An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling
American Journal of Modern Physics
Volume 6, Issue 6, November 2017, Pages: 148-152
Received: Jun. 4, 2017; Accepted: Jun. 19, 2017; Published: Nov. 10, 2017
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Author
Thomas A. Kriz, Advanced Studies, Alpha Omega Research Foundation, Cedar Park, USA
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Abstract
The initial state of the cosmos is analytically modeled as a radiation filled spherical cavity that expands from a singularity to later act as a clock and energy source in support of a 3-stage, radiation to a quark-hadron based, decoupling process. The model thereby avoids a need for Inflation and the presence of matter at start-up and during the radiation dominated phase, but nevertheless remains strongly consistent with attributes of the Guth Inflationary model. At decoupling, only quark family #1 with up-down attributes has adequate energy to successfully complete decoupling. Earlier in a 3-stage process, attempts at hadronization by quark families #2 and #3 fail due to large quark size and binding energy requirements that exceed the available radiation energy supply. These attempts decay rapidly to take a quark family #1 form. Decoupling is further modeled as half-spin based radiation resonance forms that are linked, via particle time dilation, to matter based micro-black-holes.
Keywords
Cosmic Decoupling, Expanding Radiation Filled Spherical Cavity, Quark Families, Hadron Decay
To cite this article
Thomas A. Kriz, An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling, American Journal of Modern Physics. Vol. 6, No. 6, 2017, pp. 148-152. doi: 10.11648/j.ajmp.20170606.16
Copyright
Copyright © 2017 Authors retain the copyright of this article.
This article is an open access article distributed under the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/) which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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