Characterization of the Hamamatsu R11780 12 inch Photomultiplier Tube
arXiv:1210.2765 · doi:10.1016/j.nima.2013.02.022
Abstract
Future large water Cherenkov and scintillator detectors have been proposed for measurements of long baseline neutrino oscillations, proton decay, supernova and solar neutrinos. To ensure cost-effectiveness and optimize scientific reach, one of the critical requirements for such detectors are large-area, high performance photomultiplier tubes (PMTs). One candidate for such a device is the Hamamatsu R11780, a 12" PMT that is available in both standard and high quantum efficiency versions. Measurements of the single photoelectron response characteristics, relative efficiencies of the standard and high quantum efficiency versions, a preliminary measurement of the absolute quantum efficiency of the standard quantum efficiency version, and a two-dimensional scan of the relative efficiency across the photocathode surface are presented in this paper. All single photoelectron investigations were made using a Cherenkov light source at room temperature at a gain of 1*10^7. These results show that the R11780 PMT is a excellent candidate for such large optical detectors, including the peak-to-valley ratios greater than 2, transit time spreads around 1.3 ns, and late-pulsing probabilities less than 5%.
arXiv comment20 pages, 16 figures
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- Sensitivity of a low threshold directional detector to CNO-cycle solar neutrinos
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- Sterile Neutrino Searches at the IceCube Neutrino Observatory
- Enhanced Photon Traps for Hyper-Kamiokande
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- Coincidence-based reconstruction for reactor antineutrino detection in gadolinium-doped Cherenkov detectors
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- Characterization of the ETEL D784UKFLB 11 inch Photomultiplier Tube
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