Speaker
Prof.
Dafne Guetta
(OAR INAF)
Description
I will review several models for the flux of high and ultra high energy neutrinos from astrophysical sources.
I will discuss the constraints that can be imposed from the IceCube data and that will be imposed by the next generation ultra high energy neutrino telescope like ARA.
Primary author
Prof.
Dafne Guetta
(OAR INAF)