A possible explanation of Galactic Velocity Rotation Curves in terms of a Cosmological Constant
S. B. Whitehouse, G. V. Kraniotis

TL;DR
This paper proposes that the non-gravitational component of galactic rotation curves can be explained by a negative cosmological constant, challenging dark matter interpretations and linking cosmological parameters to fundamental lengths.
Contribution
It introduces a novel explanation for galactic rotation curves using a negative cosmological constant and connects cosmological parameters to a fundamental length scale.
Findings
The experimental value of the cosmological constant matches the theoretical prediction from the Large Number Hypothesis.
Analysis of galaxy NGC 3198 supports the negative cosmological constant hypothesis.
Results favor a decelerating universe over an accelerating one.
Abstract
This paper describes how the non-gravitational contribution to Galactic Velocity Rotation Curves can be explained in terms of a negative Cosmological Constant (). It will be shown that the Cosmological Constant leads to a velocity contribution proportional to the radii, at large radii, and depending on the mass of the galaxy. This explanation contrasts with the usual interpretation that this effect is due to Dark Matter halos. The velocity rotation curve for the galaxy NGC 3198 will be analysed in detail, while several other galaxies will be studied superficially. The Cosmological Constant derived experimentally from the NGC 3198 data was found to be:. This compares favourably with the theoretical value obtained from the Large Number Hypothesis of: . The Extended LNH is then used to…
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
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
