Quantitative U/Th deposition and cleanliness control strategies in the JUNO site air

Abstract The Jiangmen Underground Neutrino Observatory (JUNO) employs a 20 kt liquid scintillator (LS) detector located 700 m underground. To meet its physics objectives, the LS must achieve an ultra-low $$^{238}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>238</mml:mn> </mml:mmultiscripts> </mml:math> U/ $$^{232}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>232</mml:mn> </mml:mmultiscripts> </mml:math> Th content of 10 $$^{-17}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>17</mml:mn> </mml:mrow> </mml:mmultiscripts> </mml:math> g/g. Given that airborne dust exhibits radioactivity about 12 orders of magnitude higher, exceptional cleanliness is essential during on-site installation. The total permissible dust mass in the 20 kt LS is only about 8 mg. To attain this, the acrylic vessel interior must comply with class 1000 cleanliness. Pre-filling water spray cleaning improves cleanliness by roughly two orders of magnitude, requiring the overall environment to be maintained between class 10,000 and 100,000. At JUNO, a cleanroom management system has been implemented across the 120,000 m $$^3$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>3</mml:mn> </mml:mmultiscripts> </mml:math> underground experimental hall. Since May 2022, continuous laser particle monitoring has consistently achieved an average cleanliness class of 74,000. Furthermore, we developed a method to directly measure $$^{238}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>238</mml:mn> </mml:mmultiscripts> </mml:math> U/ $$^{232}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>232</mml:mn> </mml:mmultiscripts> </mml:math> Th deposition rates on detector surfaces. Using ICP-MS, sensitivity reaches sub-ppt levels ( $$&lt;10^{-12}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mo>&lt;</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>12</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> g/g), enabling effective cleanliness control and assessment of external contamination during detector construction.

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Publication Details

Journal
The European Physical Journal C
Published
2026-03-08
DOI
https://doi.org/10.1140/epjc/s10052-026-15483-9
Primary Topic
Neutrino Physics Research
Type
article
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article

Quantitative U/Th deposition and cleanliness control strategies in the JUNO site air

Gaosong Li, Jie Zhao, Monica Sisti, Chenyang Cui et al.
The European Physical Journal C
Neutrino Physics Research
article

Quantitative U/Th deposition and cleanliness control strategies in the JUNO site air

Gaosong Li, Jie Zhao, Monica Sisti, Chenyang Cui, Yongpeng Zhang, Nan Wang
article en

Abstract

Abstract The Jiangmen Underground Neutrino Observatory (JUNO) employs a 20 kt liquid scintillator (LS) detector located 700 m underground. To meet its physics objectives, the LS must achieve an ultra-low $$^{238}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>238</mml:mn> </mml:mmultiscripts> </mml:math> U/ $$^{232}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>232</mml:mn> </mml:mmultiscripts> </mml:math> Th content of 10 $$^{-17}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>17</mml:mn> </mml:mrow> </mml:mmultiscripts> </mml:math> g/g. Given that airborne dust exhibits radioactivity about 12 orders of magnitude higher, exceptional cleanliness is essential during on-site installation. The total permissible dust mass in the 20 kt LS is only about 8 mg. To attain this, the acrylic vessel interior must comply with class 1000 cleanliness. Pre-filling water spray cleaning improves cleanliness by roughly two orders of magnitude, requiring the overall environment to be maintained between class 10,000 and 100,000. At JUNO, a cleanroom management system has been implemented across the 120,000 m $$^3$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>3</mml:mn> </mml:mmultiscripts> </mml:math> underground experimental hall. Since May 2022, continuous laser particle monitoring has consistently achieved an average cleanliness class of 74,000. Furthermore, we developed a method to directly measure $$^{238}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>238</mml:mn> </mml:mmultiscripts> </mml:math> U/ $$^{232}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mrow/> <mml:mn>232</mml:mn> </mml:mmultiscripts> </mml:math> Th deposition rates on detector surfaces. Using ICP-MS, sensitivity reaches sub-ppt levels ( $$&lt;10^{-12}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mo>&lt;</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>12</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> g/g), enabling effective cleanliness control and assessment of external contamination during detector construction.

The European Physical Journal CVol. 86(3)
Chinese Academy of Sciences (CN), Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca (IT), University of Chinese Academy of Sciences (CN), University of Milano-Bicocca (IT)
Industry, innovation and infrastructure
Openalex Percentile: Top 29%
Neutrino Physics Research
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