Abstract
We present observational confirmation of Hawking’s black-hole area theorem based on data from GW150914, finding agreement with the prediction with 97% (95%) probability when we model the ringdown including (excluding) overtones of the quadrupolar mode. We obtain this result from a new time-domain analysis of the pre- and postmerger data. We also confirm that the inspiral and ringdown portions of the signal are consistent with the same remnant mass and spin, in agreement with general relativity.
- Received 8 December 2020
- Accepted 26 May 2021
DOI:https://doi.org/10.1103/PhysRevLett.127.011103
© 2021 American Physical Society
Physics Subject Headings (PhySH)
synopsis
Black Hole Area Law Tested
Published 1 July 2021
By comparing the sizes of black holes before and after a merger, researchers have tested Hawking’s theorem on black hole areas.
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