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arxiv: astro-ph/9605086 · v1 · submitted 1996-05-15 · 🌌 astro-ph

Ingredients and Equations for Making a Magnetic Field in the Early Universe

Sacha Davidson This is my paper
classification 🌌 astro-ph
keywords fieldmagneticearlyingredientsuniversebaryogenesisclassicalcoherent
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The ingredients required to create a magnetic field in the early Universe are identified, and compared with Sakharov's conditions for baryogenesis. It is also shown that a long range coherent magnetic field is not generated by the classical rolling Higgs vacuum expectation value during the electroweak phase transition.

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  1. Revisiting constraints on magnetogenesis from baryon asymmetry

    hep-ph 2025-09 unverdicted novelty 5.0

    Maximally helical primordial U(1)_Y magnetic fields can generate both intergalactic magnetic fields and baryon asymmetry; non-helical fields may work if Higgs dynamics compensate helicity loss to ≲10^{-9-10} precision...