Study of TTS for a 20-inch dynode PMT

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Dong-Hao Liao, Hong-Bang Liu, Yi-Xiong Zhou, Feng-Jiao Luo, Zhi-Min Wang, An-Bo Yang, Mei-Hang Xu, Wan Xie and Zhong-Hua Qin. Study of TTS for a 20-inch dynode PMT[J]. Chinese Physics C, 2017, 41(7): 076001. doi: 10.1088/1674-1137/41/7/076001
Dong-Hao Liao, Hong-Bang Liu, Yi-Xiong Zhou, Feng-Jiao Luo, Zhi-Min Wang, An-Bo Yang, Mei-Hang Xu, Wan Xie and Zhong-Hua Qin. Study of TTS for a 20-inch dynode PMT[J]. Chinese Physics C, 2017, 41(7): 076001.  doi: 10.1088/1674-1137/41/7/076001 shu
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Received: 2017-01-04
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    Supported by Strategic Priority Research Program of the Chinese Academy of Sciences (XDA10011100) and National Natural Science Foundation of China (U1431109, 11265003)

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Study of TTS for a 20-inch dynode PMT

    Corresponding author: Hong-Bang Liu,
    Corresponding author: Zhong-Hua Qin,
  • 1. Guangxi Key Laboratory for Relativistic Astrophysics, Guangxi University, Nanning 530004, China
  • 2. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 3. University of Chinese Academy of Science, Beijing 10049,China
  • 4. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 5.  Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
Fund Project:  Supported by Strategic Priority Research Program of the Chinese Academy of Sciences (XDA10011100) and National Natural Science Foundation of China (U1431109, 11265003)

Abstract: The neutrino detector for the Jiangmen Underground Neutrino Observatory (JUNO) requires a large number of photomultiplier tubes (PMTs), including 15000 MCP PMTs and 5000 dynode PMTs. The TTS (transit time spread) of the PMTs is very important for vertex and track reconstruction of the neutrinos in the detector. In this paper, we study the TTS of a 20-inch dynode PMT (R12860) from Hamamatsu for different high voltage, light intensity, light spot size and different photocathode regions. The impact from Earth's magnetic field is also studied. The results achieved in this paper will be very useful for the JUNO experiment.

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