High accuracy binary black hole simulations with an extended wave zone
نویسندگان
چکیده
منابع مشابه
Status of black-hole-binary simulations for gravitational-wave detection
It is now possible to theoretically calculate the gravitational-wave signal from the inspiral, merger and ringdown of a black-hole-binary system. The late inspiral, merger and ringdown can be calculated in full general relativity using numerical methods. The numerical waveforms can then be either stitched to inspiral waveforms predicted by approximation techniques (in particular postNewtonian c...
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Abdul H. Mroué, Mark A. Scheel, Béla Szilágyi, Harald P. Pfeiffer, 3 Michael Boyle, Daniel A. Hemberger, 4 Lawrence E. Kidder, Geoffrey Lovelace, 2 Serguei Ossokine, 6 Nicholas W. Taylor, Anıl Zenginoğlu, Luisa T. Buchman, Tony Chu, Evan Foley, Matthew Giesler, Robert Owen, and Saul A. Teukolsky Canadian Institute for Theoretical Astrophysics, 60 St. George Street, University of Toronto, Toront...
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In 1915 Albert Einstein derived the fundamental laws of General Relativity, which predict the existence of gravitational radiation. While indirect evidence is by now well established and led in 1993 to the Nobel Prize in Physics being awarded to Hulse and Taylor, no direct detection has occurred to date. This is because gravitational waves reaching Earth are extremely weak. Recently, researcher...
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ژورنال
عنوان ژورنال: Physical Review D
سال: 2011
ISSN: 1550-7998,1550-2368
DOI: 10.1103/physrevd.83.044045