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. 2010 Jun 23;13(1):3. doi: 10.12942/lrr-2010-3

Figure 4.

Figure 4

Evolution of γ versus the redshift z in the model (4.83) with n = 1 and μ = 1.55 for four different values of k. For these model parameters the dispersion of γ with respect to k is very small. All the perturbation modes shown in the figure have reached the scalar-tensor regime (M2k2/a2) by today. From [589].