A simple model for the evolution of a dust medium

Details A simple model for the evolution of a dust medium A simple model for the evolution of a dust medium

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995tmf....10..161f&link_type=abstract

Teoreticheskaya i Matematicheskaya Fizika, vol. 10, p. 161

Mathematics

Astronomical Models, Planetary Rings, Interplanetary Dust, Galactic Evolution, Galactic Structure, Cosmic Dust, Kinetic Equations, Nonequilibrium Conditions, Attractors (Mathematics)

Scientific paper

A simple model is proposed which 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 structures.
The stable formation of typical galactic structures is related to their
evolution to dissipative attractors.

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