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Lecture
Relativity and Cosmology II
Description
This lecture covers the main points of Lecture 1, the metric of homogeneous and isotropic 3-dimensional space, the Friedmann equations, Einstein equations for FRW metric, the concept of a static Universe, energy-momentum conservation, and the Hubble law. It delves into the implications of the expanding Universe, the luminosity distance, and the red shift in the context of General Relativity.
Official source
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