Background suppression in the COSINUS experiment: Active muon veto and radiopure materials selection
M. Stukel, G. Angloher, Mukund Raghunath Bharadwaj, I. Dafinei , N. Di Marco, L. Einfalt, F. Ferroni, S. Fichtinger, A. Filipponi, T. Frank, M. Friedl, A. Fuss , Z. Ge, M. Heikinheimo, K. Huitu, M. Kellermann, R. Maji, M. Mancuso, L. Pagnanini, F. Petricca, S. Pirro, F. Pröbst, G. Profeta, A. Puiu, F. Reindl, K. Schäffner, J. Schieck, D. Schmiedmayer, C. Schwertner, M. Stahlberg, A. Stendahl, F. Wagner, S. Yue, V. Zema, Y. Zhu
SciPost Phys. Proc. 12, 032 (2023) · published 4 July 2023
- doi: 10.21468/SciPostPhysProc.12.032
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Proceedings event
14th International Conference on Identification of Dark Matter
Abstract
For over twenty-five years the DAMA/LIBRA experiment has reported an annual modulation signal that is consistent with a dark matter explanation. This signal is, currently, in tension with the null results observed by other searches that utilize different target detectors. The COSINUS experiment will perform a model-independent cross-check of the DAMA/LIBRA result by using the same target material, NaI crystals, operated as scintillating calorimeters. By measuring both temperature and light the NaI crystals in COSINUS will be able to distinguish between electron and nuclear recoils on an event-by-event basis. However, background events induced by cosmic-rays, environmental radioactivity or the intrinsic contamination of the materials used in the crystal, shielding and infrastructure can pose an issue to any analysis and must be fully understood. We report on the status of the development of the simulation for an active water Cherenkov muon veto, as well as the results of the beginning radiogenic material screening.
Authors / Affiliations: mappings to Contributors and Organizations
See all Organizations.- 1 2 Matthew Stukel,
- 3 G. Angloher,
- 3 Mukund Raghunath Bharadwaj,
- 2 4 I. Dafinei,
- 1 2 N. Di Marco,
- 5 6 Leonie Einfalt,
- 2 4 F. Ferroni,
- 6 S. Fichtinger,
- 1 7 A. Filipponi,
- 3 T. Frank,
- 6 Markus Friedl,
- 5 6 A. Fuss,
- 8 Z. Ge,
- 9 Matti Heikinheimo,
- 9 Katri Huitu,
- 3 M. Kellermann,
- 5 6 R. Maji,
- 3 M. Mancuso,
- 1 2 L. Pagnanini,
- 3 Federica Petricca,
- 1 S. Pirro,
- 3 F. Pröbst,
- 1 7 G. Profeta,
- 1 2 A. Puiu,
- 5 6 Florian Reindl,
- 3 K. Schäffner,
- 5 6 J. Schieck,
- 5 6 D. Schmiedmayer,
- 5 6 C. Schwertner,
- 3 Martin Stahlberg,
- 9 A. Stendahl,
- 6 F. Wagner,
- 8 S. Yue,
- 3 Vanessa Zema,
- 8 Y. Zhu
- 1 Laboratori Nazionali del Gran Sasso / Gran Sasso National Laboratory [LNGS]
- 2 Gran Sasso Science Institute [GSSI]
- 3 Max-Planck-Institut für Physik / Max Planck Institute for Physics [MPP]
- 4 INFN Sezione di Roma-1 / INFN Sezione di Roma-1
- 5 Atominstitut [ATI]
- 6 Österreichische Akademie der Wissenschaften / Austrian Academy of Sciences [ÖAW]
- 7 Università degli Studi dell'Aquila / University of L'Aquila
- 8 中国科学院上海硅酸盐研究所 / Shanghai Institute of Ceramics [SICCAS]
- 9 Helsinki Institute of Physics