  We generalize nested multiply warped braneworld models by incorporating
non-zero brane curvature caused by an effective cosmological constant {\Omega}
induced on the 3-branes. Starting with the doubly warped model, we first
analyze the case where the maximally warped brane is identified as the visible
brane. For {\Omega} < 0, resolution of the gauge hierarchy problem imposes a
small upper bound on |{\Omega}|, and can possibly lead to positivity of all the
3-brane tensions. For {\Omega} > 0, the latter is not possible but the tuning
of the cosmological constant to its tiny observed value is linked to the tuning
of the extra dimensional moduli close to the inverse Planck length, justifying
the original flat brane approximation. In both regimes, we study the dependence
of the scale-clustering of the pair of TeV-branes on the brane cosmological
constant and hence its potential role in generating a fermion mass hierarchy
between these branes. Identifying the near-maximally warped brane as the
visible brane instead opens up regions in the parameter space that allow
positive 3-brane tensions for both anti de Sitter and de Sitter branes, subject
to non-trivial constraints on the warping parameters. We conclude by
generalizing the key results to arbitrary n-fold nested warped braneworlds.
