On destabilising quasi-normal modes with a radially concentrated perturbation
In this work we explore some aspects of the spectral instability of back hole quasi-normal modes, using a specific model as an example. The model is that of a small bump perturbation to the effective potential of linear axial gravitational waves on a Schwarzschild background, and our focus is on thr...
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Frontiers Media S.A.
2025-01-01
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| Serie: | Frontiers in Physics |
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| Accesso online: | https://www.frontiersin.org/articles/10.3389/fphy.2024.1511757/full |
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