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Computational solution to the Einstein Field Equations for the purposes of modeling black hole spacetimes.
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Binary Black Hole mergers provide strong detectable sources of gravitational radiation.
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Accurate predictions of waveforms expected to enhance the detectability of gravity waves, build database of waveforms
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Computational simulations of black hole mergers are important for accurate detection and characterization of GW.
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Simulations of Binary Black Hole mergers will provide insights into strong field GR as well as provide a solution to the two-body problem of GR.
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