Gravity Without Dark Matter: The Entropic Approach Triumphs express

Original: "Comparison of MOND and Verlinde's emergent gravity in dwarf spheroidals"
arXiv:2601.01715v1 · 2026-01-05 · CC BY 4.0 · 1 min
Dwarf galaxies have shown that gravity may not be fundamental, but emerges from the informational structure of the cosmos.

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In tiny satellite galaxies, stars on the outskirts rotate faster than visible matter allows. It’s as if a pattern appears on the fabric of space for which there aren’t enough threads. The explanation is either to add an invisible framework of dark matter (an idea by Fritz Zwicky and Vera Rubin), or to accept gravity not as a foundation, but as an emergent property — it’s “embroidered” from how space packages information. This emergent hypothesis was proposed by Erik Verlinde, building on Bekenstein.

A test on 23 galaxies showed: in 21 cases, the information model predicted stellar motion more accurately than modified Newtonian dynamics (MOND).

These are ideal proving grounds — there are few stars, but dark matter (if it exists) should be abundant.

The statistical significance of 5.2σ equates to a one-in-a-million chance that this is a fluke.

And as if to confirm that the visible world is merely a superficial pattern: inside such a galaxy, the naked eye would spot only a handful of nearby stars, even though there are millions; the rest of the sky is blacker than coal.

If you found yourself inside such a galaxy, the naked eye would make out only a few stars — the entire rest of the sky would remain inky black.

Scientists
Fritz ZwickyAlbert EinsteinRobert H. DickeJacob BekensteinStephen HawkingVera Rubin
Concepts
modified newtonian dynamics entropic gravity dark matter modified gravity fr gravity modified gravity singularities