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arxiv: 1808.02609 · v2 · submitted 2018-08-08 · 🌀 gr-qc · hep-th

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Instability of Reissner-Nordstr\"{o}m black hole in Einstein-Maxwell-scalar theory

Yun Soo Myung , De-Cheng Zou
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classification 🌀 gr-qc hep-th
keywords blackreissner-nordstrholeeinstein-maxwell-scalarinstabilitytheoryappearanceclosely
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The scalarization of Reissner-Nordstr\"{o}m black holes was recently proposed in the Einstein-Maxwell-scalar theory. Here, we show that the appearance of the scalarized Reissner-Nordstr\"{o}m black hole is closely related to the Gregory-Laflamme instability of the Reissner-Nordstr\"{o}m black hole without scalar hair.

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Cited by 2 Pith papers

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

  1. Spin-Induced Nonlinear Scalarization of Kerr Black Holes in Einstein-scalar-Gauss-Bonnet Gravity

    gr-qc 2026-04 unverdicted novelty 7.0

    Kerr black holes in an EsGB model without linear instability undergo nonlinear scalarization above spin 0.5, existing in a finite low-mass high-spin wedge rather than a narrow band.

  2. Spin-charge induced scalarization of Kerr-Newman black holes in the Einstein-Maxwell-scalar theory with scalar potential

    gr-qc 2026-04 unverdicted novelty 6.0

    Kerr-Newman black holes in EMS theory with scalar potential scalarize for spins below a threshold set by charge, scalar mass, and coupling strength.