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Abstract
The CRESST-III experiment, located in the Gran Sasso underground laboratory (LNGS, Italy), aims at the direct detection of dark matter (DM) particles. Scintillating CaWO4 crystals operated as cryogenic detectors are used as target material for DM-nucleus scattering. The simultaneous measurement of the phonon signal from the CaWO4 crystal and of the emitted scintillation light in a separate cryogenic light detector is used to discriminate backgrounds from a possible dark matter signal. The experiment aims to significantly improve the sensitivity for low-mass (≲ 5-10 GeV/c2) DM particles by using optimized detector modules with a nuclear recoil-energy threshold ≲ 100 eV. The current status of the experiment as well as projections of the sensitivity for spin-independent DM-nucleon scattering will be presented.
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Details
1 Physik-Department, Technische Universität München, D-85748 Garching, Germany
2 Max-Planck-Institut für Physik, D-80805 München, Germany
3 Departamento de Fisica, Universidade de Coimbra, P3004 516 Coimbra, Portugal
4 INFN, Laboratori Nazionali del Gran Sasso, I-67010 Assergi, Italy
5 Physik-Department, Technische Universität München, D-85748 Garching, Germany; Walther-Meißner-Institut für Tieftemperaturforschung, D-85748 Garching, Germany
6 Institute for High energy Physics, Austrian Academy of Sciences, 1050 Vienna, Austria; Atominstitut, Technische Universität Wien, 1040 Vienna, Austria
7 Eberhard-Karls-Universität Tübingen, D-72076 Tübingen, Germany
8 Department of Physics, University of Oxford, Oxford OX1 3RH, United Kingdom