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تسجيل مستخدم جديدWaveform propagation in black hole spacetimes: evaluating the quality of numerical solutions
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L. Rezzolla
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We compute the propagation and scattering of linear gravitational waves off a Schwarzschild black hole using a numerical code which solves a generalization of the Zerilli equation to a three dimensional cartesian coordinate system. Since the solution to this problem is well understood it represents a very good testbed for evaluating our ability to perform three dimensional computations of gravitational waves in spacetimes in which a black hole event horizon is present.
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