Phys. Rev. D 54, 4849–4857 (1996)Implementing an apparent-horizon finder in three dimensionsReceived 6 June 1996; published in the issue dated 15 October 1996 Locating apparent horizons is not only important for a complete understanding of numerically generated spacetimes, but it may also be a crucial component of the technique for evolving black-hole spacetimes accurately. A scheme proposed by Libson, Massó, Seidel, and Suen, based on expanding the location of the apparent horizon in terms of symmetric trace-free tensors, seems very promising for use with three-dimensional numerical data sets. In this paper, we generalize this scheme and perform a number of code tests to fully calibrate its behavior in black-hole spacetimes similar to those we expect to encounter in solving the binary black-hole coalescence problem. An important aspect of the generalization is that we can compute the symmetric trace-free tensor expansion to any order. This enables us to determine how far we must carry the expansion to achieve results of a desired accuracy. To accomplish this generalization, we describe a new and very convenient set of recurrence relations which apply to symmetric trace-free tensors. © 1996 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.54.4849
DOI:
10.1103/PhysRevD.54.4849
PACS:
04.20.Cv, 02.60.Cb, 02.70.Rw, 04.25.Dm
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