  Using the effective equations in our Loop Quantum Cosmology (LQC) -- inspired
models, we resolve the $(n + 2)$ dimensional black hole singularity. This
resolution in the four dimensional case is same as that given recently by
Ashtekar, Olmedo, and Singh. We then study the fate of a massive collapsing
star in $(n + 2)$ dimensions, focussing on a singularity resolved black hole, a
string theoretic fuzz ball, and a Loop quantum star -- which is a solution to
the the effective modified equations for static spherically symmetric stars we
obtained recently using LQC ideas. We find qualitatively that a massive
collapsing star is likely to become a Loop quantum star : it is likely to have
a macroscopic core region with Planckian densities and pressures which is
surrounded by a low density corona region extending to the Schwarzschild
radius.
