학술논문
Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $^{136}$Xe
Document Type
Working Paper
Author
Agostini, F.; Maouloud, S. E. M. Ahmed; Althueser, L.; Amaro, F.; Antunovic, B.; Aprile, E.; Baudis, L.; Baur, D.; Biondi, Y.; Bismark, A.; Breur, P. A.; Brown, A.; Bruno, G.; Budnik, R.; Capelli, C.; Cardoso, J.; Cichon, D.; Clark, M.; Colijn, A. P.; Cuenca-García, J. J.; Cussonneau, J. P.; Decowski, M. P.; Depoian, A.; Dierle, J.; Di Gangi, P.; Di Giovanni, A.; Diglio, S.; Santos, J. M. F. dos; Drexlin, G.; Eitel, K.; Engel, R.; Ferella, A. D.; Fischer, H.; Galloway, M.; Gao, F.; Girard, F.; Glück, F.; Grandi, L.; Größle, R.; Gumbsheimer, R.; Hansmann-Menzemer, S.; Jörg, F.; Khundzakishvili, G.; Kopec, A.; Kuger, F.; Krauss, L. M.; Landsman, H.; Lang, R. F.; Lindemann, S.; Lindner, M.; Lopes, J. A. M.; Villalpando, A. Loya; Macolino, C.; Manfredini, A.; Undagoitia, T. Marrodán; Masbou, J.; Masson, E.; Meinhardt, P.; Milutinovic, S.; Molinario, A.; Monteiro, C. M. B.; Murra, M.; Oberlack, U. G.; Pandurovic, M.; Peres, R.; Pienaar, J.; Pierre, M.; Pizzella, V.; Qin, J.; García, D. Ramírez; Reichard, S.; Rupp, N.; Sanchez-Lucas, P.; Sartorelli, G.; Schulte, D.; Schumann, M.; Lavina, L. Scotto; Selvi, M.; Silva, M.; Simgen, H.; Steidl, M.; Terliuk, A.; Therreau, C.; Thers, D.; Thieme, K.; Trotta, R.; Tunnell, C. D.; Valerius, K.; Volta, G.; Vorkapic, D.; Weinheimer, C.; Wittweg, C.; Wolf, J.; Zopounidis, J. P.; Zuber, K.
Source
Eur. Phys. J. C 80, 808 (2020)
Subject
Language
Abstract
The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $^{136}$Xe. Out of its 50$\,$t total natural xenon inventory, 40$\,$t will be the active target of a time projection chamber which thus contains about 3.6 t of $^{136}$Xe. Here, we show that its projected half-life sensitivity is $2.4\times10^{27}\,$yr, using a fiducial volume of 5t of natural xenon and 10$\,$yr of operation with a background rate of less than 0.2$~$events/(t$\cdot$yr) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $^{136}$Xe.
Comment: 12 pages, 9 figures
Comment: 12 pages, 9 figures