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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/3053 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/3053 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/3053 archive 131 disk0/00/00/07/76 2014-01-30 12:53:17 2015-03-27 07:08:55 2014-01-30 12:53:17 article show Kahniashvili Tina tinatin@iliauni.edu.ge Brandenburg Axel Campanelli Leonardo Ratra Bharat Tevzadze Alexander pub QB QC public We study the evolution of an inflation-generated magnetic field, due to its coupling to fluid motions, during cosmological phase transitions. We find that the magnetic field stays almost unchanged on large scales, while on small scales, the spectrum is modified in such a way that power at small scales becomes progressively suppressed. We also show that the magnetic field generates turbulent motions in the initially turbulence-free plasma. On large scales, the slope of the resulting kinetic energy spectrum is consistent with that of white noise. 2012 published Physical Review D 86 103005 TRUE