dorsal/arxiv
View SchemaCosmological pressure fluctuations and spatial expansion
| Authors | Dale R. Koehler |
|---|---|
| Categories | |
| ArXiv ID | physics/0508136 |
| URL | https://arxiv.org/abs/physics/0508136 |
| Journal | Benton, C. V. Trends in General Relativity and Quantum Cosmology; Nova Science, Publishers: New York, 2006, vol 253,chapter 7 |
Abstract
Most recently, experimental determinations of the spectrometric characteristics and internal structural velocities of galaxies have suggested the presence of massive central black holes. In the present work, we examine whether conditions existed in the early universe, that could have led to the formation of gravitational structures possessing such unusual characteristics. We propose an early-time pressure-fluctuation model, which would have generated a radiation based energy distribution possessing the characteristic of a centrally collapsed zone isolated from its surrounding environment and thereby manifesting such a black hole behavior. Einstein's gravitational equations are assumed to apply within the radiation-dominated hole-core spatial domain and, with utilization of a spherically symmetric isotropic metric, are used in order to calculate the evolutionary time expansion characteristics. Birth times for the radiation structures are uniquely correlated with the size of the spheres and are primarily determined from the early time energy densities and the apparent curvatures presented by the gravitational equations. The model displays an early time pressure fluctuation collapse, tentatively interpreted to be the formation of a galaxy hole, and therein provides a theoretical basis for the experimental data.
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"abstract": "Most recently, experimental determinations of the spectrometric\ncharacteristics and internal structural velocities of galaxies have suggested\nthe presence of massive central black holes. In the present work, we examine\nwhether conditions existed in the early universe, that could have led to the\nformation of gravitational structures possessing such unusual characteristics.\nWe propose an early-time pressure-fluctuation model, which would have generated\na radiation based energy distribution possessing the characteristic of a\ncentrally collapsed zone isolated from its surrounding environment and thereby\nmanifesting such a black hole behavior. Einstein\u0027s gravitational equations are\nassumed to apply within the radiation-dominated hole-core spatial domain and,\nwith utilization of a spherically symmetric isotropic metric, are used in order\nto calculate the evolutionary time expansion characteristics. Birth times for\nthe radiation structures are uniquely correlated with the size of the spheres\nand are primarily determined from the early time energy densities and the\napparent curvatures presented by the gravitational equations. The model\ndisplays an early time pressure fluctuation collapse, tentatively interpreted\nto be the formation of a galaxy hole, and therein provides a theoretical basis\nfor the experimental data.",
"arxiv_id": "physics/0508136",
"authors": [
"Dale R. Koehler"
],
"categories": [
"physics.gen-ph"
],
"journal_ref": "Benton, C. V. Trends in General Relativity and Quantum Cosmology;\n Nova Science, Publishers: New York, 2006, vol 253,chapter 7",
"title": "Cosmological pressure fluctuations and spatial expansion",
"url": "https://arxiv.org/abs/physics/0508136"
},
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