Zobrazeno 1 - 10
of 14
pro vyhledávání: '"C D, Tunnell"'
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
Autor:
DARWIN Collaboration, J. Aalbers, F. Agostini, S. E. M. Ahmed Maouloud, M. Alfonsi, L. Althueser, F. D. Amaro, J. Angevaare, V. C. Antochi, B. Antunovic, E. Aprile, L. Arazi, F. Arneodo, M. Balzer, L. Baudis, D. Baur, M. L. Benabderrahmane, Y. Biondi, A. Bismark, C. Bourgeois, A. Breskin, P. A. Breur, A. Brown, E. Brown, S. Brünner, G. Bruno, R. Budnik, C. Capelli, J. Cardoso, D. Cichon, M. Clark, A. P. Colijn, J. Conrad, J. J. Cuenca-García, J. P. Cussonneau, M. P. Decowski, A. Depoian, J. Dierle, P. Di Gangi, A. Di Giovanni, S. Diglio, D. Douillet, G. Drexlin, K. Eitel, R. Engel, E. Erdal, A. D. Ferella, H. Fischer, P. Fischer, W. Fulgione, P. Gaemers, M. Galloway, F. Gao, D. Giovagnoli, F. Girard, R. Glade-Beucke, F. Glück, L. Grandi, S. Grohmann, R. Größle, R. Gumbsheimer, V. Hannen, S. Hansmann-Menzemer, C. Hils, B. Holzapfel, J. Howlett, G. Iaquaniello, F. Jörg, M. Keller, J. Kellerer, G. Khundzakishvili, B. Kilminster, M. Kleifges, T. K. Kleiner, G. Koltmann, A. Kopec, A. Kopmann, L. M. Krauss, F. Kuger, L. LaCascio, H. Landsman, R. F. Lang, S. Lindemann, M. Lindner, F. Lombardi, J. A. M. Lopes, A. Loya Villalpando, Y. Ma, C. Macolino, J. Mahlstedt, A. Manfredini, T. Marrodán Undagoitia, J. Masbou, D. Masson, E. Masson, N. McFadden, P. Meinhardt, R. Meyer, B. Milosevic, S. Milutinovic, A. Molinario, C. M. B. Monteiro, K. Morå, E. Morteau, Y. Mosbacher, M. Murra, J. L. Newstead, K. Ni, U. G. Oberlack, M. Obradovic, K. Odgers, I. Ostrovskiy, J. Palacio, M. Pandurovic, B. Pelssers, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, G. Plante, J. Qi, J. Qin, D. Ramírez García, S. E. Reichard, N. Rupp, P. Sanchez-Lucas, J. M. F. dos Santos, G. Sartorelli, D. Schulte, H. C. Schultz-Coulon, H. Schulze Eißing, M. Schumann, L. Scotto Lavina, M. Selvi, P. Shagin, S. Sharma, W. Shen, M. Silva, H. Simgen, M. Steidl, S. Stern, D. Subotic, P. Szabo, A. Terliuk, C. Therreau, D. Thers, K. Thieme, F. Toennies, R. Trotta, C. D. Tunnell, K. Valerius, G. Volta, D. Vorkapic, M. Weber, Y. Wei, C. Weinheimer, M. Weiss, D. Wenz, C. Wittweg, J. Wolf, S. Wuestling, M. Wurm, Y. Xing, T. Zhu, Y. Zhu, J. P. Zopounidis, K. Zuber
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 80, Iss 12, Pp 1-10 (2020)
Abstract We detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp, $$^7$$ 7 B
Externí odkaz:
https://doaj.org/article/453323db1c824b7c9db9d09f5649c02b
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
Autor:
S Al Kharusi, S Y BenZvi, J S Bobowski, W Bonivento, V Brdar, T Brunner, E Caden, M Clark, A Coleiro, M Colomer-Molla, J I Crespo-Anadón, A Depoian, D Dornic, V Fischer, D Franco, W Fulgione, A Gallo Rosso, M Geske, S Griswold, M Gromov, D Haggard, A Habig, O Halim, A Higuera, R Hill, S Horiuchi, K Ishidoshiro, C Kato, E Katsavounidis, D Khaitan, J P Kneller, A Kopec, V Kulikovskiy, M Lai, M Lamoureux, R F Lang, H L Li, M Lincetto, C Lunardini, J Migenda, D Milisavljevic, M E McCarthy, E O Connor, E O Sullivan, G Pagliaroli, D Patel, R Peres, B W Pointon, J Qin, N Raj, A Renshaw, A Roeth, J Rumleskie, K Scholberg, A Sheshukov, T Sonley, M Strait, V Takhistov, I Tamborra, J Tseng, C D Tunnell, J Vasel, C F Vigorito, B Viren, C J Virtue, J S Wang, L J Wen, L Winslow, F L H Wolfs, X J Xu, Y Xu
Publikováno v:
New Journal of Physics, Vol 23, Iss 3, p 031201 (2021)
