Preprint Article Version 3 This version is not peer-reviewed

A Cosmological View on Milgrom’s Acceleration Constant

Version 1 : Received: 7 December 2017 / Approved: 12 December 2017 / Online: 12 December 2017 (16:55:25 UTC)
Version 2 : Received: 9 January 2018 / Approved: 10 January 2018 / Online: 10 January 2018 (10:29:21 UTC)
Version 3 : Received: 8 November 2018 / Approved: 9 November 2018 / Online: 9 November 2018 (07:52:37 UTC)
Version 4 : Received: 9 November 2018 / Approved: 12 November 2018 / Online: 12 November 2018 (08:39:24 UTC)

How to cite: Roza, E. A Cosmological View on Milgrom’s Acceleration Constant. Preprints 2017, 2017120077 (doi: 10.20944/preprints201712.0077.v3). Roza, E. A Cosmological View on Milgrom’s Acceleration Constant. Preprints 2017, 2017120077 (doi: 10.20944/preprints201712.0077.v3).

Abstract

In this article it is shown how Milgrom’s acceleration constant is related with the ΩΛ, Ωm and ΩB values of the matter distribution within observable universe as defined in the Standard Model of Cosmology, established by the Planck Collaboration Group. The result is a two-parameter model for the observable universe. The two parameters are the age of the universe and Milgrom’s acceleration constant. It is shown that these are sufficient to calculate the amounts of matter and dark energy in the universe, as well as the contributions of dark matter and baryonic matter in the matter part. The numerical results are in agreement with those of the Lamda-CDM model. 

Subject Areas

cosmological constant; MOND; dark matter; dark energy; Lamda-CDM model

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