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Close limit of grazing black hole collisions: non-spinning holes

Reinaldo Gleiser·Gaurav Khanna·Richard Price·Jorge Pullin
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Abstract

Using approximate techniques we study the final moments of the collision of two (individually non-spinnning) black holes which inspiral into each other. The approximation is based on treating the whole space-time as a single distorted black hole. We obtain estimates for the radiated energy, angular momentum and waveforms for the gravitational waves produced in such a collision. The results can be of interest for analyzing the data that will be forthcoming from gravitational wave interferometric detectors, like the LIGO, GEO, LISA, VIRGO and TAMA projects.

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Reinaldo Gleiser, Gaurav Khanna, Richard Price, Jorge Pullin. 2000-03-02. Close limit of grazing black hole collisions: non-spinning holes. https://doi.org/10.1088/1367-2630%2F2%2F1%2F303

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