A4:. Approximation Methods

Details A4:. Approximation Methods A4:. Approximation Methods

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002grg..conf..374w&link_type=abstract

GENERAL RELATIVITY AND GRAVITATION. Proceedings of the 16th International Conference. Held 15-21 July 2001 in Durban, South Afri

Computer Science

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The Workshop A4 on Approximation Methods was divided into three sessions. The first, on post-Newtonian methods, focussed on efforts to calculate the equations of motion and gravitational waveform of inspiralling compact binaries to very high order in a post-Newtonian approximation (essentially in powers of (v/c) ~ (Gm/rc2)1/2). Progress was reported on the effort to reach third post-Newtonian order and beyond. The second session focussed on perturbations of black holes and stars, with particular interest in linking black hole perturbations with numerical relativity, and in the unstable r-modes of relativistic stars. The final session was devoted to miscellaneous perturbation methods.

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