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See:
Description
| Class Summary | |
|---|---|
| DrawAngularNeutrinoFlux | |
| DrawNeutrinoFlux | |
| DrawNeutrinoFluxIntegral | |
| DrawPropagatingNeutrinoFlux | |
| DrawPropagatingNeutrinoFlux2 | |
| DrawSumFlux | |
| NeutrinoFlux | UHE Neutrino fluxes based on the following moels are calculated from the table. |
| PropagatingNeutrinoFlux | This class calculates differential flux dF/dLogE [/cm^2 sec sr] of neutrinos and charged leptons after propagation in the earth for a given model of primary cosmic neutrino production in the Universe. |
This package contains the classes to calculate primary neutrino fluxes predicted in the EHE neutrino models such as the GZK cosmogenic neutrino production. The class NeutrinoFlux is a key class to give dN/dLogE by reading out the pre-calculated table located at $CLASSPATH/iceCube/uhe/neutrinoModel.
PropagationNeutrinoFlux class convolute the propagation matrix calculated by the PropagationMatrix in the propagation package with the primary neutrino flux. It gives the neutrino/muon/tau energy spectrum and their intensities after their propagation in earth. In the PropagationNeutrinoFlux class, the full neutrino oscillation is assumed and the primary intensity of nu-mu and nu-tau given by the NeutrinoFlux is mixed up for input neutrino spectra.
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