\documentclass[portrait]{seminar}
\def\numunue{$\nu_\mu \to \nu_e$}
\def\myslideheader{\bf MINOS, SUMO and \numunue with other Long Baselines}
\def\myslidefooter{Brett Viren}
\input{preamble.tex}

\begin{document}
\slideframe{none}
\pagestyle{fancy}
\centerslidesfalse

\begin{slide*}
  \slideheading{MINOS, SUMO and \numunue with other Long Baselines}

  
  \begin{center}
    \sizedfig{0.5\textwidth}{logo.eps}
  \end{center}

  \begin{itemize}
  \item MINOS overview
  \item MINOS \numunue{} capabilities
  \item SUMO idea
  \item Survey of baselines
  \end{itemize}
\end{slide*}


\begin{slide*}
  \slideheading{Base Line}
    \begin{center}
    \sizedfig{0.9\textwidth}{map.eps}
    \sizedfig{1.0\textwidth}{earth-xsec.eps}
  \end{center}
\end{slide*}

\begin{slide*}
  \slideheading{Aerial View}

  \sizedfig{\textwidth}{aerial-photo.eps}
\end{slide*}

\begin{slide}
  \slideheading{Neutrino Production}
  \sizedfig{\textwidth}{beam-line.eps}
\end{slide}

\begin{slide*}
  \slideheading{Near Detector}
  \begin{center}
    \sizedfig{\textwidth}{neardet-layers.eps}
  \end{center}
  \begin{itemize}
  \item 1kt (0.1kt fiducial).
  \item 282 steel planes
  \item 153 scintilator planes
  \item 68 or 96 scintilator strips/plane.
  \item 1 ended readout, no multiplexing
  \end{itemize}
\end{slide*}

\begin{slide*}
  \slideheading{Far Detector}
  \begin{center}
    \sizedfig{0.8\textwidth}{far-detector-iso.eps}
  \end{center}
  \begin{itemize}
  \item 5.4kt (3.3kt fiducial)
  \item 486 steel planes (243/243)
  \item 484 scintilator planes (242/242)
  \item 192 scintilator strips/plane.
  \item 2 ended readout, 8x multiplexing

  \end{itemize}
\end{slide*}

\begin{slide}
  \slideheading{Expected Far Detector Interaction Spectra}
  \begin{center}
    \resizebox{0.9\textwidth}{!}{\rotatebox{270}{\includegraphics{spectra.eps}}}
  \end{center}
\end{slide}

\begin{slide*}
  \slideheading{Neutrino Beam Components}
  \begin{center}
    \sizedfig{0.9\textwidth}{parent-tracks-vacuum-far.eps}
    \resizebox{0.9\textwidth}{3cm}{\includegraphics{parent-tracks.eps}}
  \end{center}
\end{slide*}

\begin{slide*}
  \slideheading{Expected Signal/Background \\($\nu_e$ appearance)}
  \begin{center}
    \sizedfig{\textwidth}{nue_sigbkg.eps}    

    {\small 10 kt-yr, $U_{e3}^2 = 0.01$, $\delta m^2 = 0.003\, \mbox{eV}^2$,
    $U_{\mu 3}^2 = U_{\tau 4}^2$}
  \end{center}
\end{slide*}

\begin{slide*}
  \slideheading{Expected Efficiency \\($\nu_e$ appearance)}
  \begin{center}
    \sizedfig{\textwidth}{nue_eff.eps}    

    $\delta m^2 = 0.003\mbox{eV}^2$
  \end{center}
\end{slide*}

\begin{slide*}
  \slideheading{Expected Sensitivities \\($\nu_e$ appearance)}
  \begin{center}
    \sizedfig{\textwidth}{nue_sensitivity.eps}
  \end{center}
  \textbf{\textcolor{Green}{Green}} test point at
  $\sin^22\theta_{13}=0.08$, 
  $\sin^2\theta_{12}=1$, 
  $\sin^22\theta_{23}=1$,
  $\delta m_{12}^2 = 0.0001\mbox{eV}^2$, 
  $\delta m_{23}^2 = 0.003\mbox{eV}^2$,
  $\phi = 2\pi/3$.

  \textbf{Black} line is 1-$\sigma$, 10 kt-yr $\nu_\mu \to \nu_e$

  \textbf{\textcolor{Red}{Red}} line is 1-$\sigma$, 20 kt-yr $\bar{\nu}_\mu \to \bar{\nu}_e$

\end{slide*}

\begin{slide*}
  \slideheading{Expected Limits \\($\nu_e$ appearance)}
  \begin{center}
    \sizedfig{\textwidth}{nue_limit.eps}
  \end{center}
\end{slide*}


\begin{slide*}
  \slideheading{SUMO: 
    \underline{S}hallow
    \underline{U}nderwater
    \underline{M}ain Injector Neutrino
    \underline{O}scillation Experiement}
  \begin{center}
    (A. Habig, D. Petyt, L. Wai.  NuMI-L-780)
  \end{center}

  Main idea:
  \begin{itemize}
  \item $\sim$ SK sized water Cerenkov detector in Two Harbors, Minn.
  \item  1-2$^\circ$ off axis of NuMI beam, 631 km baseline
  \item 32 m water overburden, 0.5-1 km off shore
  \end{itemize}

  Reminder of M. Marx's ``Concrete Beach Ball'' detector idea:
  \begin{itemize}
  \item 50 -- 75 m diameter concrete sphere with spherical shell outer
    detector
  \item inner det: purified water, outer det: lake water
  \item PMTs housed in pressure vessels in concrete ID/OD separator.
  \end{itemize}
\end{slide*}

\begin{slide*}
  \slideheading{On and 9.2 mrad off axis $\nu_\mu $ CC events}
  \sizedfig{\textwidth}{sumo1.eps}
  \begin{center}
    0.4 MW NuMI, 5 yr $\times$ 5.5kton.
  \end{center}
\end{slide*}

\begin{slide*}
  \slideheading{\numunue, beam $\nu_e$ CC}
  \sizedfig{\textwidth}{sumo2.eps}
  \begin{center}
    0.4 MW NuMI, 5 yr $\times$ 20kton.    
  \end{center}
\end{slide*}

\begin{slide*}
  \enlargethispage{100pt}
  \slideheading{90\% CL regions}
  \sizedfig{\textwidth}{sumo3.eps}
  {\small
  \begin{itemize}
  \item 10\%  sys err
  \item $U^2_{\mu 3} = U^2_{\tau 3}, U^2_{e1} = U^2_{e2}$
  \item $ \left|\Delta m^2_{12} \right| = 5 \cdot 10^{-5} e \mbox{V}^2$ 
  \item CP phase $\phi = 0$    
  \end{itemize}
}
\end{slide*}

\begin{slide*}
  \slideheading{Survey of other baselines}
  \begin{itemize}
  \item Flux: NuMI at 0, 1, 2, 3$^\circ$ off axis, pure $\nu_\mu$
  \item Oscillation: full 3 neutrino, 2 $\Delta m^2$ scale matter
    effects.
  \item $\nu$ interactions from E889 proposal MC
  \item No energy resolution smearing (yet)
  \item Baselines:
  \begin{center}
    \begin{tabular}[h]{cc}
      End points &        baseline \\
      \hline
      FNAL-SUMO &         630 km \\
      FNAL-Soudan &       735 km \\
      FNAL-Canada &       911 km \\
      FNAL-Homestake &    1290 km \\
      BNL-Soudan &        1770 km \\
      BNL-Homestake &     2540 km \\
      BNL-WIPP &          2920 km 
    \end{tabular}
  \end{center}
  \end{itemize}
\end{slide*}
\end{document}