Tuesday, November 21, 2017
2:00 pm


Formation of eccentric black hole gravitational wave mergers
Johan Samsing, Einstein and Spitzer-Cotsen Fellow, Princeton University

I will show that a non negligible fraction of black hole binary mergers forming in stellar clusters, will appear in the LIGO band with an eccentricity >0.1. All previous studies have argued that eccentric GW sources are not likely, however, with a consistent implementation of post-Newtonian terms in the N-body equation of motion, I show that the real fraction is likely a factor of 100 times higher than previously thought. This brings the fraction of eccentric GW mergers up to about 5%. This has profound implications for mapping out the dynamical universe through the detection of GW black hole mergers.

Contact Sheri Stoll sstoll@caltech.edu at 626-395-6608
For more information see TAPIR at Caltech
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