Coalescing Binary Systems: An Effective Metric Approach

Details Coalescing Binary Systems: An Effective Metric Approach Coalescing Binary Systems: An Effective Metric Approach

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...9916941b&link_type=abstract

Conference Paper, Pub. in Proceedings and Recontres de Moriond (34th): Gravitational Waves and Experimental Gravity, Les Arcs, F

Astronomy and Astrophysics

Astronomy

Digital Systems, Circular Orbits, Gravitational Waves, Coalescing, Mathematical Models, Stability, Two Body Problem, Cosmology, Neutron Stars, Relativity, Black Holes (Astronomy)

Scientific paper

In order to have a more reliable description of the final stage of evolution of a binary system, the authors 'reduce' the two-body problem in general relativity to an auxilliary one-body one. The effective description defines a particular re-summation of the original post-Newtonian expanded dynamics and should be able to specify some non-perturbative characterisics of the evolution of a binary system as the existence of the innermost stable circular orbit.

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