Reducing Orbital Eccentricity in Binary Black Hole Simulations

Details Reducing Orbital Eccentricity in Binary Black Hole Simulations Reducing Orbital Eccentricity in Binary Black Hole Simulations

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1597p&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

Binary black hole simulations starting from quasi-circular (i.e., zero radial velocity) initial data have orbits with small but non-zero orbital eccentricities. Nonzero radial velocities are added to the quasi-equilibrium formalism for constructing binary black hole initial data, and it is demonstrated how the orbital frequency and radial velocities can be tuned to obtain inspiral trajectories with significantly reduced orbital eccentricity.

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