Using recently developed tools from space-adiabatic perturbation theory, in particular the construction of a non-equilibrium almost-stationary state, we give a new proof that the Kubo formula for the Hall conductivity remains valid beyond the linear response regime. In particular, we prove that, in quantum Hall systems and Chern insulators, the transverse response current is quantized up to any order in the strength of the inducing electric field. The latter is introduced as a perturbation to a periodic, spectrally gapped equilibrium Hamiltonian by means of a linear potential; existing proofs of the exactness of Kubo formula rely instead on a time-dependent magnetic potential. The result applies to both continuum and discrete crystalline systems modelling the quantum (anomalous) Hall effect.

Marcelli, G., Monaco, D. (2022). Purely linear response of the quantum Hall current to space-adiabatic perturbations. LETTERS IN MATHEMATICAL PHYSICS, 112(5) [10.1007/s11005-022-01574-7].

Purely linear response of the quantum Hall current to space-adiabatic perturbations

Marcelli G.;
2022-01-01

Abstract

Using recently developed tools from space-adiabatic perturbation theory, in particular the construction of a non-equilibrium almost-stationary state, we give a new proof that the Kubo formula for the Hall conductivity remains valid beyond the linear response regime. In particular, we prove that, in quantum Hall systems and Chern insulators, the transverse response current is quantized up to any order in the strength of the inducing electric field. The latter is introduced as a perturbation to a periodic, spectrally gapped equilibrium Hamiltonian by means of a linear potential; existing proofs of the exactness of Kubo formula rely instead on a time-dependent magnetic potential. The result applies to both continuum and discrete crystalline systems modelling the quantum (anomalous) Hall effect.
2022
Marcelli, G., Monaco, D. (2022). Purely linear response of the quantum Hall current to space-adiabatic perturbations. LETTERS IN MATHEMATICAL PHYSICS, 112(5) [10.1007/s11005-022-01574-7].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/472935
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