Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects
Figure 7
Flavor ratio as a function of at the detector for a GRB neutrino flux with the Waxman-Bahcall (WB) “plateau” (in ) between and GeV (cf. [17]). The shaded regions show the impact of the mixing angle uncertainties now (current) [81], in about 2015 (next generation, dominated by Daya Bay and T2K [82]), and in about 2025 (for a neutrino factory [83, 84]). Here is assumed for the sake of simplicity, figure taken from [30].
