Preprint Article Version 2 Preserved in Portico This version is not peer-reviewed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 CET)
Version 2 : Received: 9 January 2018 / Approved: 10 January 2018 / Online: 10 January 2018 (10:29:21 CET)
Version 3 : Received: 8 November 2018 / Approved: 9 November 2018 / Online: 9 November 2018 (07:52:37 CET)
Version 4 : Received: 9 November 2018 / Approved: 12 November 2018 / Online: 12 November 2018 (08:39:24 CET)

How to cite: Roza, E. A Cosmological View on Milgrom’s Acceleration Constant. Preprints 2017, 2017120077. Roza, E. A Cosmological View on Milgrom’s Acceleration Constant. Preprints 2017, 2017120077.


In this article a two-parameter model is developed for the 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. All this, not only for present time, but also as a function of cosmological time. The developed theory gives an adequate explanation for the phenomena of the accelerated scaling of the universe and the anomaly of the stellar rotation curves in galaxies. The numerical results are in agreement with those of the Lamda-CDM model.


Cosmological Constant; MOND; dark matter; dark energy; Lamda-CDM model


Physical Sciences, Astronomy and Astrophysics

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