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Last orbits of binary black holes
General Relativity and Quantum Cosmology · Submitted 2 May 2002
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Comparison with third order post-Newtonian calculations indicates a rather good agreement until the innermost stable circular orbit.
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The abstract, sentence by sentence
Binary black hole systems in the pre-coalescence stage are numerically constructed by demanding that the associated spacetime admits a helical Killing vector. Comparison with third order post-Newtonian calculations indicates a rather good agreement until the innermost stable circular orbit.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Binary black hole systems in the pre-coalescence stage are numerically constructed by demanding that the associated spacetime admits a helical Killing vector. | method 0.96 | 0.81 | 0.09 | asserted 1.00 |
| s1 | Comparison with third order post-Newtonian calculations indicates a rather good agreement until the innermost stable circular orbit. | result 0.99 | 0.74 | 0.35 | hedged possibility 0.97 |
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Original abstract
Binary black hole systems in the pre-coalescence stage are numerically constructed by demanding that the associated spacetime admits a helical Killing vector. Comparison with third order post-Newtonian calculations indicates a rather good agreement until the innermost stable circular orbit.
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