  We have examined a solution to the FRW model of the Einstein and de Sitter
Universe, often termed the standard model of cosmology, using wide values for
the normalized cosmological constant Omega_L and spacetime curvature Omega_k
with proposed values of normalized matter density. These solutions were
evaluated using a combination of the third type of elliptical equations and
were found to display critical points for redshift z, between 1 and 3, when
Omega_L is positive. These critical points occur at values for normalized
cosmological constant higher than those currently thought important, though we
find this solution interesting because the Omega_L term may increase in
dominance as the Universe evolves bringing this discontinuity into importance.
We also find positive Omega_L tends towards attractive at values of z which are
commonly observed for distant galaxies.
