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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2901 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2901 http://eprints.org/relation/ismediumThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2901 2911 2 8242 document 2911 small.jpg image/png 0ab5f2b4abec553214fa7d5795dc50fe MD5 1933 2014-01-27 22:26:48 http://eprints.iliauni.edu.ge/743/6/small.jpg 743 6 6 image/png other Thumbnails conversion from text to thumbnail_small ge public

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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2901 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2901 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2901 archive 131 disk0/00/00/07/43 2014-01-29 19:48:55 2015-03-27 07:01:51 2014-01-29 19:48:55 article show Kahniashvili Tina tinatin@iliauni.edu.ge Vachaspati Tanmay pub QB QC public Magnetic fields in various astrophysical settings may be helical and, in the cosmological context, may provide a measure of primordial CP violation during baryogenesis. Yet it is difficult, even in principle, to devise a scheme by which magnetic helicity may be detected, except in some very special systems. We propose that charged cosmic rays originating from known sources may be useful for this purpose. We show that the correlator of the arrival momenta of the cosmic rays is sensitive to the helicity of an intervening magnetic field. If the sources themselves are not known, the method may still be useful provided we have some knowledge of their spatial distribution. 2006 Physical Review D 73 063507 TRUE