\relax \citation{gaisser} \@writefile{toc}{\contentsline {section}{\numberline {\uppercase {i}}Introduction}{1}} \@writefile{toc}{\contentsline {section}{\numberline {\uppercase {ii}}Neutrino beam properties}{1}} \newlabel{e1}{{1}{1}} \newlabel{e2}{{2}{1}} \@writefile{toc}{\contentsline {subsection}{\numberline {A}Differential spectra}{1}} \newlabel{eq0}{{3}{1}} \newlabel{eq1}{{5}{2}} \newlabel{eq2}{{6}{2}} \@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Calculated neutrino and antineutrino fluxes at a far site located 10000 km from a neutrino factory in which $1 \times 10^{20}$ muons have decayed in the beam--forming straight section. The fluxes are shown as a function of the energy of the stored muons for negative muons (top two plots) and positive muons (bottom two plots), and for three muon polarizations as indicated. FIGURES NEEDS UPDATING}}{2}} \newlabel{flux_fig}{{1}{3}} \@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Total neutrino flux of a given flavor versus angle at the source from the beamline at $L=732$\nobreakspace {}km for $E_\mu = 10$\nobreakspace {}GeV (solid line), 20\nobreakspace {}GeV (dashed), 50\nobreakspace {}GeV (dotted), and 250\nobreakspace {}GeV (dot--dashed), assuming $1.6\times 10^{20}$ neutrinos in the beam per operational year. A Gaussian muon beam divergence of 1\nobreakspace {}mr has been folded in. The total antineutrino flux is the same. FIGURE NEEDS UPDATING}}{3}} \newlabel{flux_vs_alpha}{{2}{3}} \citation{sg_prd} \@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces Neutrino and antineutrino spectra for muon--type neutrinos (top) and electron--type neutrinos (bottom) in the beam downstream of a muon storage ring neutrino source containing unpolarized muons. }}{4}} \newlabel{spectra_fig}{{3}{4}} \@writefile{toc}{\contentsline {subsection}{\numberline {B}Fluxes}{4}} \@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces Distribution of energies for interaction muon--type neutrinos 730\nobreakspace {}km downstream of the neutrino source for the MINOS PH2 WBB (open histogram) compared with the corresponding distribution downstream of a neutrino factory (shaded histogram).}}{5}} \newlabel{minos_beam_fig}{{4}{5}} \@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Energy spectra far cf near from Heidi}}{5}} \newlabel{far_near_fig}{{5}{5}} \citation{CCFRtotal, CCFRstrange, Eeightsixtysix} \@writefile{toc}{\contentsline {subsection}{\numberline {C}Interaction rates}{6}} \newlabel{exp_a}{{17}{6}} \@writefile{lof}{\contentsline {figure}{\numberline {6}{\ignorespaces Lepton energy spectra at a neutrino factory for CC $\overline {\nu }_\mu $ (top left), $\nu _\mu $ (top right), $\nu _e$ (bottom left), and $\overline {\nu }_e$ (bottom right) interactions.}}{7}} \newlabel{elept_fig}{{6}{7}} \newlabel{eq8}{{20}{7}} \newlabel{eq9}{{21}{7}} \newlabel{eq10}{{22}{7}} \newlabel{eq11}{{23}{7}} \newlabel{eq3}{{27}{8}} \newlabel{eq4}{{29}{8}} \citation{goodman} \citation{casper} \@writefile{lof}{\contentsline {figure}{\numberline {7}{\ignorespaces Tau--neutrino CC cross-section compared with the corresponding muon--neutrino cross-section.}}{9}} \newlabel{tau_fig}{{7}{9}} \@writefile{toc}{\contentsline {subsection}{\numberline {D}Beam divergence, momentum spread, and straight-section length}{10}} \@writefile{lot}{\contentsline {table}{\numberline {\uppercase {i}}{\ignorespaces Muon neutrino and electron antineutrino CC interaction rates in the absence of oscillations, calculated for baseline length $L = 732$\nobreakspace {}km (FNAL $\rightarrow $ Soudan), for MINOS using the wide band beam and a muon storage ring with $E_\mu =10, 20, 50$ and $250$\nobreakspace {}GeV. }}{10}} \newlabel{compare_tab}{{\uppercase {i}}{10}} \newlabel{rates_tab}{{\uppercase {i}}{10}} \bibcite{review}{1} \bibcite{solar}{2} \bibcite{solarth}{3} \bibcite{superk}{4} \bibcite{atmos}{5} \bibcite{three}{6} \bibcite{bww98}{7} \bibcite{global}{8} \bibcite{hall2}{9} \bibcite{lsnd1}{10} \bibcite{lsnd2}{11} \bibcite{four}{12} \bibcite{MINOS}{13} \bibcite{K2K}{14} \bibcite{chooz}{15} \bibcite{bugey}{16} \bibcite{kam}{17} \bibcite{paloverde}{18} \bibcite{sg_prd}{19} \bibcite{derujula}{20} \bibcite{camp}{21} \bibcite{matter}{22} \bibcite{raby}{23} \bibcite{wolf}{24} \bibcite{bppw}{25} \bibcite{lang}{26} \bibcite{lipari2}{27} \bibcite{cabbibo}{28} \bibcite{bpw}{29} \bibcite{pakvasa}{30} \bibcite{CP}{31} \bibcite{status_report}{32} \bibcite{ws1}{33} \bibcite{ws2}{34} \bibcite{bww}{35} \bibcite{papers}{36} \bibcite{design}{37} \bibcite{summer_study}{38} \bibcite{vision}{39} \bibcite{cern_vision}{40} \bibcite{gaisser}{41} \bibcite{sigma}{42} \bibcite{goodman}{43} \bibcite{casper}{44} \bibcite{ydep}{45} \bibcite{MNS}{46} \bibcite{phases}{47} \bibcite{bpw80}{48} \bibcite{kuo}{49} \bibcite{totsuka}{50} \bibcite{earth}{51} \bibcite{parke}{52} \bibcite{lipari}{53} \bibcite{petcov}{54} \bibcite{other_matter}{55} \bibcite{fuller}{56} \bibcite{pantaleone}{57} \bibcite{bdppw}{58} \bibcite{hall}{59} \bibcite{smirnov}{60} \bibcite{KARMEN}{61} \bibcite{bks1}{62} \bibcite{bks2}{63} \bibcite{justso}{64} \bibcite{boone}{65}