An approximation scheme for constructing inhomogeneous universes in general relativity

Details An approximation scheme for constructing inhomogeneous universes in general relativity An approximation scheme for constructing inhomogeneous universes in general relativity

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237..187f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 187-200.

Astronomy and Astrophysics

Astronomy

80

Background Radiation, Big Bang Cosmology, Galactic Evolution, Relativistic Theory, Universe, Astronomical Models, Galactic Clusters, Perturbation Theory, Red Shift

Scientific paper

An approximation scheme was developed to construct a model of a fully inhomogeneous universe based on the post-Newtonian approximation within the framework of general relativity. Through the use of a spatial averaging procedure, the scheme makes it possible to calculate the back reaction due to the growth of local inhomogeneities on the cosmic expansion (and vice versa). In effect, it can be used to study the formation of the large-scale structure in the early universe down to the fully nonlinear stage.

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