http://arxiv.org/abs/2212.08483
We study the evolution of hypermagnetic fields (HMFs) in random plasma in the symmetric phase of the early universe. The system of kinetic equations for the spectra of the energy density and the helicity, as well as the particles asymmetries is derived. We also formulate the initial condition which involve the Kazantsev and Kolmogorov spectra of the seed HMFs. This system is solved numerically. We predict the energy spectrum of primeval gravitational waves which are produced by these HMFs. Additionally, the baryon asymmetry of the universe, generated by the lepton asymmetries, is obtained. These results allow us to constrain the strength of seed HMFs.
M. Dvornikov
Mon, 19 Dec 22
8/62
Comments: 10 pages in LaTeX2e, 6 eps figures; contribution to proceedings of the 6th International Conference on Particle Physics and Astrophysics (November 29 – December 2, 2022, Moscow, Russia)