2011
DOI: 10.1016/j.nima.2010.11.095
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Time and amplitude of afterpulse measured with a large size photomultiplier tube

Abstract: We have studied the afterpulse of a hemispherical photomultiplier tube for an upcoming reactor neutrino experiment. The timing, the amplitude, and the rate of the afterpulse for a 10 inch photomultiplier tube were measured with a 400 MHz FADC up to 16 µs time window after the initial signal generated by an LED light pulse. The time and amplitude correlation of the afterpulse shows several distinctive groups. We describe the dependencies of the afterpulse on the applied high voltage and the amplitude of the mai… Show more

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Cited by 40 publications
(17 citation statements)
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“…Outside the γ-catcher, a 70 cm thick buffer layer is filled with 76 metric tons of a non-scintillating liquid, mineral oil (MO, C n H 2n+2 , n=11~44). This provides shielding from radioactivity in the surrounding rocks and in the 354 10-inch Hamamatsu R7081 photomultiplier tubes (PMTs) that are mounted on the inner wall of the stainless steel buffer container [2,7]. The outermost layer is the 1.5 m thick veto system and filled with highly purified water.…”
Section: Detectormentioning
confidence: 99%
See 1 more Smart Citation
“…Outside the γ-catcher, a 70 cm thick buffer layer is filled with 76 metric tons of a non-scintillating liquid, mineral oil (MO, C n H 2n+2 , n=11~44). This provides shielding from radioactivity in the surrounding rocks and in the 354 10-inch Hamamatsu R7081 photomultiplier tubes (PMTs) that are mounted on the inner wall of the stainless steel buffer container [2,7]. The outermost layer is the 1.5 m thick veto system and filled with highly purified water.…”
Section: Detectormentioning
confidence: 99%
“…This layer tags events coming from outside by Cherenkov radiation and also shields against ambient cosmic-rays and neutrons from the surrounding rock. Sixty-seven 10-inch R7081 water-proof PMTs are mounted on the wall of the veto vessel [2,7]. All surfaces of the veto layer are covered with Tyvek sheets to increase the light collection.…”
Section: Detectormentioning
confidence: 99%
“…Outside of the γ-catcher, there is a 70 cm thick buffer region filled with 62.7 tons of mineral oil. The light signals emitted from the particles are detected by 354 low background 10-inch PMTs [19] mounted on the inner wall of the stainless-steel container. The 1.5 m thick OD region is filled with highly purified water and equipped with 67 10-inch PMTs mounted on the wall of the concrete veto vessel so as to catch the water Cherenkov light.…”
Section: Introductionmentioning
confidence: 99%
“…An "afterpulse" occasionally accompanies a primary pulse signal [3]. When the primary pulse is amplified in the dynode, residual gases are ionized via interactions with electrons.…”
Section: Afterpulsementioning
confidence: 99%