Exceptional points and resonance in black hole ringdown
We propose an exceptional-point (EP) framework for black-hole ringdown beyond the standard quasinormal-mode (QNM) paradigm. It provides a first-principles characterization of the resonance associated with avoided crossings near EPs, an effect that conventional QNM analysis cannot fully capture. Employing a phenomenological environmental black-hole model with the hyperboloidal framework, we identify near-coalescence of both QNM eigenvalues and eigenfunctions, and directly demonstrate that the resonance produces enhanced mode contributions in the time domain, resulting in characteristic departures from exponentially damped oscillations. Our formulation further reveals that the EP frequency, given by the average of the resonant modes, emerges as the physically relevant observable in the near-EP regime, and offers a robust foundation for modeling and extracting resonant ringdown signals.
Authors
- Rodrigo Panosso Macedo (ORCID: https://orcid.org/0000-0003-2942-5080)
- Hayato Motohashi (ORCID: https://orcid.org/0000-0002-4330-7024)
- Kei-ichiro Kubota (ORCID: https://orcid.org/0000-0002-1576-4332)
- Takuya Katagiri
Institutions
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT)
- Institute for Cosmic Ray Research (JP)
- Tokyo Metropolitan University (JP)
- Sapienza University of Rome (IT)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2026-06-17
- DOI
- https://doi.org/10.1103/5w5d-kr25
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- Villum Fonden
- European Commission
- National Research Foundation
- Danmarks Grundforskningsfond
- Ministero dell'Università e della Ricerca
- Horizon 2020 Framework Programme
- Japan Society for the Promotion of Science
- Instituto Nazionale di Fisica Nucleare
- HORIZON EUROPE Marie Sklodowska-Curie Actions