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arXiv · gr-qc/9603043

Comment on a relativistic model for coalescing neutron star binaries

R. Rieth·G. Schäfer
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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\%.

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R. Rieth, G. Schäfer. 1996-03-25. Comment on a relativistic model for coalescing neutron star binaries. https://arxiv.org/abs/gr-qc/9603043

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