MOND disproved at large scales

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SUMMARY

The paper on arXiv (2604.14327) presents evidence disproving Modified Newtonian Dynamics (MOND) at large cosmological scales based on galaxy cluster velocity measurements shown in Figures 1 and 2. MOND, originally formulated to explain galaxy rotation curves without dark matter, fails to account for mass discrepancies at the galaxy cluster and inter-cluster scales, reaffirming its known "missing mass" problem. The discussion confirms that MOND cannot be universally scale-independent, as it requires additional mass components such as sterile neutrinos or alternative dark matter candidates to reconcile observations at larger scales. Recent theoretical extensions like the Skordis-Zlosnik framework and new mass distribution ansatzes proposed by Pavel Kroupa's group aim to address these shortcomings but remain to be validated against the new data.

PREREQUISITES

  • Modified Newtonian Dynamics (MOND) theoretical framework
  • Galaxy cluster velocity dispersion measurements
  • Dark matter candidates: sterile neutrinos and alternative models
  • Skordis-Zlosnik relativistic MOND theories

NEXT STEPS

  • Study the Skordis-Zlosnik relativistic MOND theory (reference 64 in the paper)
  • Analyze Pavel Kroupa's alternative mass distribution ansatz for galaxy clusters
  • Investigate sterile neutrino dark matter models as supplements to MOND
  • Examine large-scale structure velocity measurements and their implications for gravity theories

USEFUL FOR

Astrophysicists, cosmologists, and theoretical physicists researching gravity modifications, dark matter alternatives, and galaxy cluster dynamics will benefit from this discussion. It is essential for those evaluating the viability of MOND and its extensions in explaining large-scale cosmic structures.

timmdeeg
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https://arxiv.org/pdf/2604.14327

Fig.1 and Fig.2 seem to show that MOND is disproved at large scales due to measurements of galaxy cluster velocities.

Supposed this holds, is it thinkable at all that MOND could be still true at galaxy scales?
 
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MOND is just fitting a curve to data. As such it can't be proved or disproved.
 
So is MOND a theoretical framework which makes predictions? If yes, should this framework hold scale independent?

In other words would you agree that either Gravity is modified or it isn't?
 
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It's standard MOND lore that MOND doesn't quite work for galaxy clusters - it has its own "missing mass" problem, or need for dark matter, on the cluster scale. This paper is actually extending that result to an even bigger, inter-cluster scale.

So one way to maintain MOND is to say that there is some extra mass there - sterile neutrinos, some other kind of dark matter (e.g. the Skordis-Zlosnik theorym ref 64 in this paper). There is also a recent paper coauthored by Pavel Kroupa arguing that they have found the MOND missing mass of galaxy clusters by using a different ansatz for inferring the distribution of cluster mass. Part of the MOND response to this paper, therefore, will be to see if either of these approaches can be scaled up to account for the new results.
 
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