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• W2077828384 abstract "We study the radiation of energy and linear momentum emitted to infinity by the head-on collision of binary black holes, starting from rest at a finite initial separation, in the extreme mass ratio (particle) limit. For these configurations we identify the radiation that may be attributed to a choice of the initial three geometry. This identification suggests that for evolution of holes from initial proper separations ${L}_{0}>~7M,$ the radiated energy and momentum from head-on collisions will not be dominated by that choice. For non-head-on orbits, where the amount of radiation is orders of magnitude larger, computations may be even less sensitive to the choice of initial three geometry." @default.
• W2077828384 created "2016-06-24" @default.
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• W2077828384 date "2004-04-28" @default.
• W2077828384 modified "2023-09-25" @default.
• W2077828384 title "Radiation content of conformally flat initial data" @default.
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• W2077828384 doi "https://doi.org/10.1103/physrevd.69.087503" @default.
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