Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe

Autor: F. Agostini, S. E. M. Ahmed Maouloud, L. Althueser, F. Amaro, B. Antunovic, E. Aprile, L. Baudis, D. Baur, Y. Biondi, A. Bismark, P. A. Breur, A. Brown, G. Bruno, R. Budnik, C. Capelli, J. Cardoso, D. Cichon, M. Clark, A. P. Colijn, J. J. Cuenca-García, J. P. Cussonneau, M. P. Decowski, A. Depoian, J. Dierle, P. Di Gangi, A. Di Giovanni, S. Diglio, J. M. F. dos Santos, G. Drexlin, K. Eitel, R. Engel, A. D. Ferella, H. Fischer, M. Galloway, F. Gao, F. Girard, F. Glück, L. Grandi, R. Größle, R. Gumbsheimer, S. Hansmann-Menzemer, F. Jörg, G. Khundzakishvili, A. Kopec, F. Kuger, L. M. Krauss, H. Landsman, R. F. Lang, S. Lindemann, M. Lindner, J. A. M. Lopes, A. Loya Villalpando, C. Macolino, A. Manfredini, T. Marrodán Undagoitia, J. Masbou, E. Masson, P. Meinhardt, S. Milutinovic, A. Molinario, C. M. B. Monteiro, M. Murra, U. G. Oberlack, M. Pandurovic, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, J. Qin, D. Ramírez García, S. Reichard, N. Rupp, P. Sanchez-Lucas, G. Sartorelli, D. Schulte, M. Schumann, L. Scotto Lavina, M. Selvi, M. Silva, H. Simgen, M. Steidl, A. Terliuk, C. Therreau, D. Thers, K. Thieme, R. Trotta, C. D. Tunnell, K. Valerius, G. Volta, D. Vorkapic, C. Weinheimer, C. Wittweg, J. Wolf, J. P. Zopounidis, K. Zuber, DARWIN Collaboration

Publikováno v: European Physical Journal C: Particles and Fields, Vol 83, Iss 11, Pp 1-4 (2023)

Abstract We correct an overestimation of the production rate of $$^{137}$$ 137 Xe 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 $$^8$$ 8

Externí odkaz: https://doaj.org/article/c66391b8af7a4bd29a3391d934638348

Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe

Autor: F. Agostini, S. E. M. Ahmed Maouloud, L. Althueser, F. Amaro, B. Antunovic, E. Aprile, L. Baudis, D. Baur, Y. Biondi, A. Bismark, P. A. Breur, A. Brown, G. Bruno, R. Budnik, C. Capelli, J. Cardoso, D. Cichon, M. Clark, A. P. Colijn, J. J. Cuenca-García, J. P. Cussonneau, M. P. Decowski, A. Depoian, J. Dierle, P. Di Gangi, A. Di Giovanni, S. Diglio, J. M. F. dos Santos, G. Drexlin, K. Eitel, R. Engel, A. D. Ferella, H. Fischer, M. Galloway, F. Gao, F. Girard, F. Glück, L. Grandi, R. Größle, R. Gumbsheimer, S. Hansmann-Menzemer, F. Jörg, G. Khundzakishvili, A. Kopec, F. Kuger, L. M. Krauss, H. Landsman, R. F. Lang, S. Lindemann, M. Lindner, J. A. M. Lopes, A. Loya Villalpando, C. Macolino, A. Manfredini, T. Marrodán Undagoitia, J. Masbou, E. Masson, P. Meinhardt, S. Milutinovic, A. Molinario, C. M. B. Monteiro, M. Murra, U. G. Oberlack, M. Pandurovic, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, J. Qin, D. Ramírez García, S. Reichard, N. Rupp, P. Sanchez-Lucas, G. Sartorelli, D. Schulte, M. Schumann, L. Scotto Lavina, M. Selvi, M. Silva, H. Simgen, M. Steidl, A. Terliuk, C. Therreau, D. Thers, K. Thieme, R. Trotta, C. D. Tunnell, K. Valerius, G. Volta, D. Vorkapic, C. Weinheimer, C. Wittweg, J. Wolf, J. P. Zopounidis, K. Zuber, DARWIN Collaboration

Publikováno v: European Physical Journal C: Particles and Fields, Vol 80, Iss 9, Pp 1-11 (2020)

Abstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target

Externí odkaz: https://doaj.org/article/8578e145f1c346b2ac06e5a732969a72

MAUS: The MICE Analysis User Software

Autor: R. B. S. Gardener, J. Martyniak, Kenneth Long, Ao Liu, Y. Karadzhov, E. Overton, A. Kurup, A. Dobbs, J. C. Nugent, Scott Wilbur, S. Middleton, R. Bayes, P. Franchini, T. A. Mohayai, K. Walaron, M. Winter, G. Kafka, C. Heidt, C. Pidcott, Yagmur Torun, V. Pec, C. Hunt, M. Uchida, F. Drielsma, V. Verguilov, David Colling, P. Kyberd, I. Taylor, Chris Rogers, Mike Rayner, E. M. Santos, M. Savic, D. Rajaram, J. J. Nebrensky, R. Asfandiyarov, D. Maletic, C. D. Tunnell, J. R. Greis, M. Littlefield, M. Bogomilov, Ivan Reid, Malcolm Ellis, P. Hanlet, M. Drews, M. Fedorov, V. Blackmore

The Muon Ionization Cooling Experiment (MICE) collaboration has developed the MICE Analysis User Software (MAUS) to simulate and analyze experimental data. It serves as the primary codebase for the experiment, providing for offline batch simulation a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c89b1718cc821f594f49bfc98f0b9bc

The MICE Muon Beam on ISIS and the beam-line instrumentation of the Muon Ionization Cooling Experiment

Autor: Maurizio Bonesini, J. Tarrant, A. Oates, A. Iaciofano, A. Blondel, Kenneth Long, Simone Gilardoni, Robert B. Palmer, D. Huang, T. L. Hart, S. York, R. Beuselinck, N. Collomb, Alessandra Lombardi, A. Wilson, L. M. Cremaldi, S. Griffiths, Chris Rogers, L. Howlett, H.G. Kirk, M. Khaleeq, A. DeMello, Michael A. Green, Malcolm Ellis, T.W. Bradshaw, H. Sakamoto, E. Gschwendtner, A. Lintern, C. Nelson, A. de Bari, A. Fish, Fr Pastore, Koji Yoshimura, V. Kasey, T. Hayler, P. Snopok, A. Sato, V. Blackmore, D. Clark, R. Nicholson, T. Sashalmi, J. J. Nebrensky, G. Vankova-Kirilova, Mario Parisi, G. Lucchini, P.A. Cooke, P. Owens, Paul Fraser Harrison, S. Watson, F. Masciocchi, D. A. Sanders, T. Yano, Maurizio Vretenar, A. Tonazzo, David Colling, C. D. Tunnell, K. Tilley, I. Russinov, K. Walaron, Matthew Hills, I. Mullacrane, A. Cirillo, R. Sandstrom, X. Yang, P. J. Dornan, G. Gregoire, J. Rochford, H. Wisting, C. Petitjean, Yasuo Fukui, P. Hodgson, Michael S. Zisman, Alessandro Manfredini, Richard Fletcher, L. Coney, U. Bravar, Y. Mori, P.J. Smith, D. Kolev, G. Kafka, T. Carlisle, E. Overton, A. D. Bross, J. Alexander, Max Robinson, R. Mazza, M. Courthold, A. Nichols, S. Greenwood, Y. Kuno, C. Macwaters, G. G. Hanson, C. N. Booth, P. Hanlet, W. Lau, Andrew Moss, R. Tsenov, K. Lee, A.K. Jamdagni, A. Jones, Y. Karadzhov, S. Fayer, M. Yoshida, Juan C. Gallardo, P. Kyberd, R. Hare, Patrick Janot, A. Alekou, G. Charnley, C. Heidt, S. Ricciardi, P. Gruber, Federico Ferri, Daniel M. Kaplan, Jaroslaw Pasternak, David B. Cline, Derun Li, Ben Freemire, S. Blot, H. Haseroth, G.J. Barber, Rebecca Seviour, David Neuffer, P. Bene, R. Gamet, Frank Filthaut, D.E. Baynham, M. Apollonio, Domizia Orestano, Takashi Matsushita, Holger Witte, V. Grichine, Christopher J. White, S. Ramberger, E. McKigney, R. J. Apsimon, D. Adey, F. J. P. Soler, J. S. Graulich, Klaus Hanke, L. Tortora, Mike Rayner, Steve Virostek, B. Martlew, R. Garoby, Milorad Popovic, Y. Ivaniouchenkov, Shiming Yang, Franck Cadoux, D. J. Summers, S. B. Boyd, Maiko Takahashi, Rob Edgecock, Yagmur Torun, A. Dobbs, Shota Suzuki, M. A.C. Cummings, V. Verguilov, F. Strati, F. Y. Xu, L. Wang, S.A. Kahn, R. Bertoni, M. Capponi, S. X. Zheng, T.J. Roberts, G. Cecchet, W. Spensley, S. Geer, Alfred Moretti, Yasar Onel, T. Savidge, S. Ishimoto, J. Leaver, P. Drumm, Yongsun Kim, V. Palladino, David Forrest, Robert Rimmer, F. Paleari, J.H. Cobb, D. Adams, Robert D. Preece, I. Clark, J. J. Back, M. Littlefield, M. Bogomilov, P. Barclay

