  We construct a (quantum mechanically) modified model for the
Oppenheimer-Snyder collapse scenario where the exterior of the collapsing dust
ball is a Hayward black hole spacetime and the interior is a dust
Friedmann-Robertson-Walker cosmology. This interior cosmology is entirely
determined by the junction conditions with the exterior black hole. It turns
out to be non-singular, displaying a power-law contraction which precedes a de
Sitter phase or, reversely, a power-law expansion followed by a de Sitter era.
We also analyse the global causal structure and the viability of the model.
