Spin precession along circular orbits in the Kerr spacetime: the Frenet-Serret description
arXiv:1408.4278 · doi:10.1088/0264-9381/23/10/003
Abstract
The circular motion of spinning massive test particles in the equatorial plane of a rotating black hole is investigated in the case in which the components of the spin tensor are allowed to vary along the orbit.
18 pages, 1 figure; published version. arXiv admin note: text overlap with arXiv:gr-qc/0506017
Cited by in corpus (9)
- Dynamics of Extended Spinning Masses in a Gravitational Field
- Spin-geodesic deviations in the Schwarzschild spacetime
- Gyroscope precession along bound equatorial plane orbits around a Kerr black hole
- Spin-geodesic deviations in the Kerr spacetime
- Dynamics of quadrupolar bodies in a Schwarzschild spacetime
- Spinning particle orbits around a black hole in an expanding background
- Gyroscope precession along unbound equatorial plane orbits around a Kerr black hole
- The Raychaudhuri equation for spinning test particles
- Accelerated orbits in black hole fields: the static case