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Tensor Calculus and Differential Geometry → Current Observational Constraints
This graduate-level learning path systematically explores modified gravity theories proposed to explain cosmic acceleration, including f(R) gravity, Horndeski theories, massive gravity, and screening mechanisms. It establishes the necessary foundations in general relativity, tensor calculus, differential geometry, and cosmological perturbation theory before delving into theoretical frameworks, observational tests with large-scale structure and CMB, and current constraints.
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13 steps · 3 stages. Click any step to inspect it and see it on the Path Map.
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