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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2891 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2891 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2891 archive 131 disk0/00/00/07/42 2014-01-29 19:48:54 2015-03-27 06:57:22 2014-01-29 19:48:54 article show Kahniashvili Tina tinatin@iliauni.edu.ge von Toerne Eckard Arhipova Natalia Ratra Bharat pub QB QC public Measurements of the evolution with redshift of the number density of massive galaxy clusters are used to constrain the energy density of massive neutrinos and so the sum of neutrino masses ∑<under></under>mν. We consider a spatially flat cosmological model with cosmological constant, cold dark matter, baryonic matter, and massive neutrinos. Accounting for the uncertainties in the measurements of the relevant cosmological parameters we obtain a limit of ∑<under></under>mν<2.4 eV (95% C.L.). 2005 published Physical Review D 71 125009 TRUE