Modified Teukolsky formalism: Null testing and numerical benchmarking
Fawzi Aly, Mahmoud A. Mansour, Luis Lehner, Dejan Stojkovic, Dongjun Li, Pratik Wagle

TL;DR
This paper rigorously tests a modified Teukolsky formalism for black-hole ringdown predictions, validating its accuracy and consistency through null diagnostics and numerical methods, supporting its use in strong-field gravity tests.
Contribution
It introduces null diagnostics and numerical validation methods to verify the accuracy of the modified Teukolsky framework for gravitational wave predictions.
Findings
Null tests are passed across multiple multipoles and overtones.
Numerical approaches agree with benchmark values.
Framework validated for accurate strong-field gravity predictions.
Abstract
Next-generation gravitational-wave detectors will make black-hole ringdown an increasingly sensitive probe of small departures from General Relativity in the strong-field regime. This motivates obtaining high-precision predictions of gravitational effective field theory, as spectral shifts can be quite small. Here we perform a focused stress test of the modified-Teukolsky framework by designing two null diagnostics. First, we consider an action with redundant operators that must produce zero first-order vacuum QNM shifts. Second, we exploit a Ricci-flat identity relating two physical cubic Riemann to test such a relation is satisfied by the ringdown spectra obtained. We compute the shifts using two independent numerical approaches: the eigenvalue-perturbation and generalized continued-fraction (Leaver-type) methods. Both null tests are passed across multiple multipoles and overtones,…
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.
Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Black Holes and Theoretical Physics
