This working group will focus on the capability of theoretical models and Monte Carlo generators to describe neutrino interactions. Starting from a thorough comparison of existing models with experimental data, the group will foster and participate in the improvement of event generators.
Reminder: Next CENF-ND general meeting (via vydio) in September
In preparation of that meeting, the WGs should auto-organise: define conveners and set regular WG meetings.
Given the heterogeneity of the membership, and the need to appropriate the existing knowledge, the first meeting could be devoted to summarise, merge and digest the existing studies for the topics of interest of each WG.
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