Open mvicenzi opened 1 year ago
Just for the record, I found that similar studies were done for FASER in this paper. In particular, Table 4 in that paper is what we also want to generate for FLArE regarding muon-induced background (including muons undergoing photo-nuclear interactions in the rock in front of the detector, and within the detector volume).
An important study for the CDR is the calculation of rates for gammas, neutrons and other species inside the FLArE. This will allow to determine the background rates as a function of threshold.
Foreseen requirements:
Output: