Averaging of a locally inhomogeneous realistic universe

Toshifumi Futamase
Phys. Rev. D 53, 681 – Published 15 January 1996
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Abstract

We present an averaging scheme in general relativity which allows us to study the effect of local inhomogeneity on the global behavior of the universe. The scheme uses 3+1 splitting of spacetime and introduces Isaacson averaging on the spatial hypersurface to get the averaged geometry. As a result of the averaging, the Friedmann-Robertson-Walker (FWR) geometry is derived in the first-order approximation for a wide class of inhomogeneous nonlinear matter distribution. The deviation from the FRW expansion is derived to the next order in terms of the anisotropic distribution of an effective stress-energy tensor. Using a simple model of inhomogeneity we show that the average effect of the inhomogeneity behaves like a negative spatial curvature term and thus has a tendency to extend the age of the universe. © 1996 The American Physical Society.

  • Received 7 June 1995

DOI:https://doi.org/10.1103/PhysRevD.53.681

©1996 American Physical Society

Authors & Affiliations

Toshifumi Futamase

  • Astronomical Institute, Tohoku University, Sendai 980-77, Japan

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Vol. 53, Iss. 2 — 15 January 1996

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