📝 SummarXiv

Abstract

The nature of dark matter (DM) remains one of the most fundamental open questions in physics. Among the main DM candidates are Weakly Interacting Massive Particles (WIMPs), expected to interact with matter through scattering. Directional detection offers a way to overcome the limits of conventional WIMP searches - in particular the neutrino fog - by identifying the direction of nuclear recoils (NR) and thus inferring the incoming WIMP direction. Earth's motion through the Galaxy produces an apparent WIMP wind, resulting in an anisotropic distribution of recoil tracks that no background can mimic. This thesis contributes to this effort through the development of 3D reconstruction techniques for the CYGNO/INITIUM experiment. CYGNO operates with a He:CF4 gas mixture at 1 ATM and triple-GEM amplification, producing scintillation light which is read by CMOS sensors and photomultiplier tubes (PMTs). A 3D reconstruction method was developed by combining CMOS (XY) and PMT (Z) data. A dedicated framework extracts PMT waveform information, synchronizes it with CMOS data, and reconstructs the full 3D topology and direction of tracks. The analysis focused on alpha particles, whose ionization profiles resemble WIMP-induced NRs. Alpha tracks were reconstructed with accurate direction and head-tail determination. The study characterized alpha backgrounds in LIME, confirming the presence of Rn-222 in the gas. Angular and spatial distributions also revealed U-238 and Th-232 contamination in the GEMs, cathode, and field cage. These findings clarified discrepancies with MC simulations and guided design improvements for CYGNO-04. Finally, first steps toward Negative Ion Drift (NID) operation with the MANGO prototype are presented, including a novel analysis of the first-ever NID PMT waveforms observed. These results demonstrate the potential of CYGNO for directional, low-background dark matter detection.