2012/09/25 by Masahiro Kawasaki, Masaki Yamada · 3 citations
Physics and Astronomy · #Baryogenesis #Baryon #Black Holes and Theoretical Physics #Branching fraction #Cosmology and Gravitation Theories #Electroweak interaction #Gravitino #Massless particle #Minimal Supersymmetric Standard Model #Particle physics #Particle physics theoretical and experimental studies #Physics #Quark #Supergravity #Supersymmetry #Yukawa potential #astro-ph.CO #hep-ph
paper · pdf · doi:10.1103/physrevd.87.023517
21 pages, 14 figures
arxiv created 2012/09/25 · openalex publication_date 2013/01/22 · arxiv updated 2013/05/29 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The Affleck-Dine mechanism, which is one of the most attractive candidates for baryogenesis in supersymmetric theories, often predicts the existence of baryonic Q-balls in the early universe. In this scenario, there is a possibility to explain the observed baryon-to-dark-matter ratio because Q-balls decay into supersymmetric particles as well as quarks. If the gravitino mass is small compared to the typical interaction energy, the longitudinal component of the gravitino behaves like the massless goldstino. We numerically calculate the goldstino production rates from Q-balls in the leading semiclassical approximation without using the large-radius limit or effective coupling. We also calculate the quark production rates from Q-balls in the Yukawa theory with a massive fermion. In deriving the decay rate we also take into account the scalar field configuration of the Q-ball. These results are applied to a realistic model in the gauge-mediated supersymmetry breaking and yield the branching ratio of the Q-ball decay into the gravitino. We obtain a branching ratio much smaller than the one estimated in the previous analysis.