  The strong version of the nonviolent nonlocality proposal of Giddings
predicts "strong but soft" quantum metric fluctuations near black hole horizons
in an attempt to resolve the information paradox. To study observable
signatures of this proposal, we numerically solve Einstein's equations modified
by these fluctuations and analyze the gravitational wave signal from the
inspiral and merger of two black holes. In a model of evolution for such
fluctuations, we show that they lead to significant deviations in the observed
waveform, even when the black holes are still well separated, and could
potentially be observed by aLIGO.
