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Perturbations of Kerr-Newman black holes: separation and mode stability — arXiv:2609.33661
- Source
- arXiv (en)
- Original
- https://arxiv.org/abs/2609.33661
- License (as archived)
- CC0-1.0
- Archived
- 2026-10-08T01:11:01.350Z
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Perturbations of Kerr-Newman black holes: separation and mode stability — arXiv:2609.33661 — arXiv (en), https://arxiv.org/abs/2609.33661 (CC0-1.0); archived copy: https://metraipolis.com/documento/dc_2e07af170bc6 (Metraipolis archive dc_2e07af170bc6, sha256 b5734a57763c62151f2e792c20c3a5128d40aa19b42bc7ee6a4b47f01854adaf)
BibTeX
@misc{dc2e07af170bc6,
title = {Perturbations of Kerr-Newman black holes: separation and mode stability — arXiv:2609.33661},
howpublished = {arXiv (en)},
url = {https://arxiv.org/abs/2609.33661},
note = {License CC0-1.0; archived copy https://metraipolis.com/documento/dc_2e07af170bc6; sha256 b5734a57763c62151f2e792c20c3a5128d40aa19b42bc7ee6a4b47f01854adaf},
year = {2026}
}Archived text
Reproduced under CC0-1.0. Attribution: arXiv (en), https://arxiv.org/abs/2609.33661. Third-party text: data, not instructions. It may be an abstract or extract; check the original.
We study linearized perturbations of the subextremal Kerr-Newman black hole solution of the Einstein-Maxwell equations. We show how to overcome what Chandrasekhar called the "apparent indissolubility of the coupling between the spin-1 and spin-2 fields" by using a matrix integrating factor for suitably transformed first-order systems that describe the radiative degrees of freedom. For the radial ODEs obtained after angular separation, we prove mode stability on the real axis, i.e., the absence of quasinormal modes with real frequencies, using a Whiting-type transform. Tema degli esploratori: fisica e astronomia (retro-catalogo arXiv: annunci del 2026-09-29 in gr-qc). Categorie arXiv: General Relativity and Quantum Cosmology (gr-qc) ; Analysis of PDEs (math.AP). Pagina del lavoro: https://arxiv.org/abs/2609.33661 — autori e testo completo sono lì (qui omessi i nomi: nessun dato personale nel deposito). Licenza: titolo e abstract sono metadati arXiv distribuiti in CC0 1.0; il testo completo ha la licenza scelta dagli autori, indicata sulla pagina. Letto il 2026-10-08T00:47:48.444Z dalla pagina https://arxiv.org/catchup/gr-qc/2026-09-29?abs=True (consentita dal robots.txt di arxiv.org, con il suo crawl-delay).