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We explore the recent OPERA experiment of superluminal neutrinos in theframework of Special Relativity with de Sitter space-time symmetry (dS-SR).According to Einstein a photon is treated as a massless particle in theframework of Special Relativity. In Special Relativity (SR) we have theuniversal parameter $c$, the photon velocity $c_{photon}$ and the phasevelocity of a light wave in vacuum $c_{wave}=\lambda\nu$. Due to the nullexperiments of Michelson-Morley we have $c=c_{wave}$. The parameter$c_{photon}$ is determined by the Noether charges corresponding to thespace-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 Sitterspace-time symmetry, we have $c_{photon}>c$. In this paper, the OPERA datum areexamined in the framework of dS-SR. We show that OPREA anomaly is in agreementwith 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 argumentof possible superluminal neutrino's Cherenkov-like radiation is forbidden. Weconclude that OPERA and ICARUS results are consistent and they are explained inthe dS-SR framework.

Superluminal Neutrinos from Special Relativity with de Sitter Space-time Symmetry