Video URL
https://pirsa.org/17110139Probing the strong gravity regime with binary black hole ringdown - Swetha Prabhat
APA
Prabhat, S. (2017). Probing the strong gravity regime with binary black hole ringdown - Swetha Prabhat. Perimeter Institute for Theoretical Physics. https://pirsa.org/17110139
MLA
Prabhat, Swetha. Probing the strong gravity regime with binary black hole ringdown - Swetha Prabhat. Perimeter Institute for Theoretical Physics, Nov. 16, 2017, https://pirsa.org/17110139
BibTex
@misc{ scivideos_PIRSA:17110139, doi = {10.48660/17110139}, url = {https://pirsa.org/17110139}, author = {Prabhat, Swetha}, keywords = {Strong Gravity}, language = {en}, title = {Probing the strong gravity regime with binary black hole ringdown - Swetha Prabhat}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2017}, month = {nov}, note = {PIRSA:17110139 see, \url{https://scivideos.org/index.php/pirsa/17110139}} }
Swetha Prabhat Syracuse University
Abstract
When two black holes merge, they 'ringdown' as they settle into a final Kerr black hole. The ringdown part of the gravitational wave signal probes the strong field gravity, enabling us to test the general theory of relativity (GR) in that regime. In this talk, I will focus on one particular challenge associated with the ringdown - "When does a ringdown start during a binary black hole merger?". Then I will end the talk with a brief summary of our prospects to perform GR tests with the ringdown signals using the current and future ground-based gravitational wave observatory.