Attending: Josh Klein, Tim Bolton, Matt Worcester
"1. G4 is up and running. Everything looks good and I think we will may it easily, but see below. We can put it into your CVS repository whenever you wish.
"2. The way we have planned things is not going to work out exactly as planned, I think it will work out better than planned. Here's why: our idea was that I would give you a flux function containing neutrons at the vessel and veto information which you would then read in to ReactorFSim. The problem is that we expect one unvetoed neutron per day. G4 generates events at about 2 Hz and we need to sample over 20 m^2. At 450 MWE, the rate over 20 m^2 is 3.2 Hz, so to get one neutron to put into ReactorG4Sim, I need to run G4 for a day and a half.
"In addition, you do not yet have a way to propagating a 100 MeV neutron and taking into account n-p scattering at these energies. Maybe by now you do, which is fine. In any event, what we can do, which is much easier, is this: attached is a file of neutrons generated at (0,0,-3.5m) with cos_thete=(0,1). The neutron energy is flat over 0.1-1000 MeV and the polar angle distubution is flat over (0,1). I thien let G4 propogate them through the mineral oil and flag the proton scatterings. This way, you only need worry about the what happens with the proton (Birke's law) and neutron after it hits the proton. You run all these events through ReactorFSim, but be sure to keep track of the initial neutron position and energy: if you know that, then I can use G4 to give you weights for each and we're done.
"There are some points: the way G4 moves a neutron through any sort of scattering is to destroy the initial state neutron and create a final state neutron. I just write everything into the event record:
"The first 9001 energy is the initial neutron
9004 is the scattered proton
The 9001 record just before a scattered proton gives you the neutron
The 9001 record just before a scattered proton gives you the neutron
momentum vector before the scattering; you work out the neutron momentum
vector after.
"This should be easy. I've attached a file of 500 events; you tell me and I can give you as many as you want."
Dave and Tim are about 90% done with the improved reconstruction based on their PMT data structure.
Matt has checked in code to do multiple compton scattering for the H and Gd capture gammas to ReactorFsim. He also defined two separate AV thicknesses for the 3-zone configuration.
Dave and Tim are going to add timing for scintillation light to ReactorFsim. They might be done in about 3 weeks.
Matt is going to check in new code with some bug fixes and pass the two AV thicknesses to ReactorDetector. He is also going to start the code in ReactorFsim to handle Peter's new veto events, defined above. He is going to start looking at Cherenkov light in the mineral oil.
Matthew Worcester Last modified: Fri Apr 22 13:24 CDT 2005