The LUX-ZEPLIN experiment, operated by a collaboration of 250 scientists and engineers from 39 institutions across six countries, announced its findings at the 2026 TeV Particle Astrophysics conference in Japan. The result has been submitted to a peer-reviewed journal and posted as a pre-print for community scrutiny.

The detector, managed by Lawrence Berkeley National Laboratory and located nearly a mile underground at the Sanford Underground Research Facility, uses 10 tonnes of ultrapure liquid xenon to search for Weakly Interacting Massive Particles (WIMPs) — a leading dark matter candidate. The team analyzed 220 live days of data collected between March 2023 and April 2024.

The single event they found sits in a region where dark matter signals are expected and competing backgrounds are extremely low. If caused by a WIMP, the particle would have a mass of at least 200 GeV/c², more than 200 times the mass of a proton, and would suggest a type of interaction beyond the simplest dark matter models.

Scientists are deliberately cautious. "We're very intrigued to see this event in the data," said Professor Rick Gaitskell of Brown University, the LZ collaboration spokesperson. "With only one event, we don't want to get ahead of ourselves. We are not claiming to have seen dark matter. But we have seen something interesting that we want to share."

There is roughly a 1-in-200 chance the result is a statistical fluke. The team will continue accumulating data to determine whether additional candidate events appear — a process that could take years. The collaboration is also contributing to the design of XLZD, a next-generation detector that may eventually be hosted at STFC's Boulby Underground Laboratory in the UK.