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de Sitter black hole with a conformally coupled scalar field in four dimensions

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arxiv hep-th/0205319 v2 pith:FOHWE5T5 submitted 2002-05-31 hep-th gr-qc

Cristian Martinez , Ricardo Troncoso , Jorge Zanelli This is my paper · ORCID
classification hep-thgr-qc
keywords fieldscalarblackcosmologicalcoupledholesolutionbecomes
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A four-dimensional black hole solution of the Einstein equations with a positive cosmological constant, coupled to a conformal scalar field, is given. There is a curvature singularity at the origin, and scalar field diverges inside the event horizon. The electrically charged solution, which has a fixed charge-to-mass ratio is also found. The quartic self-interacting coupling becomes bounded in terms of Newton's and the cosmological constants.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 181 citations worldwide. Full citation record

  1. Shadow constraints of charged black hole with scalar hair and gravitational waves from extreme mass ratio inspirals

    gr-qc 2025-06 conditional novelty 5.0 of 10

    EHT shadow data constrain the EMCS black hole charge and scalar hair to about 0.1 and 0.01 levels, while LISA EMRI waveforms could reach 0.01 and 0.0001 levels.

  2. A Universal Smarr Formula via Coupling Constants

    gr-qc 2025-11 conditional novelty 4.0 of 10

    Coupling constants promoted to conserved charges make the Smarr formula work for black holes in NMG, Horndeski, MTZ, and higher-curvature gravity.

  3. A new rotating axionic AdS$_4$ black hole dressed with a scalar field

    hep-th 2025-04 unverdicted novelty 4.0 of 10

    A new axionically charged rotating AdS4 black hole solution with scalar field is presented, defined by a structural function and parameters, with thermodynamics derived via Euclidean method satisfying the first law.

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