Advances in High Energy Physics / 2015 / Article / Fig 4

Research Article

Constraints on the Nonstandard Interaction in Propagation from Atmospheric Neutrinos

Figure 4

The behaviors of the difference of the numbers of the multi-GeV -like events with the standard scenario and those with NSI . The vertical axis stands for the energy bin (1 for the lower energy and 2 for the higher energy), and the horizontal axis is the zenith angle bin (1 for for . (a) The difference of the numbers of the multi-GeV -like events. (b) The difference of the numbers of the multi-GeV -like events. (c) The difference of the numbers of the multi-GeV -like and -like events.
(a) multi-GeV IH
(b) multi-GeV IH
(c) multi-GeV IH