Results and current status of the water cherenkov detector development for the auger surface array

1999 ◽  
Vol 75 (1-2) ◽  
pp. 383-385
Author(s):  
T. Kutter
Keyword(s):  
Current Status ◽  
Cherenkov Detector ◽  
Water Cherenkov Detector

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.

A CHERENKOV DETECTOR FOR WASA AT COSY

2007 ◽  
Vol 22 (02n03) ◽  
pp. 612-616
Author(s):  
PETER VLASOV ◽  
FRANK HINTERBERGER ◽  
ANATOLY POVTOREYKO ◽  
JAMES RITMAN ◽  
REGINA SIUDAK
Keyword(s):  
Detector System ◽  
Current Status ◽  
Cherenkov Detector

The WASA detector system requires upgrades of its components to be efficient at the higher beam energies available at COSY. One of the proposed items of the WASA upgrade is to add a Cherenkov Detector. The current status of its development is presented.

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.

Study on the detection efficiency and uniformity of a Water Cherenkov Detector based on Geant4

2019 ◽  
Vol 14 (09) ◽  
pp. T09003-T09003
Author(s):  
W. Yudong ◽  
A. Chiavassa ◽  
D. Martraire ◽  
C. Vigorito ◽  
Z. Rong ◽  
...  
Keyword(s):  
Detection Efficiency ◽  
Cherenkov Detector ◽  
Water Cherenkov Detector
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