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Feb 2006
39m 31s

Lecture 33: Einstein's Universe

Richard Pogge
About this episode
What are the implications of Relativity for the Universe? This lecture introduces the Cosmological Principle, which states that the Universe is Homogeneous and Isotropic on Large Scales. Applying this to his then-new General Relativyt, Einstein got a surprise: the Universe must either expand or contract in response to all the matter/energy that fills it, ... Show More
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Feb 2006
Lecture 32: Space, Time, & Gravity: General Relativity
What is gravity? Newton left that question unanswered when he formulated his inverse square law of the gravitational force, framing no hypothesis for what agency transmits gravity, only asserting it was an action at a distance. Einstein brought gravity into relativity by answerin ... Show More
47m 56s
Feb 2006
Lecture 31: A Tale of Two World Views: Special Relativity
What are space and time? To begin our exploration of the evolving Universe, we must first understand what we mean by space and time. This lecture contrasts the Newtonian view of the World, with its absolute space and absolute time, with that of Einstein, who showed that space and ... Show More
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Feb 2006
Lecture 30: Active Galaxies & Quasars
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42m 51s
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