Implications of bar{ν}_(e)e⁻to W⁻γ for high-energy bar{ν}_e observation
classification
✦ hep-ph
astro-ph
keywords
high-energyphotonenergyfinalhardstateaboveboson
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Absorption of high-energy $\bar{\nu}_e$ over electrons above the W boson production threshold is reexamined. It is pointed out that, in the case of photon emissions along the direction of incident high-energy $\bar{\nu}_e$, the kinematically allowed average energy carried by the final state hard photon can be $\leq 1%$ of the incident $\bar{\nu}_e$ energy above the W boson production threshold. The differential energy spectrum for the final state hard photon is calculated. We also discuss implications of our results for the prospective search of high-energy $\bar{\nu}_e$ through this final state hard photon.
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