Non-diffusive
transport, for which the particle mean free path grows nonlinearly in time, is
envisaged for many space and laboratory plasmas. In particular, superdiffusion,
i.e. 〈Δx2〉 ∝ tα with α > 1,
can be described in terms of a Lévy random walk, in which case the probability
of free-path lengths has power-law tails. Here, we develop a direct numerical
simulation to reproduce the Lévy random walk, as distinct from the Lévy flights. This implies that in the free-path
probability distribution Ψ(x, t) there is a space-time coupling, that is, the
free-path length is proportional to the free-path duration. A power-law
probability distribution for the free-path duration is assumed, so that the
numerical model depends on the power-law slope μ and on the scale distance x0.
The numerical model is able to reproduce the expected mean square deviation,
which grows in a superdiffusive way, and the expected propagator P(x, t), which
exhibits power-law tails, too. The difference in the power-law slope between
the Lévy flights propagator and the Lévy walks propagator is also estimated.
Website: http://www.arjonline.org/physical-sciences/american-research-journal-of-physics/
Website: http://www.arjonline.org/physical-sciences/american-research-journal-of-physics/
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