1 | \relax |
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2 | \citation{solar} |
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3 | \citation{Fukuda:1998mi} |
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4 | \citation{Ashie:2005ik} |
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5 | \citation{Araki:2004mb} |
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6 | \citation{Aliu:2004sq} |
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7 | \citation{Aliu:2004sq} |
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8 | \citation{MINOS} |
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9 | \citation{OPERA} |
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10 | \citation{CNGS} |
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11 | \citation{LSND} |
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12 | \citation{MINIBOONE} |
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13 | \citation{FOGLILISI05} |
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14 | \citation{Maltoni:2004ei} |
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15 | \citation{PMNS} |
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16 | \citation{CHOOZ} |
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17 | \citation{Maltoni:2004ei} |
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18 | \citation{Wpaper} |
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19 | \citation{T2K} |
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20 | \citation{Ayres:2004js} |
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21 | \citation{Huber:2003pm} |
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22 | \citation{T2K} |
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23 | \citation{Albrow:2005kw} |
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24 | \citation{SPL} |
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25 | \citation{BNLHS} |
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26 | \citation{zucchelli} |
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27 | \citation{Albright:2004iw} |
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28 | \citation{Albright:2004iw} |
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29 | \citation{Blondel:2004ae} |
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30 | \citation{Campagne:2004wt} |
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31 | \citation{Mezzetto:2003ub} |
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32 | \citation{memphys} |
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33 | \citation{UNO} |
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34 | \citation{T2K} |
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35 | \citation{Nakamura:2003hk} |
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36 | \citation{Huber:2005ep} |
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37 | \citation{T2K} |
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38 | \@writefile{toc}{\contentsline {section}{\numberline {1}Introduction}{2}} |
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39 | \citation{Globes} |
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40 | \citation{Huber:2002mx} |
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41 | \citation{T2K} |
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42 | \citation{Huber:2002mx} |
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43 | \citation{Nuance} |
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44 | \citation{T2K} |
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45 | \citation{Huber:2002mx} |
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46 | \@writefile{lot}{\contentsline {table}{\numberline {1}{\ignorespaces Summary of default parameters used for the simulation of the $\beta $B, SPL, and T2HK experiments.}}{3}} |
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47 | \newlabel{tab:setups}{{1}{3}} |
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48 | \@writefile{toc}{\contentsline {section}{\numberline {2}Experiments overview and analysis methods}{3}} |
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49 | \newlabel{sec:analysis}{{2}{3}} |
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50 | \citation{Globes} |
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51 | \citation{ISSpage} |
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52 | \@writefile{lot}{\contentsline {table}{\numberline {2}{\ignorespaces Number of events for appearance and disappearance signals and backgrounds for the $\beta $B, SPL, and T2HK experiments as defined in Tab.\nobreakspace {}\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `tab:setups' on page 4 undefined}. For the appearance signals the event numbers are given for several values of $\ensuremath {\qopname \relax o{sin}^22\theta _{13}}$ and $\ensuremath {\delta _{\rm CP}}= 0$ and $\pi /2$. The background as well as the disappearance event numbers correspond to $\theta _{13}=0$. For the other oscillation parameters the values of Eq.\nobreakspace {}(\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `eq:default-params' on page 4 undefined}) are used.}}{4}} |
