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\@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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\@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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\@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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\@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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\@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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\@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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\bibcite{Maltoni:2004ei}{12}
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\bibcite{CHOOZ}{14}
\bibcite{Wpaper}{15}
\bibcite{T2K}{16}
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\bibcite{Huber:2003pm}{18}
\bibcite{Albrow:2005kw}{19}
\bibcite{SPL}{20}
\bibcite{BNLHS}{21}
\bibcite{zucchelli}{22}
\bibcite{Albright:2004iw}{23}
\bibcite{Blondel:2004ae}{24}
\bibcite{Campagne:2004wt}{25}
\bibcite{Mezzetto:2003ub}{26}
\bibcite{memphys}{27}
\bibcite{UNO}{28}
\bibcite{Nakamura:2003hk}{29}
\bibcite{Huber:2005ep}{30}
\bibcite{Globes}{31}
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\bibcite{Nuance}{33}
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\bibcite{JJHigh2}{37}
\bibcite{LindnerBB}{38}
\bibcite{JJHigh1}{39}
\bibcite{Terranova}{40}
\bibcite{BB-Reviews}{41}
\bibcite{Volpe}{42}
\bibcite{Lindroos}{43}
\bibcite{Eurisol}{44}
\bibcite{Lindroos-Optimization}{45}
\bibcite{MezzettoNuFact05}{46}
\bibcite{Neugen}{47}
\bibcite{FLUKA}{48}
\bibcite{GEANT}{49}
\bibcite{HARP-MINERVA}{50}
\bibcite{Mezzetto:2003mm}{51}
\bibcite{Honda:2004yz}{52}
\bibcite{Lipari:1991ut}{53}
\bibcite{Gonzalez-Garcia:2004wg}{54}
\bibcite{Burguet-Castell:2001ez}{55}
\bibcite{Minakata:2001qm}{56}
\bibcite{Fogli:1996pv}{57}
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\bibcite{Antusch:2004yx}{61}
\bibcite{Minakata:2004pg}{62}
\bibcite{Donini:2005db}{63}
\bibcite{Peres:2003wd}{64}
\bibcite{Gonzalez-Garcia:2004cu}{65}
\bibcite{Petcov:1998su}{66}
\bibcite{Akhmedov:1998ui}{67}
\bibcite{Bernabeu:2003yp}{68}
\bibcite{Kim:1998bv}{69}
\bibcite{Kajita}{70}
\bibcite{Petcov:2005rv}{71}
\bibcite{MenaRequejo:2005hn}{72}
\bibcite{Hagiwara:2005pe}{73}
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