Eureca - The european underground rare event calorimeter array
Proceedings of the 6th International Workshop on the Identification of Dark Matter, IDM 2006 (2007) 668-677
Abstract:
EURECA (European Underground Rare Event Calorimeter Array) is a new project, searching for dark matter. The collaboration is comprised largely of the present groups of the CRESST and EDELWEISS experiments and several new groups. The aim is to explore scalar cross sections in the - 10 -9-10-10picobarn region with a target mass of up to one tonne. A major advantage of EURECA is the planned use of more that just one target material (multi target experiment for WIMP identification). In preparation for this largescale experiment, R&D for EURECA is provided through the current phases of CRESST and EDELWEISS.The 66-channel SQUID readout for CRESST II
JOURNAL OF INSTRUMENTATION 2 (2007) ARTN P11003
Scintillation properties of pure CaF2
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 566:2 (2006) 522-525
Abstract:
The temperature dependence of the decay time and scintillation light yield of pure CaFFracture processes observed with a cryogenic detector
Physics Letters Section A General Atomic and Solid State Physics 356:4-5 (2006) 262-266
Abstract:
In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time the energy release in fracture has been directly and accurately measured on a microscopic event-by-event basis. The energy threshold corresponds to the breaking of only a few hundred covalent bonds, a sensitivity some orders of magnitude greater than that of previous technique. We report some features of the data, including energy distributions, waiting time distributions, autocorrelations and the Hurst exponent. The energy distribution appear to follow a power law, d N / d E 鈭 E- 尾, similar to the power law for earthquake magnitudes, and after appropriate translation, with a similar exponent. In the time domain, the waiting time w or gap distribution between events has a power law behavior at small w and an exponential fall-off at large w, and can be fit 鈭 w- 伪 e -w / w0Optical and luminescence studies of ZnMoO4 using vacuum ultraviolet synchrotron radiation
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 562:1 (2006) 513-516