A simple model of the evolution of a dust medium

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

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995tmp...103..475f&link_type=abstract

Theoretical and Mathematical Physics, Volume 103, Issue 1, pp.475-481

Mathematics

Mathematical Physics

Scientific paper

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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