Background suppression in the COSINUS experiment: Active muon veto and radiopure materials selection

Author:

Stukel Matthew12,Angloher G.3,Raghunath Bharadwaj Mukund3,Dafinei I.24,Di Marco N.12,Einfalt Leonie56,Ferroni F.24,Fichtinger S.6,Filipponi A.17,Frank T.3,Friedl Markus6,Fuss A.56,Ge Z.8,Heikinheimo Matti9,Huitu Katri9,Kellermann M.3,Maji R.56,Mancuso M.3,Pagnanini L.12,Petricca Federica3,Pirro S.1,Pröbst F.3,Profeta G.17,Puiu A.12,Reindl Florian56,Schäffner K.3,Schieck J.56,Schmiedmayer D.56,Schwertner C.56,Stahlberg Martin3,Stendahl A.9,Wagner F.6,Yue S.8,Zema Vanessa3,Zhu Y.8

Affiliation:

1. Gran Sasso National Laboratory

2. Gran Sasso Science Institute

3. Max Planck Institute for Physics

4. INFN Sezione di Roma-1

5. Atominstitut

6. Austrian Academy of Sciences

7. University of L'Aquila

8. Shanghai Institute of Ceramics

9. Helsinki Institute of Physics

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.

Publisher

Stichting SciPost

Subject

General Medicine

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