Talk:Oppenheimer–Snyder model
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point to make on FLWR inside Schwartzchild
editI propose adding the following to the overview:
During the collapse of a star to a black hole the geometry on the outside of the sphere is the Schwarzschild geometry- that is it has the usual black hole event horizon from which nothing, not even light, can escape. However the geometry inside is, curiously enough, the same Friedmann-Lemaître-Robertson-Walker geometry or 'flat' spacetime as in the rest of the observable universe.