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- W1989170879 abstract "We describe early success in the evolution of binary black-hole spacetimes with a numerical code based on a generalization of harmonic coordinates. Indications are that with sufficient resolution this scheme is capable of evolving binary systems for enough time to extract information about the orbit, merger, and gravitational waves emitted during the event. As an example we show results from the evolution of a binary composed of two equal mass, nonspinning black holes, through a single plunge orbit, merger, and ringdown. The resultant black hole is estimated to be a Kerr black hole with angular momentum parameter $aensuremath{approx}0.70$. At present, lack of resolution far from the binary prevents an accurate estimate of the energy emitted, though a rough calculation suggests on the order of 5% of the initial rest mass of the system is radiated as gravitational waves during the final orbit and ringdown." @default.
- W1989170879 created "2016-06-24" @default.
- W1989170879 creator A5019617791 @default.
- W1989170879 date "2005-09-14" @default.
- W1989170879 modified "2023-10-18" @default.
- W1989170879 title "Evolution of Binary Black-Hole Spacetimes" @default.
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- W1989170879 doi "https://doi.org/10.1103/physrevlett.95.121101" @default.
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