Inflation, Dark Energy, and the Cosmological Constant
Inflation, Dark Energy, and the Cosmological Constant. Intro Cosmology Short Course Lecture 5 Paul Stankus, ORNL. L= 0. Recall from Lecture 4:. The Friedmann Equation. GR. yadda, yadda, yadda…. Basic Thermodynamics. Hot. Sudden expansion, fluid fills empty space without loss of energy.
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