Perturbations and Quasinormal Modes of the Dirac Field in Effective Quantum Gravity
arXiv:2409.01561 · doi:10.1016/j.aop.2025.170046
Abstract
Recently, two models of quantum-corrected Schwarzschild-like black holes were developed within Effective Quantum Gravity, and the spectra of bosonic perturbations have been analyzed in several recent studies. In this work, we investigate the quasinormal modes of a massless Dirac field perturbations around these black holes. By employing the higher-order WKB method and time-domain integration, we achieved consistency between the two approaches within their common range of validity. This concordance enables us to distinguish the two quantum-corrected black hole models from each other and from their Schwarzschild limit through their quasinormal spectra. In addition, we find approximate analytic expressions for quasinormal modes and grey-body factors in the form of expansion beyond the eikonal limit.
arXiv comment20 pages, 2 figures, revised version, the discussion is extended, references are added
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