A model problem for quasinormal ringdown on asymptotically flat or extremal black holes
Dejan Gajic, Claude Warnick

TL;DR
This paper introduces a new definition of quasinormal frequencies for wave equations near black hole horizons, proves their spectral properties, and relates them to existing computational methods, advancing understanding of wave behavior in extreme spacetime geometries.
Contribution
It proposes a novel eigenvalue-based definition of quasinormal frequencies applicable to non-analytic potentials and establishes their spectral properties and relation to existing computational methods.
Findings
QNF spectrum is discrete in a specified complex region.
Scattering resolvent is meromorphic in a certain sector.
Continued fraction method computes valid QNFs under the new definition.
Abstract
We consider a wave equation with a potential on the half-line as a model problem for wave propagation close to an extremal horizon, or the asymptotically flat end of a black hole spacetime. We propose a definition of quasinormal frequencies (QNFs) as eigenvalues of the generator of time translations for a null foliation, acting on an appropriate (Gevrey based) Hilbert space. We show that this QNF spectrum is discrete in a subset of which includes the region Re, Im for any and some . As a corollary we establish the meromorphicity of the scattering resolvent in a sector arg for some , and show that the poles occur only at quasinormal frequencies according to our definition. This result applies in situations where the method of complex scaling cannot be directly applied, as our…
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.
