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19 11. 12. 13. 14. F. Wilczek, Phys. Rev. Lett. 40, 279 (1978). M. S. Turner, Phys. Rep. 197, 67 (1990). H. A. Chan and H. J. Paik, Phys. Rev. D 35, 3551 (1987). M. V. Moody, E. R. Canavan and H. J. Paik, Rev. Sci. Instrum. 73, 3957 (2002). 15. H. B. G. Casimir, Proc. K. Ned. Akad. Wet. 5 1 , 834 (793). 16. S. K. Lamoreaux, Phys. Rev. Lett. 78, 5 (1997). Numerical Relativity A New Generalized Harmonic Evolution S y s t e m Lee Lindblom 1 , Mark A. Scheel 1 , Lawrence E. Kidder 2 , Robert Owen 1 , and Oliver Rinne 1 Theoretical Astrophysics 130-33, California Institute Pasadena, 2 Center for Radiophysics of Technology CA 91125, USA and Space Research, Cornell University Ithaca, NY 14853 USA This note describes recent work on finding a formulation of the Einstein equations suitable for constructing stable numerical evolutions.

See Husa et al. [5] and earlier reviews [6] and [7]. 3. Artificial Cosmology Although conformally regulated Minkowski spacetime (equation 10) allows wave equations to be formulated as finite difference equations all the way out to and including R = oo, boundary conditions there can still be touchy. The ingoing coordinate speed of light there is cin = - ( 1 - r/2)2 (11) 37 which is negative (dr/du < 0 on these null directions) except at the horizon I+ where it is zero. , I+. Thus this outer boundary is very different from the future boundary u = const at each stage of the solution, which is a spacelike hypersurface in the future of the initial conditions.

In these evolutions we "freeze" the values of the incoming characteristic fields on the boundaries. We performed these numerical evolutions using spectral methods as described in Ref. 10 for a range of numerical resolutions specified by Nr (the highest order radial basis function) and Lmax (the highest order spherical harmonic). L I I I I I } = {9,7} 11,7} {13,7} 5000 10000 t/M Fig. 2. Evolution of Schwarzschild initial d a t a with 70 convergence for several numerical resolutions. 72 = 1 show stability and ues of the constraint damping parameters 70 and 72.

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An Intro to Continuity, Extrema & Related Topics for general gaussian process by Adler R.

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