Helical cosmological magnetic fields from extra-dimensions
Kumar Atmjeet, T. R. Seshadri, Kandaswamy Subramanian

TL;DR
This paper explores the generation of helical cosmological magnetic fields during inflation within a higher-dimensional electromagnetic framework, showing that extra dimensions can produce observable magnetic fields consistent with current bounds.
Contribution
It introduces a higher-dimensional model with parity violation that naturally generates helical magnetic fields during inflation, providing analytical and numerical solutions for their evolution.
Findings
A scale-invariant spectrum of helical magnetic fields is achieved for D=4.
Generated magnetic fields can reach strengths of ~10^{-9} G.
The model complies with observational bounds from Planck and gamma-ray data.
Abstract
We study the inflationary generation of helical cosmological magnetic fields in a higher-dimensional generalization of the electromagnetic theory. For this purpose, we also include a parity breaking piece to the electromagnetic action. The evolution of extra-dimensional scale factor allows the breaking of conformal invariance of the effective electromagnetic action in dimensions required for such generation. Analytical solutions for the vector potential can be obtained in terms of Coulomb wave-functions for some special cases. We also present numerical solutions for the vector potential evolution in more general cases. In the presence of a higher-dimensional cosmological constant there exist solutions for the scale factors in which both normal and extra dimensional space either inflate or deflate simultaneously with the same rate. In such a scenario, with the number of extra…
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