Dirac equations in curved space-time versus Papapetrou spinning particles
arXiv:0810.0447 · doi:10.1209/0295-5075/84/30008
Abstract
We find out classical particles, starting from Dirac quantum fields on a curved space-time, by an eikonal approximation and a localization hypothesis for amplitudes. We recover the results by Mathisson-Papapetrou, hence establishing a fundamental correspondence between the coupling of classical and quantum spinning particles with the gravitational field.
6 pages, 1 figure, accepted for publication in Europhysics Letters
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- Semiclassical analysis of Dirac fields on curved spacetime
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- Highly relativistic spin-gravity coupling for fermions
- Highly relativistic spinning particle starting near in a Kerr field
- Fermions on curved backgrounds of matrix models
- Highly relativistic spin-gravity- coupling
- Bouncing Dirac particles: compatibility between MIT boundary conditions and Thomas precession
- Nonequatorial circular orbits of spinning particles in the Schwarzschild-de Sitter background
- Curved-spacetime dynamics of spin- particles in superposed states from a WKB approximation of the Dirac equation
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- Solutions of Mathisson-Papapetrou equations for highly relativistic spinning particles
- Canonical Formulation for a Non-relativistic Spinning Particle Coupled to Gravity
- The precession of particle spin in spherical symmetric spacetimes
- Dynamics of charged spin- particles in superposed states minimally coupled to electromagnetism in curved spacetime within the WKB approximation
- Discrete geodesics and cellular automata