Spatially self-similar cosmological model of Bianchi type-1(I)

Details Spatially self-similar cosmological model of Bianchi type-1(I) Spatially self-similar cosmological model of Bianchi type-1(I)

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..93..419l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 93, no. 2, June 1983, p. 419-422.

Physics

4

Anisotropic Fluids, Astronomical Models, Cosmology, Matter (Physics), Relativity, Space-Time Functions, Einstein Equations, Equations Of State, Field Theory (Physics), Hubble Constant, Hyperspaces, Ideal Fluids, Orthogonal Functions, Similarity Theorem

Scientific paper

The solution presently arrived at through the integration of the Einstein equations for a tilted, spatially self-similar Bianchi type-(1)I space-time with 'stiff' matter content represents an anisotropic model tending to isotropic expansion in a special case. Two distinct cases arise for the so-called spatially homogeneous Bianchi models: orthogonal universes, in which the matter moves orthogonally to the hypersurfaces of homogeneity, and tilted universes, in which the fluid vector u is not normal to such hypersurfaces.

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