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. 2004 Jun 21;7(1):7. doi: 10.12942/lrr-2004-7

Figure 4.

Figure 4

The evolution of the dimensionless shear parameter Ωshear = σ2/6H2 on a Bianchi I brane, for a Inline graphic model. The early and late-time expansion of the universe is isotropic, but the shear dominates during an intermediate anisotropic stage. (Figure taken from [221].)