A Historical Review of Research on the Density-Size Correlation of the Observable Universe
DOI:
https://doi.org/10.47611/jsrhs.v12i4.5780Keywords:
Fractal Cosmology, Density, Density-Size Correlation, Density-Radius Correlation, E.F. Carpenter, Gerard De Vaucouleurs, De Sitter Model, Olber's Paradox, Universe, Homogeneous Universe, Hierarchical UniverseAbstract
This literature review explores the correlation between the density and size of celestial objects - a key subject in understanding their formation, evolution, and the potential existence of higher-order clusters. It draws attention to the two seminal papers - E. F. Carpenter's density-size correlation study and Gerard De Vaucouleurs's study on matter density in groups and clusters. While acknowledging the limitations and outdated nature of Carpenter's body of work, it underscores the need for a more contemporary, comprehensive examination across various scales from neutron stars to galaxy clusters. The review highlights how such a study can clarify questions surrounding the size and shape of the universe, address Olbers' Paradox, and contribute to theories that describe the universe's origins and dynamics.
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Carpenter, E. F. (1938, October). Some Characteristics of Associated Galaxies. I. a. Density Restriction in the Metagalaxy. The Astrophysical Journal, 88(344). https://doi.org/10.1086/143987
De Vaucouleurs, G. (1960, May). The Apparent Density of Matter in Groups and Clusters of Galaxies. The Astrophysical Journal, 131(585). https://doi.org/10.1086/146871
De Vaucouleurs, G. (1970). The Case for a Hierarchical Cosmology. Science, 167(3922), 1203–1213. http://www.jstor.org/stable/1728457. https://doi.org/10.1126/science.167.3922.1203
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Copyright (c) 2023 Thomas Thomas, Nipun Nagendra, Sreekar Garimella; Shyamal Mitra
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