Angular size test on the expansion of the Universe
Martin Lopez-Corredoira

TL;DR
This paper examines galaxy angular sizes across redshifts under various cosmological models, proposing a static universe model that fits the data well without requiring strong size evolution or additional parameters.
Contribution
It introduces a simple static universe model that explains galaxy size and supernova data without ad hoc parameters, challenging standard cosmological assumptions.
Findings
A static universe model fits angular size vs. redshift data well.
The model explains supernova Hubble diagram without extra parameters.
Weak size evolution is compatible with observational data.
Abstract
Assuming the standard cosmological model as correct, the average linear size of galaxies with the same luminosity is six times smaller at z=3.2 than at z=0, and their average angular size for a given luminosity is approximately proportional to 1/z. Neither the hypothesis that galaxies which formed earlier have much higher densities nor their luminosity evolution, mergers ratio, or massive outflows due to a quasar feedback mechanism are enough to justify such a strong size evolution. Also, at high redshift, the intrinsic ultraviolet surface brightness would be prohibitively high with this evolution, and the velocity dispersion much higher than observed. We explore here another possibility to overcome this problem by considering different cosmological scenarios that might make the observed angular sizes compatible with a weaker evolution. One of the models explored, a very simple…
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 · Gamma-ray bursts and supernovae · Astronomy and Astrophysical Research
