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Home » News & Topics » [Research] Observation of Excess Events in the XENON1T Dark Matter Experiment

[Research] Observation of Excess Events in the XENON1T Dark Matter Experiment

2020.06.18

Scientists from the international XENON collaboration, an international experimental group including the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), University of Tokyo; the Institute for Cosmic Ray Research (ICRR), University of Tokyo; the Institute for Space-Earth Environmental Research (ISEE), Nagoya University; the Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI), Nagoya University; and the Graduate School of Science, Kobe University, announced today that data from their XENON1T, the world’s most sensitive dark matter experiment, show a surprising excess of events. The scientists do not claim to have found dark matter. Instead, they say to have observed an unexpected rate of events, the source of which is not yet fully understood. The signature of the excess is similar to what might result from a tiny residual amount of tritium (a hydrogen atom with one proton and two neutrons), but could also be a sign of something more exciting—such as the existence of a new particle known as the solar axion or the indication of previously unknown properties of neutrinos.

From Nagoya University, Professor. Yoshitaka Itow (KMI, ISEE), Associate Professor. Masaki Yamashita (ISEE), YLC Assistant Professor Shingo Kazama (KMI, IAR) are involved in the collaboration. 

Next phase XENONnT experiment will have three times larger liquid xenon mass than that of XENON1T and will be started to take data in 2020. Nagoya group contributes the liquid xenon purification and neutron veto counter, which will improve the detector’s sensitivity. XENONnT will explore not only WIMP dark matter but also axion and neutrinoless double beta decay. I am very much looking forward to seeing the new data. (Masaki YAMASHITA, Designated Associate Professor / ISEE)

XENONnT experiment, which will start its operation this year, can confirm if the excess observed in the XENON1T comes from a new physics beyond the Standard Model or a  background contaminant with just several months’ data. As a leader of the analysis group for the XENONnT experiment, I’ll do my best to realize the world’s largest and most sensitive detector for the excess observed in the XENON1T as well as for the WIMP dark matter.(Shingo Kazama,  YLC Assistant Professor / KMI)

 

Press Release

 

XENON collaboration
Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo (Kavli IPMU)
Institute for Cosmic Ray Research, The University of Tokyo (ICRR)
Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University
Graduate School of Science, Kobe University

 

 

Scientists from the international XENON collaboration, an international ex-perimental group including the Kavli Institute for the Physics and Mathemat-ics of the Universe (Kavli IPMU), University of Tokyo; the Institute for Cos-mic Ray Research (ICRR), University of Tokyo; the Institute for Space-Earth Environmental Research (ISEE), Nagoya University; the Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI), Nagoya Universi-ty; and the Graduate School of Science, Kobe University, announced today that data from their XENON1T, the world’s most sensitive dark matter exper-iment, show a surprising excess of events. The scientists do not claim to have found dark matter. Instead, they say to have observed an unexpected rate of events, the source of which is not yet fully understood. The signature of the excess is similar to what might result from a tiny residual amount of tritium (a hydrogen atom with one proton and two neutrons), but could also be a sign of something more exciting—such as the existence of a new particle known as the solar axion or the indication of previously unknown properties of neu-trinos.

XENON1T was operated deep underground at the INFN Laboratori Na-zionali del Gran Sasso in Italy, from 2016 to 2018. It was primarily designed to detect dark matter, which makes up 85% of the matter in the universe. So far, scientists have only observed indirect evidence of dark matter, and a de-finitive, direct detection is yet to be made. So-called WIMPs (Weakly Inter-acting Massive Particles) are among the theoretically preferred candidates, and XENON1T has thus far set the best limit on their interaction probability over a wide range of WIMP masses. In addition to WIMP dark matter, XEN-ON1T was also sensitive to different types of new particles and interactions that could explain other open questions in physics. Last year, using the same detector, these scientists published in Nature the observation of the rarest nuclear decay ever directly measured.

The XENON1T detector was filled with 3.2 tonnes of ultra-pure liquefied xenon, 2.0 t of which served as a target for particle interactions. When a par-ticle crosses the target, it can generate tiny signals of light and free electrons from a xenon atom. Most of these interactions occur from particles that are known to exist. Scientists therefore carefully estimated the number of back-ground events in XENON1T. When data of XENON1T were compared to known backgrounds, a surprising excess of 53 events over the expected 232 events was observed.

This raises the exciting question: where is this excess coming from? One explanation could be a new, previously unconsidered source of back-ground, caused by the presence of tiny amounts of tritium in the XENON1T detector. Tritium, a radioactive isotope of hydrogen, spontaneously decays by emitting an electron with an energy similar to what was observed. Only a few tritium atoms for every 1025 (10,000,000,000,000,000,000,000,000!) xenon atoms would be needed to explain the excess. Currently, there are no inde-pendent measurements that can confirm or disprove the presence of tritium at that level in the detector, so a definitive answer to this explanation is not yet possible.

