Extrapolating Eqs. (27.71)–(27.73) into the strong-gravity regime, estimate the maximum gravitational- wave amplitude and emitted power for a nonspinning binary black hole with equal masses and with unequal masses. Compare with the results from numerical relativity discussed in the text.

Equations.

Transcribed Image Text:

Ф Ф + =(ер Дер-ёр дер), = 12 гдө 1 Ә r sin 0 аф =(ед дефтер дер); (27.71a)