Cryogenic Composite Detectors for the Dark Matter Experiments CRESST and EURECA
S. Roth, C. Ciemniak, C. Coppi, F. v. Feilitzsch, A. Guetlein, C., Isaila, J.-C. Lanfranchi, S. Pfister, W. Potzel, and W. Westphal

TL;DR
This paper discusses the development and optimization of cryogenic composite detectors for dark matter experiments like CRESST and EURECA, focusing on detecting WIMP interactions via phonons and scintillation light.
Contribution
It introduces a composite detector design (CDD) that decouples TES production from target material choice, enabling pretesting and improved detector performance.
Findings
Extended thermal detector model for composite detectors
Potential for scalable, pretested detector production
Enhanced understanding of detector optimization
Abstract
Weakly Interacting Massive Particles (WIMPs) are candidates for non-baryonic Dark Matter. WIMPs are supposed to interact with baryonic matter via scattering off nuclei producing a nuclear recoil with energies up to a few 10 keV with a very low interaction rate of ~10^(-6) events per kg of target material and day in the energy region of interest. The Dark Matter experiment CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) and the EURECA project (European Underground Rare Event Calorimeter Array) are aimed at the direct detection of WIMPs with the help of very sensitive modularised cryogenic detectors that basically consist of a transition edge sensor (TES) in combination with a massive absorber crystal. In the CRESST experiment the search for coherent WIMP-nucleon scattering events is validated by the detection of two processes. In the scintillating absorber single…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Atomic and Subatomic Physics Research
