Black hole ringdown and quasinormal modes
APA
Zimmerman, A. (2016). Black hole ringdown and quasinormal modes. Perimeter Institute. https://pirsa.org/16060014
MLA
Zimmerman, Aaron. Black hole ringdown and quasinormal modes. Perimeter Institute, Jun. 15, 2016, https://pirsa.org/16060014
BibTex
@misc{ pirsa_PIRSA:16060014, doi = {10.48660/16060014}, url = {https://pirsa.org/16060014}, author = {Zimmerman, Aaron}, keywords = {Cosmology}, language = {en}, title = {Black hole ringdown and quasinormal modes}, publisher = {Perimeter Institute}, year = {2016}, month = {jun}, note = {PIRSA:16060014 see, \url{https://pirsa.org}} }
The University of Texas at Austin
Talk Type
Subject
Abstract
The first detection of gravitational waves came with an unexpected windfall: a clear signal from the merger of two black holes into a final, spinning black hole. General Relativity predicts that following merger, the final black hole relaxes by emitting radiation in a characteristic spectrum of decaying modes. I will discuss these ``quasinormal modes'' and what can be learned from them, as well as the black hole ringdown observed in GW150914. I will also explore the exotic side of ringdown, including the modes of nearly extremal black holes, and a tool for understanding the ringdown of black holes which differ from the standard Kerr solution.