  We study the big rip scienario in Swiss-cheese Brane-worlds. The results
obtained have been found to be independent of the value of the cosmological
constant $\Lambda$ whether its positive, negative or zero. Negative tension
branes are not allowed in the current model. There is a sign flipping in cosmic
pressure corresponding to the sign flipping in the deceleration parameter from
positive to negative. The evolution of the EOS parameter shows the presence of
three phases: the matter dominant decelerating era,The accelerated-Quitessence
phase, and the phantom phase. The evolution of the potential and Kinetic term
also shows a change of sign. The energy conditions and cosmographic parameters
have also been investigated.
