Tuesday, April 10, 2012

1201.1322 (B. F. L. Ward)

Estimates of Radiation by Superluminal Neutrinos    [PDF]

B. F. L. Ward
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.
View original: http://arxiv.org/abs/1201.1322

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