%0 Conference Paper %1 2016TAUP_CRESST-III-Detector %A Strauss, R %A Angloher, G %A Bento, A %A Bucci, C %A Canonica, L %A Defay, X %A Erb, A %A von Feilitzsch, F %A Iachellini, N Ferreiro %A Gorla, P %A Gütlein, A %A Hauff, D %A Jochum, J %A Kiefer, M %A Kluck, H %A Kraus, H %A Lanfranchi, J C %A Loebell, J %A Münster, A %A Pagliarone, C %A Petricca, F %A Potzel, W %A Pröbst, F %A Reindl, F %A Schäffner, K %A Schieck, J %A Schönert, S %A Seidel, W %A Stodolsky, L %A Strandhagen, C %A Tanzke, A %A Thi, H H Trinh %A Türkoglu, C %A Ufflnger, M %A Ulrich, A %A Usherov, I %A Wawoczny, S %A Willers, M %A Wüstrich, M %A Zöller, A %D 2016 %J Journal of Physics: Conference Series %K cresst darkmatter myown %N 4 %P 042048 %T The CRESST-III low-mass WIMP detector %U http://stacks.iop.org/1742-6596/718/i=4/a=042048 %V 718 %X The next generation direct dark matter experiment CRESST-III has a high potential to significantly increase the sensitivity to low-mass WIMPs ( m x ≲10GeV/c 2 ). We present the new CRESST detector module: it consists of a 24 g CaWO 4 crystal operated as a phonon detector and a 20×20 mm 2 silicon-on-sapphire light detector. The phonon energy threshold is lowered to ~100eV and a light detector resolution of typically 5eV is achieved. A fully-scintillating inner detector housing is realised which efficiently rejects events from surface-alpha decays. The CaWO 4 sticks holding the target crystal are also operated as calorimeters to discriminate all possible artefacts related to the support structure. A projection for the sensitivity to spin-independent WIMP-nucleon scattering is given for the first phase of CRESST-III which will start beginning of 2016.

@inproceedings{2016TAUP_CRESST-III-Detector, abstract = {The next generation direct dark matter experiment CRESST-III has a high potential to significantly increase the sensitivity to low-mass WIMPs ( m x ≲10GeV/c 2 ). We present the new CRESST detector module: it consists of a 24 g CaWO 4 crystal operated as a phonon detector and a 20×20 mm 2 silicon-on-sapphire light detector. The phonon energy threshold is lowered to ~100eV and a light detector resolution of typically 5eV is achieved. A fully-scintillating inner detector housing is realised which efficiently rejects events from surface-alpha decays. The CaWO 4 sticks holding the target crystal are also operated as calorimeters to discriminate all possible artefacts related to the support structure. A projection for the sensitivity to spin-independent WIMP-nucleon scattering is given for the first phase of CRESST-III which will start beginning of 2016.}, added-at = {2017-01-20T14:32:19.000+0100}, author = {Strauss, R and Angloher, G and Bento, A and Bucci, C and Canonica, L and Defay, X and Erb, A and von Feilitzsch, F and Iachellini, N Ferreiro and Gorla, P and Gütlein, A and Hauff, D and Jochum, J and Kiefer, M and Kluck, H and Kraus, H and Lanfranchi, J C and Loebell, J and Münster, A and Pagliarone, C and Petricca, F and Potzel, W and Pröbst, F and Reindl, F and Schäffner, K and Schieck, J and Schönert, S and Seidel, W and Stodolsky, L and Strandhagen, C and Tanzke, A and Thi, H H Trinh and Türkoglu, C and Ufflnger, M and Ulrich, A and Usherov, I and Wawoczny, S and Willers, M and Wüstrich, M and Zöller, A}, biburl = {https://www.bibsonomy.org/bibtex/26cff665663557ccec4e3efe335649f11/strandhagen}, description = {The CRESST-III low-mass WIMP detector - IOPscience}, interhash = {aecd9337c370ad57953dc38cb14fb395}, intrahash = {6cff665663557ccec4e3efe335649f11}, journal = {Journal of Physics: Conference Series}, keywords = {cresst darkmatter myown}, number = 4, pages = 042048, timestamp = {2017-01-20T14:32:19.000+0100}, title = {The CRESST-III low-mass WIMP detector}, url = {http://stacks.iop.org/1742-6596/718/i=4/a=042048}, volume = 718, year = 2016 }