| 1 | \tocdepth@munge |
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| 2 | \contentsline {section}{\numberline {}Contents}{1}{} |
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| 3 | \tocdepth@restore |
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| 4 | \contentsline {section}{\numberline {I}Physics Motivation}{2}{} |
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| 5 | \contentsline {section}{\numberline {II}Brief detector description}{3}{} |
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| 6 | \contentsline {subsection}{\numberline {A}Liquid Argon TPC}{3}{} |
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| 7 | \contentsline {subsection}{\numberline {B}Liquid Scintillator}{4}{} |
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| 8 | \contentsline {subsection}{\numberline {C}Water \v {C}erenkov}{4}{} |
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| 9 | \contentsline {section}{\numberline {III}Underground sites}{5}{} |
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| 10 | \contentsline {section}{\numberline {IV}Proton decay sensitivity}{5}{} |
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| 11 | \contentsline {subsection}{\numberline {A}$p \rightarrow e^+\pi ^0$}{8}{} |
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| 12 | \contentsline {subsection}{\numberline {B}$p \rightarrow \overline {\nu }K^+$}{9}{} |
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| 13 | \contentsline {subsection}{\numberline {C}Comparison between the detectors}{10}{} |
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| 14 | \contentsline {section}{\numberline {V}Supernova neutrinos}{10}{} |
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| 15 | \contentsline {subsection}{\numberline {A}SN neutrino emission and oscillations}{10}{} |
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| 16 | \contentsline {subsection}{\numberline {B}SN neutrino detection}{11}{} |
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| 17 | \contentsline {subsection}{\numberline {C}Diffuse Supernova Neutrino Background}{12}{} |
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| 18 | \contentsline {section}{\numberline {VI}Solar neutrinos}{14}{} |
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| 19 | \contentsline {section}{\numberline {VII}Atmospheric Neutrinos}{15}{} |
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| 20 | \contentsline {subsection}{\numberline {A}Introduction}{15}{} |
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| 21 | \contentsline {subsection}{\numberline {B}Oscillation physics}{16}{} |
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| 22 | \contentsline {subsection}{\numberline {C}Direct detection of $\nu _\tau $ in the atmospheric neutrino flux}{17}{} |
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| 23 | \contentsline {subsection}{\numberline {D}New phenomena beyond the "Standard Model"}{18}{} |
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| 24 | \contentsline {section}{\numberline {VIII}Geoneutrinos}{18}{} |
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| 25 | \contentsline {section}{\numberline {IX}Indirect Search for Dark Matter}{19}{} |
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| 26 | \contentsline {section}{\numberline {X}Neutrinos from reactors}{20}{} |
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| 27 | \contentsline {section}{\numberline {XI}Neutrinos from beams}{21}{} |
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| 28 | \contentsline {subsection}{\numberline {A}Introduction}{21}{} |
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| 29 | \contentsline {subsection}{\numberline {B}CNGS upgraded beam}{22}{} |
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| 30 | \contentsline {subsection}{\numberline {C}The CERN-SPL Super Beam}{22}{} |
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| 31 | \contentsline {subsection}{\numberline {D}The CERN-$\beta $B\ baseline scenario}{23}{} |
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| 32 | \contentsline {subsection}{\numberline {E}combining SPL Beam and $\beta $B\ with MEMPHYS at Fréjus}{24}{} |
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| 33 | \contentsline {subsection}{\numberline {F}Neutrino Factory LAr detector}{25}{} |
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| 34 | \contentsline {section}{\numberline {XII}Summary}{26}{} |
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| 35 | \contentsline {section}{\numberline {}Acknowledgments}{26}{} |
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| 36 | \contentsline {section}{\numberline {}References}{26}{} |
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