The equatorial motion of the charged test particles in Kerr-Newman-Taub-NUT spacetime
arXiv:1702.02760 · doi:10.1007/s10714-019-2569-3
Abstract
In this work, we perform a detailed analysis of the equatorial motion of the charged test particles in Kerr-Newman-Taub-NUT spacetime. By working out the orbit equation in the radial direction, we examine possible orbit types. We investigate the conditions for existence of bound orbits in causality-preserving region as well as the conditions for existence of circular orbits for charged and uncharged particles. We also study the effect of NUT parameter on Newtonian orbits. Finally, we give exact analytical solutions of equations of equatorial motion for a charged test particle.
title changed , revised version
References in corpus (10)
- Geodesics of electrically and magnetically charged test particles in the Reissner-Nordström space-time: analytical solutions
- Equatorial circular orbits in the Kerr-de Sitter spacetimes
- Analytic treatment of complete and incomplete geodesics in Taub-NUT space-times
- Particle Acceleration on the Background of the Kerr-Taub-NUT Spacetime
- Penrose Process in Kerr-Taub-NUT Spacetime
- Particle Motion and Electromagnetic Fields of Rotating Compact Gravitating Objects with Gravitomagnetic Charge
- Does the gravitomagnetic monopole exist? A clue from a black hole x-ray binary
- On some novel features of the Kerr-Newman-NUT Spacetime
- Rotating Spacetimes with Asymptotic Non-Flat Structure and the Gyromagnetic Ratio
- Observers in Kerr spacetimes: the ergoregion on the equatorial plane
Cited by in corpus (5)
- Dynamics and Fundamental Frequencies of Test Particles Orbiting Kerr-Newman-NUT-Kiselev Blacks Hole in Rastall Gravity
- Dynamics of Charged and Rotating NUT Black Holes in Rastall Gravity
- Rotating traversable wormholes in Einstein-Maxwell theory
- Rotating and charged Taub-NUT-(A)dS spacetimes on a 3-brane
- Geodesic structure of a noncommutative black hole