Spinning-Black-Hole Binary Systems with Quasicircular orbits

Details Spinning-Black-Hole Binary Systems with Quasicircular orbits Spinning-Black-Hole Binary Systems with Quasicircular orbits

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aps..ses..jd09c&link_type=abstract

American Physical Society, 66th Annual Meeting of the Southeastern Section of the American Physical Society November 7-9, 1999 C

Astronomy and Astrophysics

Astrophysics

Scientific paper

The coalescence of a pair of black holes is quite likely going to be the first astrophysical source observed by the new generation of gravitational-wave observatories currently being constructed. And yet, even today, we do not have a quantitative understanding of what the merger waveforms from such a coalescence will look like. A great deal of effort is going into numerical modeling of these events. A necessary first step is to construct and fully understand the initial conditions for binary black hole numerical simulations. Here, I will describe recent work on understanding the initial data for black holes with spins either parallel or antiparallel to the orbital angular momentum of the binary system.

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