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Events (observed/expected) from accelerator ${{\mathit \nu}_{{\mu}}}$ experiments.
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Events (observed/expected) from reactor ${{\overline{\mathit \nu}}_{{e}}}$ experiments.
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R(${{\mathit \mu}}/{{\mathit e}}$) = (Measured Ratio ${{\mathit \mu}}/{{\mathit e}}$) $/$ (Expected Ratio ${{\mathit \mu}}/{{\mathit e}}$)
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R(${{\mathit \nu}_{{\mu}}}$) = (Measured Flux of ${{\mathit \nu}_{{\mu}}}$) $/$ (Expected Flux of ${{\mathit \nu}_{{\mu}}}$)
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R(${{\mathit \mu}}$/total) = (Measured Ratio ${{\mathit \mu}}$/total) $/$ (Expected Ratio ${{\mathit \mu}}$/total)
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$\mathit N_{{\mathrm {up}}}({{\mathit \mu}})/\mathit N_{{\mathrm {down}}}({{\mathit \mu}}$)
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$\mathit N_{{\mathrm {up}}}({{\mathit e}})/\mathit N_{{\mathrm {down}}}({{\mathit e}}$)
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R(up/down; ${{\mathit \mu}}$) = (Measured up/down; ${{\mathit \mu}}$) $/$ (Expected up/down; ${{\mathit \mu}}$)
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N(${{\mathit \mu}^{+}})/N({{\mathit \mu}^{-}}$)
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R(${{\mathit \mu}^{+}}/{{\mathit \mu}^{-}}$) = (Measured N(${{\mathit \mu}^{+}})/N({{\mathit \mu}^{-}}$)) $/$ (Expected N(${{\mathit \mu}^{+}})/N({{\mathit \mu}^{-}}$))
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${{\mathit \nu}_{{e}}}$ Capture Rates from Radiochemical Experiments
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$\phi _{\mathit ES}$ (${}^{8}\mathrm {B}$)
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$\phi _{\mathit CC}$ (${}^{8}\mathrm {B}$)
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$\phi _{\mathit NC}$ (${}^{8}\mathrm {B}$)
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$\phi _{{{\mathit \nu}_{{\mu}}}+{{\mathit \nu}_{{\tau}}}}$ (${}^{8}\mathrm {B}$)
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Total Flux of Active ${}^{8}\mathrm {B}$ Solar Neutrinos
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Day-Night Asymmetry (${}^{8}\mathrm {B}$)
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$0.033 \pm0.011$
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$\phi _{\mathit ES}$ (${}^{7}\mathrm {Be}$)
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$\phi _{\mathit ES}$ ( ${{\mathit p}}{{\mathit e}}{{\mathit p}}$ )
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$\phi _{\mathit ES}$ (CNO)
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$\phi _{ES}({{\mathit p}{\mathit p}}$)
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$\phi _{CC}({{\mathit p}{\mathit p}}$)
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$\phi _{\mathit ES}$ (hep)
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$\phi _{{{\overline{\mathit \nu}}_{{e}}}}$ (${}^{8}\mathrm {B}$)
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sin$^2(\theta _{12})$
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$0.307 \pm0.013$
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$\Delta $m${}^{2}_{21}$
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$(7.53 \pm0.18) \times 10^{-5}$ eV${}^{2}$
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sin$^2(\theta _{23})$
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$0.51 \pm0.04$
...
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$\Delta $m${}^{2}_{32}$
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$0.00245 \pm0.00005$ eV${}^{2}$
...
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sin$^2(\theta _{13})$
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$0.0210 \pm0.0011$
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$\delta $, $\mathit CP$ violating phase
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$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\mathit \nu}_{{\mu}}}$ $\rightarrow$ ${{\mathit \nu}_{{e}}}$ )
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sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\mathit \nu}_{{\mu}}}$ $\rightarrow$ ${{\mathit \nu}_{{e}}}$ )
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$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\overline{\mathit \nu}}_{{\mu}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
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sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\overline{\mathit \nu}}_{{\mu}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
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$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\mathit \nu}_{{\mu}}}$ ( ${{\overline{\mathit \nu}}_{{\mu}}}$ ) $\rightarrow$ ${{\mathit \nu}_{{e}}}$ ( ${{\overline{\mathit \nu}}_{{e}}}$ ))
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$<0.075$ eV${}^{2}$ CL=90.0%
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sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\mathit \nu}_{{\mu}}}$ ( ${{\overline{\mathit \nu}}_{{\mu}}}$ ) $\rightarrow$ ${{\mathit \nu}_{{e}}}$ ( ${{\overline{\mathit \nu}}_{{e}}}$ ))
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$<1.8 \times 10^{-3}$ CL=90.0%
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$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\overline{\mathit \nu}}_{{e}}}$ $\nrightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
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sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\overline{\mathit \nu}}_{{e}}}$ $\nrightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
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$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 (${{\mathit \nu}_{{\mu}}}$ $\rightarrow$ ${{\mathit \nu}_{{s}}}$)
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Search for ${{\mathit \nu}_{{\mu}}}$ or ${{\mathit \nu}_{{e}}}$ $\rightarrow$ ${{\mathit \nu}_{{s}}}$
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$\langle \Delta {{\mathit m}^{2}}_{\mathrm {21}}−\Delta {{\overline{\mathit m}}}{}^{2}_{21}\rangle $
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$\langle \Delta {{\mathit m}^{2}}_{\mathrm {32}}−\Delta {{\overline{\mathit m}}}{}^{2}_{32}\rangle $
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