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53 | \newlabel{tab:events}{{2}{4}} |
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54 | \citation{FOGLILISI05} |
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55 | \citation{Maltoni:2004ei} |
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56 | \citation{memphys} |
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57 | \citation{UNO} |
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58 | \citation{Nakamura:2003hk} |
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59 | \citation{zucchelli} |
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60 | \citation{Mezzetto:2003ub} |
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61 | \citation{MyNufact04} |
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62 | \citation{Donini:2004hu} |
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63 | \citation{JJHigh2} |
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64 | \citation{JJHigh2} |
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65 | \citation{LindnerBB} |
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66 | \citation{JJHigh2} |
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67 | \citation{JJHigh1} |
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68 | \citation{LindnerBB} |
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69 | \citation{LindnerBB} |
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70 | \citation{JJHigh1} |
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71 | \citation{Terranova} |
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72 | \citation{BB-Reviews} |
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73 | \citation{Volpe} |
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74 | \citation{Lindroos} |
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75 | \citation{Eurisol} |
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76 | \citation{Lindroos} |
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77 | \citation{Lindroos-Optimization} |
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78 | \newlabel{eq:default-params}{{1}{5}} |
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79 | \@writefile{toc}{\contentsline {section}{\numberline {3}The CERN--MEMPHYS experiments}{5}} |
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80 | \newlabel{sec:experiments}{{3}{5}} |
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81 | \@writefile{toc}{\contentsline {subsection}{\numberline {3.1}The MEMPHYS detector}{5}} |
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82 | \@writefile{toc}{\contentsline {subsection}{\numberline {3.2}The $\gamma = 100\times 100$ baseline Beta Beam}{5}} |
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83 | \citation{LindnerBB} |
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84 | \citation{JJHigh2} |
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85 | \citation{Nuance} |
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86 | \citation{JJHigh2} |
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87 | \citation{MyNufact04} |
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88 | \citation{MezzettoNuFact05} |
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89 | \citation{Neugen} |
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90 | \@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Sketch of the MEMPHYS detector under the Fr\'ejus mountain.}}{6}} |
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91 | \newlabel{fig:MEMPHYS}{{1}{6}} |
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92 | \citation{zucchelli} |
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93 | \citation{JJHigh2} |
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94 | \citation{JJHigh1} |
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95 | \citation{MezzettoNuFact05} |
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96 | \citation{MezzettoNuFact05} |
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97 | \citation{MezzettoNuFact05} |
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98 | \@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Energy resolution for \ensuremath {\nu _{e}}\ interactions in the 200--300\nobreakspace {}MeV energy range. The quantity displayed is the difference between the reconstructed and the true neutrino energy.}}{7}} |
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99 | \newlabel{fig:QE-Energy}{{2}{7}} |
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100 | \@writefile{lot}{\contentsline {table}{\numberline {3}{\ignorespaces Events for the $\beta $B\ in a 4400\nobreakspace {}kt\nobreakspace {}yr exposure. \ensuremath {\nu _{\mu }\ }(\ensuremath {\overline {\nu }_{\mu }}) CC events are computed assuming full oscillations ($P_{\nu _e\to \nu _\mu } = 1$), and pion backgrounds are computed from \ensuremath {\nu _{e}}(\ensuremath {\overline {\nu }_{e}}) CC+NC events. In the rows we give the number events generated within the fiducial volume (``Generated ev.''), after muon particle identification (``Particle ID''), and after applying a further identification requiring the detection of the Michel electron (``Decay''). }}{7}} |
