A Dark Force for Baryons

          @misc{ scivideos_PIRSA:11090076,
            doi = {10.48660/11090076},
            url = {https://pirsa.org/11090076},
            author = {Vecchi, Luca},
            keywords = {Particle Physics},
            language = {en},
            title = {A Dark Force for Baryons},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {sep},
            note = {PIRSA:11090076 see, \url{https://scivideos.org/index.php/pirsa/11090076}}
          }
          

Abstract

We suggest the existence of a fundamental connection between baryonic and dark matter. This is motivated by both the stability of these two types of matter as well as the observed similarity of their present-day densities. A unified genesis of baryonic and dark matter arises naturally in models in which proton stability is ensured by promoting the baryon number to a local symmetry. This is illustrated in a specific class of SUSY models using the Affleck-Dine mechanism. The dark matter candidate in these scenarios is charged under the baryon gauge symmetry and is required to have a mass at the weak scale. We discuss the collider constraints from B-factories, LEP, Tevatron, and LHC, as well as direct detection bounds. A baryonic dark force is shown to be consistent with all data for mediators as light as the GeV scale.