Video URL
https://pirsa.org/23100103The quasinormal-mode content of black hole ringdowns
APA
Cheung, M. (2023). The quasinormal-mode content of black hole ringdowns. Perimeter Institute for Theoretical Physics. https://pirsa.org/23100103
MLA
Cheung, Mark. The quasinormal-mode content of black hole ringdowns. Perimeter Institute for Theoretical Physics, Oct. 19, 2023, https://pirsa.org/23100103
BibTex
@misc{ scivideos_PIRSA:23100103, doi = {10.48660/23100103}, url = {https://pirsa.org/23100103}, author = {Cheung, Mark}, keywords = {Strong Gravity}, language = {en}, title = {The quasinormal-mode content of black hole ringdowns}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2023}, month = {oct}, note = {PIRSA:23100103 see, \url{https://scivideos.org/index.php/pirsa/23100103}} }
Mark Cheung Johns Hopkins University
Abstract
In general relativity, the remnant black hole of a binary black hole merger emits “ringdown” radiation: a superposition of quasinormal modes with characteristic complex frequencies. The detection of more than one of these frequencies would serve as smoking-gun evidence of a black hole and would enable a test of the no-hair theorem. In this talk, I will discuss strategies for identifying quasinormal modes within simulated ringdown waveforms both in linear perturbation theory and full general relativity. I will show that a rich spectrum of modes could exist in the ringdown, including overtones, retrograde modes and nonlinear modes, and that interesting quasi-universal relationships exist between some of their amplitudes. I will also discuss the spectral instability of quasinormal modes and its potential imprints on the ringdown waveform. These results could guide the analysis of real ringdown signals detected by gravitational-wave detectors.
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Zoom link https://pitp.zoom.us/j/92002625163?pwd=bHNDVVZKYnVNTENLNXJBLzVNKzVSQT09