(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.

$\langle \Delta {{\boldsymbol m}^{2}}_{\mathrm {21}}−\Delta {{\overline{\boldsymbol m}}}{}^{2}_{21}\rangle $ INSPIRE search

VALUE ($ 10^{-4} $ eV${}^{2}$) CL% DOCUMENT ID TECN  COMMENT
$\bf{<1.1}$ 99.7 1
DEGOUVEA
2005
FIT solar vs. reactor
1  DEGOUVEA 2005 obtained this bound at the 3${{\mathit \sigma}}$ CL from the KamLAND (ARAKI 2005 ) and solar neutrino data.
  Conservation Laws:
$\mathit CPT$ INVARIANCE
  References:
DEGOUVEA 2005
PR D71 093002 Probing New Physics by Comparing Solar and KamLAND Data