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We present numerical evolutions of three equal-mass black holes using the moving puncture approach.
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The first proof of principle simulation showing that puncture evolutions generalize to three or more black holes with minimal changes to a binary code was performed in 1997 Brügmann 1997 . Since this was an unpublished report, we summarize one of these simulations here. 30 black holes were arranged in a planar configuration using Brill-Lindquist data. Evolutions were performed using the fixed puncture method with the ADM formulation, maximal slicing, and vanishing shift, using an early version of the BAM
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