Nothing known is denser than the densest of neutron stars except
a gravitational singularity (Black hole). The upper limit of the
inward pressure a neutron star can handle before further implosion
is dictated by neutron degeneracy pressure.
However, theoretically (Not yet observed but probably out there)
the next step would be a quark star, that is, a star that is held
from implosion by quark degeneracy pressure. Then the next stage
would be a black hole.
Technically there is yet another stage in between a qaurk star
and a singularity called preon degeneracy prssure but the preon
models are too flawed to even consider.