| Class | Description |
|---|---|
| DrawAngularNeutrinoFlux | |
| DrawAngularQuickNeutrinoFlux | |
| DrawCRFlux | |
| DrawEvolutionZmaxContour | |
| DrawIntegralNeutrinoFlux | |
| DrawNeutrinoFlux | |
| DrawNeutrinoFluxFunction | |
| DrawNeutrinoFluxIntegral | |
| DrawNeutrinoFluxRatio | |
| DrawNeutrinoFluxwzOsci | |
| DrawNeutrinoFluxYield | |
| DrawPropagatingNeutrinoFlux | |
| DrawPropagatingNeutrinoFlux2 | |
| DrawSumFlux | |
| MakeNeutrinoFluxTable | |
| NeutrinoFlux |
UHE Neutrino fluxes based on the following moels
are calculated from the table.
|
| NeutrinoFluxFromSource |
Calculate the source neutrino flux by the analytical functions
|
| NeutrinoFluxFunction |
Calculate the cosmic neutrino flux by the analytical functions.
|
| NeutrinoFluxFunctionEnergetics |
Calculate the GZK neutrino flux by the energetics argument
|
| PrintIntensityOnEvolutionZmaxPlane | |
| 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.
|
| QuickPropagatingNeutrinoFlux |
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.
|
| SearchEvolution |
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.