LUX-ZEPLIN

Abstract:

EURECA (European Underground Rare Event Calorimeter Array) is an astro-particle physics facility aiming to directly detect galactic dark matter. The Laboratoire Souterrain de Modane has been selected as host laboratory. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. EURECA will use a target mass of up to one ton, enough to explore WIMP - nucleon scalar scattering cross sections in the region of 10-9 - 10-10 picobarn. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification). © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

Abstract:

The latest results on the low-temperature characterisation of scintillation materials selected for rare event search are reviewed. The temperature dependences of the light output and decay time are analysed on the basis of the current understanding of the underlying physical processes that control the emission of light in solids. It is shown that scintillation properties of the materials under study are adequate for the purpose of cryogenic experiments searching for rare events. From the analysis of the performance characteristics it is concluded that currently ZnWO4 is the most suitable scintillation target for dark matter search.

Abstract:

The prospects for the use of molybdates and tungstates in the opto-electronic devises prompted studies of the structure, as well as luminescence and scintillation properties of MgWO4-MgMoO4 system. The powder samples of (1-x)MgMoO4xMgWO4 (x = 0; 0.01; 0.05; 0.1; 0.3; 0.5; 0.7; 0.9, and 1.0) were synthesised by the solid state reaction technique at 900°C. The results of the X-ray structure analysis identified three types of crystal structure in the pseudo-binary MgWO4-MgMoO4 system, i. e. β-MgMoO4, cuprosheelite α-MgMoO4, and wolframite MgWO4. It is shown that a single-phase solid solution MgMo1-xWxO4 with β-MgMoO4 structure is formed at x < 0.10, whereas at higher concentration of tungsten the mixture of different phases is created. The phase composition of the sample determines the luminescence spectra; the maximum of the emission band is observed at 520 nm for β-MgMoO4, 590 nm for α-MgMoO4, and 480 nm for MgWO4. A possible correlation between the emission spectra and peculiarities of crystal structure are discussed in terms of the canonical configuration coordinate model. The emission efficiency of magnesium tungstate is found to be highest within the compounds under investigation. The scintillation light yield of MgWO4 at T = 295 K is found to be 0.90±0.15 of that of ZnWO4 and remains high with the decrease of temperature.