More excitingly, another explanation could be the existence of a new parti-cle. In fact, the excess observed has an energy spectrum similar to that ex-pected from axions produced in the Sun. Axions are hypothetical particles that were proposed to preserve a time-reversal symmetry of the nuclear force, and the Sun may be a strong source of them. While these solar axions are not dark matter candidates, their detection would mark the first observation of a well-motivated but never observed class of new particles, with a large impact on our understanding of fundamental physics, but also on astrophysical phe-nomena. Moreover, axions produced in the early universe could also be the source of dark matter.

Alternatively, the excess could also be due to neutrinos, trillions of which pass through your body, unhindered, every second. One explanation could be that the magnetic moment (a property of all particles) of neutrinos is larger than its value in the Standard Model of elementary particles. This would be a strong hint to some other new physics needed to explain it.

Of the three explanations considered by the XENON collaboration, the ob-served excess is most consistent with a solar axion signal. In statistical terms, the solar axion hypothesis has a significance of 3.5 sigma, meaning that there is about a 2/10,000 chance that the observed excess is due to a random fluc-tuation rather than a signal. While this significance is fairly high, it is not large enough to conclude that axions exist. The significance of both the triti-um and neutrino magnetic moment hypotheses corresponds to 3.2 sigma, meaning that they are also consistent with the data.

XENON1T is now upgrading to its next phase–XENONnT–with an active xenon mass three times larger and a background that is expected to be lower than that of XENON1T. With better data from XENONnT, the XENON col-laboration is confident it will soon find out whether this excess is a mere sta-tistical fluke, a background contaminant, or something far more exciting: a new particle or interaction that goes beyond known physics. The XENON collaboration comprises 163 scientists from 28 institutions across 11 countries. Results from this research were announced during an online seminar for researchers by the XENON collaboration on Wednesday, June 17 (16:00, Central European Summer Time; 23:00, Japan Standard Time)

Reference URL: Press release by XENON collaboration (English)

http://www.xenon1t.org

Paper details

Journal: [[arXiv]] Title: Observation of Excess Electronic Recoil Events in XENON1T
Author: XENON Collaboration

Pre-print (arXiv.org page) https://arxiv.org/abs/2006.09721

 

The bottom of the XENON1T time projection chamber from below. The back ends of the photomultiplier tubes recording the scintillation light from events inside the chamber are clearly visible in their PTFE holding structure, as are the copper rings in the cylinder walls that shape the drift field which guides the ionisation signal electrons to the top of the chamber. Credit: XENON Collaboration
The XENON1T detector suspended at the center of its surrounding water Cherenkov shield. The detector is a time projection chamber filled with liquid xenon. It is encased in a double walled stainless steel container for heat insulation. The surrounding water Cherenkov detector tags cosmic ray muons using the same detector technology as Super-Kamiokande, and was first used to shield a dark matter detector at the XMASS experiment in Kamioka. Credit: XENON Collaboration

Glossary

XENON collaboration

An international alliance consisting of 163 researchers from 28 institutions in 10 countries and regions, mainly in Europe, the United States, and Japan. Institutions from Japan include the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), University of Tokyo; the Institute for Cosmic Ray Research (ICRR), University of Tokyo; the Institute for Space-Earth Environmental Research (ISEE), Nagoya University; the Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI), Nagoya University; and the Graduate School of Science, Kobe University.

 

Tritium

A rare, radioactive, unstable isotope of hydrogen, Tritium has a nucleus containing one proton and two neutrons—unlike common hydrogen atoms, which contain one proton (hydrogen-1) or one proton and one neutron (hydrogen-2). Tritium is produced when cosmic rays fall down to Earth and react with oxygen and nitrogen in the atmosphere. Only very small amounts of the isotope can be found in the natural world.

 

Axion

An undiscovered but theoretically predicted elementary particle. The phenomenon that CP-symmetry is preserved has not been observed in experiments involving the strong nuclear force (strong interaction) only, and yet quantum chromodynamics (QCD), which describes the strong force, seems to preserve CP-symmetry. As there is no known basis in QCD why it should be preserved, this gives rise to a contradiction—called the strong CP problem. Particle physicists Roberto Peccei and Helen Quinn proposed a solution to this contradiction. The new symmetry shown by the Peccei-Quinn theory tries to resolve the CP problem by a spontaneous process of symmetry breaking that predicts—and results in—axions, the search for which is still being undertaken via various experiments.

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