Anand, SampurnSampurnAnandBhatt, Jitesh R.Jitesh R.BhattPandey, Arun KumarArun KumarPandey2025-08-302025-08-302017-07-2810.1088/1475-7516/2017/07/0512-s2.0-85026804766http://repository.iitgn.ac.in/handle/IITG2025/22425We study the generation and evolution of magnetic field in the presence of chiral imbalance and gravitational anomaly which gives an additional contribution to the vortical current. The contribution due to gravitational anomaly is proportional to T² which can generate seed magnetic field irrespective of plasma being chirally charged or neutral. We estimate the order of magnitude of the magnetic field to be 10³⁰ G at T∼ 10⁹ GeV, with a typical length scale of the order of 10^-18 cm, which is much smaller than the Hubble radius at that temperature (10^-8 cm). Moreover, such a system possess scaling symmetry. We show that the T² term in the vorticity current along with scaling symmetry leads to more power transfer from lower to higher length scale as compared to only chiral anomaly without scaling symmetry.falsebaryon asymmetry | Magnetohydrodynamics | physics of the early universe | primordial magnetic fieldsArticlehttps://arxiv.org/pdf/1705.036831475751628 July 201712051arJournal14