Reconstruction of Cosmological Evolution in the Presence of Extra
  Dimensions
  The model of Physics resulting from a Kaluza-Klein dimensional reduction
procedure offers very good dark matter candidates in the form of Light
Kaluza-Klein Particles, and thus becomes relevant to Cosmology. In this work we
recover a late-time cosmological picture, similar to that of the $\Lambda$CDM,
in a multidimensional scenario, in the general framework of Universal Extra
Dimensions. This is achieved by utilizing a special, Kasner-type solution that
is analytically known, and acts as an attractor for a plethora of pairs of
initial conditions of the usual and extra spatial Hubble parameters. The
phenomenology of fundamental interactions dictates the stabilization of the
extra dimensional evolution from a very early epoch in these scenarios. Without
an explicit mechanism, this is achieved through particular behaviors of the
usual and extra spatial fluids, which have to be motivated by a more
fundamental theory.
