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要旨:
The experiment XENON1T aims at directly detecting dark matter via interactions of weakly
interacting massive particles (WIMPs) with xenon nuclei. The goal of XENON1T is to
improve the sensitivity compared to its predecessor experiment XENON100 by 2 orders
of magnitude by using a larger xenon volume and by reducing the amount of background
events. The XENON1T inner detector, which contains 2:2 t of liquid xenon, will be equipped
with 248 photomultiplier tubes (PMTs) to detect the scintillation light induced by a possible
WIMP interaction. For this purpose 3 00 R11410-21 PMTs with low intrinsic radioactivity
and high quantum eciency are being manufactured by Hamamatsu. One part of this thesis
describes the tests of the rst 90 R11410-21 PMTs. Important features like the dark count
rate and the gain were measured at room- and liquid xenon temperature. The second part
of this thesis is dedicated to investigating the scintillation light propagation and the light
collection eciency (LCE) in a XENON1T-like detector. A Monte Carlo simulation based
on GEANT4 was developed to test how dierent assignments of quantum eciency (QE)
values to the PMT positions aect the LCE. In a rst approach, it is found that optimizing
the PMT arrangement, considering the QE values, can enhance the LCE value by a factor
of 7% at most, which would result in a 7% higher light yield for XENON1T.
