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Nonreciprocal Acoustic and Optical Phonon Dispersion Mediated by Berry Curvature in Chiral Weyl Semimetals

Sanghita Sengupta

TL;DR

This work addresses how Berry curvature and orbital magnetic moment in chiral Weyl semimetals imprint onto phonon dispersions under a magnetic field, producing a phonon magnetochiral effect (PMCE). It develops a semiclassical framework combining the Boltzmann kinetic equation for Weyl electrons with elasticity theory, incorporating node-dependent Weyl properties and magnetic-field–driven chiral imbalance to compute both acoustic and non-polar optical phonon dispersions. The results show zero-field renormalizations of acoustic and optical branches and magnetic-field–induced nonreciprocity, with acoustic effects dominated by attenuation and a small real shift, while optical modes exhibit linear-in-wavevector PMCE. The findings advance phonons as probes of topological band geometry and dynamical anomaly physics and point to polar-mode extensions and strain-engineering possibilities for enhanced nonreciprocal phononics.

Abstract

We investigate the phonon magnetochiral effect (PMCE) in chiral Weyl semimetals by deriving the nonreciprocal dispersion relations of both acoustic and non-polar optical phonons in the presence of a magnetic field. Using a semiclassical Boltzmann kinetic framework that incorporates Berry curvature, orbital magnetic moment, and node-dependent electronic structure, we obtain analytic expressions for the magnetic-field-induced corrections to the phonon dynamical matrix. Inequivalent Weyl nodes with distinct Fermi velocities, Fermi energies, and relaxation times generate a dynamical chiral imbalance that alters the phonon dispersion. For acoustic phonons, the formalism yields the magnetic-field-dependent corrections to the longitudinal mode, while for optical phonons we identify an optical analogue of the PMCE that produces a corresponding shift in the optical branch. Together, these results provide a unified theoretical description of how band-geometric properties of Weyl fermions influence both acoustic and optical phonon dispersions in chiral Weyl semimetals.

Nonreciprocal Acoustic and Optical Phonon Dispersion Mediated by Berry Curvature in Chiral Weyl Semimetals

TL;DR

This work addresses how Berry curvature and orbital magnetic moment in chiral Weyl semimetals imprint onto phonon dispersions under a magnetic field, producing a phonon magnetochiral effect (PMCE). It develops a semiclassical framework combining the Boltzmann kinetic equation for Weyl electrons with elasticity theory, incorporating node-dependent Weyl properties and magnetic-field–driven chiral imbalance to compute both acoustic and non-polar optical phonon dispersions. The results show zero-field renormalizations of acoustic and optical branches and magnetic-field–induced nonreciprocity, with acoustic effects dominated by attenuation and a small real shift, while optical modes exhibit linear-in-wavevector PMCE. The findings advance phonons as probes of topological band geometry and dynamical anomaly physics and point to polar-mode extensions and strain-engineering possibilities for enhanced nonreciprocal phononics.

Abstract

We investigate the phonon magnetochiral effect (PMCE) in chiral Weyl semimetals by deriving the nonreciprocal dispersion relations of both acoustic and non-polar optical phonons in the presence of a magnetic field. Using a semiclassical Boltzmann kinetic framework that incorporates Berry curvature, orbital magnetic moment, and node-dependent electronic structure, we obtain analytic expressions for the magnetic-field-induced corrections to the phonon dynamical matrix. Inequivalent Weyl nodes with distinct Fermi velocities, Fermi energies, and relaxation times generate a dynamical chiral imbalance that alters the phonon dispersion. For acoustic phonons, the formalism yields the magnetic-field-dependent corrections to the longitudinal mode, while for optical phonons we identify an optical analogue of the PMCE that produces a corresponding shift in the optical branch. Together, these results provide a unified theoretical description of how band-geometric properties of Weyl fermions influence both acoustic and optical phonon dispersions in chiral Weyl semimetals.

Paper Structure

This paper contains 19 sections, 83 equations, 3 figures.

Figures (3)

  • Figure 1: (a) Geometry of the phonon magnetochiral effect (PMCE): the relative orientation of the magnetic field $\mathbf{B}$ and the phonon wave vector $\mathbf{q}$ determines the nonreciprocal correction to the phonon dispersion. Reversing the direction of $\mathbf{B}$ (or equivalently $\mathbf{q}$) leads to unequal phonon frequencies, $\omega \neq \omega'$, reflecting the odd-in-$B$ and odd-in-$q$ nature of the effect. (b) Schematic depiction of a chiral Weyl semimetal with two inequivalent Weyl nodes characterized by different Fermi velocities, Fermi energies, and strong Berry curvature and orbital magnetic moments. The quantities $\Gamma_{A}$ and $\Gamma_{E}$ denote the intra-node and inter-node relaxation rates, respectively, which govern local equilibration and chiral charge transfer between Weyl nodes.
  • Figure 2: Acoustic phonon dispersion in a chiral Weyl semimetal for zero magnetic field ($\omega^{(0)}$) and for finite fields $B>0$ and $B<0$, the latter corresponding to phonon propagation parallel and antiparallel to $\mathbf{B}$. The top-left panel displays the real part of the dispersion, where the zero-field curve $\omega^{(0)}$ represents the electron–phonon renormalized longitudinal mode. A finite magnetic field introduces a small magnetochiral splitting between the $\omega_{\pm}$ (for $B>0$) and $\omega_{\pm}$ (for $B<0$) branches. The magnitude of this shift, shown in the top-right panel, is small but experimentally resolvable senguptapmce. In contrast, the imaginary part of the dispersion (bottom-left) exhibits a substantially larger nonreciprocal correction, as quantified in the bottom-right panel.
  • Figure 3: Optical phonon dispersion for zero magnetic field and for finite fields $B>0$ and $B<0$ in a chiral Weyl semimetal. The zero-field dispersion ($\omega^{(0)}$) represents the electron–phonon renormalized non-polar optical mode. Applying a magnetic field produces a linear magnetochiral splitting between the $\omega(B>0)$ and $\omega(B<0)$ branches: the real part (top-left) shifts by a small but finite amount, while the imaginary part (bottom-left) exhibits a significant directional asymmetry in attenuation. The right-hand panels quantify the magnetochiral effects, showing that the optical-phonon PMCE increases linearly with $q$.