Angular and radial stabilities of spontaneously scalarized black holes in the presence of scalar-Gauss-Bonnet couplings
arXiv:2403.10048 · doi:10.1103/PhysRevD.109.104057
Abstract
We study the linear stability of spontaneously scalarized black holes (BHs) induced by a scalar field coupled to a Gauss-Bonnet (GB) invariant . For the scalar-GB coupling , where and are constants, we first show that there are no angular Laplacian instabilities of even-parity perturbations far away from the horizon for large multipoles . The deviation of angular propagation speeds from the speed of light is largest on the horizon, whose property can be used to put constraints on the model parameters. For , the region in which the scalarized BH is subject to angular Laplacian instabilities can emerge. Provided that and , where is the field value on the horizon with a unit of the reduced Planck mass , there are scalarized BH solutions satisfying all the linear stability conditions throughout the horizon exterior. We also study the stability of spontaneously scalarized BHs in scalar-GB theories with a nonminimal coupling , where is a positive constant and is a Ricci scalar. As the amplitude of the field on the horizon approaches an upper limit , one of the squared angular propagation speeds enters the instability region . So long as is smaller than a maximum value determined for each in the range , however, the scalarized BHs are linearly stable in both angular and radial directions.
arXiv comment21 pages, 5 figures
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