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