M. Opher et R. Opher, MAGNETIC-FIELD SPECTRUM IN A PLASMA IN THERMAL-EQUILIBRIUM IN THE EPOCH OF PRIMORDIAL NUCLEOSYNTHESIS, Physical review. D. Particles and fields, 56(6), 1997, pp. 3296-3306
The low-frequency magnetic field spectrum in the primordial plasma is
of particular interest as a possible origin of magnetic fields in the
universe (e.g., Tajima and co-workers and Cable and Tajima). We derive
the magnetic field spectrum in the primordial plasma, in particular,
at the epoch of primordial nucleosynthesis. The pioneering study of Ca
ble and Tajima of the electromagnetic fluctuations, based on the fluct
uation-dissipation theorem, is extended. Our model describes both the
thermal and collisional effects in a plasma. It is based on a kinetic
description with the Bhatnagar, Gross, and Krook (BGK) collision term.
It is shown that the zero-frequency peak found by Cable and Tajima de
creases. At high frequencies, the blackbody spectrum is obtained natur
ally without the necessity of the link procedure used by them. At low
frequencies (omega less than or equal to 4 omega(pe), where omega(pe)
is the electron plasma frequency), it is shown that the magnetic field
spectrum has more energy than the blackbody spectrum in vacuum.