Orbital motion of a space GW detector creates sideband patterns that differ between gravitational waves and ultralight dark matter, enabling discrimination by counting harmonics.
hp(t) denotes the time-domain GW waveforms, which is related to that in the radiation frame by h× ± ih+ = e∓2iψ(hrad × ± ihrad + ) with ψ the polarization angle
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Identifying Monochromatic Signals in LISA and Taiji via Spectral Split: Gravitational Waves versus Ultralight Dark Matter
Orbital motion of a space GW detector creates sideband patterns that differ between gravitational waves and ultralight dark matter, enabling discrimination by counting harmonics.