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Wave equations in the Kerr-de Sitter spacetime: The full subextremal range
KTH, School of Engineering Sciences (SCI), Mathematics (Dept.).ORCID iD: 0000-0001-6781-1594
Stanford Univ, Dept Math, 450 Jane Stanford Way, Bldg 380, Stanford, CA 94305 USA.
2024 (English)In: Journal of the European Mathematical Society (Print), ISSN 1435-9855, E-ISSN 1435-9863, Vol. 27, no 8, p. 3497-3526Article in journal (Refereed) Published
Abstract [en]

We prove that solutions to linear wave equations in a subextremal Kerr-de Sitter spacetime have asymptotic expansions in quasinormal modes up to a decay order given by the normally hyperbolic trapping, extending the result of the second named author (2013). The main novelties are a different way of obtaining a Fredholm setup that defines the quasinormal modes and a new analysis of the trapping of lightlike geodesics in the Kerr-de Sitter spacetime, both of which apply in the full subextremal range. In particular, this reduces the question of decay for solutions to wave equations to the question of mode stability.

Place, publisher, year, edition, pages
European Mathematical Society - EMS - Publishing House GmbH , 2024. Vol. 27, no 8, p. 3497-3526
Keywords [en]
subextremal Kerr-de Sitter spacetime, resonances, quasinormal modes, radial points, normally hyperbolic trapping
National Category
Computational Mathematics
Identifiers
URN: urn:nbn:se:kth:diva-367879DOI: 10.4171/JEMS/1448ISI: 001504695800008Scopus ID: 2-s2.0-105006698456OAI: oai:DiVA.org:kth-367879DiVA, id: diva2:1987014
Note

QC 20250804

Available from: 2025-08-04 Created: 2025-08-04 Last updated: 2025-08-04Bibliographically approved

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Lindblad Petersen, Oliver

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