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Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites
dc.creator | Adrover, M. | |
dc.creator | Althueser, L. | |
dc.creator | Andrieu, B. | |
dc.creator | Angelino, E. | |
dc.creator | Angevaare, J. R. | |
dc.creator | Antunović, Biljana | |
dc.creator | Aprile, E. | |
dc.creator | Babicz, M. | |
dc.creator | Bajpai, D. | |
dc.creator | Barberio, E. | |
dc.creator | Baudis, L. | |
dc.creator | Bazyk, M. | |
dc.creator | Bell, N. | |
dc.creator | Bellagamba, L. | |
dc.creator | Biondi, R. | |
dc.creator | Biondi, Y. | |
dc.creator | Bismark, A. | |
dc.creator | Boehm, C. | |
dc.creator | Breskin, A. | |
dc.creator | Brookes, E. J. | |
dc.creator | Brown, A. | |
dc.creator | Bruno, G. | |
dc.creator | Budnik, R. | |
dc.creator | Capelli, C. | |
dc.creator | Cardoso, J. M. R. | |
dc.creator | Chauvin, A. | |
dc.creator | Cimental Chavez, A. P. | |
dc.creator | Colijn, A. P. | |
dc.creator | Conrad, J. | |
dc.creator | Cuenca-García, J. J. | |
dc.creator | D’Andrea, V. | |
dc.creator | Decowski, M. P. | |
dc.creator | Deisting, A. | |
dc.creator | Di Gangi, P. | |
dc.creator | Diglio, S. | |
dc.creator | Doerenkamp, M. | |
dc.creator | Drexlin, G. | |
dc.creator | Eitel, K. | |
dc.creator | Elykov, A. | |
dc.creator | Engel, R. | |
dc.creator | Farrell, S. | |
dc.creator | Ferella, A. D. | |
dc.creator | Ferrari, C. | |
dc.creator | Fischer, H. | |
dc.creator | Flierman, M. | |
dc.creator | Fulgione, W. | |
dc.creator | Gaemers, P. | |
dc.creator | Gaior, R. | |
dc.creator | Galloway, M. | |
dc.creator | Garroum, N. | |
dc.creator | Ghosh, S. | |
dc.creator | Girard, F. | |
dc.creator | Glade-Beucke, R. | |
dc.creator | Glück, F. | |
dc.creator | Grandi, L. | |
dc.creator | Grigat, J. | |
dc.creator | Größle, R. | |
dc.creator | Guan, H. | |
dc.creator | Guida, M. | |
dc.creator | Hammann, R. | |
dc.creator | Hannen, V. | |
dc.creator | Hansmann-Menzemer, S. | |
dc.creator | Hargittai, N. | |
dc.creator | Hasegawa, T. | |
dc.creator | Hils, C. | |
dc.creator | Higuera, A. | |
dc.creator | Hiraoka, K. | |
dc.creator | Hoetzsch, L. | |
dc.creator | Iacovacci, M. | |
dc.creator | Itow, Y. | |
dc.creator | Jakob, J. | |
dc.creator | Jörg, F. | |
dc.creator | Kara, M. | |
dc.creator | Kavrigin, P. | |
dc.creator | Kazama, S. | |
dc.creator | Keller, M. | |
dc.creator | Kilminster, B. | |
dc.creator | Kleifges, M. | |
dc.creator | Kobayashi, M. | |
dc.creator | Kopec, A. | |
dc.creator | von Krosigk, B. | |
dc.creator | Kuger, F. | |
dc.creator | Landsman, H. | |
dc.creator | Lang, R. F. | |
dc.creator | Li, I. | |
dc.creator | Li, S. | |
dc.creator | Liang, S. | |
dc.creator | Lindemann, S. | |
dc.creator | Lindner, M. | |
dc.creator | Lombardi, F. | |
dc.creator | Loizeau, J. | |
dc.creator | Luce, T. | |
dc.creator | Ma, Y. | |
dc.creator | Macolino, C. | |
dc.creator | Mahlstedt, J. | |
dc.creator | Mancuso, A. | |
dc.creator | Marrodán Undagoitia, T. | |
dc.creator | Lopes, J. A. M. | |
dc.creator | Marignetti, F. | |
dc.creator | Martens, K. | |
dc.creator | Masbou, J. | |
dc.creator | Mastroianni, S. | |
dc.creator | Milutinovic, S. | |
dc.creator | Miuchi, K. | |
dc.creator | Miyata, R. | |
dc.creator | Molinario, A. | |
dc.creator | Monteiro, C. M. B. | |
dc.creator | Morå, K. | |
dc.creator | Morteau, E. | |
dc.creator | Mosbacher, Y. | |
dc.creator | Müller, J. | |
dc.creator | Murra, M. | |
dc.creator | Newstead, J. L. | |
dc.creator | Ni, K. | |
dc.creator | Oberlack, U. G. | |
dc.creator | Ostrovskiy, I. | |
dc.creator | Paetsch, B. | |
dc.creator | Pandurovic, M. | |
dc.creator | Pellegrini, Q. | |
dc.creator | Peres, R. | |
dc.creator | Pienaar, J. | |
dc.creator | Pierre, M. | |
dc.creator | Piotter, M. | |
dc.creator | Plante, G. | |
dc.creator | Pollmann, T. R. | |
dc.creator | Principe, L. | |
dc.creator | Qi, J. | |
dc.creator | Qin, J. | |
dc.creator | Rajado Silva, M. | |
dc.creator | Ramírez García, D. | |
dc.creator | Razeto, A. | |
dc.creator | Sakamoto, S. | |
