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.