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Rotating charged Black Holes in Einstein-Born-Infeld theories and their ADM mass

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arxiv gr-qc/0603066 v2 pith:YEFBFA7O submitted 2006-03-16 gr-qc hep-th

Diego Julio Cirilo-Lombardo This is my paper · ORCID
classification gr-qchep-th
keywords blackholemassrotatingsolutionanalyzedangularbeen
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In this work, the solution of the Einstein equations for a slowly rotating black hole with Born-Infeld charge is obtained. Geometrical properties and horizons of this solution are analyzed. The conditions when the ADM mass (as in the nonlinear static cases) and the ADM angular momentum of the system have been modified by the non linear electromagnetic field of the black hole, are considered.

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  1. Rotating Black Holes in Einstein-Born-Infeld Theory

    gr-qc 2025-07 conditional novelty 7.0 of 10

    Exact rotating charged Einstein-Born-Infeld black holes are constructed numerically; they show charge-dependent extremal or naked-singularity endpoints, gyromagnetic ratio above 2, and ISCO radii below Kerr-Newman values.

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