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Solar neutrino results from Borexino and main future perspectives

  • Marco Pallavicini
  • , G. Bellini
  • , J. Benziger
  • , S. Bonetti
  • , M. Buizza Avanzini
  • , B. Caccianiga
  • , L. Cadonati
  • , F. Calaprice
  • , C. Carraro
  • , A. Chavarria
  • , F. Dalnoki-Veress
  • , D. D'Angelo
  • , H. De Kerret
  • , S. Davini
  • , A. Derbin
  • , A. Etenko
  • , K. Fomenko
  • , D. Franco
  • , C. Galbiati
  • , S. Gazzana
  • M. Giammarchi, M. Goeger-Neff, A. Goretti, C. Grieb, E. Guardincerri, S. Hardy, Aldo Ianni, Andrea Ianni, M. Joyce, V. Kobychev, G. Korga, D. Kryn, M. Laubenstein, M. Leung, T. Lewke, E. Litvinovich, B. Loer, P. Lombardi, L. Ludhova, I. MacHulin, S. Manecki, W. Maneschg, G. Manuzio, F. Masetti, K. McCarty, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, D. Montanari, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, R. S. Raghavan, G. Ranucci, A. Razeto, P. Risso, A. Romani, D. Rountree, A. Sabelnikov, R. Saldanha, C. Salvo, S. Schonert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R. B. Vogelaar, F. Von Feilitzsch, M. Wojcik, M. Wurm, O. Zaimidoroga, S. Zavatarelli, G. Zuzel
  • University of Genoa
  • University of Milano
  • Princeton University
  • Massachusetts Institute of Technology
  • Princeton University
  • Università di Milano-Bicocca
  • Astroparticule and Cosmol APC
  • Petersburg Nuclear Physics Institute (PNPI)
  • Kurchatov Institute
  • Joint Institute for Nuclear Research, Dubna
  • Laboratori Nazionali del Gran Sasso
  • Technical University of Munich
  • Virginia Polytechnic Institute and State University
  • Max-Planck-Institut für Kernphysik
  • INFN Sezione di Perugia
  • Jagiellonian University

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

Borexino is a solar neutrino experiment running at the Laboratori Nazionali del Gran Sasso, Italy. The radioactive background levels in the liquid scintillator target meet or even exceed design goals, opening unanticipated opportunities. The main results, so far, are the measurement of the 7Be solar neutrino flux (the first ever done) and the measurement of the 8B neutrino flux performed with electron energy threshold of 2.8 MeV. The short and medium term perspectives are summarized in the conclusions.

langue originaleAnglais
Pages (de - à)210-213
Nombre de pages4
journalNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume630
Numéro de publication1
Les DOIs
étatPublié - 21 févr. 2011
Modification externeOui

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