Three-dimensional track reconstruction for directional Dark Matter detection
J. Billard (1), F. Mayet (1), D. Santos (1) ((1) LPSC Grenoble)

TL;DR
This paper introduces a likelihood-based 3D track reconstruction method for directional Dark Matter detection, achieving sub-millimeter spatial resolution and moderate angular resolution, enhancing detector capabilities for Dark Matter searches.
Contribution
It presents a novel likelihood method for 3D track reconstruction in directional detectors, enabling improved spatial resolution and analysis of recoil directions for Dark Matter detection.
Findings
Achieves sub-mm spatial resolution in the anode plane
Angular resolution ranges from 20° to 80° depending on recoil energy
Sense recognition efficiency is limited, suggesting focus on axial data below 100 keV
Abstract
Directional detection of Dark Matter is a promising search strategy. However, to perform such detection, a given set of parameters has to be retrieved from the recoiling tracks : direction, sense and position in the detector volume. In order to optimize the track reconstruction and to fully exploit the data of forthcoming directional detectors, we present a likelihood method dedicated to 3D track reconstruction. This new analysis method is applied to the MIMAC detector. It requires a full simulation of track measurements in order to compare real tracks to simulated ones. We conclude that a good spatial resolution can be achieved, i.e. sub-mm in the anode plane and cm along the drift axis. This opens the possibility to perform a fiducialization of directional detectors. The angular resolution is shown to range between 20 to 80, depending on the recoil energy, which is…
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