Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/86785
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Type: Journal article
Title: The distance modulus determined from Carmeli's cosmology fits the accelerating universe data of the high-redshift type Ia supernovae without dark matter
Author: Hartnett, J.
Citation: Foundations of Physics: an international journal devoted to the conceptual and fundamental theories of modern physics, biophysics, and cosmology, 2006; 36(6):839-861
Publisher: Springer
Issue Date: 2006
ISSN: 0015-9018
1572-9516
Statement of
Responsibility: 
John G. Hartnett
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 magnitude–redshift 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 Ωm ≈ 0.021, which falls well within the measured values of the baryonic matter density. And the best estimate of ΩΛ+ Ωm ≈ 1.021 at the present epoch. The analysis also clearly distinguishes that the Hubble expansion of the universe is speed-limited.
Keywords: Carmeli cosmology; high redshift type Ia supernovae
Rights: © 2006 Springer Science+Business Media, Inc.
DOI: 10.1007/s10701-006-9047-y
Appears in Collections:Aurora harvest 7
Physics publications

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