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arxiv: 1502.04051 · v2 · pith:KYEVN45Xnew · submitted 2015-02-13 · ❄️ cond-mat.stat-mech · astro-ph.GA· astro-ph.SR

Temperature inversion in long-range interacting systems

classification ❄️ cond-mat.stat-mech astro-ph.GAastro-ph.SR
keywords temperaturesystemsequilibriumlong-rangestatessystemthermalinteraction
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Temperature inversions occur in nature, e.g., in the solar corona and in interstellar molecular clouds: somewhat counterintuitively, denser parts of the system are colder than dilute ones. We propose a simple and appealing way to spontaneously generate temperature inversions in systems with long-range interactions, by preparing them in inhomogeneous thermal equilibrium states and then applying an impulsive perturbation. In similar situations, short-range systems would typically relax to another thermal equilibrium, with uniform temperature profile. By contrast, in long-range systems, the interplay between wave-particle interaction and spatial inhomogeneity drives the system to nonequilibrium stationary states that generically exhibit temperature inversion. We demonstrate this mechanism in a simple mean-field model and in a two-dimensional self-gravitating system. Our work underlines the crucial role the range of interparticle interaction plays in determining the nature of steady states out of thermal equilibrium.

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