Freeze-In Dark Matter and Leptogenesis: a 'SM route
Abstract
We investigate the possibility of freeze-in dark matter production and baryogenesis via leptogenesis in a 'SM model, which is an E6 extension of the Standard Model, featuring a residual U(1)' gauge symmetry. This symmetry arises from a linear combination of U(1) and U(1), both of which are subgroups of the E6. The spontaneous breaking of U(1)' symmetry governs the dynamics of a singlet fermion, which serves as a freeze-in dark matter candidate. The dark matter mass arises from dimension-five operators, and a discrete symmetry ensures its stability. We show that freeze-in production from scalar decay can yield the correct relic abundance for dark matter masses between a few MeV to a few hundred GeV. Simultaneously, heavy right-handed neutrinos generate light neutrino masses via the type-I seesaw and produce the observed baryon asymmetry via leptogenesis.
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.