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The classic solution of the Einstein field equations that describes a homogeneous and isotropic universe is called the Friedmann–Lemaître–Robertson–Walker metric, or FLRW, after Friedmann, Georges Lemaître, Howard Percy Robertson and Arthur Geoffrey Walker, who worked on the problem in 1920's and 30's independently of Friedmann.
The cosmologist Georges Lemaître, the Big Bang theorist, was a former graduate student 1923-24 at the college, supervised by Sir Arthur Eddington.