Convolutional Neural Networks for Direct Detection of Dark Matter
Charanjit K. Khosa (1), Lucy Mars (1), Joel Richards (1), Veronica, Sanz (1, 2, 3) ((1) Department of Physics, Astronomy, University of, Sussex, Brighton, UK, (2) Alan Turing Institute, British Library, London, UK, and (3) Instituto de F\'isica Corpuscular (IFIC), Universidad de

TL;DR
This paper demonstrates that convolutional neural networks can effectively distinguish dark matter signals from background noise in liquid Xenon detectors, achieving high recall and accuracy in simulated data.
Contribution
The study introduces CNN-based analysis for direct dark matter detection, showing improved event classification without data manipulation.
Findings
CNN achieved 93.4% recall for WIMP events
Precision of 81.2% in distinguishing backgrounds
Overall accuracy of 87.2% in simulations
Abstract
The XENON1T experiment uses a time projection chamber (TPC) with liquid Xenon to search for Weakly Interacting Massive Particles (WIMPs), a proposed Dark Matter particle, via direct detection. As this experiment relies on capturing rare events, the focus is on achieving a high recall of WIMP events. Hence the ability to distinguish between WIMP and the background is extremely important. To accomplish this, we suggest using Convolutional Neural Networks (CNNs); a Machine Learning procedure mainly used in image recognition tasks. To explore this technique we use XENON collaboration open-source software to simulate the TPC graphical output of Dark Matter signals and main backgrounds. A CNN turns out to be a suitable tool for this purpose, as it can identify features in the images that differentiate the two types of events without the need to manipulate or remove data in order to focus on a…
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