The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields beca
Externí odkaz:
https://doaj.org/article/6bbda9d6120c404bb8f2f3628555ad72
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
Autor:
E. D. Hallman, G. Prior, Benjamin Monreal, E. D. Earle, P. J. Doe, S. J. M. Peeters, K. J. Keeter, T. Tsui, F. A. Duncan, P. Skensved, M. DiMarco, K. Boudjemline, Yuen-Dat Chan, J. M. Wouters, J. Heise, S. Habib, K. Graham, X. Dai, S. M. Oser, J. A. Detwiler, Keith Rielage, H. Wan Chan Tseung, M. L. Miller, A. B. McDonald, R. D. Martin, Andrew Hime, I. Levine, Jocelyn Monroe, Alain Bellerive, D. L. Wark, R. J. Ford, T. J. Sonley, R. L. Hahn, H. Fergani, R. G. H. Robertson, M. H. Schwendener, R. MacLellan, Monica Dunford, J. Maneira, B. Beltran, Mark Guy Boulay, Bei Cai, David A. Sinclair, C. A. Duba, F. Zhang, J. Law, D. Chauhan, Peter Watson, B. Jamieson, A. W. P. Poon, Christopher C. M. Kyba, P.-L. Drouin, N. Tolich, C. B. Krauss, N. S. Oblath, B. Aharmim, T.H. Burritt, Kai Zuber, C. D. Tunnell, A. L. Hallin, R. L. Helmer, B. Morissette, J. A. Secrest, I. T. Lawson, C. Kraus, B. T. Cleveland, S. R. Seibert, D. Waller, G. A. Cox, R. A. Ott, N. West, W. J. Heintzelman, K. T. Lesko, J. R. Wilson, M. Kos, A. Wright, O. Simard, E. W. Beier, B.A. VanDevender, L. C. Stonehill, C. Howard, J. Farine, A. J. Noble, C. J. Virtue, B. C. Robertson, G. Doucas, E. Guillian, T. Kutter, N. Barros, Joseph A. Formaggio, Minfang Yeh, J. C. Loach, N. A. Jelley, Hal Evans, S. D. Reitzner, S. N. Ahmed, Joshua R. Klein, M. Bergevin, N. McCauley, R. Van Berg, M. L. Chen, S. Majerus, L. L. Kormos, G. T. Ewan, N. Gagnon, R. Hazama, G. D. Orebi Gann, H. Deng, B. L. Wall, H. M. O'Keeffe, H. B. Mak, S. McGee, S. D. Biller, Bernie G. Nickel, P. J. Harvey, J. F. Wilkerson, Steven Elliott, M. A. Howe, M. Huang, G. Tešić, J. R. Leslie, F. Fleurot, A. E. Anthony, J. Tm. Goon
We have performed three searches for high-frequency signals in the solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO), motivated by the possibility that solar $g$-mode oscillations could affect the production or propagation of sol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7a565760970b0aea6abf3a64d2576bb
https://doi.org/10.1088/0004-637x/710/1/540
https://doi.org/10.1088/0004-637x/710/1/540
Autor:
M. DiMarco, R. J. Ford, R. W. Ollerhead, R. MacLellan, Mark Guy Boulay, P. Jagam, M. H. Schwendener, A. Krüger, B. C. Robertson, J. Tm. Goon, N. Gagnon, G. Doucas, F. Zhang, J. R. Wilson, J. B. Wilhelmy, S. Habib, R. L. Helmer, S. R. Seibert, J. Law, T. Kutter, J. Heise, N. West, P.-L. Drouin, P. Skensved, Hal Evans, F. Fleurot, G. D. Orebi Gann, J. F. Amsbaugh, Ryuta Hazama, H. Wan Chan Tseung, M. L. Miller, A. E. Anthony, J. V. Germani, E. D. Hallman, W. J. Heintzelman, H. Deng, K. M. Heeger, E. Guillian, C. Kraus, S. D. Biller, J. R. Leslie, S. Majerus, Yuen-Dat Chan, K. Boudjemline, K. Graham, M. W.E. Smith, L. L. Kormos, Alain Bellerive, Bernie G. Nickel, J. Wendland, S. M. Oser, S. R. Elliott, G. T. Ewan, Andrew Hime, Joshua R. Klein, A. W. Myers, P. J. Harvey, Juan-Manuel Anaya, J. Banar, K. T. Lesko, Monica Dunford, J. Maneira, M. A. Howe, M. Huang, Reyco Henning, P. M. Thornewell, N. Barros, T. J. Sonley, A. W. P. Poon, S. D. Reitzner, S. N. Ahmed, R. D. Martin, J. J. Simpson, Malcolm M. Fowler, Kai Zuber, T. J. Bowles, C. D. Tunnell, P. J. Doe, G. Tešić, J. A. Formaggio, M. Bergevin, C. A. Duba, N. McCauley, A. Goldschmidt, Bei