Electromagnetic Field Fluctuations in the Early Universe

Details Electromagnetic Field Fluctuations in the Early Universe Electromagnetic Field Fluctuations in the Early Universe

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..dpp.f3s41s&link_type=abstract

American Physical Society, Division of Plasma Physics Meeting, November 16-20, 1998 New Orleans, LA, abstract #F3S.41

Physics

Plasma Physics

Scientific paper

Employing the fluctuation-dissipation theorem (FDT) to analyze an equilibrium plasma of the Early Universe at z ~ 10^11, Tajima et al Ap. J. 390, 309, (1992) calculate that the plasma is capable of sustaining large low frequency electromagnetic fields, ^1/2 ~ 10^14 G. A more accurate description in this regime suggests that certain assumptions of the FDT are violated. In fact, the field correlations and the dominant part of the low frequency plasma resistivity depend on each other, and therefore should be determined self-consistently. We derive a system of nonlinear equations, which describe these quantities in a self-consistent manner.

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