People present: Jim, Richard, Philippe, Akshay, Vasia, Matt, Rafal
Philippe started the meeting with a brief overview of what was done with the MMT test array, and pointing out that an estimate (with uncertainties) of the material in front of the array would be needed for interpreting the negative SQUID results as monopole production limits. We need to start implementing the material geometry of relevant cavern components into LHCb software. In the long term, this will be essential to all MoEDAL searches.
Then Akshay went through his slides. Using images from the Panoramix event viewer it is clear that very little has been implemented on the MoEDAL side of the LHCb geometry. On this side, the VELO vacuum vessel appears as just a cylinder in the geometry, lacking even the back cover. On the other hand, this component was implemented by Matthias Carakson in a radiation protection study, but in another format using another software. It needs to be included into the Gauss framework.
Action plan
-- The most important component is the vacuum vessel. We will start by implementing it into Gauss.