dc.creator | Sanchez, L. | |
dc.creator | Sanchez-Lucas, P. | |
dc.creator | dos Santos, J. M. F. | |
dc.creator | Sartorelli, G. | |
dc.creator | Scaffidi, A. | |
dc.creator | Schulte, P. | |
dc.creator | Schultz-Coulon, H.-C. | |
dc.creator | Schulze Eißing, H. | |
dc.creator | Schumann, M. | |
dc.creator | Scotto Lavina, L. | |
dc.creator | Selvi, M. | |
dc.creator | Semeria, F. | |
dc.creator | Shagin, P. | |
dc.creator | Sharma, S. | |
dc.creator | Shen, W. | |
dc.creator | Silva, M. | |
dc.creator | Simgen, H. | |
dc.creator | Singh, R. | |
dc.creator | Solmaz, M. | |
dc.creator | Stanley, O. | |
dc.creator | Steidl, M. | |
dc.creator | Tan, P.-L. | |
dc.creator | Terliuk, A. | |
dc.creator | Thers, D. | |
dc.creator | Thümmler, T. | |
dc.creator | Tönnies, F. | |
dc.creator | Toschi, F. | |
dc.creator | Trinchero, G. | |
dc.creator | Trotta, R. | |
dc.creator | Tunnell, C. | |
dc.creator | Urquijo, P. | |
dc.creator | Valerius, K. | |
dc.creator | Vecchi, S. | |
dc.creator | Vetter, S. | |
dc.creator | Volta, G. | |
dc.creator | Vorkapic, D. | |
dc.creator | Wang, W. | |
dc.creator | Weerman, K. M. | |
dc.creator | Weinheimer, C. | |
dc.creator | Weiss, M. | |
dc.creator | Wenz, D. | |
dc.creator | Wittweg, C. | |
dc.creator | Wolf, J. | |
dc.creator | Wolf, T. | |
dc.creator | Wu, V. H. S. | |
dc.creator | Wurm, M. | |
dc.creator | Xing, Y. | |
dc.creator | Yamashita, M. | |
dc.creator | Ye, J. | |
dc.creator | Zavattini, G. | |
dc.creator | Zuber, K. | |
dc.date.accessioned | 2024-02-27T08:28:34Z | |
dc.date.available | 2024-02-27T08:28:34Z | |
dc.date.issued | 2024 | |
dc.identifier.issn | 1434-6052 | |
dc.identifier.uri | https://vinar.vin.bg.ac.rs/handle/123456789/12876 | |
dc.description.abstract | Xenon dual-phase time projections chambers (TPCs) have proven to be a successful technology in studying physical phenomena that require low-background conditions. With 40t of liquid xenon (LXe) in the TPC baseline design, DARWIN will have a high sensitivity for the detection of particle dark matter, neutrinoless double beta decay (0 ν β β), and axion-like particles (ALPs). Although cosmic muons are a source of background that cannot be entirely eliminated, they may be greatly diminished by placing the detector deep underground. In this study, we used Monte Carlo simulations to model the cosmogenic background expected for the DARWIN observatory at four underground laboratories: Laboratori Nazionali del Gran Sasso (LNGS), Sanford Underground Research Facility (SURF), Laboratoire Souterrain de Modane (LSM) and SNOLAB. We present here the results of simulations performed to determine the production rate of 137 Xe, the most crucial isotope in the search for 0 ν β β of 136 Xe. Additionally, we explore the contribution that other muon-induced spallation products, such as other unstable xenon isotopes and tritium, may have on the cosmogenic background. | en |
dc.relation | US National Science Foundation [No. 1719271, 1940209] | en |
dc.relation | European Research Council [No. 724320, 742789] | en |
dc.relation | Horizon 2020 Framework Programme [200020-162501, 200020-175863] | en |
dc.relation | H2020 Marie Skłodowska-Curie Actions [674896, 690575, 691164] | en |
dc.relation | Science and Technology Facilities Council [Grant ST/N000838/1] | en |
dc.relation | Ministry of Education, Science and Technological Development of the Republic of Serbia | en |
dc.rights | openAccess | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.source | The European Physical Journal C | en |
dc.title | Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites | en |
dc.type | article | en |
dc.rights.license | BY | |
dc.citation.volume | 84 | |
dc.citation.issue | 1 | |
dc.identifier.doi | 10.1140/epjc/s10052-023-12298-w | |
dc.type.version | publishedVersion | |
dc.identifier.scopus | 2-s2.0-85183882121 | |
dc.identifier.fulltext | http://vinar.vin.bg.ac.rs/bitstream/id/35570/s10052-023-12298-w.pdf |
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