Understand
Using lattice techniques we investigate the generation of long range cosmological magnetic fields during a cold electroweak transition.
- We will show how magnetic fields arise, during bubble collisions, in the form of magnetic strings.
- We conjecture that these magnetic strings originate from the alignment of magnetic dipoles associated with EW sphaleron-like configurations.
- We also discuss the early thermalisation of photons and the turbulent behaviour of the scalar fields after tachyonic preheating.
Built on
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A. Díaz-Gil, J. García-Bellido, M. García Pérez, A. González-Arroyo, in proceedings of Lattice 2005 conference , \pos
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A. Díaz-Gil, J. García-Bellido, M. García Pérez, A. González-Arroyo, in preparation
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