SciFi Hit Efficinecy Monitoring/SciFi Hit Resolution First Principles Model

The present report aims to illustrate the work carried out during the CERN Summer student internship concerning the Hit Efficiency of the SciFi tracker while simultaneously introducing a first principle model regarding Hit Resolution as a function of momentum $p$ and the track's projected slopes $t_x$ (xz plane) and $t_y$ (yz plane). The hit resolution problem was initially investigated with respect to the 2D Random Planar Walks and subsequently examined through Rossi's theory of multiple scattering.