Cosmological deductions from the relativistic stability of clusters of galaxies

With the object of theoretically predicting clusters to be as empirically observed with regard to mass, density and size, a model of non-compact clusters is obtained by adopting the Schwarzschild interior metric inside the cluster, with a Robertson /Walker metric outside. Implications include that t...

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Published in:Astrophysics and space science 1974-12, Vol.31 (2), p.333-339
Main Author: Wesson, Paul S.
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Language:English
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description With the object of theoretically predicting clusters to be as empirically observed with regard to mass, density and size, a model of non-compact clusters is obtained by adopting the Schwarzschild interior metric inside the cluster, with a Robertson /Walker metric outside. Implications include that there is no scope for the postulation of large amounts of dark matter in clusters; that the mass density of the universe is therefore close to that given by the luminous matter; thus, that the universe is open. Metric conditions, conditions on the clusters, and cosmological parameters and clusters are dealt with separately.
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title Cosmological deductions from the relativistic stability of clusters of galaxies
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