Predicting Dark Energy Survey Results Using the Flat Space Cosmology Model

HTML  XML Download Download as PDF (Size: 393KB)  PP. 1083-1089  
DOI: 10.4236/jmp.2019.109070    506 Downloads   1,240 Views  Citations

ABSTRACT

The Flat Space Cosmology (FSC) model is utilized to show how this model predicts the value of the Hubble parameter at each epoch of cosmic expansion. Specific attention in this paper is given to correlating the observable galactic redshifts since the beginning of the “cosmic dawn” reionization epoch. A graph of the log of the Hubble parameter as a function of redshift z is presented as the FSC prediction of the pending Dark Energy Survey results. In the process, it is discovered that the obvious tension between the SHOES local Hubble constant value and the 2018 Planck Survey and the 2018 Dark Energy Survey global Hubble constant values may be explained by a time-variable, scalar, Hubble parameter acting in accordance with the FSC model.

Share and Cite:

Tatum​, E. and Seshavatharam, U. (2019) Predicting Dark Energy Survey Results Using the Flat Space Cosmology Model. Journal of Modern Physics, 10, 1083-1089. doi: 10.4236/jmp.2019.109070.

Copyright © 2024 by authors and Scientific Research Publishing Inc.

Creative Commons License

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.