Geodesic structure of the Born-Infeld black hole

Details Geodesic structure of the Born-Infeld black hole Geodesic structure of the Born-Infeld black hole

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19..601b&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 4, pp. 601-612 (2002).

Physics

8

Scientific paper

In this paper we study the trajectories of test particles in a geometry that is the nonlinear electromagnetic generalization of the Reissner-Nordström black hole. The solution was originally derived by García, Salazar and Plebañski (1984 Nuovo Cimento 84 65-90). The studied spacetime is an Einstein-Born-Infeld solution, nonsingular outside a regular event horizon and characterized by three parameters: mass M, charge Q and the Born-Infeld parameter b related to the magnitude of the electric field at the origin. Asymptotically it is a Reissner-Nordström solution.

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