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We present a study of the mixing properties of the simulated intra clusterMedium, using tracers particles that are advected by the gas flow during theevolution of cosmic structures. Using a sample of seven galaxy clusters (withmasses in the range of M=2-3 10^14Msol/h) simulated with a peak resolution of25kpc/h up to the distance of two virial radii from their centers, weinvestigate the application of tracers to some important problems concerningthe mixing of the ICM. The transport properties of the evolving ICM are studiedthrough the analysis of pair dispersion statistics and mixing distributions. Asan application, we focus on the transport of metals in the ICM. We adopt simplescenarios for the injection of metal tracers in the ICM, and find remarkabledifferences of metallicity profiles in relaxed and merger systems, also throughthe analysis of simulated emission from Doppler-shifted Fe XXIII lines.

The Mixing and Transport Properties of the Intra Cluster Medium: a numerical study using tracers particles