Non-paraxial relativistic wave packets with orbital angular momentum
Dmitry Karlovets

TL;DR
This paper introduces a relativistic wave packet model with high orbital angular momentum, revealing enhanced non-paraxial effects and potential observable consequences in electron and atomic physics experiments.
Contribution
It presents a Lorentz-invariant, localized wave packet model for vortex particles with high orbital angular momentum, extending Laguerre-Gaussian beams to the relativistic regime.
Findings
Non-paraxial corrections are amplified by orbital angular momentum.
Relativistic wave packets can reach non-paraxial effects of order 10^{-3}.
The model predicts increased invariant mass and spin-orbit coupling effects.
Abstract
One of the reasons for the tremendous success of a plane-wave approximation in particle physics is that the non-paraxial corrections to such observables as energy, magnetic moment, scattering cross section, and so on are attenuated as where is a beam width and is a Compton wavelength. This amounts to less than for modern electron accelerators and less than for electron microscopes. Here we show that these corrections are times enhanced for vortex particles with high orbital angular momenta , which can already be as large as . We put forward the relativistic wave packets, both for vortex bosons and fermions, which transform correctly under the Lorentz boosts, are localized in a 3D space, and represent a non-paraxial generalization of the Laguerre-Gaussian…
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Taxonomy
TopicsOrbital Angular Momentum in Optics · Radio Wave Propagation Studies · Nonlinear Waves and Solitons
