Accès ouvert déclaré 2023 preprint

Detector development for the CRESST experiment

G. Angloher, S. Banik, G. Benato, A. Bento, A. Bertolini, R. Breier, C. Bucci, J. Burkhart, L. Canonica, A. D’Addabbo, S. Di Lorenzo, L. Einfalt, A. Erb, F. von Feilitzsch, S. Fichtinger, D. Fuchs, Abhijit Garai, V. M. Ghete, P. Gorla, P. V. Guillaumon, Subham Gupta, D. Hauff, M. Jes̆kovský, 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, Pavel P. Povinec, F. Proebst, F. Pucci, F. Reindl, J. Rothe, K. Schäeffner, J. Schieck, S. Schoenert, C. Schwertner, M. Stahlberg, L. Stodolsky, C. Strandhagen, Du Toit Strauss, I. Usherov, F. Wagner, M. Willers, V. Zema

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Le résumé fourni par la source

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.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

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Les sujets associés

Dark Matter and Cosmic PhenomenaParticle Detector Development and PerformanceScientific Research and Discoveries

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