Can Massive Gravity Explain the Mass Discrepancy - Acceleration Relation of Disk Galaxies?
Sascha Trippe (SNU Seoul)

TL;DR
This paper evaluates whether a gravity model based on massive gravitons can explain the observed mass discrepancy-acceleration relation in disk galaxies, finding it fits the data well and aligns with observed galactic dynamics.
Contribution
It introduces a graviton-based modified gravity model that successfully predicts the MDA relation, providing a potential alternative to dark matter explanations.
Findings
The 'simple mu' function fits the MDA data well.
The best-fit Milgrom's constant is approximately 1.06 x 10^-10 m/s^2.
The graviton picture explains galactic dynamics across a wide range of scales.
Abstract
The empirical mass discrepancy-acceleration (MDA) relation of disk galaxies provides a key test for models of galactic dynamics. In terms of modified laws of gravity and/or inertia, the MDA relation quantifies the transition from Newtonian to modified dynamics at low centripetal accelerations a_c < 10^-10 m/s^2. As yet, neither dynamical models based on dark matter nor proposed modifications of the laws of gravity/inertia have predicted the functional form of the MDA relation. In this work, I revisit the MDA data and compare them to four different theoretical scaling laws. Three of these scaling laws are entirely empirical, the fourth one - the "simple mu" function of Modified Newtonian Dynamics - derives from a toy model of gravity based on massive gravitons (the "graviton picture"). All theoretical MDA relations comprise one free parameter of the dimension of an acceleration,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
