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Description of CRESST-II data

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arxiv 1701.08157 v3 pith:E4ZI62ON submitted 2017-01-27 physics.ins-det

G. Angloher , P. Bauer , A. Bento , C. Bucci , L. Canonica , X. Defay , A. Erb , F. v. Feilitzsch
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N. Ferreiro Iachellini P. Gorla A. Gütlein D. Hauff J. Jochum M. Kiefer C. Kistner H. Kluck H. Kraus J.-C. Lanfranchi J. Loebell M. Mancuso A. Münster C. Pagliarone F. Petricca W. Potzel F. Pröbst R. Puig F. Reindl S. Roth K. Rottler C. Sailer K. Schäffner J. Schieck J. Schmaler S. Scholl S. Schönert W. Seidel M.v. Sivers L. Stodolsky C. Strandhagen R. Strauss A. Tanzke H.H. Trinh Thi C. Türkoǧlu M. Uffinger A. Ulrich I. Usherov S. Wawoczny M. Willers M. Wüstrich A. Zöller
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classification physics.ins-det
keywords datacresst-iidark-matterdetectordocumentenergieseventsmodules
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abstract

In Phase 2 of CRESST-II 18 detector modules were operated for about two years (July 2013 - August 2015). Together with this document we are publishing data from two detector modules which have been used for direct dark-matter searches. With these data-sets we were able to set world-leading limits on the cross section for spin-independent elastic scattering of dark matter particles off nuclei. We publish the energies of all events within the acceptance regions for dark-matter searches. In addition, we also publish the energies of the events within the electron-recoil band. This data set can be used to study interactions with electrons of CaWO$_4$. In this document we describe how to use these data sets. In particular, we explain the cut-survival probabilities required for comparisons of models with the data sets.

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  1. Boosted dark matter from semi-annihilations in the galactic center

    hep-ph 2025-01 conditional novelty 6.0 of 10

    Galactic Center semi-annihilations produce monoenergetic boosted dark matter that lets XENONnT, CRESST, and future DARWIN/DUNE probe spin-independent scattering down to about 1e-36 to 1e-38 cm2 for sub-GeV dark matter.

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