Search arXivSearch

arXiv · 2511.14590

Initial performance results of the JUNO detector

Angel Abusleme·Thomas Adam·Kai Adamowicz·David Adey·Shakeel Ahmad·Rizwan Ahmed·Timo Ahola·Sebastiano Aiello·Fengpeng An·Guangpeng An·Costas Andreopoulos·Giuseppe Andronico·João Pedro Athayde Marcondes de André·Nikolay Anfimov·Vito Antonelli·Tatiana Antoshkina·Burin Asavapibhop·Didier Auguste·Margherita Buizza Avanzini·Andrej Babic·Jingzhi Bai·Weidong Bai·Nikita Balashov·Roberto Barbera·Andrea Barresi·Davide Basilico·Eric Baussan·Beatrice Bellantonio·Marco Bellato·JeanLuc Beney·Marco Beretta·Antonio Bergnoli·Enrico Bernieri·Nikita Bessonov·David Biaré·Daniel Bick·Lukas Bieger·Svetlana Biktemerova·Thilo Birkenfeld·David Blum·Simon Blyth·Sara Boarin·Manuel Boehles·Anastasia Bolshakova·Mathieu Bongrand·Aurélie Bonhomme·Clément Bordereau·Matteo Borghesi·Augusto Brigatti·Timothee Brugiere·Riccardo Brugnera·Riccardo Bruno·Jonas Buchholz·Antonio Budano·Max Buesken·Mario Buscemi·Severino Bussino·Jose Busto·Ilya Butorov·Marcel Büchner·Anatael Cabrera·Barbara Caccianiga·Boshuai Cai·Hao Cai·Xiao Cai·Yanke Cai·Yi-zhou Cai·Zhiyan Cai·Stéphane Callier·Steven Calvez·Antonio Cammi·Agustin Campeny·Dechang Cai·Chuanya Cao·Dewen Cao·Guofu Cao·Jun Cao·Yaoqi Cao·Rossella Caruso·Aurelio Caslini·Cédric Cerna·Vanessa Cerrone·Daniele Cesini·Chi Chan·Jinfan Chang·Yun Chang·Milo Charavet·Tim Charissé·Auttakit Chatrabhuti·Chao Chen·Guoming Chen·Haitao Chen·Haotian Chen·Jiahui Chen·Jian Chen·Jing Chen·Junyou Chen·Lihao Chen·Mali Chen·Mingming Chen

Abstract

The Jiangmen Underground Neutrino Observatory (JUNO) started physics data taking on 26 August 2025. JUNO consists of a 20-kton liquid scintillator central detector, surrounded by a 35 kton water pool serving as a Cherenkov veto, and almost 1000 m$^2$ of plastic scintillator veto on top. The detector is located in a shallow underground laboratory with an overburden of 1800 m.w.e. This paper presents the performance results of the detector, extensively studied during the commissioning of the water phase, the subsequent liquid scintillator filling phase, and the first physics runs. The liquid scintillator achieved an attenuation length of 20.6 m at 430 nm, while the high coverage PMT system and scintillator together yielded about 1785 photoelectrons per MeV of energy deposit at the detector centre, measured using the 2.223 MeV $γ$ from neutron captures on hydrogen with an Am-C calibration source. The reconstructed energy resolution is 3.4% for two 0.511 MeV $γ$ at the detector centre and 2.9% for the 0.93 MeV quenched Po-214 alpha decays from natural radioactive sources. The energy nonlinearity is calibrated to better than 1%. Intrinsic contaminations of U-238 and Th-232 in the liquid scintillator are below 10$^{-16}$ g/g, assuming secular equilibrium. The water Cherenkov detector achieves a muon detection efficiency better than 99.9% for muons traversing the liquid scintillator volume. During the initial science runs, the data acquisition duty cycle exceeded 97.8%, demonstrating the excellent stability and readiness of JUNO for high-precision neutrino physics.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Angel Abusleme, Thomas Adam, Kai Adamowicz, David Adey, Shakeel Ahmad, Rizwan Ahmed, Timo Ahola, Sebastiano Aiello, Fengpeng An, Guangpeng An, Costas Andreopoulos, Giuseppe Andronico, João Pedro Athayde Marcondes de André, Nikolay Anfimov, Vito Antonelli, Tatiana Antoshkina, Burin Asavapibhop, Didier Auguste, Margherita Buizza Avanzini, Andrej Babic, Jingzhi Bai, Weidong Bai, Nikita Balashov, Roberto Barbera, Andrea Barresi, Davide Basilico, Eric Baussan, Beatrice Bellantonio, Marco Bellato, JeanLuc Beney, Marco Beretta, Antonio Bergnoli, Enrico Bernieri, Nikita Bessonov, David Biaré, Daniel Bick, Lukas Bieger, Svetlana Biktemerova, Thilo Birkenfeld, David Blum, Simon Blyth, Sara Boarin, Manuel Boehles, Anastasia Bolshakova, Mathieu Bongrand, Aurélie Bonhomme, Clément Bordereau, Matteo Borghesi, Augusto Brigatti, Timothee Brugiere, Riccardo Brugnera, Riccardo Bruno, Jonas Buchholz, Antonio Budano, Max Buesken, Mario Buscemi, Severino Bussino, Jose Busto, Ilya Butorov, Marcel Büchner, Anatael Cabrera, Barbara Caccianiga, Boshuai Cai, Hao Cai, Xiao Cai, Yanke Cai, Yi-zhou Cai, Zhiyan Cai, Stéphane Callier, Steven Calvez, Antonio Cammi, Agustin Campeny, Dechang Cai, Chuanya Cao, Dewen Cao, Guofu Cao, Jun Cao, Yaoqi Cao, Rossella Caruso, Aurelio Caslini, Cédric Cerna, Vanessa Cerrone, Daniele Cesini, Chi Chan, Jinfan Chang, Yun Chang, Milo Charavet, Tim Charissé, Auttakit Chatrabhuti, Chao Chen, Guoming Chen, Haitao Chen, Haotian Chen, Jiahui Chen, Jian Chen, Jing Chen, Junyou Chen, Lihao Chen, Mali Chen, Mingming Chen. 2025-11-18. Initial performance results of the JUNO detector. https://arxiv.org/abs/2511.14590

