PIRSA:25010079

Video URL

https://pirsa.org/25010079

Matter-Antimatter Asymmetry: With the SM and Beyond

(2025). Matter-Antimatter Asymmetry: With the SM and Beyond. Perimeter Institute for Theoretical Physics. https://pirsa.org/25010079

Matter-Antimatter Asymmetry: With the SM and Beyond. Perimeter Institute for Theoretical Physics, Jan. 21, 2025, https://pirsa.org/25010079 

          @misc{ scivideos_PIRSA:25010079,
            doi = {10.48660/25010079},
            url = {https://pirsa.org/25010079},
            author = {},
            keywords = {Particle Physics},
            language = {en},
            title = {Matter-Antimatter Asymmetry: With the SM and Beyond},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2025},
            month = {jan},
            note = {PIRSA:25010079 see, \url{https://scivideos.org/index.php/pirsa/25010079}}
          }
Seyda Ipek
Talk numberPIRSA:25010079
DOI10.48660/25010079
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

There is more matter than antimatter in the universe. This asymmetry requires three conditions: 1- Baryon (or lepton) number violation, 2- C and CP violation and 3- out-of-thermal equilibrium conditions in the early universe, before BBN. Although the SM does not have any out-of-equilibrium process, it does provide baryon number violation and CP violation. Still, it is commonly accepted that the SM CP violation is not enough for producing the observed baryon asymmetry. I will present one new physics model in which the SM CP violation, that is measured in the B meson system, is in fact enough to generate the baryon asymmetry.