Dark Count Rate Stability of JUNO 20-inch PMTs in Mass Testing

Fuente: arXiv
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Main Authors: Li, Min, Rodphai, Narongkiat, Liu, Caimei, Wang, Zhimin, Peng, Zhaoyuan, Wang, Jun, Anfimov, Nikolay, Korablev, Denis, Lachenmaier, Tobias, Olshevskiy, Alexander G., Qin, Zhonghua, Sterr, Tobias, Tietzsch, Alexander Felix, Zhao, Rong, Wang, Wei, Wen, Kaile, Wonsak, Bjoern Soenke, Xie, Wan, Xu, Meihang, Zhang, Yu
Format: Preprint
Published: 2025
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author Li, Min
Rodphai, Narongkiat
Liu, Caimei
Wang, Zhimin
Peng, Zhaoyuan
Wang, Jun
Anfimov, Nikolay
Korablev, Denis
Lachenmaier, Tobias
Olshevskiy, Alexander G.
Qin, Zhonghua
Sterr, Tobias
Tietzsch, Alexander Felix
Zhao, Rong
Wang, Wei
Wen, Kaile
Wonsak, Bjoern Soenke
Xie, Wan
Xu, Meihang
Zhang, Yu
author_facet Li, Min
Rodphai, Narongkiat
Liu, Caimei
Wang, Zhimin
Peng, Zhaoyuan
Wang, Jun
Anfimov, Nikolay
Korablev, Denis
Lachenmaier, Tobias
Olshevskiy, Alexander G.
Qin, Zhonghua
Sterr, Tobias
Tietzsch, Alexander Felix
Zhao, Rong
Wang, Wei
Wen, Kaile
Wonsak, Bjoern Soenke
Xie, Wan
Xu, Meihang
Zhang, Yu
contents The Jiangmen Underground Neutrino Observatory (JUNO) is an ambitious multipurpose neutrino experiment designed to determine the neutrino mass ordering, with an impressive energy resolution goal of at least 3% at 1 MeV. To achieve a photon detection coverage of approximately 75%, JUNO will utilize two types of 20-inch photomultiplier tubes (PMTs): the large PMT (LPMT) and the microchannel plate PMT (MCP-PMT). A significant concern in high-precision neutrino measurements is the dark count rate (DCR) of PMTs, which introduces noise that can adversely affect energy measurement accuracy. During the mass testing phase of the JUNO 20-inch PMTs, comprehensive measurements of the DCR were undertaken. These measurements not only captured the DCR values of individual PMTs but also examined the stability and temperature dependence of the DCR at an operating gain of (1x10^7). This paper presents a detailed characterization of the DCR of the JUNO 20-inch PMTs, investigating factors such as cooling time, temperature variations, and long-term stability using the JUNO Pan-Asia PMT testing facilities. The results reveal distinct DCR characteristics between the two types of PMTs, providing valuable insights into the nature of DCR and its implications for JUNO's scientific objectives. In addition to performance characterization, we implemented a monitoring system to track DCR stability over time. Notably, several spikes in DCR were identified, prompting a preliminary investigation into their causes. Potential factors contributing to these spikes, such as flasher events, were explored using coincidence rate analysis and complementary imaging techniques. The findings from this study are crucial for optimizing the performance of PMTs in JUNO, ultimately aiding the experiment in achieving its goals related to neutrino physics.
format Preprint
id arxiv_https___arxiv_org_abs_2506_15164
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Dark Count Rate Stability of JUNO 20-inch PMTs in Mass Testing
Li, Min
Rodphai, Narongkiat
Liu, Caimei
Wang, Zhimin
Peng, Zhaoyuan
Wang, Jun
Anfimov, Nikolay
Korablev, Denis
Lachenmaier, Tobias
Olshevskiy, Alexander G.
Qin, Zhonghua
Sterr, Tobias
Tietzsch, Alexander Felix
Zhao, Rong
Wang, Wei
Wen, Kaile
Wonsak, Bjoern Soenke
Xie, Wan
Xu, Meihang
Zhang, Yu
Instrumentation and Detectors
High Energy Physics - Experiment
The Jiangmen Underground Neutrino Observatory (JUNO) is an ambitious multipurpose neutrino experiment designed to determine the neutrino mass ordering, with an impressive energy resolution goal of at least 3% at 1 MeV. To achieve a photon detection coverage of approximately 75%, JUNO will utilize two types of 20-inch photomultiplier tubes (PMTs): the large PMT (LPMT) and the microchannel plate PMT (MCP-PMT). A significant concern in high-precision neutrino measurements is the dark count rate (DCR) of PMTs, which introduces noise that can adversely affect energy measurement accuracy. During the mass testing phase of the JUNO 20-inch PMTs, comprehensive measurements of the DCR were undertaken. These measurements not only captured the DCR values of individual PMTs but also examined the stability and temperature dependence of the DCR at an operating gain of (1x10^7). This paper presents a detailed characterization of the DCR of the JUNO 20-inch PMTs, investigating factors such as cooling time, temperature variations, and long-term stability using the JUNO Pan-Asia PMT testing facilities. The results reveal distinct DCR characteristics between the two types of PMTs, providing valuable insights into the nature of DCR and its implications for JUNO's scientific objectives. In addition to performance characterization, we implemented a monitoring system to track DCR stability over time. Notably, several spikes in DCR were identified, prompting a preliminary investigation into their causes. Potential factors contributing to these spikes, such as flasher events, were explored using coincidence rate analysis and complementary imaging techniques. The findings from this study are crucial for optimizing the performance of PMTs in JUNO, ultimately aiding the experiment in achieving its goals related to neutrino physics.
title Dark Count Rate Stability of JUNO 20-inch PMTs in Mass Testing
topic Instrumentation and Detectors
High Energy Physics - Experiment
url https://arxiv.org/abs/2506.15164