Article
Version 2
This version is not peer-reviewed
The CMB Luminosity Distance and Cosmological Redshifts
Version 1
: Received: 28 September 2024 / Approved: 30 September 2024 / Online: 30 September 2024 (17:13:24 CEST)
Version 2 : Received: 9 October 2024 / Approved: 10 October 2024 / Online: 10 October 2024 (08:29:41 CEST)
Version 2 : Received: 9 October 2024 / Approved: 10 October 2024 / Online: 10 October 2024 (08:29:41 CEST)
How to cite: Haug, E. The CMB Luminosity Distance and Cosmological Redshifts. Preprints 2024, 2024092443. https://doi.org/10.20944/preprints202409.2443.v2 Haug, E. The CMB Luminosity Distance and Cosmological Redshifts. Preprints 2024, 2024092443. https://doi.org/10.20944/preprints202409.2443.v2
Abstract
We will outline the relationship between luminosity distance and cosmological redshifts, demonstrating that it is consistent with a new cosmological model recently proposed by Haug and Tatum [1], which appears to resolve the Hubble tension within the Rh = ct cosmology.
Keywords
Luminosity distance, angular distance and co-moving distance.
Subject
Physical Sciences, Astronomy and Astrophysics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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