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Detector development for the CRESST experiment

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arxiv 2311.07318 v1 pith:V5T77RQU submitted 2023-11-13 physics.ins-det astro-ph.IM

Detector development for the CRESST experiment

G. Angloher , S. Banik , G. Benato , A. Bento , A. Bertolini , R. Breier , C. Bucci , J. Burkhart
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L. Canonica A. D'Addabbo S. Di Lorenzo L. Einfalt A. Erb F.v. Feilitzsch S. Fichtinger D. Fuchs A. Garai V.M. Ghete P. Gorla P.V. Guillaumon S. Gupta D. Hauff M. Je\v{s}kovsk\'y J. Jochum M. Kaznacheeva A. Kinast H. Kluck H. Kraus S. Kuckuk A. Langenkaemper M. Mancuso L. Marini B. Mauri L. Meyer V. Mokina M. Olmi T. Ortmann C. Pagliarone L. Pattavina F. Petricca W. Potzel P. Povinec F. Proebst F. Pucci F. Reindl J. Rothe K. Schaeffner J. Schieck S. Schoenert C. Schwertner M. Stahlberg L. Stodolsky C. Strandhagen R. Strauss I. Usherov F. Wagner M. Willers V. Zema
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classification physics.ins-det astro-ph.IM
keywords detectorbackgroundbeencresstexperimentreachbecamebelow
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Recently low-mass dark matter direct searches have been hindered by a low energy background, drastically reducing the physics reach of the experiments. In the CRESST-III experiment, this signal is characterised by a significant increase of events below 200 eV. As the origin of this background is still unknown, it became necessary to develop new detector designs to reach a better understanding of the observations. Within the CRESST collaboration, three new different detector layouts have been developed and they are presented in this contribution.

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