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Neutrino Flavor ratio on Earth and at Astrophysical sources K.-C. Lai, G.-L. Lin, and T. C. Liu, National Chiao Tung university Taiwan INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 31st Course Neutrinos in Cosmology, in Astro-, Particle- and Nuclear Physics Erice-Sicily: 16 - 24 September 2009
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Neutrino flavor ratio at sources (0, 0, 1) Source (1, 0, 0) Muon damped source (0, 1, 0) ● (1/3,2/3,0) Pion source ●
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Basic measured parameter definition – R : The ratio of track to shower events. – S: The ratio of two flavor shower. Experimental results are limited by number of detected events, fluctuation R and S Assumed K. Blum, Y. Nir and E. Waxman, arXiv:0706.2070 [hep-ph].
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Basic idea I: What is the real source we observed. From measured data to original source: P True flavor ratio at source Measured flavor ratio at Earth R i,th and S i,th R i,exp and S i,exp 22 1 region 2 < 2.3 2 < 11.8 3 region. 00 ’0’0 ’0’0 + Choubey et al., PHYSICAL REVIEW D 77, 113006 (2008)
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# 1: Only 10% R For E < 0.3PeV, difficult to distinguish e from . Only R Even at R/R ~ 10%, could not resolve muon damp source from pion source. muon damp source Pion source R only is unable to determine the original source. Measuring S is necessary. M. C. Gonzalez-Garcia and M. Maltoni, Phys. Rep. 460, 1 (2008); M. Maltoni, T. Schwetz, M. A. Tortola, and J. W. F. Valle, New J. Phys. 6, 122 (2004); S. Choubey, Phys. At. Nucl. 69, 1930 (2006); S. Goswami, Int. J. Mod. Phys. A 21, 1901 (2006); A. Bandyopadhyay, S. Choubey, S. Goswami, S. T. Petcov, and D. P. Roy, Phys. Lett. B 608, 115 (2005); G. L. Fogli et al., Prog. Part. Nucl. Phys. 57, 742 (2006).
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# 2-1: sin 2 13 =0 for Can rule-out pion source from muon-damped source under R/R ~ 10%, S /S ~ (11~14)% Astrophysical hidden source (1/2, a, (2/3 –a)) can be rule-out too. 2015/5/126 sin 2 23 =0.45 sin 2 23 =0.55 muon damp source Pion source Astrophysical Hidden source O. Mena, et al., PRD, 2007
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# 2-2: sin 2 13 = 0 for Can't rule-out muon-damped source from pion source under R/R ~ 10%, S /S ~ (11~12)%, sin 2 23 =0.45sin 2 23 =0.55 muon damp source Pion source
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# 3-1: CP phase , Under R/R ~ 10%, S /S ~ 13% 2015/5/128 muon damp source sin 2 13 = 0 sin 2 13 = 0.016 0.01 (non zero) Gray: =0 Blue: = /2 Red: = Pion source No dependence on CP phase when (sin 2 13 ) best-fit = 0
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# 3-2: CP phase for muon damp source sin 2 13 = 0 sin 2 13 = 0.016 0.01 Gray: =0 Blue: = /2 Red: = Pion source Under R/R ~ 10%, S /S ~ 13%
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# 4-1: Critical uncertainty R /R = 13% S /S = 16% R /R = 5% S /S = 6% Need several hundreds of neutrino events to confirm the source.
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Basic idea II: From Oscillation mechanism to new physics flavor ratio measured on Earth oscillation Possible source flavor ratio oo ij, Decay ij, Other mechanism
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Normal hierarchy: sin 2 θ 13 < 0.14 and 0.37 < sin 2 θ 23 <0.65 Inverted hierarchy: sin 2 θ 13 < 0.27 and 0.37 < sin 2 θ 23 <0.69 Possible measured region with different strategy Pion source with normal hierarchy Muon source with normal hierarchy Pion source with inverted hierarchy Muon source with inverted hierarchy * * Inverted hierarchy is only possible # # Allow both hierarchy Super-Kamiokande Collaboration Phys. Rev. D 74, 032002 (2006)
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All possible measured ratio for neutrino oscillation mechanism Neutrino oscillation # # New physics Beyond osciallation normal hierarchy inverted hierarchy measured ratio All possible source
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One example: Decay with normal mixing angle # # #: Only decay in this region is available. Michele Maltoni et al JHEP07(2008)064
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Another example: Decay with inverted hierarchy mixing angle # # # #: Only decay in this region is available.
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Conclusion Part I Measuring the R ratio only is not sufficient to determine the source type. The Critical uncertainties required to distinguish between pion and muon damped source: for pion source: R /R = 5% S /S = 6% for muon source: R /R = 13% S /S = 16% Part II New method to probe new physics.
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Reference:
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The exact form of oscillation probability matrix K.-C. Lai, G.-L. Lin, and T. C. Liu, arXiv:0905.4003 [hep-ph] ω ≡ sin 2 2θ 12, Δ ≡ cos 2 θ 23, D ≡ sinθ 13, δ the CP phase.
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