X-Nico

unusual facts about Riemannian metric



Alexander Friedmann

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.

Canonical quantum gravity

where {}^{(3)}R is the spatial scalar curvature computed with respect to the Riemannian metric \gamma {ij} and K {ij} is the extrinsic curvature,


see also