Pseudospectrum and Black Hole Quasinormal Mode Instability
We study the stability of quasinormal modes (QNM) in asymptotically flat black hole spacetimes by means of a pseudospectrum analysis. The construction of the Schwarzschild QNM pseudospectrum reveals the following: (i) the stability of the slowest-decaying QNM under perturbations respecting the asymp...
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Formato: | article |
Lenguaje: | EN |
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American Physical Society
2021
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Acceso en línea: | https://doaj.org/article/113c2317a1c64352bc01aeb604d57321 |
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