Analytical proof of the isospectrality of quasinormal modes for Schwarzschild-de Sitter and Schwarzschild-Anti de Sitter spacetimes
The deep reason why the equations describing axial and polar perturbations of Schwarzschild black holes have the same spectrum is far from trivial. In this article, we revisit the original proof and try to make it clearer. Still focusing on uncharged and non-rotating black holes, we extend the resul...
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| Veröffentlicht in: | Gen.Rel.Grav 2020, Vol.52 (8), Article 82 |
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| creator | Moulin, Flora Barrau, Aurélien |
| description | The deep reason why the equations describing axial and polar perturbations of Schwarzschild black holes have the same spectrum is far from trivial. In this article, we revisit the original proof and try to make it clearer. Still focusing on uncharged and non-rotating black holes, we extend the results to spacetimes including a cosmological constant, which have so far mostly been investigated numerically from this perspective. |
| doi_str_mv | 10.1007/s10714-020-02737-4 |
| format | Article |
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| subjects | Astronomy Astrophysics and Cosmology Classical and Quantum Gravitation Cosmological constant Differential Geometry General Relativity and Quantum Cosmology Gravity High Energy Physics - Theory Mathematical and Computational Physics Physics Physics and Astronomy Quantum Physics Relativity Theory Research Article Spacetime Theoretical |
| title | Analytical proof of the isospectrality of quasinormal modes for Schwarzschild-de Sitter and Schwarzschild-Anti de Sitter spacetimes |
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