학술논문
Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136Xe
Document Type
Erratum
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.; Gangi, P. Di; Giovanni, A. Di; 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
The European Physical Journal C: Particles and Fields. 83(11)
Subject
Language
English
ISSN
1434-6052
Abstract
We correct an overestimation of the production rate of 13780νββ13622%T1/20ν=3.0×1027yrXe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic background source is now at a level similar to the irreducible background from solar 13780νββ13622%T1/20ν=3.0×1027yrB neutrinos, thus unproblematic at the LNGS depth. The projected half-life sensitivity for the neutrinoless double beta decay (13780νββ13622%T1/20ν=3.0×1027yr) of 13780νββ13622%T1/20ν=3.0×1027yrXe improves by 13780νββ13622%T1/20ν=3.0×1027yr compared to the previously reported number and is now 13780νββ13622%T1/20ν=3.0×1027yr (90% C.L.) after 10 years of DARWIN operation.