The Distance Modulus Determined from Carmeli's Cosmology Fits the Accelerating Universe Data of the Highredshift Type Ia Supernovae Without Dark Matter
Abstract
The velocity of the Hubble expansion has been added to General Relativity by Moshe Carmeli and this resulted in new equations of motion for the expanding universe. For the first time the observational magnituderedshift data derived from the high$z$ supernova teams has been analysed in the framework of the Carmeli theory and the fit to that theory is achieved without the inclusion of any dark matter. Best fits to the data yield an averaged matter density for the universe at the present epoch $\Omega_{m} \approx 0.021$, which falls well within the measured values of the baryonic matter density. And the best estimate of $\Omega_{\Lambda} + \Omega_{m} \approx 1.021$ at the present epoch. The analysis also clearly distinguishes that the Hubble expansion of the universe is speedlimited.
 Publication:

Foundations of Physics
 Pub Date:
 March 2006
 DOI:
 10.1007/s107010069047y
 arXiv:
 arXiv:astroph/0501526
 Bibcode:
 2006FoPh...36..839H
 Keywords:

 Astrophysics;
 General Relativity and Quantum Cosmology
 EPrint:
 10 pages, includes 7 figures, revised version, paper accepted in Found. Phys. Letters 2005