Mass Distribution, Rotation Curves and Gravity Theories
Rahul Datta (Space Applications Centre, Indian Space Research, Organization, Ahmedabad, India), Dilip G. Banhatti (School of Physics,, Madurai-Kamaraj University, Madurai, India)

TL;DR
This study compares galaxy rotation curves with predictions from Newtonian, MoND, and Vacuum Modified Gravity theories to evaluate the necessity of dark matter in explaining galactic mass distributions.
Contribution
It provides a comparative analysis of mass density profiles across multiple galaxies using different gravity theories without dark matter assumptions.
Findings
Newtonian gravity with negative cosmological constant fits some galaxy profiles.
MoND explains rotation curves without dark matter in certain cases.
Vacuum Modified Gravity offers alternative fits to observed data.
Abstract
{Comparison of mass density profiles of galaxies of varying sizes based on some gravity theories from observed galaxy rotation curves and assessing the need for dark matter.} We present an analysis of the rotation curves of five galaxies of varying galactic radii: NGC6822 (4.8 kpc), Large Magellanic Cloud (9 kpc), The Milky Way (17 kpc), NGC3198 (30 kpc) and UGC9133 (102.5 kpc). The mass and mass density profiles of these galaxies have been computed using the scientific computing s/w package MATLAB taking the already available velocity profiles of the galaxies as the input, and without considering any Dark Matter contribution. We have plotted these profiles after computing them according to three different theories of gravity (and dynamics): Newtonian (black line), Modified Newtonian Dynamics (MoND) (green line) and Vacuum Modified Gravity (red line). We also consider how the profile…
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.
Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · History and Developments in Astronomy
