2014/12/11 by Román Linares, Marco Maceda, Daniel Martínez-Carbajal
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Einstein #Geology #Gravitation #Motion (physics) #Particle (ecology) #Physics #Quantum mechanics #Spacetime #Test particle #Theoretical physics #gr-qc
paper · pdf · doi:10.1103/physrevd.92.024052
published as Phys. Rev. D 92, 024052 (2015) · 10 pages, 8 figures
arxiv created 2014/12/11 · openalex publication_date 2015/07/30 · arxiv updated 2015/08/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In this paper, we review the classification of the orbits followed by charged massive test particles in the gravitational background of the black hole solutions of Einstein-Born-Infeld spacetime. Even though some features are quite similar to those of Reissner-Nordstr"om spacetime, there are also important differences, particularly those related to the effective potential governing the orbital motion. Explicit solutions involving Weierstrass functions are given for a pair of specific scenarios.