talk - International Workshop on Double Beta Decay and Neutrino

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Borexino science Vacuum oscillations Matter enhancement Physics of neutrino oscillation Precision measurements of solar neutrino fluxes can help map out the transition region, sensitive to new physics. Solar physics A spectroscopic measurement of the different solar neutrino rates can verify the Standard Solar Model predictions, rule out accretion scenarios and help determine the core C+N abundance. Andrea Pocar - DBD11 - November 15, 2011 6
Gran Sasso Perugia Heidelberg Hamburg Budapest Milano Genova München Kraków Kurchatov Moscow the Borexino Collaboration JINR Dubna Princeton Virginia Tech UMass Amherst Paris St. Petersburg Andrea Pocar - DBD11 - November 15, 2011 7
Page 1 and 2: Latest results from Borexino DBD11
Page 3 and 4: Solar Fusion Reactions p-p Solar Fu
Page 5: neutrino oscillations solar, atmosp
Page 9 and 10: Borexino L’AQUILA Tunnel of 10.
Page 11 and 12: measurement of the 7 Be solar neutr
Page 13 and 14: detector calibrations 4 campaigns i
Page 15 and 16: data reduction and signal extractio
Page 17 and 18: spectral fits • Different fits: -
Page 19 and 20: Implication on solar physics • Me
Page 21 and 22: no day/night effect matter effects
Page 23 and 24: 8 B solar neutrinos at low threshol
Page 25 and 26: pep and CNO neutrinos The 125 muo
Page 27 and 28: μ Track three-fold coincidence And
Page 29 and 30: μ Track three-fold coincidence n C
Page 31 and 32: 3-fold coincidence results (not onl
Page 33 and 34: electron/positron pulse shape discr
Page 35 and 36: pep and CNO results Borexino pep
Page 37 and 38: Andrea Pocar Pocar - DBD11 - SiLAFA

talk - International Workshop on Double Beta Decay and Neutrino

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