JournalPhysical Review D (2470-0010), 110(4), 042001 ~ -
Enrollment typeSCIE
publication date 20240822
Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels.