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101 | \newlabel{tab:sigbck}{{3}{7}} |
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102 | \citation{SPL} |
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103 | \citation{Campagne:2004wt} |
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104 | \citation{FLUKA} |
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105 | \citation{GEANT} |
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106 | \citation{HARP-MINERVA} |
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107 | \citation{Campagne:2004wt} |
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108 | \citation{Mezzetto:2003mm} |
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109 | \citation{Mezzetto:2003mm} |
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110 | \citation{Donini:2004hu} |
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111 | \citation{T2K} |
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112 | \citation{Nuance} |
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113 | \@writefile{toc}{\contentsline {subsection}{\numberline {3.3}The $3.5$-GeV SPL Super Beam}{8}} |
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114 | \@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces Neutrino fluxes, at $130$\nobreakspace {}km from the target with the horns focusing the positive particles (top panel) or the negative particles (bottom panel). The fluxes are computed for a SPL proton beam of $3.5$\nobreakspace {}GeV (4\nobreakspace {}MW), a decay tunnel with a length of $40$\nobreakspace {}m and a radius of $2$\nobreakspace {}m.}}{9}} |
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115 | \newlabel{fig:fluxSPLContrib}{{3}{9}} |
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116 | \@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces Comparison of the fluxes from SPL and $\beta $B.}}{9}} |
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117 | \newlabel{fig:fluxComparison}{{4}{9}} |
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118 | \citation{Huber:2005ep} |
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119 | \citation{Honda:2004yz} |
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120 | \citation{Ashie:2005ik} |
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121 | \citation{Ashie:2005ik} |
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122 | \@writefile{toc}{\contentsline {subsection}{\numberline {3.4}The atmospheric neutrino analysis}{10}} |
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123 | \newlabel{sec:atm-details}{{3.4}{10}} |
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124 | \newlabel{eq:contained}{{2}{10}} |
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125 | \citation{Lipari:1991ut} |
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126 | \citation{Gonzalez-Garcia:2004wg} |
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127 | \citation{Gonzalez-Garcia:2004wg} |
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128 | \newlabel{eq:upgoing}{{3}{11}} |
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129 | \newlabel{eq:poisson}{{4}{11}} |
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130 | \newlabel{eq:theopulls}{{5}{11}} |
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131 | \citation{Burguet-Castell:2001ez} |
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132 | \citation{Minakata:2001qm} |
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133 | \citation{Fogli:1996pv} |
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134 | \citation{Barger:2001yr} |
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135 | \citation{Huber:2002mx} |
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136 | \citation{Huber:2005ep} |
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137 | \citation{Yasuda:2004gu} |
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138 | \citation{Ishitsuka:2005qi} |
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139 | \citation{Donini:2004hu} |
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140 | \citation{Donini:2004hu} |
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141 | \citation{Huber:2005ep} |
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142 | \@writefile{toc}{\contentsline {section}{\numberline {4}Degeneracies}{12}} |
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143 | \newlabel{sec:degeneracies}{{4}{12}} |
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144 | \@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Allowed regions in $\qopname \relax o{sin}^22\theta _{13}$ and $\delta _\mathrm {CP}$ for LBL data alone (contour lines) and LBL+ATM data combined (colored regions). $\mathrm {H^{tr/wr} (O^{tr/wr})}$ refers to solutions with the true/wrong mass hierarchy (octant of $\theta _{23}$). The true parameter values are $\delta _\mathrm {CP} = -0.85 \pi $, $\qopname \relax o{sin}^22\theta _{13} = 0.03$, $\qopname \relax o{sin}^2\theta _{23} = 0.6$, and the values from Eq.\nobreakspace {}(\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `eq:default-params' on page 13 undefined}) for the other parameters.}}{13}} |
