Semiclassical analysis of Dirac fields on curved spacetime
arXiv:2212.04414 · doi:10.1103/PhysRevD.107.044029
Abstract
We present a semiclassical analysis for Dirac fields on an arbitrary spacetime background and in the presence of a fixed electromagnetic field. Our approach is based on a Wentzel-Kramers-Brillouin approximation, and the results are analyzed at leading and next-to-leading order in the small expansion parameter . Taking into account the spin-orbit coupling between the internal and external degrees of freedom of wave packets, we derive effective ray equations with spin-dependent terms. These equations describe the gravitational spin Hall effect of localized Dirac wave packets. We treat both massive and massless Dirac fields and show how a covariantly defined Berry connection and the associated Berry curvature govern the semiclassical dynamics. The gravitational spin Hall equations are shown to be particular cases of the Mathisson-Papapetrou equations for spinning objects.
References in corpus (19)
- Geometrodynamics of Spinning Light
- Berry Curvature, Triangle Anomalies, and the Chiral Magnetic Effect in Fermi Liquids
- Chiral anomaly and transport in Weyl metals
- Geometrodynamics of polarized light: Berry phase and spin Hall effect in a gradient-index medium
- Spin dynamics in gravitational fields of rotating bodies and the equivalence principle
- Geometrical Aspects in Optical Wavepacket Dynamics
- Consistent Chiral Kinetic Theory in Weyl Materials: Chiral Magnetic Plasmons
- Dirac fermions in strong gravitational fields
- Chiral effects in astrophysics and cosmology
- Berry Phase, Lorentz Covariance, and Anomalous Velocity for Dirac and Weyl Particles
- Chiral fermions as classical massless spinning particles
- General treatment of quantum and classical spinning particles in external fields
- Bobbing and Kicks in Electromagnetism and Gravity
- Propagation of polarized gravitational waves
- Wigner-Souriau translations and Lorentz symmetry of chiral fermions
- Semiclassical Dynamics of Dirac particles interacting with a Static Gravitational Field
- Dirac equations in curved space-time versus Papapetrou spinning particles
- Photonic spin Hall effect from quantum kinetic theory in curved spacetime
- Spin Hall effects and the localization of massless spinning particles
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- Gravity-induced birefringence in spherically symmetric spacetimes
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- Quantum geometric tensors from sub-bundle geometry
- Pauli equation and charged spin-1/2 particle in a weak gravitational field
- The precession of particle spin in spherical symmetric spacetimes
- Deflection of Massive Spin- Particles around Kerr Black Hole
- Spin oscillations of neutrinos scattered by the supermassive black hole in the galactic center
- Quantum interferometry in external gravitational fields
- Dynamics of charged spin- particles in superposed states minimally coupled to electromagnetism in curved spacetime within the WKB approximation
- Dirac Equation with Space Contributions Embedded in a Quantum-Corrected Gravitational Field