%0 Journal Article
%T Predicting Dark Energy Survey Results within the Haug-Tatum Cosmology Model
%A Eugene Terry Tatum
%A Espen Gaarder Haug
%J Journal of Modern Physics
%P 2220-2227
%@ 2153-120X
%D 2024
%I Scientific Research Publishing
%R 10.4236/jmp.2024.1512089
%X Given the pending completion and publication of the final Dark Energy Survey (DESI) results, this letter presents the corresponding predictions of the Haug-Tatum cosmology (HTC) model. In particular, we show in tabular and graphic form the &#8220;dark energy decay&#8221; curve which the HTC model predicts for cosmological redshifts covering the range of 0 - 2.0 <i>z</i>. Furthermore, we present the HTC model distance-vs-redshift curve in comparison to the three very different curves (for luminosity distance, angular diameter distance, and co-moving distance) calculated within the Lambda-CDM model. Whether the expansion of our universe is actually undergoing slight acceleration or the finely-tuned cosmic coasting at constant velocity of <i>R</i><i><sub>h</sub></i> =<i> ct</i> models, including HTC, will hopefully soon be answered by the many pending observational studies.
%K Haug-Tatum Cosmology
%K Dark Energy
%K Lambda-CDM Cosmology
%K Cosmological Redshift
%K Hubble Parameter
%K Upsilon Constant
%K DESI
%K <i>R</i><i><sub>h</sub></i> =<i> ct </i>Cosmology
%U http://www.scirp.org/journal/PaperInformation.aspx?PaperID=137301