Magnetized particle motion around non-Schwarzschild black hole immersed in an external uniform magnetic field

2016 ◽  
Vol 361 (9) ◽  
Author(s):  
J. R. Rayimbaev
Keyword(s):  
Magnetic Field ◽  
Black Hole ◽  
Particle Motion ◽  
Uniform Magnetic Field ◽  
Schwarzschild Black Hole ◽  
External Uniform Magnetic Field

scholarly journals ENERGY ASSOCIATED WITH SCHWARZSCHILD BLACK HOLE IN A MAGNETIC UNIVERSE

2000 ◽  
Vol 15 (19) ◽  
pp. 2979-2986 ◽  
Author(s):  
S. S. XULU
Keyword(s):  
Magnetic Field ◽  
Black Hole ◽  
Uniform Magnetic Field ◽  
Relativistic Effect ◽  
Rest Mass ◽  
Mass Energy ◽  
Schwarzschild Black Hole ◽  
General Relativistic ◽  
The Magnetic Field ◽  
General Relativistic Effect

In this paper we obtain the energy distribution associated with the Ernst space–time (geometry describing Schwarzschild black hole in Melvin's magnetic universe) in Einstein's prescription. The first term is the rest-mass energy of the Schwarzschild black hole, the second term is the classical value for the energy of the uniform magnetic field and the remaining terms in the expression are due to the general relativistic effect. The presence of the magnetic field is found to increase the energy of the system.

scholarly journals MAGNETIZED PARTICLE MOTION AROUND BLACK HOLE IN BRANEWORLD

2011 ◽  
Vol 26 (06) ◽  
pp. 399-408 ◽  
Author(s):  
O. G. RAHIMOV
Keyword(s):  
Magnetic Field ◽  
Black Hole ◽  
Effective Potential ◽  
Particle Motion ◽  
Uniform Magnetic Field ◽  
Radial Motion ◽  
Circular Orbits ◽  
Spinning Particle ◽  
Jacobi Formalism

We investigate the motion of a magnetized particle orbiting around a black hole in braneworld immersed in asymptotically uniform magnetic field. The influence of brane parameter on effective potential of the radial motion of magnetized spinning particle around the braneworld black hole using Hamilton–Jacobi formalism is studied. It is found that circular orbits for photons and slowly moving particles may become stable near r = 3M. It was argued that the radii of the innermost stable circular orbits are sensitive on the change of brane parameter. Similar discussion without Weil parameter has been considered by de Felice et al. in Refs. 1 and 2.

scholarly journals General-Relativistic MHD Simulation of Jets from a Geometrically Thin Accretion Disk Around a Schwarzschild Black Hole

2000 ◽  
Vol 195 ◽  
pp. 373-374
Author(s):  
S. I. Aoki ◽  
S. Koide ◽  
K. Shibata ◽  
T. Kudoh
Keyword(s):  
Magnetic Field ◽  
Black Hole ◽  
Accretion Disk ◽  
Uniform Magnetic Field ◽  
Strong Dependence ◽  
Lorentz Factor ◽  
Schwarzschild Black Hole ◽  
Mhd Simulation ◽  
General Relativistic ◽  
Jet Velocities

We have performed a 2.5D, nonsteady, general-relativistic MHD simulation. Initially, we assumed a uniform magnetic field, a geometrically thin accretion disk rotating at Keplerian velocity, and a hydrostatic corona around a Schwarzschild black hole. We have investigated the formation mechanism of gas-pressure driven jets expected by Koide et al. and found the strong dependence of jet velocities Lorentz factor of jets) on the ratio of the density of the accretion disk to that of the corona (ρd/ρc), where γ2j - γj ∝ (ρd/ρc)0.75.

Magnetized particle motion and acceleration around a Schwarzschild black hole in a magnetic field

2014 ◽  
Vol 89 (8) ◽  
pp. 084008 ◽  
Author(s):  
Ahmadjon Abdujabbarov ◽  
Bobomurat Ahmedov ◽  
Ozodbek Rahimov ◽  
Umar Salikhbaev
Keyword(s):  
Magnetic Field ◽  
Black Hole ◽  
Particle Motion ◽  
Schwarzschild Black Hole
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