Speaker
Sascha Weber
(JGU Mainz)
Description
I present a new framework—Asymgenesis—that connects the baryon asymmetry of the universe to the dark matter density within the standard type-I seesaw model. The mechanism starts from a primordial charge asymmetry, either in the visible or dark sector, and redistributes it via a higher-dimensional portal operator. This process generates both a nonzero $B-L$ asymmetry and an asymmetric dark matter component.
Unlike conventional ADM scenarios, Asymgenesis places minimal demands on the portal interaction: it need not violate $B-L$, and the scales of $B-L$ violation and charge transfer can be separated. This enhances flexibility and broadens the model-building landscape for ADM
Primary authors
Martin Mojahed
(JGU/ TUM)
Sascha Weber
(JGU Mainz)
