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Explaining Nonlinearities in Black Hole Ringdowns from Symmetries
It has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. We show that this nonlinear behavior is explained, both on the qualitative and quantitat...
| Autores principales: | , , , |
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| Lenguaje: | eng |
| Publicado: |
2023
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.108.L021501 http://cds.cern.ch/record/2848494 |
| _version_ | 1780976843357159424 |
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| author | Kehagias, Alex Perrone, Davide Riotto, Antonio Riva, Francesco |
| author_facet | Kehagias, Alex Perrone, Davide Riotto, Antonio Riva, Francesco |
| author_sort | Kehagias, Alex |
| collection | CERN |
| description | It has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. We show that this nonlinear behavior is explained, both on the qualitative and quantitative level, by near-horizon symmetries of the Kerr black hole within the Kerr/CFT correspondence. |
| id | cern-2848494 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2023 |
| record_format | invenio |
| spelling | cern-28484942023-07-21T02:41:40Zdoi:10.1103/PhysRevD.108.L021501http://cds.cern.ch/record/2848494engKehagias, AlexPerrone, DavideRiotto, AntonioRiva, FrancescoExplaining Nonlinearities in Black Hole Ringdowns from Symmetrieshep-thParticle Physics - Theoryhep-phParticle Physics - Phenomenologyastro-ph.COAstrophysics and Astronomygr-qcGeneral Relativity and CosmologyIt has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. We show that this nonlinear behavior is explained, both on the qualitative and quantitative level, by near-horizon symmetries of the Kerr black hole within the Kerr/CFT correspondence.It has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. We show that this nonlinear behaviour is explained, both on the qualitative and quantitative level, by near-horizon symmetries of the Kerr black hole within the Kerr/CFT correspondence.arXiv:2301.09345oai:cds.cern.ch:28484942023-01-23 |
| spellingShingle | hep-th Particle Physics - Theory hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy gr-qc General Relativity and Cosmology Kehagias, Alex Perrone, Davide Riotto, Antonio Riva, Francesco Explaining Nonlinearities in Black Hole Ringdowns from Symmetries |
| title | Explaining Nonlinearities in Black Hole Ringdowns from Symmetries |
| title_full | Explaining Nonlinearities in Black Hole Ringdowns from Symmetries |
| title_fullStr | Explaining Nonlinearities in Black Hole Ringdowns from Symmetries |
| title_full_unstemmed | Explaining Nonlinearities in Black Hole Ringdowns from Symmetries |
| title_short | Explaining Nonlinearities in Black Hole Ringdowns from Symmetries |
| title_sort | explaining nonlinearities in black hole ringdowns from symmetries |
| topic | hep-th Particle Physics - Theory hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy gr-qc General Relativity and Cosmology |
| url | https://dx.doi.org/10.1103/PhysRevD.108.L021501 http://cds.cern.ch/record/2848494 |
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