Thermal backgrounds in space. Cosmological principle and its consequences: Newtonian cosmology and types of "universes"; survey of relativistic cosmology; horizons. Overview of evolution in cosmology; radiation and element synthesis; physical models of the "early stages." Formation of large-scale structure to variability of physical laws. First and last states. Some knowledge of relativity expected. 8.962 recommended though not required.
This class has no prerequisites.
This class counts for a total of 12 credits. This is a graduate-level class.
You can find more information at the MIT + 8.942 - Google Search site.
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