A Comprehensive Study of Low-Energy Response for Xenon-Based Dark Matter Experiments

Abstract

We report a comprehensive study of the energy response to low-energy recoils in dual-phase xenon-based dark matter experiments. A recombination model is developed to explain the recombination probability as a function of recoil energy at zero field and non-zero field. The role of e-ion recombination is discussed for both parent recombination and volume recombination. We find that the volume recombination under non-zero field is constrained by a plasma effect, which is caused by a high density of charge carriers along the ionization track forming a plasma-like cloud of charge that shields the interior from the influence of the external electric field. Subsequently, the plasma time that determines the volume recombination probability at non-zero field is demonstrated to be different between electronic recoils and nuclear recoils due to the difference of ionization density between two processes. We show a weak field-dependence of the plasma time for nuclear recoils and a stronger field-dependence of the plasma time for electronic recoils. As a result, the time-dependent recombination is implemented in the determination of charge and light yield with a generic model. Our model agrees well with the available experimental data from xenon-based dark matter experiments.

30 pages and 21 figures

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• Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX data
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Cited by in corpus (6)

• A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
• Emission of Single and Few Electrons in XENON1T and Limits on Light Dark Matter
• Solar Neutrinos as a Signal and Background in Direct-Detection Experiments Searching for Sub-GeV Dark Matter With Electron Recoils
• A Review of Basic Energy Reconstruction Techniques in Liquid Xenon and Argon Detectors for Dark Matter and Neutrino Physics Using NEST
• A Review of NEST Models for Liquid Xenon and Exhaustive Comparison to Other Approaches
• Probing neutrino magnetic moments and the XENON1T excess with coherent elastic solar neutrino scattering