Quasinormal modes of self-dual black holes in loop quantum gravity
arXiv:2204.03259 · doi:10.1103/PhysRevD.106.024052
Abstract
We study the evolution of a test scalar field on the background geometry of a regular loop quantum black hole (LQBH) characterized by two loop quantum gravity (LQG) correction parameters, namely, the polymeric function and the minimum area gap. The calculations of quasinormal frequencies in asymptotically flat spacetime are performed with the help of higher-order WKB expansion and related Padé approximants, the improved asymptotic iteration method (AIM), and time-domain integration. The effects of free parameters of the theory on the quasinormal modes are studied and deviations from those of the Schwarzschild BHs are investigated. We show that the LQG correction parameters have opposite effects on the quasinormal frequencies and the LQBHs are dynamically stable.
arXiv comment15 pages, 6 captioned figures, and 16 tables. Comments are welcome; V2: Minor changes to match published version, references added
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