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Applying the Stefan-Boltzmann Law to a Cosmological Model (a Brief Note)
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作者 Eugene Terry Tatum 《Journal of Modern Physics》 2024年第11期1717-1722,共6页
This brief note brings the reader up-to-date with the recent successes of the new Haug-Tatum cosmology model. In particular, the significance of recent proof that the Stefan-Boltzmann law applies to such a model is em... This brief note brings the reader up-to-date with the recent successes of the new Haug-Tatum cosmology model. In particular, the significance of recent proof that the Stefan-Boltzmann law applies to such a model is emphasized and a rationale for this is given. Remarkably, the proposed solutions of this model have incorporated all 580 supernova redshifts in the Union2 database. Therefore, one can usefully apply this thermodynamic law in the form of a continually expanding black-body universe model. To our knowledge, no other cosmological model has achieved such high-precision observational correlation. 展开更多
关键词 Haug-Tatum Cosmology Stefan-Boltzmann Law Flat Space Cosmology CMB Cosmic Thermodynamics rh = ct Cosmology Model Black Body
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Melia’s R<sub>h</sub>= ct Model Is by No Means Flat
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作者 Rainer Burghardt 《Journal of Modern Physics》 2020年第5期703-711,共9页
With the support of numerous arguments, it has been shown that Melia’s claim that his cosmological Rh = ct model is flat and infinite is erroneous. In contrast, the model is positively curved, closed and, therefore, ... With the support of numerous arguments, it has been shown that Melia’s claim that his cosmological Rh = ct model is flat and infinite is erroneous. In contrast, the model is positively curved, closed and, therefore, finite. With respect to results of Melia’s model, it is identical to our Subluminal Model. 展开更多
关键词 Globally and Locally FLAT COSMOS Melia’s rh = ct MODEL SUBLUMINAL MODEL Curvature Parameter
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Local and Global Flatness in Cosmology
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作者 Rainer Burghardt 《Journal of Modern Physics》 2019年第12期1439-1453,共15页
We raise the question of how the curvature parameter k is related to the curvature of the universe. We also show that, for a cosmological model that can be interpreted geometrically as a pseudo-hypersphere with a time... We raise the question of how the curvature parameter k is related to the curvature of the universe. We also show that, for a cosmological model that can be interpreted geometrically as a pseudo-hypersphere with a time-dependent radius, the Einstein field equations are not sufficient to fully describe the model. In addition, the differential equation system of Bianchi identities is required to describe the temporal evolution of the universe. We discuss the facts using the example of the de Sitter universe, the subluminal universe and the Rh=ct model by Melia. In particular, we discuss the formal differences between the two latter models and claim that both models are identical. We also examine the possibility of introducing non-comoving coordinates. 展开更多
关键词 Curvature Parameter Bianchi IDENTITIES de SITTER COSMOS SUBLUMINAL COSMOS rh=ct COSMOS Geometric HORIZON
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How the Dirac Sea Idea May Apply to a Spatially-Flat Universe Model (A Brief Review)
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作者 Eugene Terry Tatum 《Journal of Modern Physics》 2019年第8期974-979,共6页
The famous Dirac sea idea can be resurrected if one replaces the concept of positive and negative matter mass with positive and negative energy. Utilizing this concept, the perpetually spatially-flat matter-generating... The famous Dirac sea idea can be resurrected if one replaces the concept of positive and negative matter mass with positive and negative energy. Utilizing this concept, the perpetually spatially-flat matter-generating FSC model can be shown to be a realistic Milne “empty universe” model. Furthermore, this may be why Rh = ct cosmological models like FSC show an excellent statistical fit with the accumulated data of the Supernova Cosmology Project. 展开更多
关键词 DIRAC SEA DIRAC Equation FLAT Space COSMOLOGY DARK Energy DARK Matter INFLATIONARY COSMOLOGY Supernova COSMOLOGY Project rh = ct Models
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Why Flat Space Cosmology Is Superior to Standard Inflationary Cosmology
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作者 Eugene Terry Tatum 《Journal of Modern Physics》 2018年第10期1867-1882,共16页
Following recent Cosmic Microwave Background (CMB) observations of global spatial flatness, only two types of viable cosmological models remain: inflationary models which almost instantaneously attain cosmic flatness ... Following recent Cosmic Microwave Background (CMB) observations of global spatial flatness, only two types of viable cosmological models remain: inflationary models which almost instantaneously attain cosmic flatness following the Big Bang;and non-inflationary models which are spatially flat from inception. Flat Space Cosmology (FSC) is the latter type of cosmological model by virtue of assumptions corresponding to the Hawking-Penrose conjecture that a universe expanding from a singularity could be modeled like a time-reversed black hole. Since current inflationary models have been criticized for their lack of falsifiability, the numerous falsifiable predictions and key features of the FSC model are herein contrasted with standard inflationary cosmology. For the reasons given, the FSC model is shown to be superior to standard cosmology in the following eleven categories: Predictions Pertaining to Primordial Gravity Waves;Cosmic Dawn Early Surprises;Predicting the Magnitude of CMB Temperature Anisotropy;Predicting the Value of Equation of State Term w;Predicting the Hubble Parameter Value;Quantifiable Entropy and the Entropic Arrow of Time;Clues to the Nature of Gravity, Dark Energy and Dark Matter;The Cosmological Constant Problem;Quantum Cosmology;Dark Matter and Dark Energy Quantitation;Requirements for New Physics. 展开更多
关键词 COSMOLOGY Theory COSMIC INFLATION Dark Energy COSMIC FLATNESS CMB Anisotropy COSMIC Entropy Emergent Gravity Black Holes FSC COSMIC DAWN rh = ct Model
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