On Properties of Vacuum Axial Symmetric Spacetime of Gravitomagnetic Monopole in Cylindrical Coordinates
arXiv:gr-qc/0608012 · doi:10.1007/s10714-006-0266-5
Abstract
We investigate general relativistic effects associated with the gravitomagnetic monopole moment of gravitational source through the analysis of the motion of test particles and electromagnetic fields distribution in the spacetime around nonrotating cylindrical NUT source. We consider the circular motion of test particles in NUT spacetime, their characteristics and the dependence of effective potential on the radial coordinate for the different values of NUT parameter and orbital momentum of test particles. It is shown that the bounds of stability for circular orbits are displaced toward the event horizon with the growth of monopole moment of the NUT object. In addition, we obtain exact analytical solutions of Maxwell equations for magnetized and charged cylindrical NUT stars.
arXiv comment16 pages, 3 figures, 1 table
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- Quantum Interference Effects in Slowly Rotating NUT Space-time
- External Electromagnetic Fields of a Slowly Rotating Magnetized Star with Gravitomagnetic Charge
- Observational constraints on the Kerr and its several single-parameter modified spacetimes using quasi-periodic oscillation data