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Nailing down the unknown neutrino mixing angle theta_13 is one of the most important goals in current lepton physics.
M. Apollonio et al
2003
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See the contributions at the International Workshop on sub-dominant oscillation effects in atmospheric neutrino experiments
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R. N. Mohapatra and A. Y. Smirnov, “Neutrino mass and new physics,” Ann. Rev. Nucl. Part. Sci. 56
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G. L. Fogli, E. Lisi, A. Marrone and A. Palazzo, “Global analysis of three-flavor neutrino masses and mixings,” Prog. Part. Nucl. Phys. 57
2006
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Super-Kamiokande Collaboration, J. Hosaka et al
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Super-Kamiokande Collaboration, J. Hosaka et al
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G. L. Fogli, E. Lisi, A. Marrone, A. Melchiorri, A. Palazzo, P. Serra, J. Silk, and A. Slosar, “Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results,” Phys. Rev. D 75
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F. Kaether, “Data Analysis of the solar neutrino experiment GALLEX” (PhD Thesis, Heidelberg, 2007)
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Neutrino 2008
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SNO Collaboration, B. Aharmim et al
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H. Robertson, in Neutrino 2008
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R.L. Hahn, in Neutrino 2008
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C. Galbiati, in Neutrino 2008
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Super-Kamiokande Collaboration, J. P. Cravens et al
2008
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G.L. Fogli, E. Lisi, A. Palazzo, and A. M. Rotunno, preprint in preparation. Preliminary geo- ν \nu results from this work have been kindly shown by J.G. Learned in his talk at Neutrino 2008
2008
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2008
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H. Gallagher, in Neutrino 2008
2008
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G.L. Fogli, E. Lisi, A. Marrone, A. Palazzo, and A.M. Rotunno, in Proceedings of NO-VE 2008
2008
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2008
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MINOS Collaboration, P. Adamson et al
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KamLAND Collaboration, S. Abe et al
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We reproduce well the official SNO-III results [ 18 ] for the mass-mixing parameter ranges and best-fit values (at θ 13 = 0 \theta_{13}=0 ). We have also checked that these ranges are not altered by including the SNO-III ES rate, which merely increases the overall χ 2 \chi^{2} by ∼ 3.5 \sim\!\!3.5 in our fit
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2008
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2008
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The SNO Collaboration members are planning a combined analysis of all their data with the lowest possible analysis threshold, see J. Klein, Colloquium on “Results and Prospects with the Sudbury Neutrino Observatory” (NIKHEF, Amsterdam, The Netherlands, 2008); available at: http://agenda.nikhef.nl/conferenceDisplay.py?confId=249
2008
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