The $a_0$ -- cosmology connection in MOND
Mordehai Milgrom

TL;DR
This paper reviews the intriguing numerical coincidence between the MOND acceleration constant and cosmological parameters, exploring its implications and potential clues to a fundamental underlying theory called FUNDAMOND.
Contribution
It highlights the MOND-$a_0$ and cosmological parameter coincidence, discussing its phenomenological consequences and possible insights into a fundamental MOND theory.
Findings
The near equality of $a_0$ and cosmological parameters has significant phenomenological implications.
This coincidence suggests a deeper connection between local galactic dynamics and cosmology.
Analogies with other physical systems may help explain the MOND coincidence.
Abstract
I limelight and review a potentially crucial aspect of MOND: The near equality of the MOND acceleration constant, -- as deduced from local, galactic phenomena -- and cosmological parameters. To wit, , where is the present value of the Hubble-Lema\^{i}tre constant, is the `cosmological constant', and is a cosmological characteristic length; e.g., the Hubble distance, or the de Sitter radius associated with . In itself, this near equality has some important phenomenological consequences, such as the impossibility of black holes, and of cosmological strong lensing, in the MOND regime. More importantly perhaps, this `coincidence' may be a pointer to the `FUNDAMOND' -- the more basic theory underlying MOND phenomenology. The manners in which such a relation emerges in existing, underlying scheme of…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Black Holes and Theoretical Physics
