2009
DOI: 10.1134/s0021364008210091
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Berry effect in acoustical polarization transport in phononic crystals

Abstract: We derive the semiclassical equations of motion of a transverse acoustical wave packet propagating in a phononic crystal subject to slowly varying perturbations. The formalism gives rise to Berry effect terms in the equations of motion, manifested as the Rytov polarization rotation law and the polarization-dependent Hall effect. We show that the formalism is also applicable to the case of non-periodic inhomogeneous media, yielding explicit expressions for the Berry effect terms.Comment: To appear in JETP Let

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Cited by 12 publications
(17 citation statements)
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“…The formalism gives rise to a Berry phase describing the rotation of the polarization vector (the Rytov law), and a Berry curvature in the semiclassical equations of motion deflecting the phonons depending on their polarization (the polarization dependent Hall effect). These, of course, reproduce the results of [19] (and [20], as far as non-periodic inhomogeneous media are concerned). We analyze the effect of classical noise on the Rytov law and derive the distribution of the Rytov rotation angle in the presence of thermal noise.…”
Section: Introductionsupporting
confidence: 85%
“…The formalism gives rise to a Berry phase describing the rotation of the polarization vector (the Rytov law), and a Berry curvature in the semiclassical equations of motion deflecting the phonons depending on their polarization (the polarization dependent Hall effect). These, of course, reproduce the results of [19] (and [20], as far as non-periodic inhomogeneous media are concerned). We analyze the effect of classical noise on the Rytov law and derive the distribution of the Rytov rotation angle in the presence of thermal noise.…”
Section: Introductionsupporting
confidence: 85%
“…The evolution of the wave packet can effectively be described by three so-called semi-classical variables: the semi-classical position r(t), momentum k(t), and composition (generalized polarization) η(t) of the wave packet in the two-fold degenerate subspace [30,31]. The evolution of those variables is described by semi-classical equations of motion [16,30,31] (see also SI), originating in electronic solid-state physics, but commonly applied to other waves such as light [32,33] or acoustic waves [34,35].…”
mentioning
confidence: 99%
“…Because of the dependence on polarization of optical and transverse acoustical wave propagation in inhomogeneous media, there occurs similar polarization rotation (the Rytov rotation), which is established to be a manifestation of the Berry phase of the quanta (photons/phonons) of the quantized wave fields [12][13][14]. In this work, we show that the cosmological birefringence likewise arises from an adiabatic noncyclic geometric phase that appears in the quntum state of the photons because of their interaction with the slowly varying pseudo-scalar field.…”
Section: Introductionmentioning
confidence: 99%