Results 21 to 30 of about 1,187,743 (285)
Measurement of the
B8
solar neutrino flux in
SNO+
with very low backgrounds [PDF]
Physical Review D, 2018 A measurement of the 8B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with the SNO+ detector during its water commissioning phase.M. Anderson, S. Andringa, S. Asahi, M. Askins, D. Auty, N. Barros, D. Bartlett, F. Barão, R. Bayes, E. Beier, A. Bialek, S. Biller, E. Blucher, R. Bonventre, M. Boulay, E. Caden, E. Callaghan, J. Caravaca, D. Chauhan, M. Chen, O. Chkvorets, B. Cleveland, C. Connors, I. Coulter, M. M. Depatie, F. Di Lodovico, F. Duncan, J. Dunger, E. Falk, V. Fischer, E. Fletcher, R. Ford, N. Gagnon, K. Gilje, C. Grant, J. Grove, A. Hallin, D. Hallman, S. Hans, J. Hartnell, W. Heintzelman, R. Helmer, J. L. Hernández-Hernández, B. Hreljac, J. Hu, A. S. Inácio, C. Jillings, T. Kaptanoglu, P. Khaghani, J. Klein, R. Knapik, L. Kormos, B. Krar, C. Kraus, C. Krauss, T. Kroupová, I. Lam, B. Land, R. Lane, A. Latorre, I. Lawson, L. Lebanowski, E. Leming, A. Li, J. Lidgard, B. Liggins, Y. Liu, V. Lozza, M. Luo, S. Maguire, A. Maio, S. Manecki, J. Maneira, R. D. Martin, E. Marzec, A. Mastbaum, N. McCauley, A. McDonald, P. Mekarski, M. Meyer, M. Mlejnek, I. Morton-Blake, S. Nae, M. Nirkko, H. O'Keeffe, G. O. Orebi Gann, M. J. Parnell, J. Paton, S. Peeters, T. Pershing, L. Pickard, D. Pracsovics, G. Prior, A. Reichold, R. Richardson, M. Rigan, J. Rose, R. Rosero, J. Rumleskie, I. Semenec, K. Singh, P. Skensved, M. Stringer, R. Svoboda, B. Tam, L. Tian, J. Tseng, E. Turner, R. Van Berg, J. Veinot, C. J. Virtue, E. V'azquez-J'auregui, J. Wang, J. J. Weigand, J. R. Wilson, P. Woosaree, A. Wright, J. Yáñez, M. Yeh, K. Zuber, A. Zummo +120 moresemanticscholar +1 more sourceLimiting neutrino magnetic moments with Borexino Phase-II solar neutrino data [PDF]
, 2017 A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment.M. Agostini, K. Altenmüller, S. Appel, V. Atroshchenko, Z. Bagdasarian, D. Basilico, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, F. Calaprice, A. Caminata, S. Caprioli, M. Carlini, P. Cavalcante, A. Chepurnov, K. Choi, L. Collica, D. D’Angelo, S. Davini, A. Derbin, X. Ding, A. D. Ludovico, L. Noto, I. Drachnev, K. Fomenko, A. Formozov, D. Franco, F. Froborg, F. Gabriele, C. Galbiati, C. Ghiano, M. Giammarchi, A. Goretti, M. Gromov, D. Guffanti, C. Hagner, T. Houdy, E. Hungerford, A. Ianni, A. Ianni, A. Jany, D. Jeschke, V. Kobychev, D. Korablev, G. Korga, D. Kryn, M. Laubenstein, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhova, G. Lukyanchenko, L. Lukyanchenko, I. Machulin, G. Manuzio, S. Marcocci, J. Martyn, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, V. Muratova, B. Neumair, L. Oberauer, B. Opitz, V. Orekhov, F. Ortica, M. Pallavicini, L. Papp, Ö. Penek, N. Pilipenko, A. Pocar, A. Porcelli, G. Ranucci, A. Razeto, A. Re, M. Redchuk, A. Romani, R. Roncin, N. Rossi, S. Schönert, D. Semenov, M. Skorokhvatov, O. Smirnov, A. Sotnikov, L. Stokes, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, M. Toropova, E. Unzhakov, A. Vishneva, R. Vogelaar, F. Feilitzsch, H. Wang, S. Weinz, M. Wójcik, M. Wurm, Z. Yokley, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel +106 moresemanticscholar +1 more sourceSolar neutrino detection [PDF]
AIP Conference Proceedings, 2009 8 pages, 5 figures. III School on Cosmic Rays and Astrophysics August 25 to September 5, 2008 Arequipa (Peru) AIP conference ...Lino Miramonti, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, Oscar Saavedra +4 moreopenaire +5 more sourcesSolar Neutrino Measurements in Super-Kamiokande-IV [PDF]
