| الملخص: | <p>There is an abundance of evidence, both astrophysical and cosmological, for the existence of non-luminous, gravitationally interacting matter that cannot be accounted for by the current Standard Model - dark matter. It is estimated that dark matter accounts for ~84% of the matter density of the Universe, but has yet to be directly detected.</p>
<p>The LUX-ZEPLIN experiment (LZ) is searching for a popular dark matter particle candidate, weakly interacting massive particles (WIMPs), in the energy range GeV/c2 – TeV/c2. The LZ detector consists of a dual-phase time projection chamber filled with a 7 t active target of liquid xenon. Recoil interactions of dark matter
contained within the galactic halo are expected to produce signals via charge and scintillation channels on the order of a few keV in the xenon target. Owing to passive and active shielding, fiducialisation and background rejection, LZ has reported the world-leading result for spin-independent WIMP–nucleon interactions with data collected during the first science run.</p>
<p>This thesis presents work characterising and constraining the background produced by the cavern environment, namely from naturally occurring radioactive material contained within the cavern rock. This results in a penetrative gamma-ray background from long-lived isotopes of 40K and 238U and 232Th decay chains. Radiogenic neutrons are also produced via spontaneous fission and (α, n) reactions. A new gamma spectroscopy experiment was conducted in the Davis cavern directly outside of the water tank housing LZ in order to gain long-exposure measurements of the gamma-ray background. Simulations are employed to compare our models with real data. The accuracy of our modelling becomes increasingly important as LZ continues to take science data, adding to the live time of the WIMP search and other rare physics searches, such as for low-energy electron recoils and neutrinoless
double-beta decay of 136Xe.</p>
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