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• W2016175541 abstract "We study a simple analytic solution to Einstein's field equations describing a thin spherical shell consisting of collisionless particles in circular orbit. We then apply two independent criteria for the identification of circular orbits, which have recently been used in the numerical construction of binary black hole solutions, and find that both yield equivalent results. Our calculation illustrates these two criteria in a particularly transparent framework and provides further evidence that the deviations found in those numerical binary black hole solutions are not caused by the different criteria for circular orbits." @default.
• W2016175541 created "2016-06-24" @default.
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• W2016175541 date "2002-11-22" @default.
• W2016175541 modified "2023-09-27" @default.
• W2016175541 title "Comparing criteria for circular orbits in general relativity" @default.
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• W2016175541 doi "https://doi.org/10.1103/physrevd.66.107501" @default.
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