Radiation emitted by relativistic particles moving in the vicinity of the Schwarzschild black hole, immersed in an external magnetic field

1978 ◽  
Vol 68 (1) ◽  
pp. 1-2 ◽  
Author(s):  
A.A. Sokolov ◽  
D.V. Galtsov ◽  
V.I. Petukhov
2005 ◽  
Vol 20 (14) ◽  
pp. 1077-1085 ◽  
Author(s):  
MARICEL AGOP ◽  
EUGEN RADU ◽  
REINOUD SLAGTER

The dilatonic Ernst solution describing a Schwarzschild black hole immersed in a background magnetic field is generalized by including a Liouville-type potential in the action principle. We prove that the thermodynamic properties of this new black hole dilaton solution are unaffected by an external magnetic field passing through it.


2002 ◽  
Vol 17 (34) ◽  
pp. 2277-2281 ◽  
Author(s):  
EUGEN RADU

We prove that the thermodynamic properties of a Schwarzschild black hole are unaffected by an external magnetic field passing through it. Apart from the background subtraction prescription, this result is also obtained by using a counterterm method.


1978 ◽  
Vol 21 (12) ◽  
pp. 1603-1605
Author(s):  
A. A. Sokolov ◽  
D. V. Gal'tsov ◽  
V. I. Petukhov

1989 ◽  
Vol 67 (10) ◽  
pp. 971-973
Author(s):  
K. D. Krori ◽  
J. C. Sarmah

In this paper, we present a study of the stable polar trajectories ([Formula: see text] = constant plane) of neutral test particles around a Schwarzschild black hole embedded in a magnetic field. We also show how the nature of these trajectories changes with the variation in the angular momentum of the test particle and the magnetic field parameter.


Sign in / Sign up

Export Citation Format

Share Document