  In this work, I present exact cosmological solutions from Wesson's Induced
Matter Model application to a general 5D metric in f(R,T) theory of gravity.
The non-conservation of the energy-momentum tensor, predicted by f(R,T) theory,
allows the derivation of a relation that describes the time evolution of the
extra coordinate, revealing its compactification. It is showed that such a
compactification could induce the effects of an accelerated expansion in the
observable universe.
