An unknown branch of the total-transmission modes for the Kerr-geometry
Gregory B. Cook, Luke S. Annichiarico, Daniel J. Vickers

TL;DR
This paper uncovers new branches of total-transmission gravitational modes in Kerr black holes, revealing their properties, special cases where they coincide with quasinormal modes, and their asymptotic behaviors.
Contribution
It identifies previously unknown branches of total-transmission modes in Kerr geometry and analyzes their properties and conditions for mode coincidence with quasinormal modes.
Findings
Discovery of new purely imaginary mode branches
Modes approach -i∞ near Schwarzschild limit
Conditions for mode coincidence with quasinormal modes
Abstract
The gravitational modes of the Kerr geometry include both quasinormal modes and total-transmission modes. Sequences of these modes are parameterized by the angular momentum of the black hole. The quasinormal and total-transmission modes are usually distinct, having mode frequencies that are different at any given value of the angular momentum. But a discrete and countably infinite subset of the left-total-transmission modes are simultaneously quasinormal modes. Most of these special modes exist along previously unknown branches of the gravitational total-transmission modes. In this paper, we give detailed plots of the total-transmission modes for harmonic indices , with special emphasis given to the modes which all contain previously unknown branches. All of these unknown branches have purely imaginary mode frequencies. We find that as we approach the Schwarzschild…
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