A perturbation-theory treatment of gravitational waves in a Robertson-Walker universe yields a next-to-leading-order correction factor to the waveform, but the quantitative expression appears to contain sign and factor errors.
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The imprint of cosmic expansion history on the propagation of gravitational waves
A perturbation-theory treatment of gravitational waves in a Robertson-Walker universe yields a next-to-leading-order correction factor to the waveform, but the quantitative expression appears to contain sign and factor errors.