The origin of the MOND critical acceleration scale
David Roscoe

TL;DR
This paper explores the fundamental origin of the MOND critical acceleration scale, proposing it is linked to a quasi-fractal universe structure with a characteristic acceleration, unifying it with the scale derived from the intergalactic medium.
Contribution
It presents a theoretical framework connecting the MOND acceleration scale to a quasi-fractal universe model, explaining its origin through geometric and mass distribution considerations.
Findings
$a_0$ and $a_F$ are shown to be equivalent.
The scaling relationship reproduces the Baryonic Tully-Fisher relation.
$a_F$ is explicitly embedded in galaxy data.
Abstract
The irrefutable successes of MOND are predicated upon the idea that a critical gravitational acceleration scale, , exists. But, beyond its role in MOND, the question: 'Why should a critical gravitational acceleration scale exist at all?' remains unanswered. There is no deep understanding about what is going on. Over roughly the same period that MOND has been a topic of controversy, Baryshev, Sylos Labini, Pietronero and others have been arguing, with equal controversy in earlier years, that, on medium scales at least, material in the universe is distributed in a quasi-fractal fashion. There is a link: if the idea of a quasi-fractal universe on medium scales is taken seriously then there is an associated characteristic mass surface density scale, say, and an associated characteristic gravitational acceleration scale, .…
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Taxonomy
TopicsRelativity and Gravitational Theory · Cosmology and Gravitation Theories · Advanced Mathematical Theories and Applications
