Abstract
Carmeli’s 5D brane cosmology has been applied to the expanding accelerating universe and it has been found that the distance redshift relation will fit the data of the high-z supernova teams without the need for dark matter. Also the vacuum energy contribution to gravity, Ω Λ indicates that the universe is asymptotically expanding towards a spatially flat state, where the total mass energy density Ω + Ω Λ → 1.
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References
S. Behar, M. Carmeli, Cosmological Relativity: A New Theory of Cosmology, Int. J. Theor. Phys. 39 (5) (2000)
M. Carmeli, Commun. Theor. Phys. 5: 159 (1996)
M. Carmeli, Cosmological Special Relativity, Singapore, World Scientific. (2002).
P.M. Garnavich et al, Constraints on Cosmological Models from Hubble Space Telescope Observations of High-z Supernovae, Bulletin of the American Astronomical Society 29 (7) (1997).
S. Perlmutter et al, emphCosmology From Type Ia Supernovae: Measurements, Calibration Techniques, and Implications., Bulletin of the American Astronomical Society 29 (5): 1351 (1997).
A.G. Riess et al, Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116 (Sept): 1009–1038 (1998)
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HARTNETT, J.G. (2006). CARMELI’S COSMOLOGY: THE UNIVERSE IS SPATIALLY FLAT WITHOUT DARK MATTER. In: SIDHARTH, B., HONSELL, F., DE ANGELIS, A. (eds) Frontiers of Fundamental Physics. Springer, Dordrecht. https://doi.org/10.1007/1-4020-4339-2_3
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DOI: https://doi.org/10.1007/1-4020-4339-2_3
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