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General Relativity and Quantum Cosmology

Title: Comment on a relativistic model for coalescing neutron star binaries

Authors: R. Rieth, G. Schäfer (Max--Plank--Society, Research Unit ,,Theory of Gravitation'' at the Friedrich Schiller University, Jena, Germany)

(Submitted on 25 Mar 1996)

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\%.

Comments:	6 pages including 1 figure in eps format, LaTeX using psfig.sty
Subjects:	General Relativity and Quantum Cosmology (gr-qc)
Report number:	AGG 44
Cite as:	arXiv:gr-qc/9603043v1

Submission history

From: R. Rieth [view email]
[v1] Mon, 25 Mar 1996 17:56:02 GMT (9kb)

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