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145 | \newlabel{fig:degeneracies}{{5}{13}} |
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146 | \@writefile{lof}{\contentsline {figure}{\numberline {6}{\ignorespaces Resolving degeneracies in SPL by successively using the appearance rate measurement, disappearance channel rate and spectrum, spectral information in the appearance channel, and atmospheric neutrinos. Allowed regions in $\qopname \relax o{sin}^22\theta _{13}$ and $\delta _\mathrm {CP}$ are shown at 95\%\nobreakspace {}CL, and $\mathrm {H^{tr/wr} (O^{tr/wr})}$ refers to solutions with the true/wrong mass hierarchy (octant of $\theta _{23}$). The true parameter values are $\delta _\mathrm {CP} = -0.85 \pi $, $\qopname \relax o{sin}^22\theta _{13} = 0.03$, $\qopname \relax o{sin}^2\theta _{23} = 0.6$, and the values from Eq.\nobreakspace {}(\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `eq:default-params' on page 13 undefined}) for the other parameters.}}{13}} |
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147 | \newlabel{fig:degeneracies_SPL}{{6}{13}} |
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148 | \citation{Minakata:2001qm} |
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149 | \citation{Donini:2004hu} |
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150 | \@writefile{lof}{\contentsline {figure}{\numberline {7}{\ignorespaces Allowed regions in $\qopname \relax o{sin}^22\theta _{13}$ and $\delta _\mathrm {CP}$ for 5\nobreakspace {}years data (neutrinos only) from $\beta $B, SPL, and the combination. $\mathrm {H^{tr/wr} (O^{tr/wr})}$ refers to solutions with the true/wrong mass hierarchy (octant of $\theta _{23}$). For the colored regions in the left panel also 5\nobreakspace {}years of atmospheric data are included; the solution with the wrong hierarchy has $\Delta \chi ^2 = 4$. The true parameter values are $\delta _\mathrm {CP} = -0.85 \pi $, $\qopname \relax o{sin}^22\theta _{13} = 0.03$, $\qopname \relax o{sin}^2\theta _{23} = 0.6$, and the values from Eq.\nobreakspace {}(\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `eq:default-params' on page 14 undefined}) for the other parameters. For the $\beta $B\ only analysis (middle panel) an external accuracy of 2\% (3\%) for $|\Delta m^2_{31}|$ ($\theta _{23}$) has been assumed, whereas for the left and right panel the default value of 10\% has been used.}}{14}} |
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151 | \newlabel{fig:degeneracies_5yrs}{{7}{14}} |
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152 | \citation{Antusch:2004yx} |
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153 | \citation{Minakata:2004pg} |
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154 | \citation{Donini:2005db} |
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155 | \citation{T2K} |
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156 | \citation{Maltoni:2004ei} |
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157 | \citation{Maltoni:2004ei} |
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158 | \citation{Donini:2005db} |
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159 | \@writefile{lot}{\contentsline {table}{\numberline {4}{\ignorespaces Accuracies at $3\sigma $ on the atmospheric parameters $|\Delta m^2_{31}|$ and $\qopname \relax o{sin}^2\theta _{23}$ for 5 years of neutrino data from T2K-I, SPL, and T2HK for the two test points shown in Fig.\nobreakspace {}\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `fig:atm-params' on page 15 undefined} ($\theta ^\mathrm {true}_{13} = 0$). The accuracy for a parameter $x$ is defined as $(x^\mathrm {upper} - x^\mathrm {lower})/(2 x^\mathrm {true})$, where $x^\mathrm {upper}$ ($x^\mathrm {lower}$) is the upper (lower) bound at 3$\sigma $ for 1\nobreakspace {}d.o.f.\ obtained by projecting the contour $\Delta \chi ^2 = 9$ onto the $x$-axis. For the accuracies for test point\nobreakspace {}2 the octant degenerate solution is neglected.}}{15}} |
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160 | \newlabel{tab:atm-params}{{4}{15}} |
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161 | \@writefile{toc}{\contentsline {section}{\numberline {5}Physics potential}{15}} |
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162 | \newlabel{sec:sensitivities}{{5}{15}} |
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163 | \@writefile{toc}{\contentsline {subsection}{\numberline {5.1}Sensitivity to the atmospheric parameters}{15}} |
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164 | \newlabel{sec:atm}{{5.1}{15}} |
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165 | \citation{Minakata:2004pg} |
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166 | \citation{Peres:2003wd} |
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167 | \citation{Gonzalez-Garcia:2004cu} |
