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    What Happens to Apparent Horizons in a Binary Black Hole Merger?

    Daniel Pook-Kolb1,2, Robie A. Hennigar3,4,5, and Ivan Booth3

    • 1Max-Planck-Institut für Gravitationsphysik (Albert Einstein Institute), Callinstrasse 38, 30167 Hannover, Germany
    • 2Leibniz Universität Hannover, 30167 Hannover, Germany
    • 3Department of Mathematics and Statistics, Memorial University of Newfoundland, St. John’s, Newfoundland and Labrador A1C 5S7, Canada
    • 4Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada
    • 5Department of Physics and Computer Science, Wilfrid Laurier University, Waterloo, Ontario N2L 3C5, Canada

    Phys. Rev. Lett. 127, 181101 – Published 25 October, 2021

    DOI: https://doi.org/10.1103/PhysRevLett.127.181101

    Abstract

    We resolve the fate of the two original apparent horizons during the head-on merger of two nonspinning black holes. We show that, following the appearance of the outer common horizon and subsequent interpenetration of the original horizons, they continue to exist for a finite period of time before they are individually annihilated by unstable marginally outer trapped surfaces (MOTSs). The inner common horizon vanishes in a similar, though independent, way. This completes the understanding of the analog of the event horizon’s “pair of pants” diagram for the apparent horizon. Our result is facilitated by a new method for locating MOTSs based on a generalized shooting method. We also discuss the role played by the MOTS stability operator in discerning which among a multitude of MOTSs should be considered as black hole boundaries.

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