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The pseudospectrum for gravitational perturbations in Kerr spacetimes
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-theory
We study the pseudospectrum of the Kerr black hole for gravitational perturbations with spin weight $s=2$, the case of greatest interest in gravitational-wave astronomy. In the hyperboloidal framework with two-dimensional Chebyshev collocation, we formulate the quasinormal mode problem as a non-self
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