7–11 Dec 2026
The University of Sydney
Australia/Sydney timezone
AIP Congress 2026

Recent results from the LUX-ZEPLIN dark matter experiment

8 Dec 2026, 12:15
15m
Belinda Hutchinson Building (The University of Sydney )

Belinda Hutchinson Building

The University of Sydney

Abercrombie St & Codrington St NSW 2008
Invited talk AIP | Astroparticle Physics (GAP) AIP GAP: Light Dark Matter

Speaker

Theresa Fruth (on behalf of the LZ collaboration) (University of Sydney)

Description

LUX-ZEPLIN (LZ) is a dark matter direct detection experiment located at the Sanford Underground Research Facility in Lead, South Dakota. At the heart of the detector is a dual-phase time projection chamber containing 7~tonnes of active liquid xenon. With a combined exposure of 4.2~tonne-years from the first two science campaigns, LZ has placed the most stringent limits on spin-independent WIMP-nucleon cross section for WIMP masses above $5~\textrm{GeV}/\textrm{c}^{2}$, reaching $2.2 \times 10^{-48}~\textrm{cm}^{2}$ for a $40~\textrm{GeV}/\textrm{c}^{2}$ WIMP mass.
LZ has also provided the first $>3~\sigma$ evidence of coherent elastic neutrino-nucleus scattering from $^{8}B$ solar neutrinos. Most recently, LZ searched an extended nuclear-recoil energy window for effective field theory and inelastic dark matter models, observing one event consistent with a nuclear recoil energy of $248 \pm 23 (stat) \pm 23 (sys)~\textrm{keV}$ in a region with low expected background. In this talk, I will give an overview of the LZ experiment, discuss its status, and report on its latest results in the search for dark matter and other rare phenomena.

The AIP 2026 Ruby Payne-Scott Award

I am the presenting author Yes

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