Estimates of radiation by superluminal neutrinos

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 traveling from CERN to Gran Sasso as has been shown to occur for those with constant superluminality by Cohen and Glashow if indeed delta similar or equal to 5 x 10(-5). In addition, we clarify the dependence of such radiative processes on the size of the superluminality.