Pseudospectrum and black hole quasi-normal mode (in)stability
APA
Panosso Macedo, R. (2021). Pseudospectrum and black hole quasi-normal mode (in)stability. Perimeter Institute. https://pirsa.org/21060015
MLA
Panosso Macedo, Rodrigo. Pseudospectrum and black hole quasi-normal mode (in)stability. Perimeter Institute, Jun. 07, 2021, https://pirsa.org/21060015
BibTex
@misc{ pirsa_PIRSA:21060015, doi = {10.48660/21060015}, url = {https://pirsa.org/21060015}, author = {Panosso Macedo, Rodrigo}, keywords = {Other}, language = {en}, title = {Pseudospectrum and black hole quasi-normal mode (in)stability}, publisher = {Perimeter Institute}, year = {2021}, month = {jun}, note = {PIRSA:21060015 see, \url{https://pirsa.org}} }
Queen Mary University of London
Talk Type
Subject
Abstract
We study the stability of quasi-normal modes (QNM) in asymptotically flat black hole spacetimes by means of a pseudospectrum analysis. The construction of the Schwarzschild QNM pseudospectrum reveals: i) the stability of the slowest decaying QNM under perturbations respecting the asymptotic structure, reassessing the instability of the fundamental QNM discussed by Nollert (1996); ii) the instability of all overtones under small scale perturbations of sufficiently high frequency, that migrate to a universal class of QNM branches along pseudospectra boundaries, shedding light on Nollert & Price's analysis (1996).