In this paper we study the trajectories of test particles in a geometry that is the nonlinear electromagnetic generalization of the Reissner-Nordstrom black hole. The solution was originally derived by Garcia, Salazar and Plebanski (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-Nordstrom solution. [References: 16]
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机译：在本文中，我们研究几何中测试粒子的轨迹，这是Reissner-Nordstrom黑洞的非线性电磁概括。该解决方案最初是由Garcia，Salazar和Plebanski（1984 Nuovo Cimento 84 65-90）派生的。所研究的时空是一个Einstein-Born-Infeld解，在常规事件视界之外是非奇异的，具有三个参数：质量M，电荷Q和与原点电场强度有关的Born-Infeld参数b。渐近地，这是一个Reissner-Nordstrom解。 [参考：16]
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