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168 | \@writefile{lof}{\contentsline {figure}{\numberline {8}{\ignorespaces Allowed regions of $\Delta m^2_{31}$ and $\qopname \relax o{sin}^2\theta _{23}$ at 99\%\nobreakspace {}CL (2 d.o.f.) after 5\nobreakspace {}yrs of neutrino data taking for SPL, T2K phase\nobreakspace {}I, T2HK, and the combination of SPL with 5\nobreakspace {}yrs of atmospheric neutrino data in the MEMPHYS detector. For the true parameter values we use $\Delta m^2_{31} = 2.2\tmspace +\thinmuskip {.1667em} (2.6) \times 10^{-3}\nobreakspace {}\mathrm {eV}^2$ and $\qopname \relax o{sin}^2\theta _{23} = 0.5 \tmspace +\thinmuskip {.1667em} (0.37)$ for the test point 1 (2), and $\theta _{13} = 0$ and the solar parameters as given in Eq.\nobreakspace {}(\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `eq:default-params' on page 16 undefined}). The shaded region corresponds to the 99\%\nobreakspace {}CL region from present SK and K2K data\nobreakspace {}\cite {Maltoni:2004ei}.}}{16}} |
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169 | \newlabel{fig:atm-params}{{8}{16}} |
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170 | \@writefile{toc}{\contentsline {subsection}{\numberline {5.2}The $\theta _{13}$ discovery potential}{16}} |
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171 | \newlabel{sec:th13}{{5.2}{16}} |
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172 | \@writefile{lof}{\contentsline {figure}{\numberline {9}{\ignorespaces $3\sigma $ discovery sensitivity to $\ensuremath {\qopname \relax o{sin}^22\theta _{13}}$ for $\beta $B, SPL, and T2HK as a function of the true value of \ensuremath {\delta _{\rm CP}}\ (left panel) and as a function of the fraction of all possible values of \ensuremath {\delta _{\rm CP}}\ (right panel). The width of the bands corresponds to values for the systematical errors between 2\% and 5\%. The black curves correspond to the combination of $\beta $B\ and SPL with 10\nobreakspace {}yrs of total data taking each for a systematical error of 2\%, and the dashed curves show the sensitivity of the $\beta $B\ when the number of ion decays/yr are reduced by a factor of two with respect to the values given in Tab.\nobreakspace {}\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `tab:setups' on page 17 undefined}.}}{17}} |
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173 | \newlabel{fig:th13}{{9}{17}} |
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174 | \@writefile{lof}{\contentsline {figure}{\numberline {10}{\ignorespaces $3\sigma $ discovery sensitivity to $\ensuremath {\qopname \relax o{sin}^22\theta _{13}}$ for the SPL as a function of the true value of \ensuremath {\delta _{\rm CP}}\ for $\qopname \relax o{sin}^2\theta _{23}^\mathrm {true} = 0.6$ and true values for the other parameters as given in Eq.\nobreakspace {}(\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `eq:default-params' on page 18 undefined}).}}{18}} |
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175 | \newlabel{fig:SPLTheta13Disco}{{10}{18}} |
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176 | \@writefile{toc}{\contentsline {subsection}{\numberline {5.3}Sensitivity to CP violation}{18}} |
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177 | \newlabel{sec:CPV}{{5.3}{18}} |
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178 | \@writefile{lof}{\contentsline {figure}{\numberline {11}{\ignorespaces CPV discovery potential for $\beta $B, SPL, and T2HK: For parameter values inside the ellipse-shaped curves CP conserving values of \ensuremath {\delta _{\rm CP}}\ can be excluded at $3\sigma $ $(\Delta \chi ^2>9)$. The width of the bands corresponds to values for the systematical errors from 2\% to 5\%. The dashed curves show the sensitivity of the $\beta $B\ when the number of ion decays/yr are reduced by a factor of two with respect to the values given in Tab.\nobreakspace {}\G@refundefinedtrue \text {\normalfont \bfseries ??}\GenericWarning { }{LaTeX Warning: Reference `tab:setups' on page 19 undefined} for 2\% systematics.}}{19}} |
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179 | \newlabel{fig:CPV}{{11}{19}} |
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180 | \@writefile{lof}{\contentsline {figure}{\numberline {12}{\ignorespaces Impact of total exposure and systematical errors on the CPV discovery potential of $\beta $B, SPL, and T2HK. We show the smallest true value of $\ensuremath {\qopname \relax o{sin}^22\theta _{13}}$ for which $\ensuremath {\delta _{\rm CP}}= \pi /2$ can be distinguished from $\ensuremath {\delta _{\rm CP}}= 0$ or $\ensuremath {\delta _{\rm CP}}= \pi $ at $3\sigma $ $(\Delta \chi ^2>9)$ as a function of the exposure in kt\nobreakspace {}yrs (left) and as a function of the systematical error on the background $\sigma _\mathrm {bkgr}$ (right). The widths of the curves in the left panel corresponds to values of $\sigma _\mathrm {bkgr}$ from 2\% to 5\%. The thin solid curves in the left panel corresponds to no systematical errors. The right plot is calculated for the standard exposure of 4400\nobreakspace {}kt\nobreakspace {}yrs. No systematical error on the signal has been assumed. }}{20}} |
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181 | \newlabel{fig:systematics}{{12}{20}} |
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182 | \citation{Ishitsuka:2005qi} |
