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Testing the Black-Hole Area Law with GW150914

Maximiliano Isi, Will M. Farr, Matthew Giesler, Mark A. Scheel, and Saul A. Teukolsky
Phys. Rev. Lett. 127, 011103 – Published 1 July 2021
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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.

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  • 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)

Gravitation, Cosmology & Astrophysics

synopsis

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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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Authors & Affiliations

Maximiliano Isi1,*, Will M. Farr2,3,†, Matthew Giesler4, Mark A. Scheel5, and Saul A. Teukolsky4,5

  • 1LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
  • 2Center for Computational Astrophysics, Flatiron Institute, 162 5th Ave, New York, New York 10010, USA
  • 3Department of Physics and Astronomy, Stony Brook University, Stony Brook, New York 11794, USA
  • 4Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, New York 14853, USA
  • 5TAPIR, Walter Burke Institute for Theoretical Physics, California Institute of Technology, Pasadena, California 91125, USA

  • *maxisi@mit.edu; NHFP Einstein fellow
  • will.farr@stonybrook.edu

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Issue

Vol. 127, Iss. 1 — 2 July 2021

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