Study of a prototype water Cherenkov detector for the Daya Bay neutrino experiment

2012 ◽  
Vol 682 ◽  
pp. 26-30 ◽  
Author(s):  
Zeyuan Yu ◽  
Haoqi Lu ◽  
Changgen Yang ◽  
Lingyu Wang ◽  
Mengyun Guan ◽  
...  
Keyword(s):  
Daya Bay ◽  
Neutrino Experiment ◽  
Cherenkov Detector ◽  
Water Cherenkov Detector

scholarly journals Offline Software of RPC Detector System in Daya Bay Reactor Neutrino Experiment

2012 ◽  
Vol 396 (2) ◽  
pp. 022061 ◽  
Author(s):  
Qingmin Zhang ◽  
Miao He ◽  
Jilei Xu ◽  
Jiaheng Zou ◽  
Zhe Ning ◽  
...  
Keyword(s):  
Detector System ◽  
Daya Bay ◽  
Neutrino Experiment ◽  
Reactor Neutrino

HYPER-KAMIOKANDE — A NEXT GENERATION WATER CHERENKOV DETECTOR

2003 ◽  
Vol 18 (22) ◽  
pp. 4053-4063 ◽  
Author(s):  
KENZO NAKAMURA
Keyword(s):  
Total Mass ◽  
Proton Synchrotron ◽  
Cherenkov Detector ◽  
Next Generation ◽  
Neutrino Sector ◽  
Long Baseline ◽  
Neutrino Oscillation Experiment ◽  
Water Cherenkov Detector ◽  
Under Construction ◽  
Oscillation Experiment

A next generation water Cherenkov detector at Kamioka with a total mass of ~1 Mton is called Hyper-Kamiokande. If the beam intensity of a 50-GeV proton synchrotron now under construction at Tokai is upgraded to 4 MW in future, a long baseline neutrino oscillation experiment with Hyper-Kamiokande as a far detector will open the possibility of measuring CP violation in the neutrino sector. Also, Hyper-Kamiokande will allow to extend nucleon decay search to τp/B(p → e+π0) > 1035 yr and [Formula: see text]. Aiming at the realization of Hyper-Kamiokande, various R&D efforts are in progress.

Chapter 3 Extra-galactic Gamma-Ray Sources

2021 ◽  
Author(s):  
Xiang-Yu Wang
Keyword(s):  
Active Galactic Nuclei ◽  
Lower Energy ◽  
Gamma Ray ◽  
Galactic Nuclei ◽  
Starburst Galaxies ◽  
Gamma Ray Bursts ◽  
Cherenkov Detector ◽  
Extragalactic Background Light ◽  
Background Light ◽  
Water Cherenkov Detector

Abstract Extra-galactic gamma-ray sources, such as gamma-ray bursts, active galactic nuclei, starburst galaxies, are interesting and important targets for LHAASO observations. In this chapter, the prospects of detecting these sources with LHAASO and their physical implications are studied. The upgrade plan for the Water Cherenkov Detector Array (WCDA), which aims to enhance the detectability of relatively lower energy photons, is also presented. In addition, a study on constraining the extragalactic background light with LHAASO observation of blazars is presented.

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