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Born-Infeld black hole in the isolated horizon framework

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arxiv hep-th/0301254 v1 pith:EZ3KXDDN submitted 2003-01-31 hep-th

Nora Breton This is my paper · ORCID
classification hep-th
keywords blackholeborn-infeldframeworkhorizonisolatedmodelashtekar
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In this work we probe the Born-Infeld (BI) black hole in the isolated horizon framework. It turns out that the BI black hole is consistent with the heuristic model for colored black holes proposed by Ashtekar et al [(2001) Class.Quant.Grav. v. 18, 919-940]. The model points to the unstability of the BI black hole.

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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. Causality Constraints on Black Hole Thermodynamics in Nonlinear Electrodynamics

    hep-th 2025-05 conditional novelty 6.0 of 10

    Causality in nonlinear electrodynamics forces the entropy-to-mass-squared ratio of black holes to decrease with mass and the extremal mass-to-charge ratio to increase with charge.

  2. Mixed-state entanglement and phase transitions in Einstein-Born-Infeld massive gravity

    hep-th 2025-12 unverdicted novelty 4.0 of 10

    In Einstein-Born-Infeld massive gravity, the second temperature derivative of the entanglement-wedge cross-section tracks the metal-insulator crossover, all entanglement measures diagnose Hawking-Page transitions, and...

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