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Rotating Black Holes in Higher Order Gravity

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arxiv 1903.05519 v1 pith:UC77RDA2 submitted 2019-03-13 hep-th astro-ph.COgr-qc

Christos Charmousis , Marco Crisostomi , Ruth Gregory , Nikolaos Stergioulas This is my paper · ORCID
classification hep-thastro-ph.COgr-qc
keywords blackhairholecosmologicalgravitationalgravityrotatingstealth
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We develop a new technique for finding black hole solutions in modified gravity that have "stealth" hair, i.e., hair whose only gravitational effect is to tune the cosmological constant. We consider scalar-tensor theories in which gravitational waves propagate at the speed of light, and show that Einstein metrics can be painted with stealth hair provided there exists a family of geodesics always normal to spacelike surfaces. We also present a novel scalar-dressed rotating black hole that has finite scalar field at both the black hole and cosmological event horizons.

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  1. Test-Field vs Physical Quasi-Normal Modes in Scalar-Tensor Theories

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Test-field QNM spectra of BCL black holes deviate strongly from physical axial gravitational QNM spectra at high overtones, while fundamental modes remain close.

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