Matter-Antimatter Asymmetry: With the SM and Beyond
APA
(2025). Matter-Antimatter Asymmetry: With the SM and Beyond. Perimeter Institute. https://pirsa.org/25010079
MLA
Matter-Antimatter Asymmetry: With the SM and Beyond. Perimeter Institute, Jan. 21, 2025, https://pirsa.org/25010079
BibTex
@misc{ pirsa_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}, year = {2025}, month = {jan}, note = {PIRSA:25010079 see, \url{https://pirsa.org}} }
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.