Abstract
The anomalous conversion of leptons into baryons during leptogenesis is shown to produce a right-handed helical magnetic field; in contrast, the magnetic field produced during electroweak baryogenesis is known to be left-handed. If the cosmological medium is turbulent, the magnetic field evolves to have a present day coherence scale ∼ 10 pc and field strength ∼ 10-18 Gauss. This result is insensitive to the energy scale at which leptogenesis took place. Observations of the amplitude, coherence scale, and helicity of the intergalactic magnetic field promise to provide a powerful probe of physics beyond the Standard Model and the very early universe.
Original language | English (US) |
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Article number | 036 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2014 |
Issue number | 2 |
DOIs | |
State | Published - Feb 2014 |
Keywords
- cosmic magnetic fields theory
- leptogenesis
- particle physics - cosmology connection
- physics of the early universe
ASJC Scopus subject areas
- Astronomy and Astrophysics