Comment on a relativistic model for coalescing neutron star binaries
arXiv:gr-qc/9603043
Abstract
The Wilson approximate dynamics and the Einstein dynamics are compared for binary systems. At the second post-Newtonian approximation, genuine two-body aspects are found to differ by up to 114\%. In the regime of a formal innermost stable circular orbit (ISCO) the both dynamics differ by up to 7\%.
arXiv comment6 pages including 1 figure in eps format, LaTeX using psfig.sty