Analytic treatment of black-hole gravitational waves at the algebraically special frequency
Alec Maassen van den Brink

TL;DR
This paper analyzes the special frequency solutions of black-hole wave equations, revealing unique properties and their implications for understanding black-hole perturbations and mode behavior.
Contribution
It provides an exact solution at the algebraically special frequency, clarifies the physical significance of SUSY relationships, and explains the nature of modes and transmission at this frequency.
Findings
No quasinormal or total-transmission modes at the special frequency for RWE.
The special frequency exhibits a cancellation of divergences and branch-cut discontinuity vanishing.
Finite rotation makes modes totally transmitting, clarifying Schwarzschild limit singularity.
Abstract
We study the Regge-Wheeler and Zerilli equations (RWE and ZE) at the `algebraically special frequency' , where these equations admit an exact solution (elaborated here), generating the SUSY relationship between them. The physical significance of the SUSY generator and of the solutions at in general is elucidated as follows. The RWE has no (quasinormal or total-transmission) modes at all; however, is nonetheless `special' in that (a) for the outgoing wave into the horizon one has a `miraculous' cancellation of a divergence expected due to the exponential potential tail, and (b) the branch-cut discontinuity at vanishes in the outgoing wave to infinity. Moreover, (a) and (b) are related. For the ZE, its only mode is the-inverse-SUSY generator, which is at the same time a quasinormal mode_and_ a total-transmission mode propagating to infinity. The…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
