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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2800 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2800 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2800 archive 131 disk0/00/00/07/26 2014-01-29 19:48:07 2015-03-27 07:04:31 2014-01-29 19:48:07 article show Kahniashvili Tina tinatin@iliauni.edu.ge Gogoberidze Grigol Ratra Bharat pub QB QC public We consider gravitational waves (GWs) generated by primordial inverse-cascade helical magneto-hydrodynamical (MHD) turbulence produced by bubble collisions at the electroweak phase transitions (EWPT). Compared to the unmagnetized EWPT case, the spectrum of MHD-turbulence-generated GWs peaks at lower frequency with larger amplitude and can be detected by the proposed Laser Interferometer Space Antenna. 2008 published Physical Review Letters 100 231301 TRUE