From the Early Universe to the Modern Universe
The birth of the Universe, its dark components, and the next fundamental level of matter are briefly discussed. The classical cosmological solution for our Universe with a Λ-term has two branches divided by a gap. The quantum process of tunneling between branches took place. A model of a sl...
| Main Author: | |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2020-03-01
|
| Series: | Symmetry |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2073-8994/12/3/382 |
| _version_ | 1798026730496065536 |
|---|---|
| author | V. V. Burdyuzha |
| author_facet | V. V. Burdyuzha |
| author_sort | V. V. Burdyuzha |
| collection | DOAJ |
| description | The birth of the Universe, its dark components, and the next fundamental level of matter are briefly discussed. The classical cosmological solution for our Universe with a Λ-term has two branches divided by a gap. The quantum process of tunneling between branches took place. A model of a slowly swelling Universe in the result of the multiple reproductions of cosmological cycles arises naturally. The occurrence of baryon asymmetry is briefly discussed. The problem of the cosmological constant is solved and, thus, the crisis of physics connected with this constant is overcome. But we note that dark energy is evolving. Dark matter (part or all) consists of familon-type pseudo-Goldstone bosons with a mass of 10<sup>−5</sup>−10<sup>−3</sup> eV. It follows the composite model of particles. This model reproduces three relativistic phase transitions in the medium of familons at different red shifts, forming a large scale structure of the Universe dark matter that was “repeated” by baryons. Here three generations of elementary particles are absolutely necessary. |
| first_indexed | 2024-04-11T18:41:03Z |
| format | Article |
| id | doaj.art-b5a53d226ed24f3fa5e846a323d0d7b2 |
| institution | Directory Open Access Journal |
| issn | 2073-8994 |
| language | English |
| last_indexed | 2024-04-11T18:41:03Z |
| publishDate | 2020-03-01 |
| publisher | MDPI AG |
| record_format | Article |
| series | Symmetry |
| spelling | doaj.art-b5a53d226ed24f3fa5e846a323d0d7b22022-12-22T04:09:00ZengMDPI AGSymmetry2073-89942020-03-0112338210.3390/sym12030382sym12030382From the Early Universe to the Modern UniverseV. V. Burdyuzha0P.N. Lebedev Physical Institute, Russian Academy of Sciences, Leninsky prospect 53, 119991 Moscow, RussiaThe birth of the Universe, its dark components, and the next fundamental level of matter are briefly discussed. The classical cosmological solution for our Universe with a Λ-term has two branches divided by a gap. The quantum process of tunneling between branches took place. A model of a slowly swelling Universe in the result of the multiple reproductions of cosmological cycles arises naturally. The occurrence of baryon asymmetry is briefly discussed. The problem of the cosmological constant is solved and, thus, the crisis of physics connected with this constant is overcome. But we note that dark energy is evolving. Dark matter (part or all) consists of familon-type pseudo-Goldstone bosons with a mass of 10<sup>−5</sup>−10<sup>−3</sup> eV. It follows the composite model of particles. This model reproduces three relativistic phase transitions in the medium of familons at different red shifts, forming a large scale structure of the Universe dark matter that was “repeated” by baryons. Here three generations of elementary particles are absolutely necessary.https://www.mdpi.com/2073-8994/12/3/382early universebaryon asymmetrydark energydark mattercomposite model |
| spellingShingle | V. V. Burdyuzha From the Early Universe to the Modern Universe Symmetry early universe baryon asymmetry dark energy dark matter composite model |
| title | From the Early Universe to the Modern Universe |
| title_full | From the Early Universe to the Modern Universe |
| title_fullStr | From the Early Universe to the Modern Universe |
| title_full_unstemmed | From the Early Universe to the Modern Universe |
| title_short | From the Early Universe to the Modern Universe |
| title_sort | from the early universe to the modern universe |
| topic | early universe baryon asymmetry dark energy dark matter composite model |
| url | https://www.mdpi.com/2073-8994/12/3/382 |
| work_keys_str_mv | AT vvburdyuzha fromtheearlyuniversetothemodernuniverse |