Inhomogeneous cosmological models and the Local Supercluster of Galaxies

Details Inhomogeneous cosmological models and the Local Supercluster of Galaxies Inhomogeneous cosmological models and the Local Supercluster of Galaxies

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976crasm.282..451m&link_type=abstract

Academie des Sciences (Paris), Comptes Rendus, Serie A - Sciences Mathematiques, vol. 282, no. 8, Feb. 23, 1976, p. 451-454. In

Physics

Fluid Dynamics

1

Astronomical Models, Big Bang Cosmology, Galactic Clusters, Relativity, Condensation, Einstein Equations, Expansion, Fluid Dynamics, Rotating Disks

Scientific paper

The following three-region cosmological model is proposed for the Local Supercluster of Galaxies: (1) Region 1 is a central condensation of spherical symmetry which can be described by a Friedmann expansion model. The Local Supercluster has the form of a rotating disk. (2) Region 2 is an intermediate zone, also of spherical symmetry which encircles region 1. This zone is assumed to be a vacuum, the so-called vacuous hole. (3) Region 3 is the expanding universe which contains the vacuous hole. The nature of the three regions is studied on the basis of an analysis of the behavior of spherically symmetrical incoherent fluids in General Relativity.

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