Axial perturbations of hairy black holes in generalised scalar-tensor theories

Andrea Maselli; Caio F. B. Macedo; Georgios Antoniou; Thomas P. Sotiriou

Axial perturbations of hairy black holes in generalised scalar-tensor theories

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arxiv 2404.02479 v1 pith:JTXQCKHV submitted 2024-04-03 gr-qc hep-th

Georgios Antoniou , Caio F. B. Macedo , Andrea Maselli , Thomas P. Sotiriou This is my paper · ORCID

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Gravitational wave observations can test the validity of General Relativity (GR) in the strong field regime. Certain classes of scalar-tensor theories indeed predict that compact objects can exhibit significant deviations from their GR counterparts. Here we explore the quasinormal modes of axial perturbations in spherically symmetric black holes in three such classes: (i) dilatonic black holes with an additional scalar-Ricci coupling (EdRGB), (ii) spontaneously scalarized black holes (EsRGB) with a quadratic coupling to the Gauss-Bonnet invariant and the Ricci scalar, (iii) spontaneously scalarized black holes with a quadratic and a quartic coupling to the Gauss-Bonnet invariant.

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Gravitational quasinormal modes of black holes in quadratic gravity
gr-qc 2024-12 conditional novelty 7.0 of 10

Axial gravitational quasinormal modes are computed for Schwarzschild and hairy black holes in Einstein-Weyl gravity, showing stability and new massive spin-2 tones.

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