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We have examined a solution to the FRW model of the Einstein and de SitterUniverse, often termed the standard model of cosmology, using wide values forthe normalized cosmological constant Omega_L and spacetime curvature Omega_kwith proposed values of normalized matter density. These solutions wereevaluated using a combination of the third type of elliptical equations andwere found to display critical points for redshift z, between 1 and 3, whenOmega_L is positive. These critical points occur at values for normalizedcosmological constant higher than those currently thought important, though wefind this solution interesting because the Omega_L term may increase indominance as the Universe evolves bringing this discontinuity into importance.We also find positive Omega_L tends towards attractive at values of z which arecommonly observed for distant galaxies.

Elliptical Solutions to the Standard Cosmology Model with Realistic Values of Matter Density