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. Preprints2024, 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
Haug, E. The Photon Energy Density Parameter Ωγ of the Universe Exactly Derived. Preprints2024, 2024031663. https://doi.org/10.20944/preprints202403.1663.v1
APA Style
Haug, E. (2024). The Photon Energy Density Parameter Ωγ of the Universe Exactly Derived. Preprints. https://doi.org/10.20944/preprints202403.1663.v1
Chicago/Turabian Style
Haug, E. 2024 "The Photon Energy Density Parameter Ωγ of the Universe Exactly Derived" Preprints. 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.