Title of article
Characterization of the Hamamatsu R11780 12 in. photomultiplier tube
Author/Authors
Brack، نويسنده , , J. and Delgado، نويسنده , , B. and Dhooghe، نويسنده , , J. and Felde، نويسنده , , J. and Gookin، نويسنده , , B. and Grullon، نويسنده , , S. and Klein، نويسنده , , J.R. and Knapik، نويسنده , , R. G. Latorre، نويسنده , , A. F. Seibert، نويسنده , , S. and Shapiro، نويسنده , , K. and Svoboda، نويسنده , , R. and Ware، نويسنده , , L. and Van Berg، نويسنده , , R.، نويسنده ,
Pages
12
From page
162
To page
173
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 in. 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 1×107. These results show that the R11780 PMT is an excellent candidate for such large optical detectors.
Keywords
Photomultiplier tube , Neutrino detectors , Photon detection , Single phase dark matter , Optical detectors
Journal title
Astroparticle Physics
Record number
2013045
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