In this talk, based on 1810.00880 and 2101.02706 , I will present a new mechanism of Baryogenesis and Dark Matter production: B-Mesogenesis. Within the B-Mesogenesis paradigm, both the dark matter relic abundance and the baryon asymmetry arise from neutral B meson oscillations and subsequent decays in the early Universe. If this mechanism is at play in the early Universe it would lead to unique collider signatures that I will describe in detail. I will also discuss various possibilities for the dark sector. Finally, I will show that a combination of measurements at BaBar, Belle, Belle II, LHCb, ATLAS & CMS can fully test B-Mesogenesis.
Meeting ID: 950 7111 3164