The experiment, developed with strong contribution from a research group from Mainz, detected signals at the lowest neutrino energy ever achieved
PRESS RELEASE OF THE XENON COLLABORATION
Every second, tens of billions of neutrinos produced by nuclear fusion in the Sun pass through every square centimetre of the Earth—and through our bodies—almost without interacting. Although they are one of the most abundant particles emitted by the Sun, their extremely weak interactions make the detection of these elusive particles one of the greatest experimental challenges in particle physics.
Today, during a seminar hosted by the INFN Laboratori Nazionali del Gran Sasso (LNGS), Italy, the XENON Collaboration announced the first observation of low-energy solar neutrinos scattering off electrons in the XENONnT detector. The measurement extends the frontier of direct neutrino observations down to neutrino energies of about 17 keV, the lowest neutrino energy threshold ever achieved. The detected signal is dominated by pp neutrinos, produced in the proton–proton fusion reactions that power the Sun and account for the vast majority of its neutrino emission.
XENONnT was originally designed for the direct search for particle dark matter in our Galaxy. At its heart is a dual-phase xenon Time Projection Chamber containing 5.9 tonnes of ultra-pure liquid xenon, installed at LNGS, 1,400 metres beneath the Gran Sasso massif. The detector is surrounded by water Cherenkov detectors that identify and reject cosmic-ray muons and neutrons, and it is capable of reconstructing the tiny flashes of light and ionization signals produced when a particle interacts with the xenon target.
Observing this feeble low-energy neutrino signal at 5σ—the statistical significance conventionally used in particle physics to claim a discovery—required not only reducing the detector backgrounds to unprecedented levels of purity but also quantifying them precisely. The dominant challenge comes from trace amounts of radioactive radon constantly released by detector materials. Over many years, the XENON Collaboration has pioneered techniques to suppress this background through extensive material screening and a dedicated online cryogenic distillation system that continuously removes radon from the xenon. The Collaboration identified and constrained every relevant background contribution at exceptionally low rates, including beta decays from lead and krypton isotopes, smaller contributions from material-induced gamma rays, as well as other subdominant components.
The result further expands the scientific reach of XENONnT. Following the recent observation of coherent elastic neutrino–nucleus scattering from higher-energy solar neutrinos, this new measurement demonstrates that the same detector can probe complementary aspects of neutrino physics, while continuing its primary search for dark matter. XENONnT is thus emerging as one of the world’s most sensitive observatories for rare low-energy particle interactions.
The measurement also builds upon a long tradition of solar-neutrino research at LNGS. GALLEX/GNO provided the first measurements of the low-energy solar neutrino flux using radiochemical techniques, while Borexino pioneered the real-time spectroscopy of individual solar neutrino interactions with a neutrino energy threshold of 335 keV.
XENONnT now extends this legacy, lowering the solar-neutrino energy threshold to 17 keV. Beyond this achievement, XENONnT offers a glimpse of the future of rare-event physics. The technologies developed to build and operate one of the cleanest particle detectors are laying the foundation for the next generation of liquid-xenon observatories. The planned XLZD experiment, with a target mass an order of magnitude larger than XENONnT, aims to extend the search for dark matter to the highest sensitivities ever achieved and to measure low-energy solar neutrinos with exceptional precision, while opening new opportunities in neutrino physics and the study of other extremely rare processes.
“This observation of low-energy solar neutrinos demonstrates how advances driven by the search for dark matter are opening entirely new windows on the Universe,” said Elena Aprile, Professor at Columbia University and spokesperson of the XENON Collaboration. “It shows that technologies originally developed to observe some of the rarest interactions in nature are now enabling us to explore fundamental questions well beyond their original scientific goals.”
Technology developed in Mainz
The participating group at Johannes Gutenberg University Mainz (JGU) is led by Professor Uwe Oberlack, co-spokesperson for the XENON collaboration, one of the project’s founding members, and a member of the PRISMA++ Cluster of Excellence. The group is in particular responsible for the innovative XENONnT neutron and muon veto systems, which are designed to identify and filter out muons and neutrons from cosmic rays. This ensures that weak signals can be correctly identified. The low-energy calibration using an argon source, which was built as an internal source at the TRIGA reactor, also contributes to the precision of today’s results.
Publication:
Image
https://download.uni-mainz.de/presse/08_prisma++_xenon_sonnenneutrinos.png
Related Links:
https://www.iph.uni-mainz.de – Institute for Physics at JGU
https://xenonexperiment.org – XENON Experiment
Read more:
https://press.uni-mainz.de/first-measurement-of-a-nuclear-recoil-signal-from-solar-neutrinos-with-xenonnt/ – press release “First measurement of a nuclear recoil signal from solar neutrinos with XENONnT” (11 July 2024)
https://press.uni-mainz.de/first-wimp-search-results-from-the-xenonnt-experiment/ – press release “First WIMP search results from the XENONnT experiment” (23 March 2023)
https://press.uni-mainz.de/surprising-signal-in-the-xenon1t-dark-matter-experiment/ – press release “Surprising signal in the XENON1T dark matter experiment” (17 June 2020)
