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Stabilization of Large Scale Structure by Adhesive Gravitational Clustering

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...

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Autor principal: Buchert, Thomas
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:http://cds.cern.ch/record/375600
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author Buchert, Thomas
author_facet Buchert, Thomas
author_sort Buchert, Thomas
collection CERN
description 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.
id cern-375600
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
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spelling cern-3756002019-09-30T06:29:59Zhttp://cds.cern.ch/record/375600engBuchert, ThomasStabilization of Large Scale Structure by Adhesive Gravitational ClusteringAstrophysics and AstronomyThe 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.astro-ph/9901002oai:cds.cern.ch:3756001999-01-05
spellingShingle Astrophysics and Astronomy
Buchert, Thomas
Stabilization of Large Scale Structure by Adhesive Gravitational Clustering
title Stabilization of Large Scale Structure by Adhesive Gravitational Clustering
title_full Stabilization of Large Scale Structure by Adhesive Gravitational Clustering
title_fullStr Stabilization of Large Scale Structure by Adhesive Gravitational Clustering
title_full_unstemmed Stabilization of Large Scale Structure by Adhesive Gravitational Clustering
title_short Stabilization of Large Scale Structure by Adhesive Gravitational Clustering
title_sort stabilization of large scale structure by adhesive gravitational clustering
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/375600
work_keys_str_mv AT buchertthomas stabilizationoflargescalestructurebyadhesivegravitationalclustering