Mathematics
Scientific paper
Jun 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183..727e&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 183, June 1978, p. 727-748. Research supported by the University Grants
Mathematics
6
Astronomical Models, Cosmic Dust, Cosmology, Newton Theory, Relativity, Anisotropic Media, Equations Of Motion, Gravitational Effects, Singularity (Mathematics), Universe
Scientific paper
Comoving metrics of relativistic dust universes are interpreted locally in terms of conventional Newtonian cosmology. Quasi-classical equations for these universes show how anistropies in the motion and the spatial curvature affect the dynamics. Though generally indeterminate, the equations have heuristic and possibly predictive value, especially as regards matter singularities and indefinite expansion, for which they offer simple classifications. Examples are provided by homogeneous world models, including some with an apparently new kind of singularity behavior.
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