2025/12/16 by Wu, David G., Hussain, Asad, Zimmerman, Aaron
#FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc)
paper · doi:10.48550/arxiv.2512.14679
The growing number of gravitational wave (GW) detections and the increasing sensitivity of GW detectors have enabled precision tests of General Relativity (GR) in the strong-field regime. The recent observation of multiple quasinormal modes (QNMs) in GW250114 marks a major advance for observational black hole spectroscopy. This clear signal, together with the growing number of GW detections, highlights the need for accurate predictions of QNM spectra in beyond-GR theories in order to carry out precision searches for new physics. In this work, we continue to lay the foundation for such predictions using a modified Teukolsky formalism in conjunction with the eigenvalue perturbation method. We compute the spectral shifts of slowly rotating Johannsen-Psaltis black holes for 2 ≤ ℓ ≤ 10, all m, and overtones n = 0, 1, 2, and confirm the large-ℓ behavior of the modes by comparing with the WKB approximation. We find that these black holes admit definite-parity modes but break the isospectrality between even- and odd-parity QNMs at all spins, and that the shifts depend linearly on m for slow spins. We further derive a general parity condition that any beyond-GR modification to the metric must satisfy to support definite-parity modes, providing new insights into isospectrality breaking and parity structure in gravitational perturbations.