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Scalarized black holes in the Einstein-Maxwell-scalar theory with a quasi-topological term

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arxiv 2011.09665 v2 pith:V4KB4ASR submitted 2020-11-18 gr-qc hep-th

classification gr-qchep-th
keywords blackholestermquasi-topologicalscalarizedcdotschargedeinstein-maxwell-scalar
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abstract

We investigate the Einstein-Maxwell-scalar theory with a quasi-topological term. Considering exponential couplings to Maxwell term, quasi-topological term, and both terms, we obtain three sets of infinite scalarized charged black holes by taking into account tachyonic instability of dyonic Reissner-Nordstr\"{o}m black hole. Each set of infinite scalarized charged black holes is classified by the number of $n=0,1,2,\cdots$, where $n=0$ is called the fundamental black hole and $n=1,2,\cdots$ denote the $n$-excited black holes. All $n=0$ black holes are stable against the radial perturbation, while all $n=1,2$ black holes are unstable.

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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. Polar perturbations of dilaton-Euler-Heisenberg black holes

    gr-qc 2026-01 conditional novelty 6.0 of 10

    Every computed fundamental quasinormal frequency for polar metric-dilaton perturbations of dilaton-Euler-Heisenberg black holes has a negative imaginary part, meaning the modes are damped, with ε=+1 and ε=−1 differing...

  2. Shadow and geometric scattering analysis of a new black hole with magnetic charge

    gr-qc 2025-05 reject novelty 4.0 of 10

    The paper derives a magnetically charged black hole metric with a tiny q^6/r^10 correction and claims EHT constraints on the charge, but its naked-singularity branches still have horizons.

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