The $\kappa$-model, a minimal model alternative to dark matter. Application to the galactic rotation problem
G.Pascoli

TL;DR
The paper introduces the ppa-model, a minimal alternative to dark matter, which explains galactic rotation curves by environmental effects, showing equivalence with MOND and challenging the dark matter paradigm.
Contribution
It proposes the ppa-model as a novel, environment-based approach to galactic dynamics, offering an alternative to dark matter and establishing equivalence with MOND.
Findings
ppa-model can mimic MOND effects in galaxy rotation
The model offers an environment-dependent explanation for gravitational phenomena
It questions the necessity of dark matter in explaining galactic rotation
Abstract
The determination of the velocities, accelerations and the gravitational field intensity at a given location in a galaxy could potentially be achieved in an unexpected manner with the environment of the observer, for instance, the local mean mass density in the galaxy. This idea, mathematically supported by the asymmetric distance concept, is illustrated here by a study regarding the rotation of spiral galaxies. This suggestion is new in the astrophysics field (in the following, it is called the \k{appa}-model) and could help to mimic the main effects seen in modified Newtonian dynamics (MOND) theory, modified gravity (MOG) models, or other related models built with the aim of eliminating dark matter that are already well-established theories. Thus, starting from two selected examples of galaxies, in section 5, we show that there is an equivalence between MOND and the \k{appa}-model. In…
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.