, 2016 Upgraded electronics, improved water system dynamics, better calibration and analysis techniques allowed Super-Kamiokande-IV to clearly observe very low-energy 8B solar neutrino interactions, with recoil electron kinetic energies as low as 3.49 MeV ...S. Abe, Y. Haga, Y. Hayato, M. Ikeda, K. Iyogi, J. Kameda, Y. Kishimoto, L. Marti, M. Miura, S. Moriyama, M. Nakahata, T. Nakajima, S. Nakayama, A. Orii, H. Sekiya, M. Shiozawa, Y. Sonoda, A. Takeda, H. Tanaka, Y. Takenaga, S. Tasaka, T. Tomura, K. Ueno, T. Yokozawa, R. Akutsu, T. Irvine, H. Kaji, T. Kajita, I. Kametani, K. Kaneyuki, K. P. Lee, Y. Nishimura, T. McLachlan, K. Okumura, E. Richard, L. Labarga, P. Fernández, F. Blaszczyk, J. Gustafson, C. Kachulis, E. Kearns, 32 J. L. Raaf, J. Stone, 32 L. R. Sulak, S. Berkman, S. Tobayama, M. Goldhaber, K. Bays, G. Carminati, N. J. Griskevich, W. Kropp, S. Mine, A. Renshaw, M. Smy, H. Sobel, V. Takhistov, P. Weatherly, K. Ganezer, B. Hartfiel, J. Hill, W. Keig, N. Hong, J. Kim, I. Lim, R. Park, T. Akiri, J. Albert, A. Himmel, Z. Li, E. O’Sullivan, K. Scholberg, C. Walter, T. Wongjirad, T. Ishizuka, T. Nakamura, J. Jang, K. Choi, J. Learned, S. Matsuno, S. Smith, M. Friend, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nishikawa, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, Y. Nakano, A. Suzuki, Y. Takeuchi, T. Yano, S. Cao, T. Hayashino, T. Hiraki, S. Hirota, K. Huang, K. Ieki, M. Jiang, T. Kikawa, A. Minamino, A. Murakami, T. Nakaya, N. Patel, K. Suzuki, S. Takahashi, R. Wendell, Y. Fukuda, Y. Itow, G. Mitsuka, F. Muto, T. Suzuki, P. Mijakowski, K. Frankiewicz, J. Hignight, J. Imber, C. Jung, X. Li, J. Palomino, G. Santucci, I. Taylor, C. Vilela, M. Wilking, C. Yanagisawa, D. Fukuda, H. Ishino, T. Kayano, A. Kibayashi, Y. Koshio, T. Mori, M. Sakuda, J. Takeuchi, R. Yamaguchi, Y. Kuno, R. Tacik, S. Kim, H. Okazawa, Y. Choi, K. Itô, K. Nishijima, M. Koshiba, Y. Totsuka, Y. Suda, M. Yokoyama, C. Bronner, R. Calland, M. Hartz, K. Martens, Y. Obayashi, Y. Suzuki, M. Vagins, C. Nantais, J. Martin, P. Perio, H. Tanaka, A. Konaka, S. Chen, H. Sui, L. Wan, Z. Yang, H. Zhang, Y. Zhang, K. Connolly, M. Dziomba, R. Observatory, Inst. for Nucl. Research, U. Tokyo, Research Center for Cosmic Neutrinos, Department of Applied Physics, U. A. Madrid, Department of Applied Physics, Boston University, Astronomy, U. Columbia, P. Department, Brookhaven National Laboratory, U. California, Irvine, California Polytechnic State University, Chonnam National University, D. University, Junior College, Fukuoka Institute of Technology, G. University, Gist College, Gwangju Institute of Science, Technology, U. Hawaii, High Energy Accelerator Research Organization, K. University, Kyoto University, Miyagi University of Education, Inst. for Nucl. Research, Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles, the Universe, N. C. F. N. Research, State University of New York at Stony Brook, O. University, Okayama, Okayama 700-8530, J. D. O. Physics, O. University, U. O. Regina, Seoul National University, Department of Informatics in Social Welfare, Shizuoka University of Welfare, S. University, T. University, T. U. O. Tokyo, K. I. F. T. Physics, M. Universe, The University of Tokyo Institutes for Advanced Study, U. Toronto, Triumf, 4004 Wesbrook Mall, Department of Applied Physics, Tsinghua University, U. Washington +222 moresemanticscholar +1 more sourceSolar neutrino flux at keV energies [PDF]
, 2017 We calculate the solar neutrino and antineutrino flux in the keV energy range. The dominant thermal source processes are photo production (γ e→ e νν̄), bremsstrahlung (e+Ze→ Ze+e+νν̄), plasmon decay (γ→νν̄), and νν̄ emission in free-bound and bound-bound E. Vitagliano, J. Redondo, G. Raffeltsemanticscholar +1 more source
