A New Parallel Method for Binary Black Hole Simulations
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Initial data for numerical evolutions of binary-black holes have been dominated by ‘‘conformally flat’’ (CF) data (i.e., initial data where the conformal background metric is chosen to be flat) because they are easy to construct. However, CF initial data cannot simulate nearly ex
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Since the breakthroughs in 2005 which have led to long term stable solutions of the binary black hole problem in numerical relativity, much progress has been made. I present here a short summary of the state of the field, including the capabilities of numerical relativity codes,
At early times in numerical evolutions of binary black holes, current simulations contain an initial burst of spurious gravitational radiation (also called “junk radiation”) which is not astrophysically realistic. The spurious radiation is a consequence of how the binary-black-ho
This Letter presents a publicly available catalog of 174 numerical binary black hole simulations following up to 35 orbits. The catalog includes 91 precessing binaries, mass ratios up to 8∶1, orbital eccentricities from a few percent to 10(-5), black hole spins up to 98% of the t
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