Studies of Ionization Backgrounds in Noble Liquid Detectors For Dark Matter Searches

dc.contributor.advisorXu, Jingkeen_US
dc.contributor.advisorHall, Carteren_US
dc.contributor.authorMizrachi, Elien_US
dc.contributor.departmentPhysicsen_US
dc.contributor.publisherDigital Repository at the University of Marylanden_US
dc.contributor.publisherUniversity of Maryland (College Park, Md.)en_US
dc.date.accessioned2024-09-23T05:45:17Z
dc.date.available2024-09-23T05:45:17Z
dc.date.issued2024en_US
dc.description.abstractDark matter is believed to make up almost 85% of the total mass of the universe, yet its identity remains unclear. Weakly Interacting Massive Particles (WIMPs) have historically been a favored dark matter candidate, and dual-phase noble liquid time projection chambers (TPCs) have set the strongest interaction limits to date on WIMPs with a mass greater than several GeV. However, because no definitive interactions have been observed, the parameter space for conventional WIMPs is highly constrained. This has sparked greater interest in new sub-GeV dark matter models. At this mass scale, dark matter interactions with xenon or argon target media may still produce detectable signals at or near the single electron limit. However, these signals are currently obscured by delayed ionization backgrounds (“electron trains”) which persist for seconds after an ionization event occurs. Electron trains have been observed in many different experiments and exhibit similar characteristics, but their cause is only partially understood. This work examines the nature of electron trains in various contexts, as well as possible strategies to mitigate them. First, a characterization of electron trains in the LZ experiment is presented, including new evidence of a dependence on detector conditions. The characterization also informed the development of an electron-train veto for LZ's first WIMP search, which set world-leading limits on the spin-independent and spin-dependent WIMP-nucleon cross-sections for medium and high-mass WIMPs. Next, to complement the analysis of LZ data, hardware upgrades were performed in XeNeu, a small xenon TPC at Lawrence Livermore National Lab. These included replacing plastics with low-outgassing metal and machinable ceramic components, as well as a replacement of XeNeu's photomultiplier tube array with silicon photomultipliers. The resulting reduction in the intensity of electron-trains and better position resolution from the respective upgrades will improve future studies of low energy interactions and phenomena. Concurrent with this work, XeNeu was used to perform a nuclear recoil calibration and a search for the Migdal effect, the latter of which can substantially enhance an experiment's low-mass dark matter sensitivity. Finally, the development of CoHerent Ionization Limits in Liquid Argon and Xenon (CHILLAX), is reported. CHILLAX is a new xenon-doped, dual-phase argon test stand that has the potential to have a higher sensitivity to low-mass dark matter interactions and lower backgrounds than current liquid xenon TPCs. The system is designed to handle high (percent level) xenon concentrations in liquid argon that can enable a range of ionization signal production and collection benefits. CHILLAX demonstrated the feasibility of such concepts by achieving a world record xenon doping concentration with stable operation.en_US
dc.identifierhttps://doi.org/10.13016/jygd-ibrg
dc.identifier.urihttp://hdl.handle.net/1903/33310
dc.language.isoenen_US
dc.subject.pqcontrolledParticle physicsen_US
dc.subject.pquncontrolleddark matteren_US
dc.subject.pquncontrolledgas samplingen_US
dc.subject.pquncontrolledionization backgroundsen_US
dc.subject.pquncontrollednoble liquiden_US
dc.subject.pquncontrolledtime projection chamberen_US
dc.subject.pquncontrolledxenon doped argonen_US
dc.titleStudies of Ionization Backgrounds in Noble Liquid Detectors For Dark Matter Searchesen_US
dc.typeDissertationen_US

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