cosmo
Cosmogenic Working Group
Members:
Angela Reisetter
Chao Zhang
Dongming Mei
Vitaly Kudryavtsev
Goals
Track the cosmic ray background from surface down to underground and calculate the flux at different level of depth.
Validate Geant4 muon propagation
Establish whether to employ MUSUN in C++ as a standard, or just work with Geant4?
Estimate the uncertainty of the cosmogenic background in different levels underground.
Establish a standard method for each site to prevent having to re-generate the muons each time
Continue to interact with Geant4 collaboration on the physics lists relevant to muon production of neutrons
Link to the Fluka v Geant working group on physics issues
cosmo.txt · Last modified: 2012/09/19 09:43 by prisca