Asymptotic quasinormal modes of string-theoretical -dimensional black holes
arXiv:2105.02616 · doi:10.1007/JHEP08(2021)078
Abstract
We compute the quasinormal frequencies of -dimensional spherically symmetric black holes with leading string corrections for tensorial gravitational perturbations in the highly damped regime. We solve perturbatively the master differential equation and we compute the monodromies of the master perturbation variable (analytically continued to the complex plane) in different contours, in order to obtain the quasinormal mode spectra. We proceed analogously for the quasinormal modes of test scalar fields. Differently than in Einstein gravity, we obtain distinct results for the two cases.
31 pages, 4 figures. v2: references added; published version
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- The isospectrality of asymptotic quasinormal modes of large Gauss-Bonnet d-dimensional black holes
- Singularities of regular black holes and the monodromy method for asymptotic quasinormal modes
- Quasinormal modes of a charged loop quantum black hole
- A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric
- Greybody factors of string-corrected d-dimensional black holes
- WKB method and quasinormal modes of string-theoretical d-dimensional black holes