Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors
This paper demonstrates that by employing additional wave plates to detect axion-like dark matter-induced birefringence, space-based gravitational wave detectors can achieve optimal sensitivity across different frequency ranges using specific time-delay interferometry combinations, with the Monitor and Beacon schemes excelling at high frequencies and ASTROD-GW capable of probing dark matter masses down to .