English

Inflationary magnetogenesis with helical coupling

Cosmology and Nongalactic Astrophysics 2019-12-02 v1 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We describe a simple scenario of inflationary magnetogenesis based on a helical coupling to electromagnetism. It allows to generate helical magnetic fields of strength of order up to 107G10^{- 7}\,\text{G}, when extrapolated to the current epoch, in a narrow spectral band centered at any physical wavenumber by adjusting the model parameters. Additional constraints on magnetic fields arise from the considerations of baryogenesis and, possibly, from the Schwinger effect of creation of charged particle-antiparticle pairs.

Keywords

Cite

@article{arxiv.1911.10424,
  title  = {Inflationary magnetogenesis with helical coupling},
  author = {Yu. V. Shtanov and M. V. Pavliuk},
  journal= {arXiv preprint arXiv:1911.10424},
  year   = {2019}
}

Comments

5 pages, 1 figure. This work is based on the results presented at the XI Bolyai-Gauss-Lobachevskii (BGL-2019) Conference: Non-Euclidean, Noncommutative Geometry and Quantum Physics, Kiev, May 19-24. Compared to arXiv:1902.05894, a smooth analytic interpolating coupling function is used with an exact solution

R2 v1 2026-06-23T12:25:19.103Z