Pauli equation and charged spin-1/2 particle in a weak gravitational field

Abstract

Using the nonrelativistic approximation in the curved-space Dirac equation, the analog of the Pauli equation is derived for a weak gravitational field with a gauge fixing condition related to the synchronous gauge, in the presence of an electromagnetic field. Different from the previous works which were employing either the exact or conventional Foldy-Wouthuysen transformations, here we perform calculations by directly performing nonrelativistic approximation which reduced in the power series expansion in the inverse mass of the spinning particle. On top of that, the equations of motion for the massive spin-$1/2$ charged particle are obtained. The two particular cases of the previously explored backgrounds, namely a) plane gravitational wave and b) homogeneous static gravitational field are considered for control. In the case a) we meet correspondence with the previous results. On the other hand, in case b), there is no correspondence with neither perturbative nor with exact Foldy-Wouthuysen transformations, which we also recalculate and agree with the previous works. The disagreement is a kind of a theoretical challenge and most likely occurs because the potential energy, in the particular case of Newtonian approximation, is proportional to the mass of the particle.

24 pages, no figures

References in corpus (7)

• Spin dynamics in gravitational fields of rotating bodies and the equivalence principle
• Equivalence principle and experimental tests of gravitational spin effects
• General treatment of quantum and classical spinning particles in external fields
• Solution of the problem of uniqueness and hermiticity of hamiltonians for Dirac particles in gravitational fields
• Hermiticity of the Dirac Hamiltonian in Curved Spacetime
• Semiclassical analysis of Dirac fields on curved spacetime
• Exact Foldy-Wouthuysen transformation for gravitational waves and magnetic field background