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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2794 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2794 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2794 archive 131 disk0/00/00/07/25 2014-01-27 20:08:02 2015-03-27 06:56:57 2014-01-27 20:08:02 article show Kahniashvili Tina tinatin@iliauni.edu.ge Gogoberidze Grigol Ratra Bharat pub QC public We show that helical turbulence produced during a first-order phase transition generates circularly polarized cosmological gravitational waves (GWs). The characteristic frequency of these GWs for an extreme case of the phase transition model is around 10-3-10-2Hz with an energy density parameter as high as 10-12-10-11. The possibility of detection is briefly discussed. 2005 published Physical Review Letters 95 151301 TRUE