Abstract
Prototype of the fast timing Cherenkov detector, applicable in high-energy collider experiments, has been developed basing on the modified Planacon XP85012 MCP-PMT and fused silica radiators. We present the reasons and description of the MCP-PMT modification, timing and amplitude characteristics of the prototype including the summary of the detector’s response on particle hits at oblique angles and MCP-PMT performance at high illumination rates.
Highlights
Modern comprehensive detection systems for the high-energy physics experiments often require relatively simple subdetectors able to generate trigger signals with the best timing in the shortest period of time
The experimental setup is shown in figure 2: time resolution of the tested device was measured relatively to the average timing of the two Cherenkov counters based on FEU-187 PMTs
Time resolution of the Cherenkov counters serving as time trigger and the tested Cherenkov modules with the standard and modified versions of the XP85012 MCP-PMT is shown in figure 3
Summary
This content has been downloaded from IOPscience. Please scroll down to see the full text. 2017 J. You may be interested in: Fast timing and trigger Cherenkov detector for collider experiments V A Grigoryev, V A Kaplin, T L Karavicheva et al A square, multi-anode, long life MCP-PMT for the detection of Cherenkov photons J S Milnes, T M Conneely, J S Lapington et al Ground detectors for the study of cosmic ray showers H Salazar and L Villasenor Scintillators and Cherenkov detectors for the registration of 10.8 MeV gamma rays J E McMillan, A Cole, A Kirby et al Overview of photon detectors for fast single photon detection Peter Križan Aerogel Cherenkov detectors in colliding beam experiments A F Danilyuk, S A Kononov, E A Kravchenko et al Quartz Cherenkov counters for fast timing: QUARTIC M G Albrow, Heejong Kim, S Los et al Cherenkov detectors for high-energy neutrino astrophysics Zh-A M Dzhilkibaev, G V Domogatsky and O V Suvorova ICF gamma-ray reaction history diagnostics H W Herrmann, C S Young, J M Mack et al
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