Gravitational anti-screening as an alternative to the ΛCDM model

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2016-11
Authors
Penner, A. Raymond
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Abstract
Previously, in Penner (2016), a theory of gravitational anti-screening was shown to lead to the Baryonic Tully-Fisher Relationship. In addition it was shown to agree with the observed rotation curve of the Galaxy, the observed features in the rotational curves of other spiral galaxies, and with observations of the Coma cluster. In this paper, the theory is now shown to be consistent with a geometrically flat universe. Using a model of the distribution of superclusters, the overall density parameter of the universe, as determined by the theory, is Ω = 1.08 ± 0.19. In addition, the energy density which falls out from the theory has a negative pressure associated with it. This, along with a model of the evolution of superclusters, leads to an acceleration of the universal expansion without the requirement of dark energy. The theory of gravitational anti-screening therefore provides an alternative to the ΛCDM model of cosmology.
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This is a pre-copyedited, author produced version of an article published as: Penner, A.R. (2016). Gravitational anti-screening as an alternative the ΛCDM model. Astrophysics and Space Science, 361(11), 1-5. DOI: 10.1007/s10509-016-2953-3 The final publication is available at Springer via http://dx.doi.org/10.1007/s10509-016-2953-3.
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