Estimates of Radiation by Superluminal Neutrinos

Details Estimates of Radiation by Superluminal Neutrinos Estimates of Radiation by Superluminal Neutrinos

2012-01-05

arxiv.org/abs/1201.1322v3

Phys. Rev. D85 (2012) 073007

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, no figures; text re-arranged for journal purposes; improved references; published version(title changed by Editors)

Scientific paper

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.

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