the modulation of the charge density significantly modifies the electronic structure. These changes can make an important contribution to superconductivity through electron-assisted hopping.
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                Author and article information

                Journal
                PRLTAO
                Physical Review Letters
                Phys. Rev. Lett.
                American Physical Society (APS)
                0031-9007
                1079-7114
                June 2019
                June 18 2019
                : 122
                : 24
                Article
                10.1103/PhysRevLett.122.246401
                31322361
                7f621dad-d0b2-466c-8ae2-2776d5491500
                © 2019

                https://link.aps.org/licenses/aps-default-license

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