Detection of gravitational waves from black holes

  • Recently the LIGO and VIRGO Collaborations reported the observation of gravitational-wave signal corresponding to the inspiral and merger of two black holes, resulting into formation of the final black hole. It was shown that the observations are consistent with the Einstein theory of gravity with high accuracy, limited mainly by the statistical error. Angular momentum and mass of the final black hole were determined with rather large allowance of tens of percents. Here we shall show that this indeterminacy in the range of the black-hole parameters allows for some non-negligible deformations of the Kerr spacetime leading to the same frequencies of the black-hole ringing. This means that at the current precision of the experiment there remains some possibility for alternative theories of gravity.

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Metadaten
Author:Roman Konoplya, Alexander Zhidenko
URN:urn:nbn:de:hebis:30:3-546732
DOI:https://doi.org/10.1016/j.physletb.2016.03.044
ISSN:1873-2445
ISSN:0370-2693
Parent Title (English):Physics Letters B
Publisher:Elsevier
Place of publication:Amsterdam
Document Type:Article
Language:English
Date of Publication (online):2016/05/10
Date of first Publication:2016/05/10
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2020/05/14
Volume:756.2016
Page Number:4
First Page:350
Last Page:353
Note:
This is an open access article under the CC BY license
(http://creativecommons.org/licenses/by/4.0/).
HeBIS-PPN:465583636
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung 4.0