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183 | \@writefile{lof}{\contentsline {figure}{\numberline {13}{\ignorespaces Impact of degeneracies on the CPV discovery potential for the $\beta $B. We show the sensitivity to CPV at $3\sigma $ $(\Delta \chi ^2>9)$ computed for 4 different combinations of the true values of the hierarchy (NH or IH) and $\theta _{23}$ ($\qopname \relax o{sin}^2\theta _{23} = 0.4$ or $0.6$). Dashed curves are computed neglecting degeneracies in the fit.}}{21}} |
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184 | \newlabel{fig:deltacp}{{13}{21}} |
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185 | \citation{Huber:2005ep} |
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186 | \citation{Huber:2005ep} |
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187 | \citation{Petcov:1998su} |
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188 | \citation{Akhmedov:1998ui} |
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189 | \citation{Bernabeu:2003yp} |
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190 | \citation{Kim:1998bv} |
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191 | \citation{Peres:2003wd} |
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192 | \citation{Gonzalez-Garcia:2004cu} |
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193 | \citation{Kajita} |
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194 | \citation{Huber:2005ep} |
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195 | \@writefile{toc}{\contentsline {section}{\numberline {6}Synergies provided by the CERN--MEMPHYS facilities}{22}} |
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196 | \newlabel{sec:synergies}{{6}{22}} |
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197 | \@writefile{toc}{\contentsline {subsection}{\numberline {6.1}Combining Beta Beam and Super Beam}{22}} |
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198 | \newlabel{sec:synergies-beams}{{6.1}{22}} |
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199 | \@writefile{toc}{\contentsline {subsection}{\numberline {6.2}Resolving degeneracies with atmospheric neutrinos}{22}} |
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200 | \newlabel{sec:atmospherics}{{6.2}{22}} |
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201 | \@writefile{lof}{\contentsline {figure}{\numberline {14}{\ignorespaces Discovery potential of a finite value of $\ensuremath {\qopname \relax o{sin}^22\theta _{13}}$ at $3\sigma $ $(\Delta \chi ^2>9)$ for 5\nobreakspace {}yrs neutrino data from $\beta $B, SPL, and the combination of $\beta $B\ + SPL compared to 10\nobreakspace {}yrs data from T2HK (2\nobreakspace {}yrs neutrinos + 8\nobreakspace {}yrs antineutrinos). }}{23}} |
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202 | \newlabel{fig:th13-5yrs}{{14}{23}} |
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203 | \@writefile{lof}{\contentsline {figure}{\numberline {15}{\ignorespaces Sensitivity to CPV at $3\sigma $ $(\Delta \chi ^2>9)$ for combining 5\nobreakspace {}yrs neutrino data from $\beta $B\ and SPL compared to 10\nobreakspace {}yrs data from T2HK (2\nobreakspace {}yrs neutrinos + 8\nobreakspace {}yrs antineutrinos). }}{23}} |
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204 | \newlabel{fig:CP-5yrs}{{15}{23}} |
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205 | \citation{Huber:2005ep} |
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206 | \citation{Ayres:2004js} |
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207 | \citation{Ayres:2004js} |
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208 | \citation{Ayres:2004js} |
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209 | \citation{Ayres:2004js} |
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210 | \citation{Huber:2005ep} |
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211 | \@writefile{lof}{\contentsline {figure}{\numberline {16}{\ignorespaces Sensitivity to the mass hierarchy at $2\sigma $ $(\Delta \chi ^2 = 4)$ as a function of the true values of $\qopname \relax o{sin}^22\theta _{13}$ and $\delta _\mathrm {CP}$ (left), and the fraction of true values of $\ensuremath {\delta _{\rm CP}}$ (right). The solid curves are the sensitivities from the combination of long-baseline and atmospheric neutrino data, the dashed curves correspond to long-baseline data only. For comparison we show in the right panel also the sensitivities of NO$\nu $A and NO$\nu $A+T2K extracted from Fig.\nobreakspace {}13.14 of Ref.\nobreakspace {}\cite {Ayres:2004js}. For the curve labeled ``NO$\nu $A (p.dr.)+T2K@4\nobreakspace {}MW'' a proton driver has been assumed for NO$\nu $A and the T2K beam has been up-graded to 4\nobreakspace {}MW, see Ref.\nobreakspace {}\cite {Ayres:2004js} for details.}}{24}} |
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212 | \newlabel{fig:hierarchy}{{16}{24}} |
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213 | \citation{Huber:2005ep} |
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214 | \citation{Petcov:2005rv} |
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215 | \citation{Ayres:2004js} |
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216 | \citation{Ayres:2004js} |
