Neutrino flux predictions for Galactic plerions
Dafne Guetta, Elena Amato
Abstract
We consider a class of plerions that have been detected in the TeV range, and investigate the possibility that the emission is due to π0 decay. From the TeV flux we derive what is the expected νflux at Earth and find that this is likely to exceed the detection threshold of the upcoming km2 neutrino detectors.
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