In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct weakly interacting massive particles (WIMP) detection. Nuclear recoils can be discriminated against electron recoils by measuring phonons and scintillation light simultaneously. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers. Results on the sensitivity of the phonon and the light channel, radiopurity, the scintillation properties of CaWO4, and on the WIMP sensitivity are presented. (C) 2003 Elsevier B.V. All rights reserved
The CRESST-II Dark Matter experiment aims at the direct detection of WIMPs via scattering off nuclei...
The goal of the CRESST Dark Matter Search is the direct detection of Weakly Interacting Massive Part...
CRESST-II detector modules rely on the ability to actively discriminate electron recoils from nuclea...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (wea...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (wea...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The goal of the CRESST Dark Matter Search is the direct detection of Weakly Interacting Massive Part...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) Dark Matter search is aim...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a...
Although it is well known that CaWO4 is a scintillator it is not often used. mainly because it has a...
The CRESST-II Dark Matter experiment aims at the direct detection of WIMPs via scattering off nuclei...
The CRESST-II Dark Matter experiment aims at the direct detection of WIMPs via scattering off nuclei...
The goal of the CRESST Dark Matter Search is the direct detection of Weakly Interacting Massive Part...
CRESST-II detector modules rely on the ability to actively discriminate electron recoils from nuclea...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (wea...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (wea...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The goal of the CRESST Dark Matter Search is the direct detection of Weakly Interacting Massive Part...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) Dark Matter search is aim...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a...
Although it is well known that CaWO4 is a scintillator it is not often used. mainly because it has a...
The CRESST-II Dark Matter experiment aims at the direct detection of WIMPs via scattering off nuclei...
The CRESST-II Dark Matter experiment aims at the direct detection of WIMPs via scattering off nuclei...
The goal of the CRESST Dark Matter Search is the direct detection of Weakly Interacting Massive Part...
CRESST-II detector modules rely on the ability to actively discriminate electron recoils from nuclea...