(C) Other neutrino mixing results

The LSND collaboration reported in AGUILAR 2001 a signal which is consistent with ${{\overline{\mathit \nu}}_{{{\mu}}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{{e}}}}$ oscillations. In a three neutrino framework, this would be a measurement of $\theta _{12}$ and $\Delta \mathit m{}^{2}_{21}$. This does not appear to be consistent with most of the other neutrino data. The following listings include results from ${{\mathit \nu}_{{{\mu}}}}$ $\rightarrow$ ${{\mathit \nu}_{{{e}}}}$ , ${{\overline{\mathit \nu}}_{{{\mu}}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{{e}}}}$ appearance and ${{\mathit \nu}_{{{\mu}}}}$, ${{\overline{\mathit \nu}}_{{{\mu}}}}$, ${{\mathit \nu}_{{{e}}}}$, and ${{\overline{\mathit \nu}}_{{{e}}}}$ disappearance experiments, and searches for $\mathit CPT$ violation.

$\Delta \mathit m{}^{2}$ for sin$^2(2{}\theta )$ = 1 ( ${{\mathit \nu}_{{{\mu}}}}$ ( ${{\overline{\mathit \nu}}_{{{\mu}}}}$ ) $\rightarrow$ ${{\mathit \nu}_{{{e}}}}$ ( ${{\overline{\mathit \nu}}_{{{e}}}}$ ))

INSPIRE   PDGID:
S067D13
VALUE (eV${}^{2}$) CL% DOCUMENT ID TECN  COMMENT
$\bf{<0.075}$ 90
BORODOVSKY
1992
CNTR BNL E776
• • We do not use the following data for averages, fits, limits, etc. • •
$<1.6$ 90 1
ROMOSAN
1997
CCFR FNAL
1  ROMOSAN 1997 uses wideband beam with a $0.5~$km decay region.
References:
ROMOSAN 1997
PRL 78 2912 A High Statistics Search for ${{\mathit \nu}_{{{\mu}}}}$ (${{\overline{\mathit \nu}}_{{{\mu}}}}$) $\rightarrow$ ${{\mathit \nu}_{{{e}}}}$ (${{\overline{\mathit \nu}}_{{{e}}}}$) Oscillations in the Small Mixing Angle Regime
BORODOVSKY 1992
PRL 68 274 Search for ${{\mathit \nu}_{{{\mu}}}}$ Oscillations ${{\mathit \nu}_{{{\mu}}}}$ $\rightarrow$ ${{\mathit \nu}_{{{e}}}}$( ${{\overline{\mathit \nu}}_{{{\mu}}}}$ $\rightarrow$ ${{\overline{\mathit \nu}}_{{{e}}}}$) in a Wide Band Neutrino Beam