Cai, Minfang Yeh, E. Rollin, R. G. H. Robertson, R. A. Ott, T.H. Burritt, D. Chauhan, R. Van Berg, H. B. Mak, C. J. Virtue, B. Jamieson, J. F. Wilkerson, T. D. Van Wechel, K. J. Keeter, A. Wright, J. C. Loach, C. Currat, N. A. Jelley, S. J. M. Peeters, T. D. Steiger, M. L. Chen, T. V. Bullard, M. Kos, A. A. Hamian, O. Simard, X. Dai, J. A. Detwiler, R. Lange, G. Prior, C. Howard, E. W. Beier, J. Farine, R. L. Hahn, M. C. Browne, A. J. Noble, L. C. Stonehill, S. McGee, J. M. Wouters, A. B. McDonald, Christopher C. M. Kyba, B. L. Wall, B. T. Cleveland, H. M. O'Keeffe, Keith Rielage, Jocelyn Monroe, B. Aharmim, B. Beltran, A. L. Hallin, C. Mifflin, N. S. Oblath, C. B. Krauss, M. R. Dragowsky, B. A. VanDevender, N. Tolich, Guthrie Miller, B. Morissette, Benjamin Monreal, E. D. Earle, G. C. Harper, F. A. Duncan, J. A. Secrest, I. T. Lawson, D. Waller, G. A. Cox, H. Fergani, T. Tsui
Publikováno v:
Physical Review C. 87
This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the Sudbury Neutrino Observatory (SNO). An array of He-3 proportional counters was installed in the heavy-water target to measure precisely the rate of ne
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
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
https://hal.in2p3.fr/in2p3-00708450
Autor:
Monica Dunford, J. Maneira, A. W. P. Poon, Christopher C. M. Kyba, J. R. Leslie, J. Tm. Goon, J. F. Wilkerson, Joseph A. Formaggio, M. Kos, Minfang Yeh, C. J. Virtue, C. B. Krauss, N. S. Oblath, M. L. Miller, E. W. Beier, J. C. Loach, B. Beltran, R. A. Ott, R. D. Martin, H. B. Mak, N. A. Jelley, Jocelyn Monroe, N. Gagnon, Andrew Hime, I. Levine, R. G. H. Robertson, E. D. Hallman, M. Huang, G. Tešić, F. A. Duncan, Howe, F. Fleurot, R. Hazama, Yuen-Dat Chan, K. Graham, A. L. Hallin, J. R. Wilson, Kai Zuber, C. D. Tunnell, S. McGee, B. C. Robertson, A. E. Anthony, S. M. Oser, G. D. Orebi Gann, S. D. Biller, N. Barros, Bernie G. Nickel, B. Aharmim, G. Doucas, A. B. McDonald, C. Kraus, S. J. M. Peeters, P. J. Harvey, J.M. Wouters, R. L. Hahn, H. Deng, T. Tsui, S. Habib, N. Tolich, T. Kutter, P. Skensved, M. DiMarco, Steven Elliott, B.A. VanDevender, P. J. Doe, R. J. Ford, M. H. Schwendener, F. Zhang, J. Law, B. L. Wall, Hal Evans, David A. Sinclair, H. M. O'Keeffe, K. Boudjemline, N. West, W. J. Heintzelman, K. T. Lesko, C. Howard, J. Farine, A. J. Noble, B. Morissette, Keith Rielage, K. J. Keeter, T. J. Sonley, Bei Cai, E. Guillian, R. MacLellan, D. Chauhan, Mark Guy Boulay, L. L. Kormos, P.-L. Drouin, B. Jamieson, R. L. Helmer, G. T. Ewan, S. D. Reitzner, S. N. Ahmed, S. R. Seibert, J. Heise, X. Dai, J. A. Detwiler, C. A. Duba, H. Fergani, J. A. Secrest, I. T. Lawson, D. Waller, G. A. Cox, Benjamin Monreal, E. D. Earle, H. Wan Chan Tseung, D. L. Wark, G. Prior, T.H. Burritt, B. T. Cleveland, A. Wright, O. Simard, Alain Bellerive, L. C. Stonehill, M. Bergevin, N. McCauley, R. Van Berg, M. L. Chen, S. Majerus, Joshua R. Klein
Publikováno v:
Physical Review C, C81
Results are reported from a joint analysis of Phase I and Phase II data from the Sudbury Neutrino Observatory. The effective electron kinetic energy threshold used is T_eff=3.5 MeV, the lowest analysis threshold yet achieved with water Cherenkov dete
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
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https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3fdd0d6145ec788d6bdd71a6716a2567