Leptogenesis and Primordial Magnetic Fields
arXiv:1309.2315 · doi:10.1088/1475-7516/2014/02/036
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 and field strength that are of astrophysical interest. 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.
v2: 21 pages, no figures; expanded JCAP version
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- Evolution of the Baryon Asymmetry through the Electroweak Crossover in the Presence of a Helical Magnetic Field
- Search for CP Violating Signature of Intergalactic Magnetic Helicity in the Gamma Ray Sky
- The Gamma-Ray Window to Intergalactic Magnetism
- Future CMB constraints on cosmic birefringence and implications for fundamental physics
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- Probing Intergalactic Magnetic Fields with Simulations of Electromagnetic Cascades
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- Scale-invariant helical magnetic field evolution and the duration of inflation
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- Parity-odd correlators of diffuse gamma rays and intergalactic magnetic fields
- Searching for Primordial Magnetic Fields with CMB B-modes
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- Thermal leptogenesis in the presence of helical hypermagnetic fields