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A Possible Role of the Energetically Excited Quantum Vacuum in Cosmology:A Potential Solution to the Horizon and Flatness Problems–The Excitation Energy Dominated Era
Version 1
: Received: 27 December 2022 / Approved: 28 December 2022 / Online: 28 December 2022 (12:46:45 CET)
How to cite:
Marosi, L. A Possible Role of the Energetically Excited Quantum Vacuum in Cosmology:A Potential Solution to the Horizon and Flatness Problems–The Excitation Energy Dominated Era. Preprints2022, 2022120545. https://doi.org/10.20944/preprints202212.0545.v1
Marosi, L. A Possible Role of the Energetically Excited Quantum Vacuum in Cosmology:A Potential Solution to the Horizon and Flatness Problems–The Excitation Energy Dominated Era. Preprints 2022, 2022120545. https://doi.org/10.20944/preprints202212.0545.v1
Marosi, L. A Possible Role of the Energetically Excited Quantum Vacuum in Cosmology:A Potential Solution to the Horizon and Flatness Problems–The Excitation Energy Dominated Era. Preprints2022, 2022120545. https://doi.org/10.20944/preprints202212.0545.v1
APA Style
Marosi, L. (2022). A Possible Role of the Energetically Excited Quantum Vacuum in Cosmology:A Potential Solution to the Horizon and Flatness Problems–The Excitation Energy Dominated Era. Preprints. https://doi.org/10.20944/preprints202212.0545.v1
Chicago/Turabian Style
Marosi, L. 2022 "A Possible Role of the Energetically Excited Quantum Vacuum in Cosmology:A Potential Solution to the Horizon and Flatness Problems–The Excitation Energy Dominated Era" Preprints. https://doi.org/10.20944/preprints202212.0545.v1
Abstract
The cosmological model presented here rests on the postulate that the universe can be described as an interacting attraction (exerted by matter) and repulsion (exerted by the excitation energy of the quantum vacuum) system in virial equilibrium. The basic parameters of the model, the matter density and the excitation energy of the quantum vacuum are determined by observations and are not adjusted to the model. The model requires only a few assumptions that can be deduced from the laws of conventional physics and from the rules of quantum field theory. Existing problems in standard cosmology, such as the flatness and the horizon problems, among others, can be resolved in a straightforward way without inflation and without recourse to dark matter and dark energy.
Copyright:
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
