Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/84317
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Type: Book chapter
Title: Extending the Hubble diagram to higher redshifts in CGR
Author: Hartnett, J.
Citation: Relativity: Modern Large-Scale Spacetime Structure of the Cosmos, 2008 / Moshe Carmeli, (ed./s), pp.363-380
Publisher: World Scientific Publishing
Publisher Place: Singapore
Issue Date: 2008
ISBN: 9789812813756
Editor: Moshe Carmeli,
Statement of
Responsibility: 
John Hartnett
Abstract: The redshift-distance modulus relation, the Hubble Diagram, derived from Cosmological General Relativity are extended to arbitrarily large redshifts. Numerical methods are employed and a density function is found that results in a valid solution of the field equations at all redshifts. The extension is compared to 302 type Ia supernova data as well as to 69 Gamma-ray burst data. The latter however do not truly represent a ‘standard candle’ as the derived distance modulii are not independent of the cosmology used. Nevertheless the analysis shows a good fit can be achieved without the need to assume the existence of dark matter. The Carmelian theory is also shown to describe a Universe that is always spatially flat. This results from the underlying assumption of the energy density of a cosmological constant ΩΛ = 1, the result of vacuum energy. The curvature of the Universe is described by a spacevelocity metric where the energy content of the curvature at any epoch is Ω𝑲 = ΩΛ – = 1 –Ω where Ω is the matter density of the Universe. Hence the total density is always Ω𝑲 + Ω = 1. The following is based on Hartnett 2008.
Rights: Copyright © 2008 by World Scientific Publishing Co. Pte. Ltd.
DOI: 10.1142/9789812813770_0014
Published version: http://dx.doi.org/10.1142/9789812813770_0014
Appears in Collections:Aurora harvest 4
Chemistry and Physics publications

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