Stability of circular orbits of spinning particles in Schwarzschild-like space-times
arXiv:1005.3110 · doi:10.1007/s10714-010-0995-3
Abstract
Circular orbits of spinning test particles and their stability in Schwarzschild-like backgrounds are investigated. For these space-times the equations of motion admit solutions representing circular orbits with particles spins being constant and normal to the plane of orbits. For the de Sitter background the orbits are always stable with particle velocity and momentum being co-linear along them. The world-line deviation equations for particles of the same spin-to-mass ratios are solved and the resulting deviation vectors are used to study the stability of orbits. It is shown that the orbits are stable against radial perturbations. The general criterion for stability against normal perturbations is obtained. Explicit calculations are performed in the case of the Schwarzschild space-time leading to the conclusion that the orbits are stable.
eps figures, submitted to General Relativity and Gravitation
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Cited by in corpus (10)
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- Mathisson-Papapetrou-Dixon equations in the Schwarzschild and Kerr backgrounds
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- Spinning and Spinning Deviation Equations for Special Types of Gauge Theories of Gravity
- The precession of particle spin in spherical symmetric spacetimes