Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Cosmic Entropy Prediction with Extremely High Precision in Rh = ct Cosmology

Version 1 : Received: 17 September 2024 / Approved: 18 September 2024 / Online: 19 September 2024 (12:09:23 CEST)

How to cite: Haug, E.; Tatum, E. Cosmic Entropy Prediction with Extremely High Precision in Rh = ct Cosmology. Preprints 2024, 2024091436. https://doi.org/10.20944/preprints202409.1436.v1 Haug, E.; Tatum, E. Cosmic Entropy Prediction with Extremely High Precision in Rh = ct Cosmology. Preprints 2024, 2024091436. https://doi.org/10.20944/preprints202409.1436.v1

Abstract

We present how the Bekenstein-Hawking entropy of a growing black hole variant of Rh = ct cosmology model can be rewritten as a function of the Cosmic Microwave Background (CMB) radiation temperature or Hubble parameter, rather than the Hubble radius, as first pointed out by Tatum and Seshavatharam [1]. We then show how our CMB temperature formulae lead to much higher precision in the estimated entropy of the Hubble radius universe, since the CMB temperature can be measured with great precision. We also briefly discuss how the Schwarzschild metric can be rewritten as a function of the Bekenstein-Hawking entropy, and how the entropy of the universe can be directly linked to recent estimates of the number of quantum operations in the universe since its beginning.

Keywords

Bekensten-Hawking entropy; black hole entropy; Hubble sphere; CMB temperature

Subject

Physical Sciences, Astronomy and Astrophysics

Comments (0)

We encourage comments and feedback from a broad range of readers. See criteria for comments and our Diversity statement.

Leave a public comment
Send a private comment to the author(s)
* All users must log in before leaving a comment
Views 0
Downloads 0
Comments 0


×
Alerts
Notify me about updates to this article or when a peer-reviewed version is published.
We use cookies on our website to ensure you get the best experience.
Read more about our cookies here.