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The large scale structures of the universe will likely be the next leading source of cosmological information.
R. Scoccimarro and J. Frieman, “Loop corrections in nonlinear cosmological perturbation theory,” Astrophys. J. Suppl
1996
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A. Lewis, A. Challinor and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys. J
2000
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