Submitted:
15 October 2024
Posted:
21 October 2024
You are already at the latest version
Abstract
This paper provides a brief overview of how the Haug and Tatum Cosmological Model (HTC) outperforms the Λ-CDM model in numerous categories. In particular, we show why the HTC model is a strong competitor to the Λ-CDM model. For example, HTC appears to resolve the Hubble tension by making use of newly-discovered fundamental relationships between the CMB temperature, the Hubble parameter, and cosmological redshift. Moreover, HTC appears to better explain certain early universe telescopic observations than the Λ-CDM model.
Keywords:
1. The Haug and Tatum Cosmological Model
2. -CDM Cannot Predict Current CMB Temperature, Whereas HTC Can Precisely Predict
“The present theory is, however, unable to predict the value of T at . It is therefore a free parameter in SC (Standard Cosmology)."
3. -CDM Cannot Derive , Whereas HTC Does So
4. -CDM Cannot Yet Resolve the Hubble Tension, Whereas HTC Appears to Resolve the Hubble Tension
5. -CDM Has Much Higher Uncertainty in Comparison to HTC in Measured
6. HTC Provides for Markedly Increased Precision in Predictions of a Series of Cosmological Parameters
7. -CDM Operates with Three Different Distances for a Given Red-Shift, Whereas They Are Unified in HTC
8. -CDM Appears to Be Less Compatible with Recent Early Universe Observations than HTC
“JWST’s recent discovery of well-formed galaxies and supermassive black holes only a few hundred million years after the Big Bang seriously challenges the timeline predicted by Λ-CDM,"
9. HTC Is Consistent with both the Standard Friedmann Equation and Our Thermodynamic Friedmann Equation, Whereas -CDM Has No Solid Mathematical Foundation Relating CMB Temperature with Other Cosmic Parameters
10. -CDM Has Horizon Problems, Whereas HTC Has No Horizon Problem
11. Summary and Conclusions
References
- E. G. Haug and E. T. Tatum. Solving the Hubble tension using the Union2 supernova database. Preprints.org, 2024. [CrossRef]
- A. Friedmann. Über die krüng des raumes. Zeitschrift für Physik, 1922; 10, 377. [CrossRef]
- A. Einstein. Näherungsweise integration der feldgleichungen der gravitation. Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften Berlin, 1916.
- Dhal, S. Singh, K. Konar, and R. K. Paul. Calculation of cosmic microwave background radiation parameters using cobe/firas dataset. Experimental Astronomy (2023), 56:715, 2023. [CrossRef]
- J. V. Narlikar and T. Padmanabhan. Standard cosmology and alternatives: A critical appraisal. Annual Review of Astronomy and Astrophysics, 1979; 39, 211. [CrossRef]
- E. T. Tatum, U. V. S. E. T. Tatum, U. V. S. Seshavatharam, and S. Lakshminarayana. The basics of flat space cosmology. International Journal of Astronomy and Astrophysics, 2015; 5, 116. [Google Scholar] [CrossRef]
- E. G. Haug and S. Wojnow. How to predict the temperature of the CMB directly using the Hubble parameter and the Planck scale using the Stefan-Boltzman law. Journal of Applied Physics and Mathematics, accepted and forthcoming, 2024. [CrossRef]
- E. G. Haug and E. T. Tatum. The Hawking Hubble temperature as a minimum temperature, the Planck temperature as a maximum temperature and the CMB temperature as their geometric mean temperature. Journal of Applied Physics and Mathematics (accepted and forthcoming), 2024.
- I. de Martino et. al. Measuring the redshift dependence of the cosmic microwave background monopole temperature with planck data. The Astrophysical Journal, 2012; 757, 144. [CrossRef]
- L. Yunyang. Constraining cosmic microwave background temperature evolution with sunyaev–zel’dovich galaxy clusters from the atacama cosmology telescope. The Astrophysical Journal, 2021; 922, 136. [CrossRef]
- D.A. Riechers, A. D.A. Riechers, A. Weiss, and F. et al. Walter. Microwave background temperature at a redshift of 6.34 from h2o absorption. Nature, 2022; 602, 58. [Google Scholar] [CrossRef]
- E. Valentino et. al. In the realm of the Hubble tension – a review of solutions. Classical and Quantum Gravity, 2021; 38, 153001. [CrossRef]
- E. G. Haug. Closed form solution to the Hubble tension based on Rh=ct cosmology for generalized cosmological redshift scaling of the form: z=(Rh/Rt)x-1 tested against the full distance ladder of observed SN Ia redshift. Preprints.org, 2024. [CrossRef]
- E. G. Haug and E. T. Tatum. Planck length from cosmological redshifts solves the Hubble tension. ResearchGate.org, 2024. [CrossRef]
- N. Aghanim et al. (the Planck Collaboration). Planck 2018 results. vi. cosmological parameters. Astronomy & Astrophysics, 2021; 652. [CrossRef]
- A. G. Riess et. al. A comprehensive measurement of the local value of the Hubble constant with 1 km s-1 Mpc-1 uncertainty from the Hubble space telescope and the sh0es team. The Astrophysical Journal, 2021; 934. [CrossRef]
- E. T. Tatum, E. G. E. T. Tatum, E. G. Haug, and S. Wojnow. High precision Hubble constant determinations based upon a new theoretical relationship between CMB temperature and H0. Journal of Modern Physics, Accepted and forthcoming. Pre-print version at Hal-archive, 2024. [Google Scholar]
- E. T. Tatum. Upsilon constants and their usefulness in Planck scale quantum cosmology. Journal of Modern Physics, 2024; 15, 167. [CrossRef]
- E. T. Tatum and E. G. Haug. Extracting a cosmic age of 14.6 billion years from all 580 type Ia supernova redshifts in the Union2 database. ResearchGate.org, 2024. [CrossRef]
- E. G. Haug and E. T. Tatum. How a thermodynamic version of the Friedmann equation appears to solve the early galaxy formation problem. PrePrints.org, 2024. [CrossRef]
- E. G. Haug and E. T. Tatum. Friedmann type equations in thermodynamic form lead to much tighter constraints on the critical density of the universe. https://www.preprints.org/manuscript/202403.1241/v2. 2024.
- E. G. Haug and E. T. Tatum. Cosmic entropy prediction with extremely high precision in Rh=ct cosmology. Preprints.org, 2024. [CrossRef]
- F. Melia. Strong observational support for the Rh=ct timeline in the early universe. Physics of the Dark Universe, 2024; 46, 101587. [CrossRef]
- F. Melia and Shevchuk A. S. H. The Rh=ct universe. Monthly Notices of the Royal Astronomical Society, 2012; 419, 2579. [CrossRef]
- F. Melia. A solution to the electroweak horizon problem in the Rh=ct universe. Eur. Phys. J. 2018; 78, 739. [CrossRef]

| Property: | Formula: | References |
|---|---|---|
| Hubble constant | [1,17] | |
| Hubble radius | ||
| Hubble time | years | [19,20] |
| Critical density | [21] | |
| Cosmic Hubble sphere entropy | [22] |
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content. |
© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).