Abstract
Motivated by recent experiments on the phonon contribution to the thermal Hall effect in the cuprates, we present an analysis of chiral phonon transport. We assume the chiral behavior arises from a nonzero phonon Hall viscosity, which is likely induced by the coupling to electrons. Phonons with a nonzero phonon Hall viscosity have an intrinsic thermal Hall conductivity, but Chen et al. [Phys. Rev. Lett. 124, 167601 (2020)] have argued that a significantly larger thermal Hall conductivity can arise from an extrinsic contribution which is inversely proportional to the density of impurities. We solve the Boltzmann equation for phonon transport and compute the temperature () dependence of the thermal Hall conductivity originating from skew scattering off pointlike impurities. We find that the dominant source for thermal Hall transport is an interference between impurity skew-scattering channels with opposite parity. The thermal Hall conductivity at low in dimensions, and has a window of -independent behavior for , where is determined by the ratio of scattering potentials with opposite parity. We also consider the role of nonspecular scattering off the sample boundary, and find that it leads to negligible corrections to thermal Hall transport at low .
- Received 8 March 2021
- Accepted 21 April 2021
DOI:https://doi.org/10.1103/PhysRevB.103.205115
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