The Jiangmen Underground Neutrino Observatory (JUNO) aims to determine the neutrino mass ordering. As a satellite experiment of JUNO, the Taishan Antineutrino Observatory (TAO) is designed to precisely measure the reactor antineutrino energy spectrum at a near site, providing essential reference data for JUNO. TAO represents a novel cryogenic liquid scintillator experiment, utilizing Silicon Photomultipliers (SiPMs) for photon detection and operating at -50∘C to suppress SiPM dark noise. A full-size prototype of the central detector of TAO (approximately 2% SiPMs installed) was assembled before its final deployment to the power plant. This paper presents the test results of the prototype using a Co-60 source at -50∘C, and using the surface flux of ground cosmic muons in the warm-up phase of the detector. The detector simulation software of TAO was adapted to the configuration of the prototype and the Monte Carlo prediction shows good agreement with the Co-60 data. A mild variation of the detector response was observed after correcting the temperature effect of the SiPM performance with the cosmic muon data.
Chen, Z., Xu, J., Li, Y., Qi, M., Anfimov, N., Cao, G., et al. (2026). Test results of the TAO prototype detector with Co-60 and cosmic muon. RADIATION DETECTION TECHNOLOGY AND METHODS [10.1007/s41605-025-00627-4].
Test results of the TAO prototype detector with Co-60 and cosmic muon
Fabbri, Andrea;Stanescu Farilla, Elia;Mari, Stefano M.;Petrucci, Fabrizio;
2026-01-01
Abstract
The Jiangmen Underground Neutrino Observatory (JUNO) aims to determine the neutrino mass ordering. As a satellite experiment of JUNO, the Taishan Antineutrino Observatory (TAO) is designed to precisely measure the reactor antineutrino energy spectrum at a near site, providing essential reference data for JUNO. TAO represents a novel cryogenic liquid scintillator experiment, utilizing Silicon Photomultipliers (SiPMs) for photon detection and operating at -50∘C to suppress SiPM dark noise. A full-size prototype of the central detector of TAO (approximately 2% SiPMs installed) was assembled before its final deployment to the power plant. This paper presents the test results of the prototype using a Co-60 source at -50∘C, and using the surface flux of ground cosmic muons in the warm-up phase of the detector. The detector simulation software of TAO was adapted to the configuration of the prototype and the Monte Carlo prediction shows good agreement with the Co-60 data. A mild variation of the detector response was observed after correcting the temperature effect of the SiPM performance with the cosmic muon data.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


