Physics > Computational Physics
[Submitted on 16 Nov 2007 (v1), last revised 2 Jul 2009 (this version, v2)]
Title:A spectral collocation approximation for the radial-infall of a compact object into a Schwarzschild black hole
View PDFAbstract: The inhomogeneous Zerilli equation is solved in time-domain numerically with the Chebyshev spectral collocation method to investigate a radial-infall of the point particle towards a Schwarzschild black hole. Singular source terms due to the point particle appear in the equation in the form of the Dirac $\delta$-function and its derivative. For the approximation of singular source terms, we use the direct derivative projection method without any regularization. The gravitational waveforms are evaluated as a function of time. We compare the results of the spectral collocation method with those of the explicit second-order central-difference method. The numerical results show that the spectral collocation approximation with the direct projection method is accurate and converges rapidly when compared with the finite-difference method.
Submission history
From: Gaurav Khanna [view email][v1] Fri, 16 Nov 2007 02:40:48 UTC (920 KB)
[v2] Thu, 2 Jul 2009 22:30:54 UTC (606 KB)
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