Article
Version 1
Preserved in Portico This version is not peer-reviewed
The Photon Energy Density Parameter Ωγ of the Universe Exactly Derived
Version 1
: Received: 26 March 2024 / Approved: 27 March 2024 / Online: 27 March 2024 (14:17:57 CET)
How to cite: Haug, E. The Photon Energy Density Parameter Ωγ of the Universe Exactly Derived. Preprints 2024, 2024031663. https://doi.org/10.20944/preprints202403.1663.v1 Haug, E. The Photon Energy Density Parameter Ωγ of the Universe Exactly Derived. Preprints 2024, 2024031663. https://doi.org/10.20944/preprints202403.1663.v1
Abstract
We will demonstrate that the photon energy density parameter Ωγ of the universe can be derived exactly in Rh = ct cosmology. We find that it must be Ωγ = 1/5760π ≈ 5.52621330180192× 10^(−5). This indicates that there is no uncertainty in the radiation density within at least somesub-classes of Rh = ct cosmology.
Keywords
Photon energy density parameter; Friedmann equation; critical density; Thermodynamical Friedmann equation
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.
Comments (0)
We encourage comments and feedback from a broad range of readers. See criteria for comments and our Diversity statement.
Leave a public commentSend a private comment to the author(s)
* All users must log in before leaving a comment