Abstract
We study the effect of an external magnetic field on the stability of circular motion of charged particles in the equatorial plane of a five-dimensional rotating black hole. Using the Hamilton–Jacobi formalism, we derive the effective potential for the radial motion of test particles around a five-dimensional magnetized Myers–Perry black hole. We show that there exist stable circular orbits in equatorial planes in the background of this metric.
Keywords
Physics
Classical mechanics
Circular orbit
Rotating black hole
Black hole (networking)
Charged black hole
Magnetic field
Formalism (music)
Charged particle
Spin-flip
Circular motion
Quantum electrodynamics
Gravitation
Astrophysics
Schwarzschild radius
Angular momentum
Quantum mechanics
Ion
Galaxy
Subject Areas
Astrophysical Phenomena and Observations
·Astronomy and Astrophysics ·Physical Sciences
Pulsars and Gravitational Waves Research
·Astronomy and Astrophysics ·Physical Sciences
Black Holes and Theoretical Physics
·Nuclear and High Energy Physics ·Physical Sciences
Citations by Year
2021: 1
2022: 1
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