For a no-slip spherical particle in a Newtonian fluid at low Reynolds number, Stokes law gives . The fluctuation-dissipation theorem then gives the Stokes–Einstein relation . Using the conventional radial Brownian displacement in three dimensions,Here is the Boltzmann constant, absolute temperature, dynamic viscosity, particle radius and elapsed time. Larger thermal forcing raises diffusion; larger viscous drag reduces it. The formula requires times long relative to momentum relaxation and neglects walls, interactions and external drift.
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