  We show that the more energetic superluminal neutrinos with quadratically
dispersed superluminalities \delta=\beta^2-1, for \beta=v/c where v is the
neutrino velocity, also lose significant energy to radiation to the \nu+e^-+e^+
final state in travelling from CERN to Gran Sasso as has been shown to occur
for those with constant superluminality by Cohen and Glashow if indeed \delta
\simeq 5\times 10^{-5}. In addition, we clarify the dependence of such
radiative processes on the size of the superluminality.

High Energy Physics - Phenomenology