2021/03/31 by Abigail Kopec, Amanda L. Baxter, Michael Clark +4 · 1 citation
Physics and Astronomy · #hep-ex #physics.ins-det
paper · pdf · doi:10.1088/1748-0221/16/07/p07014
published as JINST 16 P07014 (2021) · 16 pages, 7 figures, 1 table
arxiv created 2021/07/12 · arxiv updated 2021/07/13
We characterize single- and few-electron backgrounds that are observed in dual-phase liquid xenon time projection chambers at timescales greatly exceeding a maximum drift time after an interaction. These instrumental backgrounds limit a detector's sensitivity to dark matter and cosmogenic neutrinos. Using the ~150g liquid xenon detector at Purdue University, we investigate how these backgrounds, produced after 122keV 57Co Compton interactions, behave under different detector conditions. We find that the rates of single- and few-electron signals follow power-laws with time after the interaction. We observe linearly increasing rates with increased extraction field, and increased rates in the single-electron background with increased drift field. Normalizing the rates to the primary interaction's measured ionization signal, the rates increase linearly with the depth of the interaction. We test the hypothesis that infrared photons (1550nm) would stimulate and accelerate electron emission via photodetachment from impurities, but find that even 1 Watt of infrared light fails to reduce these backgrounds. We thus provide a characterization that can inform background models for low-energy rare event searches.