Astronomy 162 - Stars, Galaxies, & the Universe

Lecture 32: Space, Time, & Gravity: General Relativity


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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 answering
Newton's unanswered question with his General Relativity, our modern
theory of gravity. In Einstein's formulation, Matter tells spacetime how
to curve, and curved spacetime tells matter how to move. This lecture
presents the basic picture of General Relativity, and introduces some
of its observational consequences. The surprising conclusion is that
instead of space and time being a backdrop for physics in Newton's view,
united into spacetime by Relativity they are understood to be physical
and dynamic. This is important for understanding how the Universe as
a whole works.
Recorded 2006 February 21 in 1008 Evans Laboratory on the Columbus campus
of The Ohio State University.
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Astronomy 162 - Stars, Galaxies, & the UniverseBy Richard Pogge

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