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Hidden Momentum and the Absence of the Gravitational Spin Hall Effect in a Uniform Field

arXiv:2512.18096 · doi:10.3390/universe11110365

Abstract

We re-examine the recent claim that a Dirac particle freely falling in a uniform gravitational field exhibits a spin-dependent transverse deflection (gravitational spin Hall effect). Using a circulating mass model, we show that hidden momentum arises in uniform fields when an object carries angular momentum. On the quantum side, we analyze the Dirac Hamiltonian in a uniform potential, construct its Foldy--Wouthuysen form, and evaluate the Heisenberg evolution of spin-polarized Gaussian packets. The state used previously, with , is not at rest: because canonical and kinetic momenta differ, the packet carries a spin-dependent hidden momentum from . Imposing requires a compensating spin-dependent ; with this preparation to leading order in the gravitational acceleration . Generalizing, an exact Foldy--Wouthuysen transformation (linear in but to all orders in ) shows that spin-dependent transverse motion begins no earlier than at for a broad class of wave packets. We conclude that a uniform field does not produce a gravitational spin Hall effect at linear order; the previously reported drift stems from inconsistent initial states and misinterpreting canonical momentum.

Invited contribution to the Universe Special Issue Geometric Theories of Gravity

References in corpus (3)

Hidden Momentum and the Absence of the Gravitational Spin Hall Effect in a Uniform Field · wovepaper