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Geant4-based electromagnetic background model for the CRESST dark matter experiment.
Abdelhameed, A H; Angloher, G; Bauer, P; Bento, A; Bertoldo, E; Breier, R; Bucci, C; Canonica, L; D'Addabbo, A; Lorenzo, S Di; Erb, A; Feilitzsch, F V; Iachellini, N Ferreiro; Fichtinger, S; Fuss, A; Gorla, P; Hauff, D; Jes Kovský, M; Jochum, J; Kaizer, J; Kinast, A; Kluck, H; Kraus, H; Langenkämper, A; Mancuso, M; Mokina, V; Mondragón, E; Olmi, M; Ortmann, T; Pagliarone, C; Palus Ová, V; Pattavina, L; Petricca, F; Potzel, W; Povinec, P; Pröbst, F; Reindl, F; Rothe, J; Schäffner, K; Schieck, J; Schipperges, V; Schmiedmayer, D; Schönert, S; Schwertner, C; Stahlberg, M; Stodolsky, L; Strandhagen, C; Strauss, R; Türkoglu, C; Usherov, I.
Afiliação
  • Abdelhameed AH; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Angloher G; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Bauer P; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Bento A; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Bertoldo E; 9Departamento de Fisica, Universidade de Coimbra, 3004 516 Coimbra, Portugal.
  • Breier R; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Bucci C; 2Faculty of Mathematics, Physics and Informatics, Comenius University, 84248 Bratislava, Slovakia.
  • Canonica L; 3INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy.
  • D'Addabbo A; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Lorenzo SD; 3INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy.
  • Erb A; 10GSSI-Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Feilitzsch FV; 3INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy.
  • Iachellini NF; 10GSSI-Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Fichtinger S; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Fuss A; Walther-Meißner-Institut für Tieftemperaturforschung, 85748 Garching, Germany.
  • Gorla P; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Hauff D; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Jes Kovský M; 5Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, 1050 Wien, Austria.
  • Jochum J; 5Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, 1050 Wien, Austria.
  • Kaizer J; 6Atominstitut, Technische Universität Wien, 1020 Wien, Austria.
  • Kinast A; 3INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy.
  • Kluck H; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Kraus H; 2Faculty of Mathematics, Physics and Informatics, Comenius University, 84248 Bratislava, Slovakia.
  • Langenkämper A; 7Eberhard-Karls-Universität Tübingen, 72076 Tübingen, Germany.
  • Mancuso M; 2Faculty of Mathematics, Physics and Informatics, Comenius University, 84248 Bratislava, Slovakia.
  • Mokina V; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Mondragón E; 5Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, 1050 Wien, Austria.
  • Olmi M; 6Atominstitut, Technische Universität Wien, 1020 Wien, Austria.
  • Ortmann T; 8Department of Physics, University of Oxford, Oxford, OX1 3RH UK.
  • Pagliarone C; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Palus Ová V; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Pattavina L; 5Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, 1050 Wien, Austria.
  • Petricca F; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Potzel W; 3INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy.
  • Povinec P; 10GSSI-Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Pröbst F; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Reindl F; 3INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy.
  • Rothe J; 12Dipartimento di Ingegneria Civile e Meccanica, Universitá degli Studi di Cassino e del Lazio Meridionale, 03043 Cassino, Italy.
  • Schäffner K; 2Faculty of Mathematics, Physics and Informatics, Comenius University, 84248 Bratislava, Slovakia.
  • Schieck J; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Schipperges V; 10GSSI-Gran Sasso Science Institute, 67100 L'Aquila, Italy.
  • Schmiedmayer D; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Schönert S; 4Physik-Department and Excellence Cluster Universe, Technische Universität München, 85747 Garching, Germany.
  • Schwertner C; 2Faculty of Mathematics, Physics and Informatics, Comenius University, 84248 Bratislava, Slovakia.
  • Stahlberg M; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Stodolsky L; 5Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, 1050 Wien, Austria.
  • Strandhagen C; 6Atominstitut, Technische Universität Wien, 1020 Wien, Austria.
  • Strauss R; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Türkoglu C; 1Max-Planck-Institut für Physik, 80805 Munich, Germany.
  • Usherov I; 5Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, 1050 Wien, Austria.
Eur Phys J C Part Fields ; 79(10): 881, 2019.
Article em En | MEDLINE | ID: mdl-31708682
ABSTRACT
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) dark matter search experiment aims for the detection of dark matter particles via elastic scattering off nuclei in CaWO 4 crystals. To understand the CRESST electromagnetic background due to the bulk contamination in the employed materials, a model based on Monte Carlo simulations was developed using the Geant4 simulation toolkit. The results of the simulation are applied to the TUM40 detector module of CRESST-II phase 2. We are able to explain up to ( 68 ± 16 ) % of the electromagnetic background in the energy range between 1 and 40 keV .
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2019 Tipo de documento: Article País de afiliação: Alemanha
Texto completo
Adicionar na Minha BVS
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Eur Phys J C Part Fields Ano de publicação: 2019 Tipo de documento: Article País de afiliação: Alemanha