Study of TTS for a 20-inch dynode PMTSupported by Strategic Priority Research Program of the Chinese Academy of Sciences (XDA10011100) and National Natural Science Foundation of China (U1431109, 11265003)
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 t...
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Published in | Chinese physics C Vol. 41; no. 7 |
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Main Authors | , , , , , , , , |
Format | Journal Article |
Language | English |
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IOP Publishing
01.07.2017
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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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AbstractList | 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. |
Author | Luo, Feng-Jiao Yang, An-Bo Xu, Mei-Hang Zhou, Yi-Xiong Liu, Hong-Bang Xie, Wan Qin, Zhong-Hua Liao, Dong-Hao Wang, Zhi-Min |
Author_xml | – sequence: 1 givenname: Dong-Hao surname: Liao fullname: Liao, Dong-Hao organization: Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China – sequence: 2 givenname: Hong-Bang surname: Liu fullname: Liu, Hong-Bang organization: University of Chinese Academy of Science, Beijing 10049,China – sequence: 3 givenname: Yi-Xiong surname: Zhou fullname: Zhou, Yi-Xiong organization: University of Chinese Academy of Science, Beijing 10049,China – sequence: 4 givenname: Feng-Jiao surname: Luo fullname: Luo, Feng-Jiao organization: University of Chinese Academy of Science, Beijing 10049,China – sequence: 5 givenname: Zhi-Min surname: Wang fullname: Wang, Zhi-Min organization: Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China – sequence: 6 givenname: An-Bo surname: Yang fullname: Yang, An-Bo organization: University of Chinese Academy of Science, Beijing 10049,China – sequence: 7 givenname: Mei-Hang surname: Xu fullname: Xu, Mei-Hang organization: Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China – sequence: 8 givenname: Wan surname: Xie fullname: Xie, Wan organization: Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China – sequence: 9 givenname: Zhong-Hua surname: Qin fullname: Qin, Zhong-Hua organization: Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China |
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Copyright | 2017 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd |
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Snippet | The neutrino detector for the Jiangmen Underground Neutrino Observatory (JUNO) requires a large number of photomultiplier tubes (PMTs), including 15000 MCP... |
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SubjectTerms | 20-inch dynode PMT Earth's magnetic field transit time TTS |
Title | Study of TTS for a 20-inch dynode PMTSupported 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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