Bhatt, Jitesh R.Jitesh R.BhattPandey, Arun KumarArun KumarPandey2025-08-302025-08-302016-08-3010.1103/PhysRevD.94.0435362-s2.0-84989284337https://d8.irins.org/handle/IITG2025/21846We study the generation of a magnetic field in primordial plasma of standard model particles at a temperature T>80 TeV - much higher than the electroweak scale. It is assumed that there is an excess number of right-handed electrons compared to left-handed positrons in the plasma. Using the Berry-curvature modified kinetic theory to incorporate the effect of the Abelian anomaly, we show that this chiral imbalance leads to the generation of a hypermagnetic field in the plasma in both the collision dominated and collisionless regimes. It is shown that, in the collision dominated regime, the chiral-vorticity effect can generate finite vorticity in the plasma together with the magnetic field. Typical strength of the generated magnetic field is 1027 G at T∼80 TeV with the length scale 105/T, whereas the Hubble length scale is 1013/T. Furthermore, the instability can also generate a magnetic field of the order 1031 G at a typical length scale 10/T. But there may not be any vorticity generation in this regime. We show that the estimated values of the magnetic field are consistent with the bounds obtained from current observations.falsePrimordial magnetic field and kinetic theory with Berry curvatureArticlehttps://arxiv.org/pdf/1503.018782470002930 August 201616043536arJournal15