  As a follow-up to our previous paper arxiv: 1309.4244[hep-th], we determine
radion induced spherically symmetric solution using the gradient approximation
scheme, when two warped $3$-branes are slant with respect to each other such
that the radion field in this case is a radial co-ordinate varying function.
The slanting between the branes is assumed to be small. In the absence of any
on-brane matter except that induced effects of radion field, the resulting
black hole is found to be extremal Reissner-Nordstrom whose mass is
proportional to the slanting between the $3$-branes. It is however seen that
the inter-brane separation diminishes to zero for a particular value of radial
co-ordinate which can be mimicked as intersection of the branes. This situation
can be circumvented by adding traceless on-brane matter on the negative tension
brane.
