Measurement of Atmospheric Neutrino Oscillations with Very Large Volume Neutrino Telescopes

Figure 5

Expected interaction rate of electron neutrinos and antineutrinos predicted by a NO over the rate predicted assuming an IO. Using the oscillation parameters in [3]. Because of the flux ratio and the cross section difference, estimated to be 2.1 times larger for neutrinos than antineutrinos, more electron neutrino interactions are expected for a NO.