Comment on a relativistic model for coalescing neutron star binaries

Details Comment on a relativistic model for coalescing neutron star binaries Comment on a relativistic model for coalescing neutron star binaries

1996-03-25

arxiv.org/abs/gr-qc/9603043v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages including 1 figure in eps format, LaTeX using psfig.sty

Scientific paper

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\%.

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