GEM-based TPC with CCD Imaging for Directional Dark Matter Detection

TL;DR

This paper presents a high-resolution GEM-based TPC with CCD imaging designed for directional dark matter detection, demonstrating its capability to distinguish electron and nuclear recoils at low energies with potential for further sensitivity improvements.

Contribution

It introduces a novel high-resolution, high signal-to-noise GEM-based TPC with CCD readout optimized for detailed recoil track measurements in dark matter experiments.

Findings

Achieved stable gas gains > 10^5 in 100 Torr CF4

Demonstrated effective background discrimination below ~10 keVee

Potential for lower thresholds with pressure reduction and 3D tracking

Abstract

The world's leading directional dark matter experiments currently all utilize low-pressure gas Time Projection Chamber (TPC) technologies. We discuss some of the challenges for this technology, for which balancing the goal of achieving the best sensitivity with that of cost effective scale-up requires optimization over a large parameter space. Critical for this are the precision measurements of the fundamental properties of both electron and nuclear recoil tracks down to the lowest detectable energies. Such measurements are necessary to provide a benchmark for background discrimination and directional sensitivity that could be used for future optimization studies for directional dark matter experiments. In this paper we describe a small, high resolution, high signal- to-noise GEM-based TPC with a 2D CCD readout designed for this goal. The performance of the detector was characterized using alpha particles, X-rays, gamma-rays, and neutrons, enabling detailed measurements of electron and nuclear recoil tracks. Stable effective gas gains of greater than $1 \times 10^5$ were obtained in 100 Torr of pure CF$_4$ by a cascade of three standard CERN GEMs each with a 140 $\mu$m pitch. The high signal-to-noise and sub-millimeter spatial resolution of the GEM amplification and CCD readout, together with low diffusion, allow for excellent background discrimination between electron and nuclear recoils down below $\sim$10 keVee ($\sim$23 keVr fluorine recoil). Even lower thresholds, necessary for the detection of low mass WIMPs for example, might be achieved by lowering the pressure and utilizing full 3D track reconstruction. These and other paths for improvements are discussed, as are possible fundamental limitations imposed by the physics of energy loss.