  In a recent paper, a cosmological model based on El Naschie {\it E} infinity
cantorian spacetime was presented [Iovane, G.; Chaos, Solitons and Fractals,
20: 657-667, (2004)]. In that work it was claimed that the present accelerated
expansion of the Universe can be obtained as the effect of a scaling law on
newtonian cosmology with a certain time dependent gravitational constant ($G$).
In the present work we show that it may be problematic to explain the present
accelerated expansion of the Universe using the approach presented in
\cite{iovane}. As a better alternative we apply the same scaling law and a
time-dependent gravitational constant, that follows from the observational
constraints, to relativistic cosmology, i.e. the Friedmann's model. We are able
to show that for a matter-dominated flat Universe, with the scaling law and a
varying $G$, an accelerated expansion emerges in such a way that the function
luminosity distance vs redshift can be made close to the corresponding function
that comes from the usual Friedmann's model supplemented with a cosmological
constant of value $\Omega_{\Lambda}\simeq0.7$. Then the measurements of high
redshift supernovae, could be interpreted as a consequence of the fractal-self
similarity of the $G$ varying relativistic universe.
