[385] | 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} |
---|
| 234 | \bibcite{Aliu:2004sq}{5} |
---|
| 235 | \bibcite{MINOS}{6} |
---|
| 236 | \bibcite{OPERA}{7} |
---|
| 237 | \bibcite{CNGS}{8} |
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| 238 | \bibcite{LSND}{9} |
---|
| 239 | \bibcite{MINIBOONE}{10} |
---|
| 240 | \bibcite{FOGLILISI05}{11} |
---|
| 241 | \bibcite{Maltoni:2004ei}{12} |
---|
| 242 | \bibcite{PMNS}{13} |
---|
| 243 | \bibcite{CHOOZ}{14} |
---|
| 244 | \bibcite{Wpaper}{15} |
---|
| 245 | \bibcite{T2K}{16} |
---|
| 246 | \bibcite{Ayres:2004js}{17} |
---|
| 247 | \bibcite{Huber:2003pm}{18} |
---|
| 248 | \bibcite{Albrow:2005kw}{19} |
---|
| 249 | \bibcite{SPL}{20} |
---|
| 250 | \bibcite{BNLHS}{21} |
---|
| 251 | \bibcite{zucchelli}{22} |
---|
| 252 | \bibcite{Albright:2004iw}{23} |
---|
| 253 | \bibcite{Blondel:2004ae}{24} |
---|
| 254 | \bibcite{Campagne:2004wt}{25} |
---|
| 255 | \bibcite{Mezzetto:2003ub}{26} |
---|
| 256 | \bibcite{memphys}{27} |
---|
| 257 | \bibcite{UNO}{28} |
---|
| 258 | \bibcite{Nakamura:2003hk}{29} |
---|
| 259 | \bibcite{Huber:2005ep}{30} |
---|
| 260 | \bibcite{Globes}{31} |
---|
| 261 | \bibcite{Huber:2002mx}{32} |
---|
| 262 | \bibcite{Nuance}{33} |
---|
| 263 | \bibcite{ISSpage}{34} |
---|
| 264 | \bibcite{MyNufact04}{35} |
---|
| 265 | \bibcite{Donini:2004hu}{36} |
---|
| 266 | \bibcite{JJHigh2}{37} |
---|
| 267 | \bibcite{LindnerBB}{38} |
---|
| 268 | \bibcite{JJHigh1}{39} |
---|
| 269 | \bibcite{Terranova}{40} |
---|
| 270 | \bibcite{BB-Reviews}{41} |
---|
| 271 | \bibcite{Volpe}{42} |
---|
| 272 | \bibcite{Lindroos}{43} |
---|
| 273 | \bibcite{Eurisol}{44} |
---|
| 274 | \bibcite{Lindroos-Optimization}{45} |
---|
| 275 | \bibcite{MezzettoNuFact05}{46} |
---|
| 276 | \bibcite{Neugen}{47} |
---|
| 277 | \bibcite{FLUKA}{48} |
---|
| 278 | \bibcite{GEANT}{49} |
---|
| 279 | \bibcite{HARP-MINERVA}{50} |
---|
| 280 | \bibcite{Mezzetto:2003mm}{51} |
---|
| 281 | \bibcite{Honda:2004yz}{52} |
---|
| 282 | \bibcite{Lipari:1991ut}{53} |
---|
| 283 | \bibcite{Gonzalez-Garcia:2004wg}{54} |
---|
| 284 | \bibcite{Burguet-Castell:2001ez}{55} |
---|
| 285 | \bibcite{Minakata:2001qm}{56} |
---|
| 286 | \bibcite{Fogli:1996pv}{57} |
---|
| 287 | \bibcite{Barger:2001yr}{58} |
---|
| 288 | \bibcite{Yasuda:2004gu}{59} |
---|
| 289 | \bibcite{Ishitsuka:2005qi}{60} |
---|
| 290 | \bibcite{Antusch:2004yx}{61} |
---|
| 291 | \bibcite{Minakata:2004pg}{62} |
---|
| 292 | \bibcite{Donini:2005db}{63} |
---|
| 293 | \bibcite{Peres:2003wd}{64} |
---|
| 294 | \bibcite{Gonzalez-Garcia:2004cu}{65} |
---|
| 295 | \bibcite{Petcov:1998su}{66} |
---|
| 296 | \bibcite{Akhmedov:1998ui}{67} |
---|
| 297 | \bibcite{Bernabeu:2003yp}{68} |
---|
| 298 | \bibcite{Kim:1998bv}{69} |
---|
| 299 | \bibcite{Kajita}{70} |
---|
| 300 | \bibcite{Petcov:2005rv}{71} |
---|
| 301 | \bibcite{MenaRequejo:2005hn}{72} |
---|
| 302 | \bibcite{Hagiwara:2005pe}{73} |
---|
| 303 | \bibcite{Kachelriess:2004vs}{74} |
---|