English

Scale-invariant Helical Magnetic Fields from Inflation

Cosmology and Nongalactic Astrophysics 2019-09-11 v1 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We discuss a model which can generate scale-invariant helical magnetic fields on large scales (1\lesssim 1Mpc) in the primordial universe. It is also shown that the electric conductivity becomes significant and terminates magnetogenesis even before reheating is completed. By solving the electromagnetic dynamics taking conductivity into account, we find that magnetic fields with amplitude B1015GB\simeq 10^{-15}{\rm G} at present can be generated without encountering a backreaction or strong coupling problem.

Keywords

Cite

@article{arxiv.1904.11428,
  title  = {Scale-invariant Helical Magnetic Fields from Inflation},
  author = {Tomohiro Fujita and Ruth Durrer},
  journal= {arXiv preprint arXiv:1904.11428},
  year   = {2019}
}

Comments

24 pages, 6 figures

R2 v1 2026-06-23T08:49:34.151Z