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Black hole shadow of a rotating scale--dependent black hole

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arxiv 1906.06990 v4 pith:KRNQ7MO5 submitted 2019-06-17 gr-qc

Ernesto Contreras , Ángel Rincón , Grigoris Panotopoulos , Pedro Bargueño , Benjamin Koch This is my paper · ORCID
classification gr-qc
keywords blackholerotatingscale--dependentshadowsolutionalgorithmbesides
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In this work, starting from a spherically symmetric scale--dependent black hole, a rotating solution is obtained by following the Newman--Janis algorithm without complexification. Besides studying the horizon, the static conditions and causality issues of the rotating solution, we get and discuss the shape of its shadow.

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Cited by 3 Pith papers

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

  1. Quasinormal modes of Bonanno-Reuter black holes via the Spectral Method

    gr-qc 2026-07 accept novelty 6.0 of 10

    Spectral Method yields the complete QNM spectrum (fundamentals, overtones, overdamped modes) of the Bonanno-Reuter black hole, missed by prior WKB analyses.

  2. On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows

    gr-qc 2024-11 conditional novelty 5.0 of 10

    The authors introduce two new regular black hole metrics from nonlinear electrodynamics and two Limiting Curvature Condition versions, with numerical results for stability, shadows, and quasinormal modes.

  3. Minimal Geometric Deformation in a Reissner-Nordstr\"om background

    gr-qc 2019-09 conditional novelty 4.0 of 10

    New exact Reissner-Nordström black hole solutions are built via minimal geometric deformation with a linear equation of state in the added source.

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