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In order to explain cosmic acceleration without invoking "dark" physics, we consider $f(R)$ modified gravity models, which replace the standard Einstein-Hilbert action in General Relativity with a higher derivative theory.
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L. Pogosian and A. Silvestri, The pattern of growth in viable f(R) cosmologies
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F. Schmidt, A. Vikhlinin, and W. Hu, Cluster constraints on f(R) gravity
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J.-h. He, Testing f ( R ) f(R) dark energy model with the large scale structure
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S. Ferraro, F. Schmidt, and W. Hu, Cluster Abundance in f(R) Gravity Models
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I. Tereno, E. Semboloni, and T. Schrabback, COSMOS weak-lensing constraints on modified gravity
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H. Gil-Marin, F. Schmidt, W. Hu, R. Jimenez, and L. Verde, The Bispectrum of f(R) Cosmologies
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A. Hojjati, L. Pogosian, A. Silvestri, and S. Talbot, Practical solutions for perturbed f(R) gravity
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J. Dossett and M. Ishak, Spatial Curvature and Cosmological Tests of General Relativity
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J.-h. He, Weighing neutrinos in f(R) gravity
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