PIRSA:25010067

Video URL

https://pirsa.org/25010067

The Astrophysical Promise of Black Hole Ringdowns

Siegel, H. (2025). The Astrophysical Promise of Black Hole Ringdowns. Perimeter Institute for Theoretical Physics. https://pirsa.org/25010067

Siegel, Harrison. The Astrophysical Promise of Black Hole Ringdowns. Perimeter Institute for Theoretical Physics, Jan. 09, 2025, https://pirsa.org/25010067 

          @misc{ scivideos_PIRSA:25010067,
            doi = {10.48660/25010067},
            url = {https://pirsa.org/25010067},
            author = {Siegel, Harrison},
            keywords = {Strong Gravity},
            language = {en},
            title = {The Astrophysical Promise of Black Hole Ringdowns},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2025},
            month = {jan},
            note = {PIRSA:25010067 see, \url{https://scivideos.org/pirsa/25010067}}
          }

Harrison Siegel Columbia University

Talk numberPIRSA:25010067
DOI10.48660/25010067
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The remnant of a binary black hole coalescence is a perturbed black hole, which equilibrates by emitting ringdown gravitational waves. These ringdown waves not only encode information in their frequencies about the spacetime structure of the remnant black hole metric, but also have imprints in their amplitudes of the progenitor black hole binary's properties. In this talk I will highlight recent results in black hole ringdown data analysis and new understanding of astrophysical ringdown amplitudes gleaned from numerical relativity simulations, and will then discuss how ringdown analyses may become a vital tool for making inferences of binary black hole properties - even in situations where the gravitational wave signal from the binary inspiral itself is never directly observed.