Publikováno v: Journal of Instrumentation
Journal of Instrumentation, 2012, 7, pp.P05009. ⟨10.1088/1748-0221/7/05/P05009⟩
Journal of Instrumentation, Vol. 7 (2012) P. P05009
Journal of Instrumentation, IOP Publishing, 2012, 7, pp.P05009. ⟨10.1088/1748-0221/7/05/P05009⟩
JINST
Journal of Instrumentation, 7, 5, pp. P05009
Journal of Instrumentation, 7, P05009

The international Muon Ionization Cooling Experiment (MICE), which is under construction at the Rutherford Appleton Laboratory (RAL), will demonstrate the principle of ionization cooling as a technique for the reduction of the phase-space volume occu

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb7d47d59e5a7017c27d8d2df70e3d35
https://hal.in2p3.fr/in2p3-00708450

Independent measurement of the total active 8B solar neutrino flux using an array of 3He proportional counters at the sudbury neutrino observatory

Autor: B, Aharmim, S N, Ahmed, J F, Amsbaugh, A E, Anthony, J, Banar, N, Barros, E W, Beier, A, Bellerive, B, Beltran, M, Bergevin, S D, Biller, K, Boudjemline, M G, Boulay, T J, Bowles, M C, Browne, T V, Bullard, T H, Burritt, B, Cai, Y D, Chan, D, Chauhan, M, Chen, B T, Cleveland, G A, Cox-Mobrand, C A, Currat, X, Dai, H, Deng, J, Detwiler, M, DiMarco, P J, Doe, G, Doucas, P-L, Drouin, C A, Duba, F A, Duncan, M, Dunford, E D, Earle, S R, Elliott, H C, Evans, G T, Ewan, J, Farine, H, Fergani, F, Fleurot, R J, Ford, J A, Formaggio, M M, Fowler, N, Gagnon, J V, Germani, A, Goldschmidt, J T M, Goon, K, Graham, E, Guillian, S, Habib, R L, Hahn, A L, Hallin, E D, Hallman, A A, Hamian, G C, Harper, P J, Harvey, R, Hazama, K M, Heeger, W J, Heintzelman, J, Heise, R L, Helmer, R, Henning, A, Hime, C, Howard, M A, Howe, M, Huang, P, Jagam, B, Jamieson, N A, Jelley, K J, Keeter, J R, Klein, L L, Kormos, M, Kos, A, Krüger, C, Kraus, C B, Krauss, T, Kutter, C C M, Kyba, R, Lange, J, Law, I T, Lawson, K T, Lesko, J R, Leslie, J C, Loach, R, MacLellan, S, Majerus, H B, Mak, J, Maneira, R, Martin, K, McBryde, N, McCauley, A B, McDonald, S, McGee, C, Mifflin, G G, Miller, M L, Miller, B, Monreal, J, Monroe, B, Morissette, A, Myers, B G, Nickel, A J, Noble, N S, Oblath, H M, O'Keeffe, R W, Ollerhead, G D Orebi, Gann, S M, Oser, R A, Ott, S J M, Peeters, A W P, Poon, G, Prior, S D, Reitzner, K, Rielage, B C, Robertson, R G H, Robertson, E, Rollin, M H, Schwendener, J A, Secrest, S R, Seibert, O, Simard, J J, Simpson, L, Sinclair, P, Skensved, M W E, Smith, T D, Steiger, L C, Stonehill, G, Tesić, P M, Thornewell, N, Tolich, T, Tsui, C D, Tunnell, T, Van Wechel, R, Van Berg, B A, VanDevender, C J, Virtue, T J, Walker, B L, Wall, D, Waller, H Wan Chan, Tseung, J, Wendland, N, West, J B, Wilhelmy, J F, Wilkerson, J R, Wilson, J M, Wouters, A, Wright, M, Yeh, F, Zhang, K, Zuber

The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (nu_x) 8B solar neutrino flux. This technique is independen

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3fdd0d6145ec788d6bdd71a6716a2567