Cosmology and galactic rotation curves
Astrophysics
2016-08-30 v1
Abstract
We explore the possibility that the entire departure of galactic rotational velocities from their luminous Newtonian expectation be cosmological in origin, and show that within the framework of conformal gravity (but not Einstein gravity apparently) every static observer sees the overall Hubble flow as a local universal linear potential which is able to account for available data without any need for dark matter. We find that the Universe is necessarily an open one with 3-space scalar curvature given by cm.
Cite
@article{arxiv.astro-ph/9511045,
title = {Cosmology and galactic rotation curves},
author = {Philip D. Mannheim},
journal= {arXiv preprint arXiv:astro-ph/9511045},
year = {2016}
}
Comments
Plain TeX, 10 pages, plus one requestable hard copy figure (requests to mannheim@uconnvm.uconn.edu)