Technische Universität Wien, Austria
22 December 2016, Thursday, 14:40
Cavid Erginsoy Seminar Room, Physics Department, 3rd floor
Abstract: It is suggested by several astronomical observations that dark matter contributes 27 % to the overall energy density of our universe but its nature has not been understood so far. In recent years, different theory models about dark matter particles have been made and these theory models have led to different predictions. In order to test these predictions, three experimental methods have been developed: production, indirect and direct searches. The CRESST experiment aims to directly detect dark matter particle elastically scattering off nuclei. The CRESST-II detector modules are based on CaWO4 crystals which are operated at mK temperatures. The nuclear recoil energy thresholds for the CRESST-II detectors Lise and TUM40 are 0.3 keV and 0.6 keV, respectively. Such low energy thresholds make CRESST ideally suited for the detection of low-mass dark matter particles. Further increase in sensitivity is expected with CRESST-III detectors featuring a threshold of 0.1 keV. In this talk, we will present our results on the dark matter search obtained with the detector modules Lise and TUM40 of CRESST-II. We will discuss the status of CRESST-III Phase 1 which started taking data this year. Additionally, an outlook for the upgrade of the readout electronics of CRESST-III Phase 2 will be discussed. In addition to the low threshold, radio purity of the crystals is another important factor for the detection of dark matter particles. To acquire a detailed understanding of the backgrounds measured by the detectors, a Geant4 simulation of the electromagnetic backgrounds was carried out for the TUM40 detector module. The simulation includes backgrounds coming both from inside the crystal and from outside. The information taken from the background simulation will be vital for the second phase of the CRESST-III experiment.
Reminder: Tea and cookies will be in the seminar room before the seminar.