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Double instability of Schwarzschild black holes in Einstein-Weyl-scalar theory

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arxiv 2307.04060 v1 pith:KFWD4HT5 submitted 2023-07-08 gr-qc hep-th

classification gr-qchep-th
keywords blackschwarzschildtheoryholeholesinstabilitylinearizedmass
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abstract

We study the stability of Schwarzschild black hole in Einstein-Weyl-scalar (EWS) theory with a quadratic scalar coupling to the Weyl term. Its linearized theory admits the Lichnerowicz equation for Ricci tensor as well as scalar equation. The linearized Ricci-tensor carries with a regular mass term ($m^2_2$), whereas the linearized scalar has a tachyonic mass term ($-1/m^2_2$). It turns out that the double instability of Schwarzschild black hole in EWS theory is given by Gregory-Laflamme and tachyonic instabilities. In the small mass regime of $m_2<0.876$, the Schwarzschild black hole becomes unstable against Ricci-tensor perturbations, while tachyonic instability is achieved for $m_2<1.174$. The former would provide a single branch of scalarized black holes, whereas the latter would induce infinite branches of scalarized black holes.

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  1. 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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