Study of tts for a 20-inch dynode pmt
文献类型：期刊论文
| 作者 | Liao, Dong-Hao1,2; Liu, Hong-Bang1,3; Zhou, Yi-Xiong1,3; Luo, Feng-Jiao2,3; Wang, Zhi-Min2; Yang, An-Bo2,3; Xu, Mei-Hang2; Xie, Wan2; Qin, Zhong-Hua2 |
| 刊名 | Chinese physics c
 |
| 出版日期 | 2017-07-01 |
| 卷号 | 41期号:7页码:6 |
| 关键词 | Tts 20-inch dynode pmt Transit time Earth's magnetic field |
| ISSN号 | 1674-1137 |
| DOI | 10.1088/1674-1137/41/7/076001 |
| 通讯作者 | Liu, hong-bang(liuhb@gxu.edu.cn) |
| 英文摘要 | 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. |
| WOS关键词 | LARGE-AREA PHOTOMULTIPLIERS ; MAGNETIC-FIELD |
| WOS研究方向 | Physics |
| WOS类目 | Physics, Nuclear ; Physics, Particles & Fields |
| 语种 | 英语 |
| WOS记录号 | WOS:000406156700015 |
| 出版者 | CHINESE PHYSICAL SOC |
| URI标识 | http://www.irgrid.ac.cn/handle/1471x/2177254 |
| 专题 | 高能物理研究所 |
| 通讯作者 | Liu, Hong-Bang |
| 作者单位 | 1.Guangxi Univ, Guangxi Key Lab Relativist Astrophys, Nanning 530004, Peoples R China 2.Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China 3.Univ Chinese Acad Sci, Beijing 10049, Peoples R China |
| 推荐引用方式 GB/T 7714 | Liao, Dong-Hao,Liu, Hong-Bang,Zhou, Yi-Xiong,et al. Study of tts for a 20-inch dynode pmt[J]. Chinese physics c,2017,41(7):6. |
| APA | Liao, Dong-Hao.,Liu, Hong-Bang.,Zhou, Yi-Xiong.,Luo, Feng-Jiao.,Wang, Zhi-Min.,...&Qin, Zhong-Hua.(2017).Study of tts for a 20-inch dynode pmt.Chinese physics c,41(7),6. |
| MLA | Liao, Dong-Hao,et al."Study of tts for a 20-inch dynode pmt".Chinese physics c 41.7(2017):6. |
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来源：高能物理研究所
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