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https://hdl.handle.net/2440/86857
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DC Field | Value | Language |
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dc.contributor.author | Hartnett, J. | - |
dc.date.issued | 2008 | - |
dc.identifier.citation | Foundations of Physics: an international journal devoted to the conceptual and fundamental theories of modern physics, biophysics, and cosmology, 2008; 38(3):201-215 | - |
dc.identifier.issn | 0015-9018 | - |
dc.identifier.issn | 1572-9516 | - |
dc.identifier.uri | http://hdl.handle.net/2440/86857 | - |
dc.description.abstract | The redshift-distance modulus relation, the Hubble Diagram, derived from Cosmological General Relativity has been extended to arbitrarily large redshifts. Numerical methods were employed and a density function was found that results in a valid solution of the field equations at all redshifts. The extension has been 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 moduli 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 Ω K =ΩΛ−Ω=1−Ω, where Ω is the matter density of the universe. Hence the total density is always Ω K +Ω=1. | - |
dc.description.statementofresponsibility | John G. Hartnett | - |
dc.language.iso | en | - |
dc.publisher | Springer | - |
dc.rights | © Springer Science+Business Media, LLC 2007 | - |
dc.subject | Cosmological General Relativity | - |
dc.subject | High redshift type Ia supernovae | - |
dc.subject | Dark matter | - |
dc.subject | Distance modulus | - |
dc.title | Extending the redshift-distance relation in Cosmological General Relativity to higher redshifts | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1007/s10701-007-9198-5 | - |
pubs.publication-status | Published | - |
Appears in Collections: | Aurora harvest 2 Physics publications |
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