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I’ll discuss the possibility that QCD, the SU(3) encapsulating the strong nuclear force in the Standard Model, undergoes a period in the early history of the Universe in which it confines with a much larger confinement scale than is observed today. I’ll talk about the mechanics of how one can realize such a phenomenon, what the Universe would look like during this period and phenomenological implications, and potential applications to realize the observed baryon asymmetry or a modified picture for dark matter freeze out.
Tim Cohen