Energy-extraction processes from a Kerr black hole immersed in a magnetic field. II. The formalism

1984 ◽  
Vol 30 (8) ◽  
pp. 1625-1631 ◽  
Author(s):  
S. V. Dhurandhar ◽  
N. Dadhich
Galaxies ◽  
2020 ◽  
Vol 8 (4) ◽  
pp. 76
Author(s):  
Ahmadjon Abdujabbarov ◽  
Javlon Rayimbaev ◽  
Farruh Atamurotov ◽  
Bobomurat Ahmedov

In the present work we explored the dynamics of magnetized particles around the compact object in γ-spacetime in the presence of an external asymptotically-uniform magnetic field. The analysis of the circular orbits of magnetized particles around the compact object in the spacetime of a γ-object immersed in the external magnetic field has shown that the area of stable circular orbits of magnetized particles increases with the increase of γ-parameter. We have also investigated the acceleration of the magnetized particles near the γ-object and shown that the center-of-mass energy of colliding magnetized particles increases with the increase of γ-parameter. Finally, we have applied the obtained results to the astrophysical scenario and shown that the values of γ-parameter in the range of γ∈(0.5,1) can mimic the spin of Kerr black hole up to a≃0.85, while the magnetic interaction can mimic the γ-parameter at γ∈(0.8,1) and spin of a Kerr black hole up to a≃0.3.


Pramana ◽  
1985 ◽  
Vol 25 (2) ◽  
pp. 135-148 ◽  
Author(s):  
B R Iyer ◽  
C V Vishveshwara ◽  
P J Wiita ◽  
J J Goldstein

1983 ◽  
Vol 61 (8) ◽  
pp. 1192-1197 ◽  
Author(s):  
K. D. Krori ◽  
Sumita Chaudhury ◽  
S. Dowerah

We present here an investigation of the event horizon of a charged black hole embedded in a uniform magnetic field by studying the Gaussian curvature. It is shown that the Gauss–Bonnet theorem holds for this magnetized black hole and also for a magnetized Kerr black hole.


2003 ◽  
Vol 214 ◽  
pp. 87-90
Author(s):  
Shinji Koide

We have developed a numerical method for general relativistic magnetohydrodynamic simulations in Kerr space-time. The method is applied to the basic astrophysical problem of the Kerr black hole activity in the large-scale strong magnetic field. The numerical result shows that the magnetic field extracts the rotational energy of the black hole with negative energy-at-infinity and the torsional Alfven wave is induced from the ergosphere.


2018 ◽  
Vol 926 ◽  
pp. 83-94 ◽  
Author(s):  
Fen Long ◽  
Songbai Chen ◽  
Shangyun Wang ◽  
Jiliang Jing

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