Electroweak Baryogenesis
Mark Trodden
TL;DR
<3-5 sentence high-level summary> The paper surveys electroweak baryogenesis as a framework to explain the baryon asymmetry of the universe, focusing on how baryon-number-violating processes in the electroweak sector (via sphalerons) interact with CP violation and the dynamics of the electroweak phase transition. It evaluates zero- and finite-temperature baryon-number violation, discusses Standard Model and beyond-Standard Model CP-violating sources (notably in two-Higgs models and the MSSM), and analyzes both local and nonlocal baryogenesis mechanisms. The work emphasizes nonperturbative approaches, including lattice simulations and real-time dynamics, to assess the viability of EWBG, and highlights defect-mediated scenarios as alternatives that relax constraints on the phase transition. It concludes that while the SM alone cannot generate the observed BAU, plausible extensions—especially the MSSM and two-Higgs frameworks—offer testable pathways that can be probed by EDM measurements and collider experiments.
Abstract
Contrary to naive cosmological expectations, all evidence suggests that the universe contains an abundance of matter over antimatter. This article reviews the currently popular scenario in which testable physics, present in the standard model of electroweak interactions and its modest extensions, is responsible for this fundamental cosmological datum. A pedagogical explanation of the motivations and physics behind electroweak baryogenesis is provided, and analytical approaches, numerical studies, up to date developments and open questions in the field are also discussed.
