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Figure 1:
Dynamics for ![]() |
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Figure 2:
Expansion histories for different values of ![]() ![]() ![]() ![]() ![]() ![]() |
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Figure 3:
Hubble diagram (distance modulus vs. redshift) from the High-Z Supernova Team [212]. The lines represent predictions from the cosmological models with the specified parameters. The lower plot indicates the difference between observed distance modulus and that predicted in an open-universe model. |
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Figure 4:
Hubble diagram from the Supernova Cosmology Project [197]. The bottom plot shows the number of standard deviations of each point from the best-fit curve. |
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Figure 5:
Constraints in the ![]() ![]() |
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Figure 6:
Constraints in the ![]() ![]() |
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Figure 7:
CMB data (binned) and two theoretical curves: The model with a peak at ![]() ![]() |
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Figure 8:
Constraints in the ![]() ![]() |
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Figure 9:
Gravitational lens probabilities in a flat universe with ![]() ![]() ![]() ![]() |
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Figure 10:
Limits from supernovae and large-scale structure data on ![]() ![]() ![]() |
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Figure 11:
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