Lung, K;
Arisaka, K;
Bargetzi, A;
Beltrame, P;
Cahill, A;
Genma, T;
Ghag, C;
... Yoshizawa, Y; + view all
(2012)
Characterization of the Hamamatsu R11410-10 3-in. photomultiplier tube for liquid xenon dark matter direct detection experiments.
Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
, 696
pp. 32-39.
10.1016/j.nima.2012.08.052.
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Abstract
To satisfy the requirements of the next generation of dark matter detectors based on the dual phase TPC, Hamamatsu, in close collaboration with UCLA, has developed the R11410-10 photomultiplier tube. In this work, we present the detailed tests performed on this device. High QE (∼30%) accompanied by a low dark count rate (50 Hz at 0.3 PE) and high gain (1×10 7) with good single PE resolution have been observed. A comprehensive screening measurement campaign is ongoing while the manufacturer quotes a radioactivity of 20 mBq/PMT. These characteristics show the R11410-10 to be particularly suitable for the forthcoming zero background liquid xenon detectors. © 2012 Elsevier B.V.
Type: | Article |
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Title: | Characterization of the Hamamatsu R11410-10 3-in. photomultiplier tube for liquid xenon dark matter direct detection experiments |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1016/j.nima.2012.08.052 |
Publisher version: | http://dx.doi.org/10.1016/j.nima.2012.08.052 |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | Photomultiplier tubesDark matterAstroparticle physics |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/1352147 |




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