Search for low-mass Dark Matter with the CRESST Experiment
- Kluck, Holger
- Angloher, G.
- Gorla, P.
- Gütlein, A.
- Hauff, D.
- Jochum, J.
- Kiefer, M.
- Kraus, H.
- Lanfranchi, J.-C.
- Langenkämper, A.
- Loebell, J.
- Mancuso, M.
- Bauer, P.
- Mondragon, E.
- Münster, A.
- Pagliarone, C.
- Petricca, F.
- Potzel, W.
- Pröbst, F.
- Puig, R.
- Reindl, F.
- Rothe, J.
- Schäffner, K.
- Bento, A.
- Schieck, J.
- Schönert, S.
- Seidel, W.
- Stahlberg, M.
- Stodolsky, L.
- Strandhagen, C.
- Strauss, R.
- Tanzke, A.
- Trinh Thi, H. H.
- Türkoğlu, C.
- Bucci, C.
- Ulrich, A.
- Usherov, I.
- Wawoczny, S.
- Willers, M.
- Wüstrich, M.
- Canonica, L.
- Defay, X.
- Erb, A.
- Feilitzsch, F. v.
- Ferreiro Iachellini, N.
DOIAbstract
CRESST is a multi-stage experiment directly searching for dark matter (DM) using cryogenic $\mathrm{CaWO_4}$ crystals. Previous stages established leading limits for the spin-independent DM-nucleon cross section down to DM-particle masses $m_\mathrm{DM}$ below $1\,\mathrm{GeV/c^2}$. Furthermore, CRESST performed a dedicated search for dark photons (DP) which excludes new parameter space between DP masses $m_\mathrm{DP}$ of $300\,\mathrm{eV/c^2}$ to $700\,\mathrm{eV/c^2}$. In this contribution we will discuss the latest results based on the previous CRESST-II phase 2 and we will report on the status of the current CRESST-III phase 1: in this stage we have been operating 10 upgraded detectors with $24,\mathrm{g}$ target mass each and enhanced...
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