The generation of matter-antimatter asymmetries and hypermagnetic fields by the chiral vortical effect of transient fluctuations
arXiv:2001.03499 · doi:10.1140/epjc/s10052-021-09272-9
Abstract
We study the contribution of temperature-dependent chiral vortical effect to the generation and evolution of the hypermagnetic fields and the matter-antimatter asymmetries, in the symmetric phase of the early Universe, in the temperature range $100\mbox{GeV} \le T\le 10\mbox{TeV}$. Our most important result is that, due to the chiral vortical effect, small overlapping transient fluctuations in the vorticity field in the plasma and temperature of matter degrees of freedom can lead to the generation of strong hypermagnetic fields and matter-antimatter asymmetries, all starting from zero initial values. We show that, either an increase in the amplitudes of the fluctuations of vorticity or temperature, or a decrease in their widths, leads to the production of stronger hypermagnetic fields, and therefore, larger matter-antimatter asymmetries. We have the interesting result that fluctuating vorticity fields are more productive, by many orders of magnitude, as compared to vorticities that are constant in time.
22 pages, 6 figures
References in corpus (14)
- Charge separation induced by P-odd bubbles in QCD matter
- Chiral anomaly and local polarization effect from quantum kinetic approach
- Relativistic Hydrodynamics with General Anomalous Charges
- Notes on chiral hydrodynamics within effective theory approach
- Baryogenesis from Decaying Magnetic Helicity
- Constraining The Early-Universe Baryon Density And Expansion Rate
- Evolution of the Baryon Asymmetry through the Electroweak Crossover in the Presence of a Helical Magnetic Field
- A consistent description of kinetic equation with triangle anomaly
- Lepton asymmetry growth in the symmetric phase of an electroweak plasma with hypermagnetic fields versus its washing out by sphalerons
- Hypermagnetic Baryogenesis
- Primordial Nucleosynthesis: The Predicted and Observed Abundances and Their Consequences
- The effects of the U(1) Chern-Simons term and its baryonic contribution on matter asymmetries and hypermagnetic fields
- Contribution of the chiral vortical effect to the evolution of the hypermagnetic field and the matter-antimatter asymmetry in the early Universe
- Flavon Magneto-Baryogenesis