Igor Ostrovskiy
(University of Alabama)
25/05/2022 13:30
Sara Leardini
25/05/2022 13:45
Hiu Sze Wu
(Karlsruhe Institute of Technology (KIT))
25/05/2022 14:00
Florian Tönnies
(University of Freiburg)
25/05/2022 14:15
Julia Mueller
25/05/2022 14:30
Hiu-Sze Wu
(Institute of Astroparticle Physics, Karlsruhe Institute of Technology (KIT), Germany)
The DARk matter Wimp search with liquid xenoN (DARWIN) observatory is a future dark matter detector aiming at reaching the sensitivity for WIMP at the neutrino floor and covering the mass range from 5 GeV/c2 to above 10 TeV/c2 [1]. The observatory uses the technology of a dual-phase time projection chamber (TPC) with 40 t active volume of liquid xenon (LXe) for the detection [1].
The...