An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling

Thomas A. Kriz

doi:doi:10.11648/j.ajmp.20170606.16

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An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling

Thomas A. Kriz

Published in American Journal of Modern Physics (Volume 6, Issue 6)

Received: 4 June 2017 Accepted: 19 June 2017 Published: 10 November 2017

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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.

Published in	American Journal of Modern Physics (Volume 6, Issue 6)
DOI	10.11648/j.ajmp.20170606.16
Page(s)	148-152
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2017. Published by Science Publishing Group

Keywords

Cosmic Decoupling, Expanding Radiation Filled Spherical Cavity, Quark Families, Hadron Decay

References

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Thomas A. Kriz. (2017). An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling. American Journal of Modern Physics, 6(6), 148-152. https://doi.org/10.11648/j.ajmp.20170606.16

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ACS Style

Thomas A. Kriz. An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling. Am. J. Mod. Phys. 2017, 6(6), 148-152. doi: 10.11648/j.ajmp.20170606.16

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Thomas A. Kriz. An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling. Am J Mod Phys. 2017;6(6):148-152. doi: 10.11648/j.ajmp.20170606.16

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@article{10.11648/j.ajmp.20170606.16,
  author = {Thomas A. Kriz},
  title = {An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling},
  journal = {American Journal of Modern Physics},
  volume = {6},
  number = {6},
  pages = {148-152},
  doi = {10.11648/j.ajmp.20170606.16},
  url = {https://doi.org/10.11648/j.ajmp.20170606.16},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajmp.20170606.16},
  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.},
 year = {2017}
}

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TY  - JOUR
T1  - An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling
AU  - Thomas A. Kriz
Y1  - 2017/11/10
PY  - 2017
N1  - https://doi.org/10.11648/j.ajmp.20170606.16
DO  - 10.11648/j.ajmp.20170606.16
T2  - American Journal of Modern Physics
JF  - American Journal of Modern Physics
JO  - American Journal of Modern Physics
SP  - 148
EP  - 152
PB  - Science Publishing Group
SN  - 2326-8891
UR  - https://doi.org/10.11648/j.ajmp.20170606.16
AB  - 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.
VL  - 6
IS  - 6
ER  -

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Author Information

Thomas A. Kriz

Advanced Studies, Alpha Omega Research Foundation, Cedar Park, USA

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Thomas A. Kriz. (2017). An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling. American Journal of Modern Physics, 6(6), 148-152. https://doi.org/10.11648/j.ajmp.20170606.16

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ACS Style

Thomas A. Kriz. An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling. Am. J. Mod. Phys. 2017, 6(6), 148-152. doi: 10.11648/j.ajmp.20170606.16

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AMA Style

Thomas A. Kriz. An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling. Am J Mod Phys. 2017;6(6):148-152. doi: 10.11648/j.ajmp.20170606.16

Copy | Download

@article{10.11648/j.ajmp.20170606.16,
  author = {Thomas A. Kriz},
  title = {An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling},
  journal = {American Journal of Modern Physics},
  volume = {6},
  number = {6},
  pages = {148-152},
  doi = {10.11648/j.ajmp.20170606.16},
  url = {https://doi.org/10.11648/j.ajmp.20170606.16},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajmp.20170606.16},
  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.},
 year = {2017}
}

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TY  - JOUR
T1  - An Energy Based Analysis of the Quark/Hadron Impact on Cosmic Decoupling
AU  - Thomas A. Kriz
Y1  - 2017/11/10
PY  - 2017
N1  - https://doi.org/10.11648/j.ajmp.20170606.16
DO  - 10.11648/j.ajmp.20170606.16
T2  - American Journal of Modern Physics
JF  - American Journal of Modern Physics
JO  - American Journal of Modern Physics
SP  - 148
EP  - 152
PB  - Science Publishing Group
SN  - 2326-8891
UR  - https://doi.org/10.11648/j.ajmp.20170606.16
AB  - 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.
VL  - 6
IS  - 6
ER  -

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