Generation of magnetic field in the pre-recombination era
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Blackwell Publishing for the Royal Astronomical Society
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We study the possibility of generating magnetic fields during the evolution of electron, proton and photon plasma in the pre-recombination era. We show that a small magnetic field can be generated in the second order of perturbation theory for scalar modes with adiabatic initial conditions. The amplitude of the field is <~10-30G at the present epoch for scales from sub-kiloparsec to 〉~100Mpc.
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Restricted Access. An open access version is available at arXiv.org.(one of the alternative locations)
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Monthly Notices of the Royal Astronomical Society, 2005, Vol.363, Issue 2, p521-528.
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(2005) Blackwell Publishing for the Royal Astronomical Society

