Affleck-Dine curvaton
Year: 2026
Type: article
Abstract: The Standard Model of particle physics does not explain the origin of the universe’s baryon asymmetry or its primordial fluctuations. The Affleck-Dine mechanism is a well motivated scenario for generating the baryon asymmetry through the postinflationary dynamics of a complex scalar field with baryon number. The curvaton mechanism is a popular approach for producing curvature perturbations through the dynamics of a light spectator field that decays after inflation. We demonstrate that the same complex field can viably perform both roles without any modifications to the minimal realization of Affleck-Dine baryogenesis. This scenario can also accommodate appreciable levels of primordial non-Gaussianity, beyond those achievable with only a real-valued curvaton field, and may be observable with future cosmic microwave background experiments.
DOI: 10.1103/7hr7-rtvh
Authors: Aurora Ireland, Gordan Krnjaic, Takuya Okawa
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Awards: G154696372, Theory For New Fundamental Physics Experiments, G2770303603, G4521877040, G498139845, G5616713406, G585908603, Research in Particle Theory, Cosmology, and Quantum Gravity, G716412294, THEORETICAL AND EXPERIMENTAL STUDIES IN PARTICLE PHYSICS AND COSMOLOGY, G7584948965, G86560745, G969889393
OpenAlex ID: W4403580025
