On 18 December 2024, ultra-pure water begins to fill the bottom of the detector tank, above which is the spherical detector lined with photomultipliers. Image: JUNO.

Filling of the JUNO Detector Has Begun

Développements techniques Neutrino physics

The JUNO underground neutrino observatory, an international project in which CNRS Nuclear & Particle Physics is involved, has entered its final stage before commissioning its massive detector. On December 18, 2024, the filling process began in Jiangmen, southern China, at a rate of approximately 2,000 tons of ultra-pure water per day.

This operation concerns the spherical detector, the central element of the JUNO infrastructure, as well as the 44-meter-deep, 43.5-meter-diameter tank that houses it. The filling process is divided into two phases.

Une partie de l’équipe scientifique et technique de JUNO réunie au pied du détecteur juste avant le démarrage du remplissage. Désormais, l’accès est condamné et l’ensemble du volume va être immergé dans des dizaines de milliers de tonnes d’eau ultra pure. Image : JUNO
Part of the JUNO scientific and technical team gathered at the foot of the detector just before the filling process began. Access has now been blocked and the entire volume will be immersed in tens of thousands of tonnes of ultra-pure water. Image : JUNO

During the first phase, which will last two months, both the sphere and the tank will be filled simultaneously with ultra-pure water. This approach ensures a balanced pressure between the two components. It will also allow for an initial data-taking phase to calibrate the detector.

The second phase, set to begin in early February, will involve gradually replacing the ultra-pure water inside the sphere with a scintillating liquid. Once the detector is operational, this liquid will provide the instrument with its full sensitivity.

It is the interaction between neutrinos and this scintillating liquid that will produce light, which will then be captured, amplified, and converted into an electrical signal by the photomultiplier tubes lining the inner wall of the spherical detector. Meanwhile, the ultra-pure water in the tank surrounding the detector will serve both as a shield and as a detector of background radiation. It will work in conjunction with a cosmic muon detector positioned above the setup to identify and eliminate background noise from the atmosphere and surrounding rock.

As of January 27, 95% of the central detector had been filled with water. The filling of the scintillating liquid, expected to be completed by July 2025, will pave the way for the start of experimental data collection in August.

The JUNO Collaboration and French Laboratories

JUNO is a versatile neutrino experiment designed to determine the mass hierarchy of these elusive, omnipresent particles and to precisely measure their oscillation parameters. The JUNO detector is being developed and built by an international collaboration of more than 700 members from 17 countries and regions.

Several CNRS Nuclear & Particle Physics laboratories are contributing to the project, including CPPM (CNRS / Aix-Marseille University), IJCLab (CNRS / Paris-Saclay University), IPHC (CNRS / University of Strasbourg), LP2iB (CNRS / University of Bordeaux) and Subatech (CNRS / IMT Atlantique). 

These laboratories are actively involved in the development of the Top Tracker (muon veto system), the photomultiplier system of the central detector, and the data analysis efforts.

Contact

Cécile Jollet
Chercheuse au LP2I
Thomas Hortala
Chargé de communication
Laurent Vacavant
IN2P3 deputy scientific director for particle physics