Model-independent searches of new physics in DARWIN with a semi-supervised deep learning pipeline
J. Aalbers, K. Abe, M. Adrover, S. Ahmed Maouloud, L. Althueser, D. W. P. Amaral, B. Andrieu, E. Angelino, D. Ant\'on Martin, B. Antunovic, E. Aprile, M. Babicz, D. Bajpai, M. Balzer, E. Barberio, L. Baudis, M. Bazyk, N. F. Bell, L. Bellagamba, R. Biondi, Y. Biondi, A. Bismark

TL;DR
This paper introduces a deep learning pipeline for model-independent, likelihood-free detection of anomalous events in the DARWIN liquid Xenon experiment, outperforming traditional methods and enabling more efficient analysis.
Contribution
A novel semi-supervised deep learning approach using variational autoencoders and classifiers for model-independent anomaly detection in dark matter searches.
Findings
Outperforms classical likelihood-based background rejection tests.
Learns relevant energy features directly from high-dimensional detector data.
Reduces computational effort and information loss by avoiding data compression.
Abstract
We present a novel deep learning pipeline to perform a model-independent, likelihood-free search for anomalous (i.e., non-background) events in the proposed next generation multi-ton scale liquid Xenon-based direct detection experiment, DARWIN. We train an anomaly detector comprising a variational autoencoder and a classifier on extensive, high-dimensional simulated detector response data and construct a one-dimensional anomaly score optimised to reject the background only hypothesis in the presence of an excess of non-background-like events. We benchmark the procedure with a sensitivity study that determines its power to reject the background-only hypothesis in the presence of an injected WIMP dark matter signal, outperforming the classical, likelihood-based background rejection test. We show that our neural networks learn relevant energy features of the events from low-level,…
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