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The diffusion coefficient is calculated for a concentrated magnetic fluid in the absence of a magnetic field, taking into account the many-body correlations. The ferroparticle density distribution in a gravitational field is determined using both Monte Carlo simulations and theoretical modeling. Numerical and theoretical results are in good agreement.doi:10.1016/j.phpro.2010.11.024 fatcat:s3rr65mdk5hkxjy3hlvqwep6si