Global Predictions of the Universal Constant of Expansion

Abstract

The new spatial condensation cosmological theory, based on the new universal constant of expansion, kappa = G Rho t^2 = 3/(32 Pi), is used to predict measurements of the supernova Ia data with no acceleration of the expansion rate of the universe. That goal was accomplished with the key assumption that radiation travels on great circles on the surface of the supporting 4-D ball towards the detector at the compounded velocity of Vc = Hr - c. The radiation has traveled great distances from emission to measurement in the expanding universe and is exactly suited to test the global predictions of a cosmological theory. Problems of the current big bang theory are discussed. It will be shown that a new method of analyzing the data does indeed show the simplicity and consistency of the new theory in contrast to the old Friedmann big bang model.