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18 April 2024
 
  » arxiv » 1410.1753

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A detector module with highly efficient surface-alpha event rejection operated in CRESST-II Phase 2
R. Strauss ; G. Angloher ; A. Bento ; C. Bucci ; L. Canonica ; A. Erb ; F.v. Feilitzsch ; N. Ferreiro ; P. Gorla ; A. Gütlein ; D. Hauff ; J. Jochum ; M. Kiefer ; H. Kluck ; H. Kraus ; J.-C. Lanfranchi ; J. Loebell ; A. Münster ; F. Petricca ; W. Potzel ; F. Pröbst ; F. Reindl ; S. Roth ; K. Rottler ; C. Sailer ; K. Schäffner ; J. Schieck ; S. Scholl ; S. Schönert ; W. Seidel ; M.v. Sivers ; M. Stanger ; L. Stodolsky ; C. Strandhagen ; A. Tanzke ; M. Uffinger ; A. Ulrich ; I. Usherov ; S. Wawoczny ; M. Willers ; M. Wüstrich ; A. Zöller ;
Date 7 Oct 2014
AbstractThe cryogenic dark matter experiment CRESST-II aims at the direct detection of WIMPs via elastic scattering off nuclei in scintillating CaWO$_4$ crystals. We present a new, highly improved, detector design installed in the current run of CRESST-II Phase 2 with an efficient active rejection of surface-alpha backgrounds. Using CaWO$_4$ sticks to hold the target crystal a detector housing with fully-scintillating inner surface could be realized. The presented detector (TUM40) provides an excellent threshold of ${sim},0.60,$keV and a resolution of $sigma,{approx},0.090,$keV (at 2.60$,$keV). With significantly reduced background levels, TUM40 sets stringent limits on the spin-independent WIMP-nucleon scattering cross section and probes a new region of parameter space for WIMP masses below 3$,$GeV/c$^2$. In this paper, we discuss the novel detector design and the surface-alpha event rejection in detail.
Source arXiv, 1410.1753
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