Go to the U of M home page
School of Physics & Astronomy
Assay and Acquisition of Radiopure Materials

User Tools


cosmo

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Next revision
Previous revision
cosmo [2012/09/19 09:12] – created chao.zhangcosmo [2012/09/19 09:43] (current) prisca
Line 11: Line 11:
  
   * Track the cosmic ray background from surface down to underground and calculate the flux at different level of depth.   * 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.   * 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.1348063923.txt.gz · Last modified: 2012/09/19 09:12 by chao.zhang