UV surface brightness of galaxies from the local Universe to z ~ 5
Eric J. Lerner, Renato Falomo, Riccardo Scarpa

TL;DR
This study analyzes UV surface brightness of galaxies from the local universe to z ~ 5, finding it remains constant, supporting a static Euclidean universe model over the expanding universe paradigm.
Contribution
It demonstrates that galaxy surface brightness data are consistent with a static Euclidean universe, challenging the standard cosmological model.
Findings
Surface brightness remains constant up to z ~ 5
Data supports a static Euclidean universe model
Re-analysis confirms previous lower-redshift results
Abstract
The Tolman test for surface brightness dimming was originally proposed as a test for the expansion of the Universe. The test, which is independent of the details of the assumed cosmology,is based on comparisons of the surface brightness (SB) of identical objects at different cosmological distances. Claims have been made that the Tolman test provides compelling evidence against a static model for the Universe. In this paper we reconsider this subject by adopting a static Euclidean Universe with a linear Hubble relation at all z (which is not the standard Einstein- de Sitter model),resulting in a relation between flux and luminosity that is virtually indistinguishable from the one used for LCDM models. Based on the analysis of the UV surface brightness of luminous disk galaxies from HUDF and GALEX datasets, reaching from the local Universe to z ~ 5 we show that the surface brightness…
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