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217 | \citation{Ishitsuka:2005qi} |
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218 | \citation{MenaRequejo:2005hn} |
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219 | \citation{Hagiwara:2005pe} |
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220 | \citation{Kachelriess:2004vs} |
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221 | \citation{Huber:2005ep} |
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222 | \citation{Huber:2005ep} |
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223 | \citation{Gonzalez-Garcia:2004cu} |
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224 | \citation{Ishitsuka:2005qi} |
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225 | \@writefile{lof}{\contentsline {figure}{\numberline {17}{\ignorespaces $\Delta \chi ^2$ of the solution with the wrong octant of $\theta _{23}$ as a function of the true value of $\qopname \relax o{sin}^2\theta _{23}$. We have assumed a true value of $\theta _{13} = 0$.}}{26}} |
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226 | \newlabel{fig:octant}{{17}{26}} |
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227 | \@writefile{toc}{\contentsline {section}{\numberline {7}Summary}{26}} |
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228 | \newlabel{sec:conclusions}{{7}{26}} |
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229 | \citation{ISSpage} |
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230 | \bibcite{solar}{1} |
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231 | \bibcite{Fukuda:1998mi}{2} |
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232 | \bibcite{Ashie:2005ik}{3} |
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233 | \bibcite{Araki:2004mb}{4} |
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234 | \bibcite{Aliu:2004sq}{5} |
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235 | \bibcite{MINOS}{6} |
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236 | \bibcite{OPERA}{7} |
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237 | \bibcite{CNGS}{8} |
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238 | \bibcite{LSND}{9} |
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239 | \bibcite{MINIBOONE}{10} |
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240 | \bibcite{FOGLILISI05}{11} |
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241 | \bibcite{Maltoni:2004ei}{12} |
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242 | \bibcite{PMNS}{13} |
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243 | \bibcite{CHOOZ}{14} |
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244 | \bibcite{Wpaper}{15} |
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245 | \bibcite{T2K}{16} |
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246 | \bibcite{Ayres:2004js}{17} |
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247 | \bibcite{Huber:2003pm}{18} |
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248 | \bibcite{Albrow:2005kw}{19} |
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249 | \bibcite{SPL}{20} |
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250 | \bibcite{BNLHS}{21} |
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251 | \bibcite{zucchelli}{22} |
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252 | \bibcite{Albright:2004iw}{23} |
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253 | \bibcite{Blondel:2004ae}{24} |
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254 | \bibcite{Campagne:2004wt}{25} |
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255 | \bibcite{Mezzetto:2003ub}{26} |
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263 | \bibcite{ISSpage}{34} |
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264 | \bibcite{MyNufact04}{35} |
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265 | \bibcite{Donini:2004hu}{36} |
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266 | \bibcite{JJHigh2}{37} |
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267 | \bibcite{LindnerBB}{38} |
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268 | \bibcite{JJHigh1}{39} |
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269 | \bibcite{Terranova}{40} |
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270 | \bibcite{BB-Reviews}{41} |
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271 | \bibcite{Volpe}{42} |
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287 | \bibcite{Barger:2001yr}{58} |
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288 | \bibcite{Yasuda:2004gu}{59} |
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290 | \bibcite{Antusch:2004yx}{61} |
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291 | \bibcite{Minakata:2004pg}{62} |
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292 | \bibcite{Donini:2005db}{63} |
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293 | \bibcite{Peres:2003wd}{64} |
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294 | \bibcite{Gonzalez-Garcia:2004cu}{65} |
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295 | \bibcite{Petcov:1998su}{66} |
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