24–27 Mar 2025
UCLA Physics and Astronomy Building 1-425
US/Pacific timezone

R&D for XLZD, the Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics

Not scheduled
20m
UCLA Physics and Astronomy Building 1-425

UCLA Physics and Astronomy Building 1-425

475 Portola Plaza, Los Angeles, CA 90095 darkmatter@physics.ucla.edu
Poster

Speaker

Yanina Biondi (Karlruhe Institute for Technology)

Description

Liquid xenon time projection chambers (LXe TPCs) represent the forefront of sensitivity in WIMP dark matter direct detection. The goal of the next-generation experiment XLZD (XENON-LZ-DARWIN) is to explore the WIMP parameter space down to the neutrino fog, where coherent neutrino-nucleus scattering dominates. Achieving this demands a combination of ultra-low background levels and a tenfold increase in active target mass compared to current detectors. The XLZD detector is designed for a 60-tonne active mass. Together with further improvements on radon and neutron backgrounds, this opens up a plethora of science channels, including the neutrino-less double-beta decay of ^{136}Xe, axions and axion-like particles, neutrinos from supernovae and different rare nuclear processes. A broad R&D program is currently addressing technical challenges towards the realization of the experiment. Key areas include scaling up dual-phase TPC technology while ensuring ultra-low radioactivity materials, advanced purification techniques, and enhanced detection efficiencies. This presentation will delve into the progress of the R&D program that combines the expertise of three international collaborations.

Author

Yanina Biondi (Karlruhe Institute for Technology)

Presentation materials

There are no materials yet.