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Using the recently established formalism of a worldline quantum field theory (WQFT) description of the classical scattering of two spinless black holes, we compute the far-field time-domain waveform of the gravitational waves produced in the encounter at leading order in the post-Minkowskian (weak field, but generic velocity) expansion.
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Ira Z. Rothstein, “Progress in effective field theory approach to the binary inspiral problem,” Gen. Rel. Grav. 46
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