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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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Lenguaje: | eng |
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1999
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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 |
record_format | invenio |
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 |