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Our Standard Model of particle physics may be the most successful theory to date, yet it falls short in painting the full picture of our Universe. To explain the deficiencies, physicists have proposed various “Beyond the Standard Model” theories, including the presence of a mysterious, non-luminous mass component called “dark matter”. The nature of dark matter (DM), yet to be directly observed, is at the very forefront of physics research today. Direct detection experiments, who seek to observe interactions of DM particles with atoms in Earth-based detectors, have been extensively searching for Weakly Interacting Massive Particles (WIMPs), however have not yet been able to detect the historically favoured candidate. Another well-motivated DM theory is “asymmetric” DM, which postulates that the abundance of DM today has the same origin as the asymmetry of matter over anti-matter that we observe. In this model, DM candidates have masses on the order of the mass of the proton (~ 1 GeV), much lighter than the high mass WIMPs that most direct detection experiments are designed to search for. In this talk, I outline my proposal to use innovative (& quantum) detector instrumentation and sophisticated analysis strategies to perform a comprehensive and holistic search for this low mass DM, using both the largest DM experiment under construction to date, DarkSide-20k, and one of the smallest, QUEST-DMC.