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Black Holes With Many Horizons in the Theories of Nonlinear Electrodynamics

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arxiv 2106.13486 v3 pith:QPGXVZVF submitted 2021-06-25 gr-qc

classification gr-qc
keywords blackholeshorizonselectrodynamichorizonmanynonlineartheories
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In this article, we construct exact black hole solutions with many horizons (more than number two) in the Einstein-nonlinear electrodynamic theories. In particular, we acquire the explicit expression of nonlinear electrodynamic Lagrangian for the 3-horizon black holes. Then we make the investigations of 3-horizon black holes on the horizons, the null and timelike geodesics, the Love numbers and the thermodynamics.

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Cited by 4 Pith papers

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

  1. Black holes and causal nonlinear electrodynamics

    hep-th 2026-01 accept novelty 7.0 of 10

    Causal nonlinear electrodynamics forces a singular center and at most three phases for RN-asymptotic black holes, with monotonicity proofs showing reduced mass and entropy for extreme dyonic cases.

  2. Taming the Aretakis instability: extremal black holes with multi-degenerate horizons

    gr-qc 2026-04 unverdicted novelty 6.0 of 10

    Black holes with infinitely degenerate horizons are proposed to be stable against Aretakis instability, potentially serving as end states.

  3. Scalarization of Einstein-Euler-Heisenberg black hole with multiple horizons

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Stable, positive-mass scalarized EEH black holes exist only in an intermediate primary-scalar-charge window for low/cold horizons and above a lower bound for hot horizons.

  4. Topologically equivalent yet radiatively distinct orbits in EMRI system

    gr-qc 2026-04 unverdicted novelty 5.0 of 10

    In dyonic black holes, periodic orbits with identical rotation numbers but spanning different curvature regions generate radiatively distinct gravitational waveforms in EMRIs.

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