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Physical Review

Translational Inertial Spin Effect with Moving Particles

O. Costa de Beauregard

Published Apr 27, 1964• 16 citations
Publisher

Abstract

Although the final conclusion of a preceding paper was incorrect, as we shall explain, the main point remains, and should entail the existence of sui generis recoil effects associated with nonzero values of curl $\ensuremath{\sigma}$ ($\ensuremath{\sigma}$ is the spin density). These should be observed by testing, not with solids as was previously proposed, but with the probability fluids associated with moving particles; this more refined type of experiment should be able to select, among the set of integrally equivalent energy-momentum tensors, the one describing locally the true or physical energy-momentum flux. In this paper it is shown, by an explicit calculation, that cylindrical type solutions of the extreme relativistic Dirac equation exist with no $z$ dependence of the wave function (and thus no ${k}_{z}$ component of the momentum) but still with a $z$ component of the Dirac probability current; as this conclusion is reached with a $t$ dependence of the wave function of strictly the form $\mathrm{exp}(\ensuremath{-}\frac{\mathrm{iWt}}{\ensuremath{\hbar}})$, there is no question of having to perform a Foldy-Wouthuysen transformation to extract the positive energy contribution (or equivalently, to use the Newton-Wigner position operator). The "transverse inertial spin effect" we predict is locally described by the flux of the Dirac current per time $\mathrm{dt}$ and surface $d\mathrm{s}$, and corresponds to the local transition probabilities between the dynamical state of the beam and a pointlike localization of the incident particles.

DOI
10.1103/physrev.134.b471

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Although the final conclusion of a preceding paper was incorrect, as we shall explain, the main point remains, and should entail the existence of sui generis recoil effects associated with nonzero values of curl \ensuremathσ\ensuremath{\sigma}\ensuremathσ (\ensuremathσ\ensuremath{\sigma}\ensuremathσ is the spin density). These should be observed by testing, not with solids as was previously proposed, but with the probability fluids associated with moving particles; this more refined type of experiment should be able to select, among the set of integrally equivalent energy-momentum tensors, the one describing locally the true or physical energy-momentum flux. In this paper it is shown, by an explicit calculation, that cylindrical type solutions of the extreme relativistic Dirac equation exist with no zzz dependence of the wave function (and thus no kz{k}_{z}kz​ component of the momentum) but still with a zzz component of the Dirac probability current; as this conclusion is reached with a ttt dependence of the wave function of strictly the form exp(\ensuremath−iWt\ensuremathℏ)\mathrm{exp}(\ensuremath{-}\frac{\mathrm{iWt}}{\ensuremath{\hbar}})exp(\ensuremath−\ensuremathℏiWt​), there is no question of having to perform a Foldy-Wouthuysen transformation to extract the positive energy contribution (or equivalently, to use the Newton-Wigner position operator). The "transverse inertial spin effect" we predict is locally described by the flux of the Dirac current per time dt\mathrm{dt}dt and surface dsd\mathrm{s}ds, and corresponds to the local transition probabilities between the dynamical state of the beam and a pointlike localization of the incident particles.
Zitterbewegung (ZBW), arising from the interference between positive- and negative-energy solutions of the Dirac equation, is a characteristic feature of relativistic single-particle dynamics, but its explicit manifestation depends on the choice of position operator. We formulate relativistic vortex electron wave packets as coherent superpositions of Dirac plane-wave states and derive their exact spacetime evolution. For the canonical Dirac position, we show that orbital angular momentum substantially enhances and spatially structures the relative-coordinate contribution conventionally associated with ZBW. We then analyze the operator dependence of this result by separating the canonical position into a Foldy–Wouthuysen/Newton–Wigner (FW/NW) mean position and an oscillatory relative coordinate. For the vortex packets considered here, the FW/NW mean position exhibits only the ordinary centroid drift and no transverse trembling. However, the same vortex-enhanced radial scale survives in the positive-energy sector as a Berry-type geometric dressing of the projected position operator. The present work therefore identifies not a representation-independent trembling of the one-particle centroid, but a vortex-amplified remnant of Dirac interband mixing in an operationally meaningful position observable.
Motivated by recent interest in relativistic electron vortex states, we revisit the spin and orbital angular momentum properties of Dirac electrons. These are uniquely determined by the choice of the position operator for a relativistic electron. We consider two main approaches discussed in the literature: (i) the projection of operators onto the positive-energy subspace, which removes the Zitterbewegung effects and correctly describes spin-orbit interaction effects, and (ii) the use of Newton-Wigner-Foldy-Wouthuysen operators based on the inverse Foldy-Wouthuysen transformation. We argue that the first approach [previously described in application to Dirac vortex beams in K. Y. Bliokh et al., Phys. Rev. Lett. 107, 174802 (2011)] has a more natural physical interpretation, including spin-orbit interactions and a nonsingular zero-mass limit, than the second one [S. M. Barnett, Phys. Rev. Lett. 118, 114802 (2017)].