Hi all, I’m working to build a G4 simulation of an X-ray telescope. It uses cerium bromide scintillators. I have parameters set up such as scintillation yield(s), indices of refraction, etc. and optical photons are produced and propagated correctly.
From what I can tell, in G4, the energy resolution "RESOLUTIONSCALE"
of a scintillating material is a constant value. However, for cerium bromide, the energy resolution (FWHM) is not constant, but rather a linear function of energy—see, for instance, Quarati et al., figure 7..
Main question: Has anyone used or implemented energy-dependent scintillation resolution in the past?
Am I misinterpreting the energy resolution parameter "RESOLUTIONSCALE"
available for scintillation? My understanding is that it is a fixed parameter that does not very with energy, so it is not a good model of CeBr3 resolution. At the moment I am thinking to modify the G4 scintillation source to incorporate energy-dependent resolution. I would be happy to share this modification with anyone in the future.
Thank you in advance!
~ William