Massive scalar field perturbation on Kerr black holes in dynamical Chern-Simons gravity

Abstract

We study massive scalar field perturbation on Kerr black holes in dynamical Chern-Simons gravity by performing a $(2+1)$-dimensional simulation. Object pictures of the wave dynamics in time domain are obtained. The tachyonic instability is found to always occur for any nonzero black hole spin and any scalar field mass as long as the coupling constant exceeds a critical value. The presence of the mass term suppresses or even quenches the instability. The quantitative dependence of the onset of the tachyonic instability on the coupling constant, the scalar field mass and the black hole spin is given numerically.

arXiv commentv1:14 pages, 4 figures;v2: minor modification, refs added. v3: minor modification, more refs, match published version

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Cited by in corpus (8)

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• Spin-Charge induced spontaneous scalarization of Kerr-Newman black holes
• Magnetic-induced Spontaneous Scalarization in Dynamcial Chern-Simons Gravity
• Spin-induced scalarization of Kerr-Newman black holes in Einstein-Maxwell-scalar theory
• Black hole scalarizations induced by parity violations
• Tachyonic instability and spontaneous scalarization in parameterized Schwarzschild-like black holes
• Tachyonic Instability of Reissner-Nordström-Melvin Black Holes in Einstein-Maxwell-Scalar Theory