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This is the primary tracking issue for integrating Celeritas with the simulation workflow for DUNE. The primary Celeritas contact points are the "assignees" to the right.
Notes from today's meeting (compiled an hour later so hopefully I remember the important bits):
Cherenkov is neglected in current simulations; it's only a few percent, and the detectors weren't designed for it. (There's currently no directional capabilities, the detector geometry doesn't favor capturing the light, and the photodetectors can't discriminate against UV light.)
The optical photon mapping includes time dependence, but a finely resolved grid (necessary for higher fidelity) requires too much memory
Currently the framework decouples energy deposition from optical responses at a framework level: energy deposition from steps are gathered during the Geant4 simulation, and afterward another stage of processing does the optical response calculation
Future work could move back to a model where optical photons are simulated during the main simulation
DUNE uses GDML for input (we have a copy)
They have a limited closed-source standalone simulation we might be able to try out
Surface physics is important; there will soon be reflective materials to worry about
This is the primary tracking issue for integrating Celeritas with the simulation workflow for DUNE. The primary Celeritas contact points are the "assignees" to the right.
Core capabilities
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