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EFT Approach to Black Hole Scalarization and its Compatibility with Cosmic Evolution

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arxiv 2203.06030 v1 pith:A6OJRZF5 submitted 2022-03-11 gr-qc astro-ph.COhep-th

EFT Approach to Black Hole Scalarization and its Compatibility with Cosmic Evolution

classification gr-qc astro-ph.COhep-th
keywords scalarizationblackholecompatibilitycosmicactuallyaddressadmitting
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We address the issue of black hole scalarization and its compatibility with cosmic inflation and big bang cosmology from an effective field theory (EFT) point of view. In practice, using a well-defined and healthy toy model which (in part) has been broadly considered in the literature, we consider how higher-order theories of gravity, up to cubic operators in Riemann curvature, fit within this context. Interestingly enough, we find that already at this minimal level, there is a non-trivial interplay between the Wilson coefficients which are otherwise completely independent, constraining the parameter space where scalarization may actually occur. Conclusively, we claim that the EFT does exhibit black hole scalarization, remaining compatible with the inflationary paradigm, and admitting General Relativity as a cosmological attractor.

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Cited by 1 Pith paper

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  1. Thermodynamic Phase Transitions in Einstein-Maxwell-Scalar-Gauss-Bonnet Gravity

    hep-th 2026-04 unverdicted novelty 6.0

    Scalarization in EMSGB gravity enables free-energy crossings between scalarized and Reissner-Nordström black holes, producing up to three phase transitions whose order changes with coupling strength.