%0 Journal Article
%T Final results of Borexino Phase-I on low energy solar neutrino spectroscopy
%A Borexino Collaboration
%A G. Bellini
%A J. Benziger
%A D. Bick
%A G. Bonfini
%A D. Bravo
%A M. B. Avanzini
%A B. Caccianiga
%A L. Cadonati
%A F. Calaprice
%A P. Cavalcante
%A A. Chavarria
%A A. Chepurnov
%A D. D'Angelo
%A S. Davini
%A A. Derbin
%A A. Empl
%A A. Etenko
%A K. Fomenko
%A D. Franco
%A C. Galbiati
%A S. Gazzana
%A C. Ghiano
%A M. Giammarchi
%A M. Goeger-Neff
%A A. Goretti
%A L. Grandi
%A C. Hagner
%A E. Hungerford
%A Aldo Ianni
%A Andrea Ianni
%A V. Kobychev
%A D. Korablev
%A G. Korga
%A D. Kryn
%A M. Laubenstein
%A T. Lewke
%A E. Litvinovich
%A B. Loer
%A F. Lombardi
%A P. Lombardi
%A L. Ludhova
%A G. Lukyanchenko
%A I. Machulin
%A S. Manecki
%A W. Maneschg
%A G. Manuzio
%A Q. Meindl
%A E. Meroni
%A L. Miramonti
%A M. Misiaszek
%A P. Mosteiro
%A V. Muratova
%A L. Oberauer
%A M. Obolensky
%A F. Ortica
%A K. Otis
%A M. Pallavicini
%A L. Papp
%A C. Pena-Garay
%A L. Perasso
%A S. Perasso
%A A. Pocar
%A G. Ranucci
%A A. Razeto
%A A. Re
%A A. Romani
%A N. Rossi
%A R. Saldanha
%A C. Salvo
%A S. Schoenert
%A H. Simgen
%A M. Skorokhvatov
%A O. Smirnov
%A A. Sotnikov
%A S. Sukhotin
%A Y. Suvorov
%A R. Tartaglia
%A G. Testera
%A D. Vignaud
%A R. B. Vogelaar
%A F. von Feilitzsch
%A J. Winter
%A M. Wojcik
%A A. Wright
%A M. Wurm
%A J. Xu
%A O. Zaimidoroga
%A S. Zavatarelli
%A G. Zuzel
%J Physics
%D 2013
%I arXiv
%R 10.1103/PhysRevD.89.112007
%X Borexino has been running since May 2007 at the LNGS with the primary goal of detecting solar neutrinos. The detector, a large, unsegmented liquid scintillator calorimeter characterized by unprecedented low levels of intrinsic radioactivity, is optimized for the study of the lower energy part of the spectrum. During the Phase-I (2007-2010) Borexino first detected and then precisely measured the flux of the 7Be solar neutrinos, ruled out any significant day-night asymmetry of their interaction rate, made the first direct observation of the pep neutrinos, and set the tightest upper limit on the flux of CNO neutrinos. In this paper we discuss the signal signature and provide a comprehensive description of the backgrounds, quantify their event rates, describe the methods for their identification, selection or subtraction, and describe data analysis. Key features are an extensive in situ calibration program using radioactive sources, the detailed modeling of the detector response, the ability to define an innermost fiducial volume with extremely low background via software cuts, and the excellent pulse-shape discrimination capability of the scintillator that allows particle identification. We report a measurement of the annual modulation of the 7 Be neutrino interaction rate. The period, the amplitude, and the phase of the observed modulation are consistent with the solar origin of these events, and the absence of their annual modulation is rejected with higher than 99% C.L. The physics implications of phase-I results in the context of the neutrino oscillation physics and solar models are presented.
%U http://arxiv.org/abs/1308.0443v2