The main goal of this project is to produce a definite recommendation on how to proceed beyond the current state-of-the-art in the modeling of the VHE gamma-ray emission from pulsars. This may involve the design and successful implementation of hybrid FFE/MHD-PIC simulations with particle acceleration, γ-ray emission, and radiation reaction. We expect that the joint effort of representatives from all the major international groups working together in the same Team will make this a reality.