  In a previous paper, some of us studied general relativistic homogeneous
gravitational collapses for dust and radiation, in which the density profile
was replaced by an effective density justified by some quantum gravity models.
It was found that the effective density introduces an effective pressure that
becomes negative and dominant in the strong-field regime. With this set-up, the
central singularity is replaced by a bounce, after which the cloud starts
expanding. Motivated by the fact that in the classical case homogeneous and
inhomogeneous collapse models have different properties, here we extend our
previous work to the inhomogeneous case. As in the quantum-inspired homogeneous
collapse model, the classical central singularity is replaced by a bounce, but
the inhomogeneities strongly affect the structure of the bounce curve and of
the trapped region.
