# Mirror magnetic field and its impact on dark matter distribution in   galaxies

**Authors:** Ekaterina Kryukova

arXiv: 1902.04512 · 2019-10-02

## TL;DR

This paper investigates the evolution of mirror magnetic fields across cosmological epochs and explores their potential influence on mirror matter distribution within galaxies, considering dynamo amplification and kinetic mixing effects.

## Contribution

It provides a detailed estimation of mirror magnetic field values during different cosmological stages and discusses their impact on galaxy structure, introducing a generalized model with kinetic mixing.

## Key findings

- Mirror magnetic fields are generated during radiation era and post-recombination.
- Dynamo amplification can enhance galactic mirror magnetic fields.
- Mirror magnetic fields may affect the distribution of mirror matter in galaxies.

## Abstract

We obtain the value of the mirror magnetic field during different stages of cosmological evolution. We consider the magnetic field generation in the radiation-dominated era and the post-recombination epoch. We also estimate its galactic low-scale value in the process of dynamo amplification. We discuss a possible effect of the mirror magnetic field on the mirror matter distribution in a galaxy. The model can be generalized by assuming the existence of kinetic mixing between ordinary and mirror particles.

## Full text

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## Figures

2 figures with captions in the complete paper: https://tomesphere.com/paper/1902.04512/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1902.04512/full.md

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Source: https://tomesphere.com/paper/1902.04512