arXiv · 2401.02898
Quasinormal modes of rapidly rotating Ellis-Bronnikov wormholes
Abstract
We present for the first time a study of the quasinormal modes of rapidly rotating Ellis-Bronnikov wormholes in General Relativity. We compute the spectrum of the wormholes using a spectral decomposition of the metric perturbations on a numerical background. We focus on the $M_z=2,3$ sector of the perturbations, and show that the triple isospectrality of the symmetric and static Ellis-Bronnikov wormhole is broken due to rotation, giving rise to a much richer spectrum than the spectrum of Kerr black holes. We do not find any instabilities for $M_z=2,3$ perturbations.
Explore related subjects
Keep this discovery
Fech Scen Khoo, Bahareh Azad, Jose Luis Blázquez-Salcedo, Luis Manuel González-Romero, Burkhard Kleihaus, Jutta Kunz, Francisco Navarro-Lérida. 2024-01-05. Quasinormal modes of rapidly rotating Ellis-Bronnikov wormholes. https://doi.org/10.1103/physrevd.109.084013
Cite the original work for its findings. Save a collection to share your selection of sources.