Last Borexino Result
نویسنده
چکیده
C. Arpesella, H. O. Back, M. Balata, G. Bellini, J. Benziger, S. Bonetti, A. Brigatti, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, G. Cecchet, A. Chavarria, M. Chen, F. Dalnoki-Veress, D. DÁngelo, A. de Bari, A. de Bellefon, H. de Kerret, A. Derbin, M. Deutsch, A. di Credico, G. di Pietro, R. Eisenstein, F. Elisei, A. Etenko, R. Fernholz, K. Fomenko, R. Ford, D. Franco, B. Freudiger, C. Galbiati, F. Gatti, S. Gazzana, M. Giammarchi, D. Giugni, M. Goeger-Neff, T. Goldbrunner, A. Goretti, C. Grieb, C. Hagner, W. Hampel, E. Harding, S. Hardy, F. X. Hartman, T. Hertrich, G. Heusser, Aldo Ianni, Andrea Ianni, M. Joyce, J. Kiko, T. Kirsten, V. Kobychev, G. Korga, G. Korschinek, D. Kryn, V. Lagomarsino, P. Lamarche, M. Laubenstein, C. Lendvai, M. Leung, T. Lewke, E. Litvinovich, B. Loer, P. Lombardi, L. Ludhova, I. Machulin, S. Malvezzi, S. Manecki, J. Maneira, W. Maneschg, I. Manno, D. Manuzio, G. Manuzio, A. Martemianov, F. Masetti, U. Mazzucato, K. McCarty, D. McKinsey, Q. Meindl, E. Meroni, L. Miramonti, D. Montanari, M. E. Monzani, V. Muratova, P. Musico, H. Neder, A. Nelson, L. Niedermeier, L. Oberauer, M. Obolensky, M. Orsini, F. Ortica, M. Pallavicini, L. Papp, S. Parmeggiano, L. Perasso, A. Pocar, R. S. Raghavan, G. Ranucci, W. Rau, A. Razeto, E. Resconi, P. Risso, A. Romani, D. Rountree, A. Sabelnikov, R. Saldanha, C. Salvo, D. Schimizzi, S. SchÃűnert, T. Shutt, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sonnenschein, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, S. Vitale, R. B. Vogelaar, F. von Feilitzsch, R. von Hentig, T. von Hentig, M. Wojcik, M. Wurm, O. Zaimidoroga, S. Zavatarelli and G. Zuzel
منابع مشابه
Status of Borexino experiment and Physics results with its Counting Test Facility (CTF)
Borexino is a solar neutrino experiment located under the Gran Sasso mountain in Italy. It is currently in the commissioning phase and will start taking data in 2007. Its main goal is to detect low-energy neutrinos coming from the sun in real-time, via the scattering reaction ν e − → ν e−. Borexino exploits 300 tons of liquid scintillator as active target for neutrinos and 2200 photomultiplier ...
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In this paper an overview of the Borexino experiment will be give. The physics motivations and the background requirements are discussed.Furthermore, the main results from the Counting Test Facility of Borexino will be reported. The intention of this paper is to give answers to the following questions: \how are neutrinos measured in Borexino?", \why 7 Be neutrinos?" and \what can Borexino tell ...
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The solar neutrino deficit observed in Homestake, SAGE, GALLEX and Kamiokande experiments [1] has been confirmed by the new result from Super-Kamiokande experiment [2]. The most successful explanation of the deficit is given by the resonant flavor conversion of neutrinos (MSW mechanism) [3] in the solar interior. Based on the result obtained in ref. [4], where we have studied the impact of rand...
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