News Release 

Observation of Excess Events in the XENON1T Dark Matter Experiment

Kavli Institute for the Physics and Mathematics of the Universe

June 16, 2020 Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU)

The content of the press release is embargoed until 16:00 Central European Summer Time (23:00, Japan Standard Time)on 17, June 2020. Journalists should credit the XENON collaboration as the source of stories covered.

Observation of Excess Events in the XENON1T Dark Matter Experiment

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.

XENON1T was operated deep underground at the INFN Laboratori Nazionali 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 definitive, direct detection is yet to be made. So-called WIMPs (Weakly Interacting 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, XENON1T 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 particle 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 background 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 background, 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 independent 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 particle. In fact, the excess observed has an energy spectrum similar to that expected 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 phenomena. 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 observed 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 fluctuation 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 tritium 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 collaboration is confident it will soon find out whether this excess is a mere statistical fluke, a background contaminant, or something far more exciting: a new particle or interaction that goes beyond known physics.

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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)

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*Activities related to the XENON1T and XENONnT experiments of the Japan Group are supported by the Japan Society for the Promotion of Science and the Grants-in-Aid for Scientific Research (KAKENHI) (18H03697, 18KK0082, 19H05802, 19H05805, 19H00675, 19H01920).

Reference URL: Press release by XENON collaboration (English)
http://www.xenon1t.org
The press release will be available above shortly after the embargo date and time expires

Paper details
Journal: [[arXiv]]
Title: Observation of Excess Events in the XENON1T Dark Matter Experiment
Author: XENON Collaboration
Pre-print (arXiv.org page)
https://arxiv.org
*The paper will be released to arXiv after the XENON collaboration online seminar.

Notes
The content of the press release is embargoed until 16:00 (Central European Summer Time; 23:00 (Japan Standard Time)) on 17, June 2020.

Research contact
Kai Martens
Principal Investigator and Associate Professor
Kavli Institute for the Physics and Mathematics of the Universe; Director, Kamioka Branch Office
XENON Experimental International Collaborative Research Group; Japan Representative
E-mail: kai.martens@ipmu.jp
Tel: 0578-85-9513

Moriyama Shigetaka
Professor
Institute for Cosmic Ray Research; Kavli Institute for the Physics and Mathematics of the Universe
The University of Tokyo
E-mail: moriyama@icrr.u-tokyo.ac.jp
Tel: 0578-85-9604

Itow Yoshitaka
Professor
Institute for Space-Earth Environmental Research; Kobayashi-Maskawa Institute for the Origin of Particles and the Universe
Nagoya University
E-mail: itow@isee.nagoya-u.ac.jp
Tel: 052-789-4319

Miuchi Kentaro
Associate Professor
Graduate School of Science
Kobe University
E-mail: miuchi@phys.sci.kobe-u.ac.jp
Tel: 078-803-5637

Media Contact
John Amari
Press officer
Kavli Institute for the Physics and Mathematics of the Universe
The University of Tokyo
E-mail: press@ipmu.jp
TEL: 080-4056- 2767

Nakamura Makio
Public Relations Office
Institute for Cosmic Ray Research
The University of Tokyo
E-mail: icrr-pr@icrr.u-tokyo.ac.jp Tel: 080-4869-4539

Minamizaki Azusa
Public Relations Office
Kobayashi-Maskawa Institute for the Origin of Particles and the Universe
Nagoya University
E-mail: pr-office@kmi.nagoya-u.ac.jp Tel: 052-789-2896

Public Relations Division, General Affairs Department
Kobe University
E-mail: ppr-kouhoushitsu@office.kobe-u.ac.jp Tel: 078-803-6678

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Image captions
detectorWithOnePerson:
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.?

x1t-closed:
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.

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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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