  We explore the recent OPERA experiment of superluminal neutrinos in the
framework of Special Relativity with de Sitter space-time symmetry (dS-SR).
According to Einstein a photon is treated as a massless particle in the
framework of Special Relativity. In Special Relativity (SR) we have the
universal parameter $c$, the photon velocity $c_{photon}$ and the phase
velocity of a light wave in vacuum $c_{wave}=\lambda\nu$. Due to the null
experiments of Michelson-Morley we have $c=c_{wave}$. The parameter
$c_{photon}$ is determined by the Noether charges corresponding to the
space-time symmetries of SR. In Einstein's Special Relativity (E-SR) we have
$c=c_{photon}$. In dS-SR, i.e. the Special Relativity with SO(4,1) de Sitter
space-time symmetry, we have $c_{photon}>c$. In this paper, the OPERA datum are
examined in the framework of dS-SR. We show that OPREA anomaly is in agreement
with the prediction of dS-SR with $R\simeq 1.95\times 10^{12}l.y.$ Based on the
$p$-$E$ relation of dS-SR, we also prove that the Cohen and Glashow's argument
of possible superluminal neutrino's Cherenkov-like radiation is forbidden. We
conclude that OPERA and ICARUS results are consistent and they are explained in
the dS-SR framework.
