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Latest News

JUNO experiment delivers first physics results with world-leading precision just two months after completion

Fundamental Forces and Cosmic Evolution, Accelerated Scientific Discovery, ORIGINS, Research, Physics | 21.11.2025

Early data show that JUNO is ready to deliver frontier measurements in neutrino physics

Color photograph of a large research infrastructure, JUNO, which looks like golden glass bubbles
The Central Detector of JUNO from inside during the final phase of construction. 20,000 large and 25,000 small photomultiplier tubes are now detecting the scintillation light caused by neutrino interactions in the 35.4 m acrylic sphere filled with a liquid scintillation medium. Photo: JUNO Collaboration

The Institute of High Energy Physics (IHEP) of the Chinese Academy of Sciences held a press conference in Jiangmen City on November 19, 2025, to announce the successful completion of the Jiangmen Underground Neutrino Observatory (JUNO) and the release of its first physics results. After more than a decade of design, construction, and international collaboration, JUNO has become the world’s first next-generation, large-scale, high-precision neutrino detector to begin operation. 

Early data show that the detector’s key performance indicators fully meet or surpass design expectations, confirming that JUNO is ready to deliver frontier measurements in neutrino physics. A detailed paper describing the detector performance has been submitted to Chinese Physics C and was posted on the arXiv preprint server on November 18. 

At the press conference, Prof. Wen Liangjian, physics analysis coordinator of the JUNO Collaboration, presented the experiment’s first physics results. 

Using data collected between August 26 and November 2, 2025 — just 59 days after the start of operation — JUNO has already measured the so-called solar neutrino oscillation parameters, θ12 and Δm221, with a factor of 1.6 better precision than all previous experiments combined. 

These parameters, originally determined using solar neutrinos, can also be precisely measured by reactor antineutrinos. Earlier results from the two approaches showed a mild 1.5-sigma discrepancy, sometimes called the solar neutrino tension, hinting at possible new physics. The new JUNO measurement confirmed this difference, which can be proved or disproved by the JUNO experiment only using both solar and reactor neutrinos. A second detailed paper reporting these findings has been submitted for publication and was posted on the arXiv preprint server on November 18. 

“Achieving such precision within only two months of operation shows that JUNO is performing exactly as designed,” said Prof. Yifang Wang, JUNO project manager and spokesperson. “With this level of accuracy, JUNO will soon determine the neutrino mass ordering, test the three-flavor oscillation framework, and search for new physics beyond it.” 

JUNO is a major international collaboration led by IHEP. The project involves more than 700 scientists from 74 institutions across 17 countries and regions. “As Chair of the JUNO Institutional Board, I am proud to see this global effort reach such a milestone. JUNO’s success reflects the commitment and creativity of our entire international community.” said Prof. Marcos Dracos of the University of Strasbourg and CNRS/IN2P3 in France. 

“The scientific outcome announced today witnesses how fruitful the decade long effort of the JUNO Collaboration has been to assemble a state-of-the-art detector, incorporating many cutting-edge technical solutions, that will dominate the landscape of neutrino physics over the next years, providing results of exquisite precision. Many factors contributed to this success, among which the convergence of experience and expertise in liquid scintillator detectors and related analysis techniques—brought together by groups from around the world—was surely pivotal in achieving JUNO’s unprecedented level of performance”, added Dr. Gioacchino Ranucci of the Italian National Institute for Nuclear Physics (INFN) of Milano in Italy, deputy spokesperson of JUNO. 

The concept of JUNO was proposed in 2008 and received approval and funding from the Chinese Academy of Sciences and the Guangdong Provincial Government in 2013, followed by international contributions in 2014. Civil construction of the underground laboratory began in 2015, with detector installation starting in 2021 and completing in December 2024. After filling the detector with ultrapure water and 20 kilotons of liquid scintillator, JUNO began physics data taking on August 26, 2025. 

Years of dedicated R&D led to breakthroughs in key technologies, including high-efficiency photomultiplier tubes, ultra-transparent liquid scintillator, low-background materials, and precision calibration systems. At the heart of the experiment is a 35.4-metre-diameter acrylic sphere holding 20,000 tons of liquid scintillator, viewed by more than 20,000 large and 25,000 small photomultiplier tubes immersed in a 44-metre-deep water pool for shielding and muon tagging. 

“With its unprecedented detection sensitivity, JUNO will determine the neutrino mass ordering and measure oscillation parameters with sub-percent precision. It will also study solar, atmospheric, supernova, and geoneutrinos, and search for physics beyond the Standard Model. Designed for a scientific lifetime of about 30 years, JUNO can be upgraded into one of the world’s most sensitive detectors for neutrinoless double-beta decay, probing the absolute neutrino-mass scale and testing whether neutrinos are Majorana particles” said Dr. Hans Steiger, who heads TUM's contributions to JUNO. 

“JUNO will continue to produce important results and train new generations of physicists for decades to come,” said Prof. Jun Cao, director of IHEP and JUNO deputy spokesperson. 

“Our team is proud to have contributed its share to JUNO’s foundation,” added Dr. Steiger. “This experiment is a rare place where many independent streams of expertise from around the world converge into one coherent effort. JUNO’s first results show what this collective strength can achieve — and they open the way to discoveries that will shape neutrino physics for years to come.” 

 

Further information and links 

  • The research project is part of the ORIGINS cluster funded by the German Research Foundation (DFG) and the DFG's Collaborative Research Center (SFB) 1258 “Neutrinos and Dark Matter in Astro- and Particle Physics”.
  • JUNO Research project at TUM https://www.ph.nat.tum.de/en/e66/research/neutrino-physics-dark-matter-searches-with-large-volume-liquid-detectors/juno/
  • New research group established in particle physics https://uni-tuebingen.de/news-default/article/neue-forschungsgruppe-in-der-teilchenphysik-eingerichtet/ (in German) 

 

Contact for this article 

Dr. Hans Th. J. Steiger 
Technical University of Munich 
TUM School of Natural Sciences 
Chair of Precision Measurements under Extreme Conditions 
Collaborative Research Center 1258 ‘Neutrinos and Dark Matter in Astro- and Particle Physics’ 
hans.steiger@tum.de 

 

Press contact
communications(at)nat.tum.de
Our team

 

Original article: https://english.ihep.cas.cn/nw/han/y25/202511/t20251119_1132377.html 

 


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