CORDIS Project
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This project aims to explore the nature of ultralight dark matter by utilizing gravitational wave detectors. It will develop new methods to distinguish between different types of ultralight dark matter signals and improve detection capabilities in unexplored frequency ranges.
Despite compelling astrophysical and cosmological evidence for dark matter, its nature remains unknown.
Ultralight dark matter (ULDM) is a well-motivated candidate, producing distinctive signatures that can be probed with gravitational wave (GW) interferometers.
Spin-0, spin-1, and spin-2 ULDM couple differently to Standard Model particles, inducing measurable effects in GW detectors, but distinguishing between ULDM spins, and between ULDM and continuous astrophysical GWs, is challenging due to…
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