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Cryogenic Composite Detectors for the Dark Matter Experiments CRESST and EURECA
S. Roth, C. Ciemniak, C. Coppi +7
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…
Neutron Scattering Facility for Characterization of CRESST and EURECA Detectors at mK Temperatures
J. -C. Lanfranchi, C. Ciemniak, C. Coppi +15
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 m…
Commissioning Run of the CRESST-II Dark Matter Search
G. Angloher, M. Bauer, I. Bavykina +40
The CRESST cryogenic direct dark matter search at Gran Sasso, searching for WIMPs via nuclear recoil, has been upgraded to CRESST-II by several changes and improvements.We present…
Detection potential for the diffuse supernova neutrino background in the large liquid-scintillator detector LENA
M. Wurm, F. von Feilitzsch, M. Goeger-Neff +4
The large-volume liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) will provide high-grade background discrimination and enable the detection of diffuse supernova n…
The CRESST Dark Matter Search
B. Majorovits, G. Angloher, C. Bucci +23
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from sel…
Limits on WIMP dark matter using scintillating CaWO4 cryogenic detectors with active background suppression
G. Angloher, C. Bucci, P. Christ +21
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Dat…