Differences between V 1.2.0 and 1.1.3¶
Lepton fluxes¶
The origin of this changes is a bug in the scripts used for the generation of the decay tables. The bug was a “wrong” formula for the boost discovered by Matthias Huber, thx. The effect is strongest at low energies as seen in the plots. At high energies there are no changes. For fluxes the changes are most striking in the zenith distribution of muons. For neutrinos the effect is mostly related to the spectral index. For electron neutrinos there is some effect for the zenith distribution at tens of GeV and will affect predictions made for IceCube DeepCore or KM3Net-ORCA. Update and recomputation of expectations is therefore recommended. For high energies, i.e. IceCube/P-ONE/ARCA recomputation is not necessary.
Muons in air showers¶
For MCEq computations for a single primary, the resulting spectra constitute the spectrum of particles in air showers. There is a ~10% change for the muon number.
Other changes¶
Some particle “mappings” have been updated and synchronized between the development version of CORSIKA 8. This has minor impact on the hadron ratios within the cascade and can lead to percent/sub-percent changes here and there.
Acknowledgements¶
The author is grateful to Matthias Huber (TUM) for helping with the discovery of the “decay bug”. And to Maximilian Reininghaus and Ralf Ulrich (KIT) for making thorough and very detailed cross checks with various versions of CORSIKA.