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- W2015370531 abstract "Primordial turbulence in the radiation era generates a weak seed magnetic field on all scales of the turbulence. This field is stochastically amplified by turbulence motions, and it is possible for magnetic and small-scale kinetic energies to attain equipartition within an expansion time. Field generation ceases at the epoch of equal radiation and matter densities, when the field strength is of the order of 1 G. It is estimated that the present intergalactic magnetic field has an intensity of ensuremath{sim}${10}^{ensuremath{-}8}$ G and a scale-length of ensuremath{sim}Mparsec." @default.
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- W2015370531 date "1973-01-29" @default.
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- W2015370531 title "Origin of Magnetic Fields in the Early Universe" @default.
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- W2015370531 doi "https://doi.org/10.1103/physrevlett.30.188" @default.
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