Abstract
In this paper we discuss the particle trajectories in a uniform magnetic field superimposed on Kerr geometry. The rotation axis of the Kerr black hole makes an angle with the asymptotic magnetic field. We find that the particle is trapped for suitable initial conditions.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Chakraborty, D.K. and Prasanna, A.R.: 1982, Pramana J. Phys. 19, 141.
King, A.R.: 1976, Phys. Lett. 56A, 339.
King, A.R. and Lasota, J.P.: 1977, Astron. Astrophys. 58, 175.
Kinnersley, W.J.: 1969, J. Math. Phys. 10, 1195.
Prasanna, A.R.: 1991, Prasanna 36, 445.
Prasanna, A.R. and Vishveshwara, C.V.: 1978, Pramana J. Phys. 11, 359.
Prasanna, A.R. and Sengupta, S.: 1994, Phys. Lett. A 193, 25.
Wald, R.M.: 1974, Phys. Rev. D 10, 1680.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Mishra, K., Chakraborty, D. Orbits of a Charged Particle in a Skew Uniform Magnetic Field on Kerr Back Ground Geometry. Astrophysics and Space Science 260, 441–454 (1998). https://doi.org/10.1023/A:1001701802525
Issue Date:
DOI: https://doi.org/10.1023/A:1001701802525