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Figure 1:
Schematic of confinement of matter to the brane, while gravity propagates in the bulk (from [51]). |
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Figure 2:
The RS 2-brane model. (Figure taken from [58].) |
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Figure 3:
Gravitational field of a small point particle on the brane in RS gauge. (Figure taken from [105].) |
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Figure 4:
The evolution of the dimensionless shear parameter ![]() ![]() |
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Figure 5:
The relation between the inflaton mass ![]() ![]() ![]() ![]() |
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Figure 6:
Constraints from WMAP data on inflation models with quadratic and quartic potentials, where ![]() ![]() ![]() ![]() |
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Figure 7:
Brane-world instanton. (Figure taken from [104].) |
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Figure 8:
The evolution of the covariant variable ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
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Figure 9:
The evolution of ![]() |
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Figure 10:
Graviton “volcano” potential around the ![]() |
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Figure 11:
Damping of brane-world gravity waves on horizon re-entry due to massive mode generation. The solid curve is the numerical solution, the short-dashed curve the low-energy approximation, and the long-dashed curve the standard general relativity solution. ![]() ![]() |
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Figure 12:
The CMB power spectrum with brane-world effects, encoded in the dark radiation fluctuation parameter ![]() ![]() |
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Figure 13:
The CMB power spectrum with brane-world moduli effects from the field ![]() ![]() ![]() |
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