Charged spinning particles on circular orbits in the Reissner-Nordström spacetime
arXiv:1408.4272 · doi:10.1142/S0218271805007358
Abstract
The behaviour of charged spinning test particles moving along circular orbits in the equatorial plane of the Reissner-Nordström spacetime is studied in the framework of the Dixon-Souriau model completed with standard choices of supplementary conditions. The gravitomagnetic " clock effect", i.e. the delay in the arrival times of two oppositely circulating particles as measured by a static observer, is derived and discussed in the cases in which the particles have equal/opposite charge and spin, the latter being directed along the -axis.
arXiv comment19 pages, 4 figures; published version. arXiv admin note: text overlap with arXiv:gr-qc/0410082
References in corpus (4)
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- Dynamics of quadrupolar bodies in a Schwarzschild spacetime
- Highly relativistic spinning particle in the Schwarzschild field: Circular and other orbits
- Stability of circular orbits of spinning particles in Schwarzschild-like space-times
- Particle dynamics and deviation effects in the field of a strong electromagnetic wave
- Spinning charged test particle dynamics around a Schwarzschild black hole embedded in a homogeneous magnetic field