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A simple model of the evolution of a dust medium

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Abstract

A simple model is proposed that describes the kinetics of a dust medium and reproduces some observed nonequilibrium processes that lead to the formation of planetary rings, galaxies, and large-scale fold-type structures in space. The stable formation of typical galactic structures is attributed to their relaxation to stationary dissipative attractors.

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Authors and Affiliations

  1. Physicotechnical Institute, Donetsk

    A. É. Filippov

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  1. A. É. Filippov
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Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 103, No. 1, pp. 161–169, April, 1995.

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Filippov, A.É. A simple model of the evolution of a dust medium. Theor Math Phys 103, 475–481 (1995). https://doi.org/10.1007/BF02069790

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  • DOI: https://doi.org/10.1007/BF02069790

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