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In numerical simulations of black hole binaries, Pretorius and Khurana [Class.
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V. Cardoso et al., NR/HEP: roadmap for the future, arXiv:1201.5118
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Ref. [ 7 ] quotes a maximum fraction of energy radiated of 23 % 23\% , while its Fig. 2 shows a maximum number of 1.7 1.7 orbits; we have divided the former by the latter. For a boost of 2.9 2.9 , the maximal energy radiated went up to 35 % 35\% , but the maximal number of orbits is not given
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