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Charged Black Hole Solutions in Einstein-Born-Infeld gravity with a Cosmological constant

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arxiv hep-th/0306120 v3 pith:HRMNW7CH submitted 2003-06-12 hep-th

Sharmanthie Fernando , Don Krug This is my paper · ORCID
classification hep-th
keywords blacksolutionschargedconstantcosmologicalgravityholeconstruct
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We construct black hole solutions to Einstein-Born-Infeld gravity with a cosmological constant. Since an elliptic function appears in the solutions for the metric, we construct horizons numerically. The causal structure of these solutions differ drastically from their counterparts in Einstein-Maxwell gravity with a cosmological constant. The charged de-Sitter black holes can have up to three horizons and the charged anti-de Sitter black hole can have one or two depending on the parameters chosen.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  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.

  2. Properties of black holes in non-linear electrodynamics

    hep-th 2026-04 unverdicted novelty 5.0 of 10

    Nonlinear electrodynamics black holes with non-monotonic lapse functions admit stable light rings and trapped near-horizon photon orbits that generate additional longer-lived quasinormal mode branches.

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