arXiv · hep-ph/9602357
Electrical conductivity in the early universe
Abstract
We solve numerically the Boltzmann equation in the early universe in the presence of a constant electric field and find the electrical conductivity $σ$ in the range $1\MeV\lsim T\lsim M_W$. The main contribution to $σ$ is shown to be due to leptonic interactions. For $T\lsim 100\MeV$ we find $σ\simeq 0.76T$ while at $T\simeq M_W$ we obtain $σ\simeq 6.7T$
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Jarkko Ahonen, Kari Enqvist. 1996-02-21. Electrical conductivity in the early universe. https://doi.org/10.1016/0370-2693(96)00633-8
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