Quasinormal resonances of rapidly-spinning Kerr black holes and the universal relaxation bound
The universal relaxation bound suggests that the relaxation times of perturbed thermodynamical systems is bounded from below by the simple time-times-temperature (TTT) quantum relation τ×T≥ħπ. It is known that some perturbation modes of near-extremal Kerr black holes in the regime MTBH/ħ≪m−2 are cha...
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| Formato: | article |
| Lenguaje: | EN |
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Elsevier
2021
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| Acceso en línea: | https://doaj.org/article/08e983a1a2b44504943d50afb5b2127e |
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