Neutron Scattering Facility for Characterization of CRESST and EURECA Detectors at mK Temperatures
J.-C. Lanfranchi, C. Ciemniak, C. Coppi, F. von Feilitzsch, A., G\"utlein, H. Hagn, C. Isaila, J. Jochum, M. Kimmerle, S. Pfister, W. Potzel,, W. Rau, S. Roth, K. Rottler, C. Sailer, S. Scholl, I. Usherov, W. Westphal

TL;DR
This paper describes the development of a neutron scattering facility at millikelvin temperatures to characterize detector responses for dark matter experiments like CRESST and EURECA, improving background discrimination.
Contribution
It introduces a specialized neutron scattering setup at mK temperatures for detailed recoil behavior studies in dark matter detector materials, aiding future multi-target experiments.
Findings
Facility successfully installed and commissioned at Garching.
Enables recoil behavior analysis for Ca, O, W nuclei.
Supports research for background rejection in dark matter detection.
Abstract
CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is an experiment located at the Gran Sasso underground laboratory and aimed at the direct detection of dark matter in the form of WIMPs. The setup has just completed a one year commissioning run in 2007 and is presently starting a physics run with an increased target mass. Scintillating single crystals, operated at temperatures of a few millikelvin, are used as target to detect the tiny nuclear recoil induced by a WIMP. The powerful background identification and rejection of , e and events is realized via the simultaneous measurement of a phonon and a scintillation signal generated in the crystal. However, neutrons could still be misidentified as a WIMP signature. Therefore, a detailed understanding of the individual recoil behaviour in terms of phonon…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Particle physics theoretical and experimental studies
