We study Q-ball formation in the expanding universe on 1D, 2D and 3D lattice simulations. We obtain detailed Q-ball charge distributions, and find that the distribution is peaked at Q3Dpeak ≈ 1.9 × 10-2(|Φin|/m)2, which is greater than the existing result by about 60%. Based on the numerical simulations, we discuss how the Q-ball formation proceeds. Also we make a comment on possible deviation of the charge distributions from what was conjectured in the past.
- cosmology of theories beyond the SM
- physics of the early universe
- supersymmetry and cosmology
ASJC Scopus subject areas
- Astronomy and Astrophysics