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Charged Nariai Black Holes With a Dilaton

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arxiv gr-qc/9608053 v1 pith:P52MN2HW submitted 1996-08-22 gr-qc hep-th

Raphael Bousso (DAMTP , Cambridge) This is my paper · ORCID
classification gr-qchep-th
keywords blackchargeddilatonholesnariaisolutionsdilatonictheories
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The Reissner-Nordstrom-de Sitter black holes of standard Einstein-Maxwell theory with a cosmological constant have no analogue in dilatonic theories with a Liouville potential. The only exception are the solutions of maximal mass, the Charged Nariai solutions. We show that the structure of the solution space of the Dilatonic Charged Nariai black holes is quite different from the non-dilatonic case. Its dimensionality depends on the exponential coupling constants of the dilaton. We discuss the possibility of pair creating such black holes on a suitable background. We find conditions for the existence of Charged Nariai solutions in theories with general dilaton potentials, and consider specifically a massive dilaton.

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Cited by 4 Pith papers

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

  1. The Fate of Nucleated Black Holes in de Sitter Quantum Gravity

    hep-th 2026-05 unverdicted novelty 6.0 of 10

    Nucleated maximal-mass black holes in de Sitter space undergo thermal Hawking evaporation in smooth quantum states and return fully to the empty de Sitter vacuum.

  2. Semiclassical decay of de Sitter space into black holes with vortex-deformed horizons

    hep-th 2026-06 unverdicted novelty 5.0 of 10

    De Sitter space decays into vortex-dressed black holes via a regular Euclidean instanton that generalizes the Nariai solution, with rates organized by topological charge of the vortices.

  3. Quasinormal frequencies in Reissner-Nordstr\"om de Sitter black holes: constraints from space-time and scalar field parameters

    gr-qc 2025-01 conditional novelty 4.0 of 10

    For charged, massive scalar fields around Reissner-Nordström de Sitter black holes, the effective potential has a single barrier for ℓ≥1, and the critical mass below which damping is anomalous is ℓ-independent for zer...

  4. A note on Strong Cosmic Censorship and its violation in Reissner-Nordstr\"om de Sitter black hole space-times

    gr-qc 2025-01 conditional novelty 4.0 of 10

    A WKB-based scan of quasinormal mode decay rates shows Strong Cosmic Censorship is violated in a region of the Reissner-Nordström de Sitter parameter space near extremality.

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