Stabilization of Large Scale Structure by Adhesive Gravitational Clustering

Details Stabilization of Large Scale Structure by Adhesive Gravitational Clustering Stabilization of Large Scale Structure by Adhesive Gravitational Clustering

1999-01-02

arxiv.org/abs/astro-ph/9901002v2

Ann.Shanghai.Obs.Acad.Sin.21:85-92,2000

Astronomy and Astrophysics

Astrophysics

LaTeX 8 pages, incl. 2 figures; uses paspconf.sty, epsf.sty, matches published version, `From Stars to the Universe', Workshop

Scientific paper

The interplay between gravitational and dispersive forces in a multi-streamed medium leads to an effect which is exposed in the present note as the genuine driving force of stabilization of large-scale structure. The conception of `adhesive gravitational clustering' is advanced to interlock the fairly well-understood epoch of formation of large-scale structure and the onset of virialization into objects that are dynamically in equilibrium with their large-scale structure environment. The classical `adhesion model' is opposed to a class of more general models traced from the physical origin of adhesion in kinetic theory.

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