PIRSA:10060068  ( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?

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

Collection: Theory Meets Data Analysis at Comparable and Extreme Mass Ratios - 2010

URL: http://pirsa.org/10060068/  Share: