10,192 research outputs found

    The distribution of localization centers in some discrete random systems

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    As a supplement of our previous work, we consider the localized region of the random Schroedinger operators on l2(Zd)l^2({\bf Z}^d) and study the point process composed of their eigenvalues and corresponding localization centers. For the Anderson model, we show that, this point process in the natural scaling limit converges in distribution to the Poisson process on the product space of energy and space. In other models with suitable Wegner-type bounds, we can at least show that any limiting point processes are infinitely divisible

    Comparison of Post-Newtonian and Numerical Evolutions of Black-Hole Binaries

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    In this paper, we compare the waveforms from the post-Newtonian (PN) approach with the numerical simulations of generic black-hole binaries which have mass ratio q∼0.8q\sim0.8, arbitrarily oriented spins with magnitudes S1/m12∼0.6S_1/m_1^2\sim0.6 and S2/m22∼0.4S_2/m_2^2\sim0.4, and orbit 9 times from an initial orbital separation of r≈11Mr\approx11M prior to merger. We observe a reasonably good agreement between the PN and numerical waveforms, with an overlap of over 98% for the first six cycles of the (ℓ=2,m=±2)(\ell=2,m=\pm2) mode and over 90% for the (ℓ=2,m=1)(\ell=2,m=1) and (ℓ=3,m=3)(\ell=3,m=3) modes.Comment: 4 pages, 2 figures, prepared for the proceedings of the 18th workshop on general relativity and gravitation, Hiroshima, Japan, Nov.17 - Nov.21, 200

    Intermediate Mass Ratio Black Hole Binaries: Numerical Relativity meets Perturbation Theory

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    We study black-hole binaries in the intermediate-mass-ratio regime 0.01 < q < 0.1 with a new technique that makes use of nonlinear numerical trajectories and efficient perturbative evolutions to compute waveforms at large radii for the leading and nonleading modes. As a proof-of-concept, we compute waveforms for q=1/10. We discuss applications of these techniques for LIGO/VIRGO data analysis and the possibility that our technique can be extended to produce accurate waveform templates from a modest number of fully-nonlinear numerical simulations.Comment: 4 pages, 5 figures, revtex
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