Speaker
Huan Zhang
Description
LUX-ZEPLIN(LZ) and its next generation XENON-LZ-DARWIN(XLZD) are designed to search for dark matter using two-phase liquid xenon time projection chambers. LZ has been processing its WS2024 upper-limits for dark matter candidates, like axion-like particles(ALPs). Meanwhile, XLZD has been projecting sensitivity for several signal’s models, including weakly interacting massive particles(WIMPs), solar axion, neutrinos, and ALPs. In this poster, I will show LZ most up-to-date upper-limits and XLZD projected sensitivities for signal models of low-energy electron-recoil(ER) group.
