The LSND Experiment and the Zee Model
| dc.creator | Wolfenstein, Lincoln | |
| dc.date | 1995-06-16 | |
| dc.date.accessioned | 2026-07-07T03:57:46Z | |
| dc.date.available | 2026-07-07T03:57:46Z | |
| dc.description | A recent experiment LSND at Los Alamos has provided\cite{1} an indication of $\overlineν_μ - \overlineν_e$ oscillations with $Δm^2$ of order 1ev$^2$ or greater and $\sin^2 2 θ_{e μ}$ between $2 \times 10^{-3}$ and $10^{2}$. Such a value of $Δm^2$ for $ν_μ - ν_e$ oscillations was not expected in the standard see-saw model\cite{2} suggested by SO(10) with a large mass hierarchy because it leads to too large a value of $m(ν_τ)$ to fit cosmological constraints. Furthermore within that model the LSND result is inconsistent with the indications of oscillations from both atmospheric neutrinos\cite{3} and solar neutrinos.\cite{4} | |
| dc.description | 3 pages, latex, no figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9506352 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9506352 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45570 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | The LSND Experiment and the Zee Model | |
| dc.type | text |