Astrophysics

   

Inhomogeneous Distribution of the Universe’s Matter Density as a Physical Basis for MOND’s Acceleration a0

Authors: Antonio Francino, Gabriel Simón

One of the most effective theories for dark matter is Milgrom’s Modified Newtonian Dynamics, where a modified law of gravity based on a fixed acceleration scale a0 is postulated that provides a correct description of the gravitational fields in galaxies. However, the significance of a0 is unknown, and the whole theory is generally viewed as a phenomenological description of the observations. Based on Newton’s gravitational law as applied to a uniform continuous mass we posit a non-homogeneous distribution of mass at cosmological scales that would give rise to a constant acceleration that agrees with MOND’s a0. The implications for MOND as a viable theory of dark matter and for the problem of dark energy are discussed.

Comments: 16 Pages. Slightly corrected and improved version, with some necessary references added. Main argument and conclusions unaltered.

Download: PDF

Submission history

[v1] 2023-07-04 17:23:06
[v2] 2023-07-08 21:31:11
[v3] 2023-07-13 00:33:57
[v4] 2023-08-10 08:11:52

Unique-IP document downloads: 459 times

Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.

Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.

comments powered by Disqus