Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime

We give a quantitative refinement and simple proofs of mode stability type statements for the wave equation on Kerr backgrounds in the full sub-extremal range (|a| <  M). As an application, we are able to quantitatively control the energy flux along the horizon and null infinity and establish int...

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Main Author: Shlapentokh-Rothman, Yakov Mordechai
Other Authors: Massachusetts Institute of Technology. Department of Mathematics
Format: Article
Language:English
Published: Springer Basel 2019
Online Access:http://hdl.handle.net/1721.1/121094
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author Shlapentokh-Rothman, Yakov Mordechai
author2 Massachusetts Institute of Technology. Department of Mathematics
author_facet Massachusetts Institute of Technology. Department of Mathematics
Shlapentokh-Rothman, Yakov Mordechai
author_sort Shlapentokh-Rothman, Yakov Mordechai
collection MIT
description We give a quantitative refinement and simple proofs of mode stability type statements for the wave equation on Kerr backgrounds in the full sub-extremal range (|a| <  M). As an application, we are able to quantitatively control the energy flux along the horizon and null infinity and establish integrated local energy decay for solutions to the wave equation in any bounded-frequency regime. Keywords: Black Hole, Wave Equation, Half Plane, Quasinormal Mode, Mode Stability
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spelling mit-1721.1/1210942022-09-29T23:38:44Z Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime Shlapentokh-Rothman, Yakov Mordechai Massachusetts Institute of Technology. Department of Mathematics Shlapentokh-Rothman, Yakov Mordechai We give a quantitative refinement and simple proofs of mode stability type statements for the wave equation on Kerr backgrounds in the full sub-extremal range (|a| <  M). As an application, we are able to quantitatively control the energy flux along the horizon and null infinity and establish integrated local energy decay for solutions to the wave equation in any bounded-frequency regime. Keywords: Black Hole, Wave Equation, Half Plane, Quasinormal Mode, Mode Stability 2019-03-26T13:56:39Z 2019-03-26T13:56:39Z 2014-01 2013-02 2019-02-02T04:45:59Z Article http://purl.org/eprint/type/JournalArticle 1424-0637 1424-0661 http://hdl.handle.net/1721.1/121094 Shlapentokh-Rothman, Yakov. “Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime.” Annales Henri Poincaré 16, no. 1 (January 31, 2014): 289–345. en https://doi.org/10.1007/s00023-014-0315-7 Annales Henri Poincaré Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. Springer Basel application/pdf Springer Basel Springer Basel
spellingShingle Shlapentokh-Rothman, Yakov Mordechai
Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime
title Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime
title_full Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime
title_fullStr Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime
title_full_unstemmed Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime
title_short Quantitative Mode Stability for the Wave Equation on the Kerr Spacetime
title_sort quantitative mode stability for the wave equation on the kerr spacetime
url http://hdl.handle.net/1721.1/121094
work_keys_str_mv AT shlapentokhrothmanyakovmordechai quantitativemodestabilityforthewaveequationonthekerrspacetime