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Search for dark matter in a signature with a four-prong large-radius jet in proton-proton collisions at $\sqrt{s}$ = 13 TeV

A search for a pair of nonprompt dark matter (DM) candidates produced in association with an initial-state radiation jet, in a signature containing a four-prong large-radius jet, is presented. The signal model contains a heavy vector or axial-vector mediator, which produces long-lived dark-sector particles that decay to a stable DM particle and a light boson, which decays to quarks. The analysis is based on data collected in the years 2016$-$2018 with the CMS detector at the LHC in proton-proton collisions at $\sqrt{s}$ = 13 TeV, corresponding to an integrated luminosity of 138 fb$^{-1}$. Signal candidates feature large-radius jets, which are identified using a jet substructure tagger based on a graph neural network. The large-radius jet aims to reconstruct the decay of light DM mediators into four quarks, which are produced in association with two stable DM particles. The standard model background contributions are estimated from data using dedicated control regions. The missing transverse momentum spectrum is probed for a potential signal over the expected background. No significant excess over the standard model expectation is observed. Upper limits at 95% confidence level are set on the signal strength as functions of either the mediator mass or the relevant coupling. This is the first search for a pair of nonprompt DM candidates in the Lorentz-boosted topology, characterized by a large-radius jet and large missing transverse momentum.

hep-ex

Charge-dependent atmospheric muon flux at 17 GV geomagnetic cutoff with the mini-ICAL detector

The Iron CALorimeter (ICAL) detector at the India-Based Neutrino Observatory (INO) was conceived as an underground experiment designed to measure atmospheric neutrino oscillation parameters. As part of the R\&D programme, a scaled prototype (mini-ICAL), 85\,ton, approximately 1/600$^{\mathrm{th}}$ the mass of the full detector, was constructed at the IICHEP Transit Campus, Madurai (altitude 150\,m; latitude 9.9372$^\circ$\,N; longitude 78.013$^\circ$\,E; geomagnetic latitude 1.44$^\circ$\,N; vertical cutoff rigidity 17\,GV) and operated between 2018 and 2022. The prototype enabled measurements of charge-dependent cosmic muon spectra in the vicinity of the geomagnetic equator and provided an important validation of detector performance, reconstruction algorithms, and simulation frameworks for the ICAL experiment. Differential fluxes of $μ^{-}$ and $μ^{+}$ were measured over the momentum range $\sim$\,1--5\,GeV/c. The obtained momentum spectra are systematically lower than those reported at sites with smaller geomagnetic cutoff rigidities, consistent with the suppression of low- and intermediate-rigidity primary cosmic rays at the 17\,GV cutoff. The measurements are compared with predictions from different hadronic interaction models available in CORSIKA simulations.

hep-ex

Laboratory constraints on peV-scale mass splitting between ordinary and sterile neutron states

Sterile states of matter, represented by a parallel ``mirror'' sector, may contribute to the observed dark matter in the Universe. We investigated the parameter space of neutron $(n)$ to mirror-neutron $(n')$ oscillations, in the case where the two states are not necessarily mass-degenerate, taking into account interactions in the mirror sector. By tuning the magnitude of an applied magnetic-field in the range $5~μ\mathrm{T} < B < 360~μ\mathrm{T}$ to corresponding resonance conditions for finite mass splitting, we derive exclusion limits for the $n-n'$ oscillation time constant reaching about $20~\text{s}$ over the mass-difference range $0.3 - 22~\text{peV}$. In parts of this parameter range, our limits exceed the model-dependent neutron-star-cooling bound, providing the first experimental constraints in this scenario that are more stringent than this astrophysical estimate.

hep-ex