Comment on a relativistic model for coalescing neutron star binaries
General Relativity and Quantum Cosmology
2019-08-15 v1
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\%.
Keywords
Cite
@article{arxiv.gr-qc/9603043,
title = {Comment on a relativistic model for coalescing neutron star binaries},
author = {R. Rieth and G. Schäfer},
journal= {arXiv preprint arXiv:gr-qc/9603043},
year = {2019}
}
Comments
6 pages including 1 figure in eps format, LaTeX using psfig.sty