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PERIMETER INSTITUTE RECORDED SEMINAR ARCHIVE

11 Orbit inspiral of unequal mass black-hole binaries
Speaker(s): Ulrich Sperhake
Abstract: We present simulations of non-spinning unequal mass black-hole binaries with mass ratio q=1/4 covering approximately 11 orbits prior to coalescence and merger obtained with the moving puncture technique. Accuracy of the simulations and matching to post-Newtonian waveforms is discussed.
Date: 24/06/2010 - 5:10 pm
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