LEPTONS
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Neutrino Mixing

Reviews:
Introductory Text to Neutrino Mixing
Introduction to Three-Neutrino Mixing Parameters Listing (rev.)
(A) Neutrino fluxes and event ratios
Events (observed/expected) from accelerator ${{\mathit \nu}_{{\mu}}}$ experiments.
Events (observed/expected) from reactor ${{\overline{\mathit \nu}}_{{e}}}$ experiments.
Atmospheric neutrinos
R(${{\mathit \mu}}/{{\mathit e}}$) = (Measured Ratio ${{\mathit \mu}}/{{\mathit e}}$) $/$ (Expected Ratio ${{\mathit \mu}}/{{\mathit e}}$)
R(${{\mathit \nu}_{{\mu}}}$) = (Measured Flux of ${{\mathit \nu}_{{\mu}}}$) $/$ (Expected Flux of ${{\mathit \nu}_{{\mu}}}$)
R(${{\mathit \mu}}$/total) = (Measured Ratio ${{\mathit \mu}}$/total) $/$ (Expected Ratio ${{\mathit \mu}}$/total)
$\mathit N_{{\mathrm {up}}}({{\mathit \mu}})/\mathit N_{{\mathrm {down}}}({{\mathit \mu}}$)
$\mathit N_{{\mathrm {up}}}({{\mathit e}})/\mathit N_{{\mathrm {down}}}({{\mathit e}}$)
R(up/down; ${{\mathit \mu}}$) = (Measured up/down; ${{\mathit \mu}}$) $/$ (Expected up/down; ${{\mathit \mu}}$)
N(${{\mathit \mu}^{+}})/N({{\mathit \mu}^{-}}$)
R(${{\mathit \mu}^{+}}/{{\mathit \mu}^{-}}$) = (Measured N(${{\mathit \mu}^{+}})/N({{\mathit \mu}^{-}}$)) $/$ (Expected N(${{\mathit \mu}^{+}})/N({{\mathit \mu}^{-}}$))
Solar neutrinos
${{\mathit \nu}_{{e}}}$ Capture Rates from Radiochemical Experiments
$\phi _{\mathit ES}$ (${}^{8}\mathrm {B}$)
$\phi _{\mathit CC}$ (${}^{8}\mathrm {B}$)
$\phi _{\mathit NC}$ (${}^{8}\mathrm {B}$)
$\phi _{{{\mathit \nu}_{{\mu}}}+{{\mathit \nu}_{{\tau}}}}$ (${}^{8}\mathrm {B}$)
Total Flux of Active ${}^{8}\mathrm {B}$ Solar Neutrinos
Day-Night Asymmetry (${}^{8}\mathrm {B}$)   $0.033 \pm0.011$  
$\phi _{\mathit ES}$ (${}^{7}\mathrm {Be}$)
$\phi _{\mathit ES}$ ( ${{\mathit p}}{{\mathit e}}{{\mathit p}}$ )
$\phi _{\mathit ES}$ (CNO)
$\phi _{ES}({{\mathit p}{\mathit p}}$)
$\phi _{CC}({{\mathit p}{\mathit p}}$)
$\phi _{\mathit ES}$ (hep)
$\phi _{{{\overline{\mathit \nu}}_{{e}}}}$ (${}^{8}\mathrm {B}$)
(B) Three-neutrino mixing parameters
see data
sin$^2(\theta _{12})$   $0.307 \pm0.013$  
$\Delta $m${}^{2}_{21}$   $(7.53 \pm0.18) \times 10^{-5}$ eV${}^{2}$ 
sin$^2(\theta _{23})$   $0.51 \pm0.04$    ...
$\Delta $m${}^{2}_{32}$   $0.00245 \pm0.00005$ eV${}^{2}$   ...
sin$^2(\theta _{13})$   $0.0210 \pm0.0011$  
$\mathit CP$ violating phase
$\delta $, $\mathit CP$ violating phase
(C) Other neutrino mixing results
$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\mathit \nu}_{{\mu}}}$ $\rightarrow$ ${{\mathit \nu}_{{e}}}$ )
sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\mathit \nu}_{{\mu}}}$ $\rightarrow$ ${{\mathit \nu}_{{e}}}$ )
$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\overline{\mathit \nu}}_{{\mu}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\overline{\mathit \nu}}_{{\mu}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\mathit \nu}_{{\mu}}}$ ( ${{\overline{\mathit \nu}}_{{\mu}}}$ ) $\rightarrow$ ${{\mathit \nu}_{{e}}}$ ( ${{\overline{\mathit \nu}}_{{e}}}$ ))   $<0.075$ eV${}^{2}$  CL=90.0%
sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\mathit \nu}_{{\mu}}}$ ( ${{\overline{\mathit \nu}}_{{\mu}}}$ ) $\rightarrow$ ${{\mathit \nu}_{{e}}}$ ( ${{\overline{\mathit \nu}}_{{e}}}$ ))   $<1.8 \times 10^{-3}$   CL=90.0%
$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\overline{\mathit \nu}}_{{e}}}$ $\nrightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
sin$^2(2{}\theta )$ for ``Large'' $\Delta \mathit m{}^{2}$ ( ${{\overline{\mathit \nu}}_{{e}}}$ $\nrightarrow$ ${{\overline{\mathit \nu}}_{{e}}}$ )
Sterile neutrino limits
$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 (${{\mathit \nu}_{{\mu}}}$ $\rightarrow$ ${{\mathit \nu}_{{s}}}$)
Search for ${{\mathit \nu}_{{\mu}}}$ or ${{\mathit \nu}_{{e}}}$ $\rightarrow$ ${{\mathit \nu}_{{s}}}$
$\mathit CPT$ tests
$\langle \Delta {{\mathit m}^{2}}_{\mathrm {21}}−\Delta {{\overline{\mathit m}}}{}^{2}_{21}\rangle $
$\langle \Delta {{\mathit m}^{2}}_{\mathrm {32}}−\Delta {{\overline{\mathit m}}}{}^{2}_{32}\rangle $