Adaptive event horizon tracking and critical phenomena in binary black hole coalescence

Scott A. Caveny and Richard A. Matzner
Phys. Rev. D 68, 104003 – Published 5 November 2003
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Abstract

This work establishes critical phenomena in the topological transition of black hole coalescence. We describe and validate a computational front tracking event horizon solver, developed for generic studies of the black hole coalescence problem. We then apply this to the Kastor-Traschen axisymmetric analytic solution of the extremal Maxwell-Einstein black hole merger with a cosmological constant. The surprising result of this computational analysis is a power law scaling of the minimal throat proportional to time. The minimal throat connecting the two holes obeys this power law during a short time immediately at the beginning of merger. We also confirm the behavior analytically. Thus, at least in one axisymmetric situation a critical phenomenon exists. We give arguments for a broader universality class than the restricted requirements of the Kastor-Traschen solution.

  • Received 1 April 2003

DOI:https://doi.org/10.1103/PhysRevD.68.104003

©2003 American Physical Society

Authors & Affiliations

Scott A. Caveny and Richard A. Matzner

  • Center for Relativity, The University of Texas at Austin, Austin, Texas 78712-1081, USA

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Issue

Vol. 68, Iss. 10 — 15 November 2003

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