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Conformally coupled theories and their deformed compact objects: from black holes, radiating spacetimes to eternal wormholes

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arxiv 2206.11013 v1 pith:ZY4IQAXI submitted 2022-06-22 gr-qc hep-th

classification gr-qchep-th
keywords scalartheoryasymptoticallyblackconformallycoupledeternalflat
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We study a higher order conformally coupled scalar tensor theory endowed with a covariant geometric constraint relating the scalar curvature with the Gauss-Bonnet scalar. It is a particular Horndeski theory including a canonical kinetic term but without shift or parity symmetry for the scalar. The theory also stems from a Kaluza-Klein reduction of a well defined higher dimensional metric theory. Properties of an asymptotically flat spherically symmetric black hole are analyzed, and new slowly rotating and radiating extensions are found. Through disformal transformations of the static configurations, gravitating monopole-like solutions and eternal wormholes are presented. The latter are shown to extract from spacetime possible naked singularities, yielding completely regular and asymptotically flat spacetimes.

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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. Thermodynamics of four-dimensional regular black holes with an infinite tower of regularized curvature corrections

    gr-qc 2025-05 conditional novelty 5.0 of 10

    Planar regular black holes from an infinite tower of higher-curvature corrections are thermodynamically indistinguishable from singular GR black holes, while spherical horizons may lift this degeneracy.

  2. The lack of influence of the scalar hair on the DC conductivity

    hep-th 2024-12 conditional novelty 4.0 of 10

    The DC conductivity of beyond-Horndeski axionic black holes is shown to be independent of the primary scalar hair parameter, depending only on horizon data and axion and charge parameters.

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