Binary black hole spectroscopy : A no-hair test of GW190814 and GW190412

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dc.identifier.uri http://dx.doi.org/10.15488/10645
dc.identifier.uri https://www.repo.uni-hannover.de/handle/123456789/10723
dc.contributor.author Capano, Collin D.
dc.contributor.author Nitz, Alexander H.
dc.date.accessioned 2021-03-26T10:06:21Z
dc.date.available 2021-03-26T10:06:21Z
dc.date.issued 2020
dc.identifier.citation Capano, C.D.; Nitz, A.H.: Binary black hole spectroscopy: A no-hair test of GW190814 and GW190412. In: Physical Review D 102 (2020), Nr. 12, 124070. DOI: https://doi.org/10.1103/PhysRevD.102.124070
dc.description.abstract Gravitational waves provide a window to probe general relativity (GR) under extreme conditions. The recent observations of GW190412 and GW190814 are unique high-mass-ratio mergers that enable the observation of gravitational-wave harmonics beyond the dominant (ℓ,m)=(2,2) mode. Using these events, we search for physics beyond GR by allowing the source parameters measured from the subdominant harmonics to deviate from that of the dominant mode. All results are consistent with GR. We constrain the chirp mass as measured by the (ℓ,m)=(3,3) mode to be within 0-3+5% of the dominant mode when we allow both the masses and spins of the subdominant modes to deviate. If we allow only the mass parameters to deviate, we constrain the chirp mass of the (3,3) mode to be within ±1% of the expected value from GR. © 2020 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Open access publication funded by the Max Planck Society. eng
dc.language.iso eng
dc.publisher College Park, MD : American Physical Society
dc.relation.ispartofseries Physical Review D 102 (2020), Nr. 12
dc.rights CC BY 4.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by/4.0/
dc.subject Condensed matter eng
dc.subject Nuclear physics eng
dc.subject Particles (Nuclear physics) eng
dc.subject Quantum gravity eng
dc.subject General relativity (Physics) eng
dc.subject Gravitation eng
dc.subject Fluid dynamics eng
dc.subject.ddc 530 | Physik ger
dc.title Binary black hole spectroscopy : A no-hair test of GW190814 and GW190412
dc.type article
dc.type Text
dc.relation.essn 1089-4918
dc.relation.essn 1550-2368
dc.relation.essn 2470-0029
dc.relation.issn 2470-0010
dc.relation.doi https://doi.org/10.1103/PhysRevD.102.124070
dc.bibliographicCitation.issue 12
dc.bibliographicCitation.volume 102
dc.bibliographicCitation.firstPage 124070
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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