# From primordial seed magnetic fields to the galactic dynamo

**Authors:** Kandaswamy Subramanian

arXiv: 1903.03744 · 2019-08-12

## TL;DR

This paper reviews the origins of cosmic magnetic fields, discussing primordial seed fields, astrophysical batteries, and dynamo mechanisms, highlighting current challenges and the processes that amplify and sustain galactic magnetic fields.

## Contribution

It provides a comprehensive overview of the theoretical models for magnetic field origins and the dynamo processes, emphasizing recent challenges and potential resolutions.

## Key findings

- Primordial fields from early universe phases could serve as seed fields.
- Turbulent dynamos are crucial for amplifying seed magnetic fields in galaxies.
- Current theoretical challenges in dynamo theory are identified and discussed.

## Abstract

The origin and maintenance of coherent magnetic fields in the Universe is reviewed with an emphasis on the possible challenges that arise in their theoretical understanding. We begin with the interesting possibility that magnetic fields originated at some level from the early universe. This could be during inflation, the electroweak or the quark-hadron phase transitions. These mechanisms can give rise to fields which could be strong, but often with much smaller coherence scales than galactic scales. Their subsequent turbulent decay decreases their strength but increases their coherence. We then turn to astrophysical batteries which can generate seed magnetic fields. Here the coherence scale can be large, but the field strength is generally very small. These seed fields need to be further amplified and maintained by a dynamo to explain observed magnetic fields in galaxies. Basic ideas behind both small and large-scale turbulent dynamos are outlined. The small-scale dynamo may help understand the first magnetization of young galaxies, while the large-scale dynamo is important for the generation of fields with scales larger than the stirring scale, as observed in nearby disk galaxies. The current theoretical challenges that turbulent dynamos encounter and their possible resolution are discussed.

## Full text

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## References

147 references — full list in the complete paper: https://tomesphere.com/paper/1903.03744/full.md

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Source: https://tomesphere.com/paper/1903.03744