Why do phonons in many insulators show a thermal Hall effect?
In plain words
Sideways heat flow in a magnetic field appears in magnetic and non-magnetic insulators alike, with roughly similar size relative to the ordinary heat flow. No single coupling between phonons and the field explains all cases.
Precise statement
In insulators including $\mathrm{SrTiO_3}$, cuprate parent compounds, Kitaev candidates, garnets, quartz, MgO and intrinsic Si and Ge, fields of tens of kG produce a thermal Hall conductivity $\kappa_{xy}$ carried by phonons, with thermal Hall angle $\kappa_{xy}/\kappa_{xx}$ up to $\sim 3 \times 10^{-3}\text{ at }9 \times 10^{4}\,\mathrm{G}$, typically peaking near the maximum of $\kappa_{xx}$. Identify the coupling: intrinsic Berry curvature of phonon bands from spin-lattice or ionic Lorentz-type coupling, skew scattering off charged or magnetic defects, or resonant scattering by dynamical defects. An answer predicts magnitude, sign and temperature dependence across materials.
What would settle it
A theory predicting $\kappa_{xy}/\kappa_{xx}$ with sign in several unrelated insulators from measured parameters, confirmed by controlled defect doping.
Status in the literature
Unverified note: it names recent work and was partly written without a live literature search; it awaits a check by an editor.
Phonon thermal Hall signals with a common scaling $\kappa_{xy} \sim \kappa_{xx}^2$ were reported in many nonmagnetic crystals ($\mathrm{SrTiO_3}$, quartz, MgO, $\mathrm{MgAl_2O_4}$, Si, Ge; Jin et al., arXiv 2404.02863, 2024); no coupling mechanism accounts for magnitude and sign across materials.
Problems built on this one
Special cases
- Origin of the large phonon thermal Hall effect in cuprates · open
- Intrinsic versus defect-driven phonon thermal Hall effect in $\mathrm{SrTiO_3}$ · open
- How do phonons couple to a magnetic field in nonmagnetic insulators? · open
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