On the Physics of Primordial Magnetic Fields
E. Battaner & H. Lesch

TL;DR
This paper discusses the origins of cosmic magnetic fields, emphasizing the importance of their spatial coherence scales and suggesting that large-scale fields originate from inflation, while small-scale fields are generated later during galaxy formation.
Contribution
It provides astrophysical arguments to distinguish between large and small-scale primordial magnetic fields, challenging many existing theories based on their coherence scales and timing.
Findings
Large-scale magnetic fields likely originated during inflation.
Small-scale fields cannot survive the radiation era and are generated after recombination.
Including large-scale magnetic fields can improve structure formation models.
Abstract
There are at present more then 30 theories about the origin of cosmic magnetic fields at galactic and intergalactic scales. Most of them rely on concepts of elementary particle physics, like phase transitions in the early Universe, string theory and processes during the inflationary epoch. Here we present some more astrophysical arguments to provide some guidance through this large number and variety of models. Especially the fact that the evolution of magnetic fields depends on the spatial coherence scale of the fields leds to some interesting conclusions, which may rule out the majority of the theoretical scenarios. In principle one has to distinguish between the large-scale and small-scale magnetic fields. Large scale fields are defined as those as becoming sub-horizon at that redshift at which the mass energy density becomes equal to the photon energy density, which we name as…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Scientific Research and Discoveries · Geomagnetism and Paleomagnetism Studies
