Electroweak Phase Transitions in Einstein’s Static Universe
We suggest using Einstein’s static universe metric for the metastable state after reheating, instead of the Friedman-Robertson-Walker spacetime. In this case, strong static gravitational potential leads to the effective reduction of the Higgs vacuum expectation value, which is found to be compatible...
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| Format: | Article |
| Language: | English |
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Wiley
2018-01-01
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| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2018/4653202 |
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| _version_ | 1832549414259916800 |
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| author | M. Gogberashvili |
| author_facet | M. Gogberashvili |
| author_sort | M. Gogberashvili |
| collection | DOAJ |
| description | We suggest using Einstein’s static universe metric for the metastable state after reheating, instead of the Friedman-Robertson-Walker spacetime. In this case, strong static gravitational potential leads to the effective reduction of the Higgs vacuum expectation value, which is found to be compatible with the Standard Model first-order electroweak phase transition conditions. Gravity could also increase the CP-violating effects for particles that cross the new phase bubble walls and thus is able to lead to the successful electroweak baryogenesis scenario. |
| format | Article |
| id | doaj-art-f58f04e2ab9f48f59c568f73fb31241e |
| institution | Kabale University |
| issn | 1687-7357 1687-7365 |
| language | English |
| publishDate | 2018-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| spelling | doaj-art-f58f04e2ab9f48f59c568f73fb31241e2025-02-03T06:11:26ZengWileyAdvances in High Energy Physics1687-73571687-73652018-01-01201810.1155/2018/46532024653202Electroweak Phase Transitions in Einstein’s Static UniverseM. Gogberashvili0Javakhishvili Tbilisi State University, 3 Chavchavadze Avenue, 0179 Tbilisi, GeorgiaWe suggest using Einstein’s static universe metric for the metastable state after reheating, instead of the Friedman-Robertson-Walker spacetime. In this case, strong static gravitational potential leads to the effective reduction of the Higgs vacuum expectation value, which is found to be compatible with the Standard Model first-order electroweak phase transition conditions. Gravity could also increase the CP-violating effects for particles that cross the new phase bubble walls and thus is able to lead to the successful electroweak baryogenesis scenario.http://dx.doi.org/10.1155/2018/4653202 |
| spellingShingle | M. Gogberashvili Electroweak Phase Transitions in Einstein’s Static Universe Advances in High Energy Physics |
| title | Electroweak Phase Transitions in Einstein’s Static Universe |
| title_full | Electroweak Phase Transitions in Einstein’s Static Universe |
| title_fullStr | Electroweak Phase Transitions in Einstein’s Static Universe |
| title_full_unstemmed | Electroweak Phase Transitions in Einstein’s Static Universe |
| title_short | Electroweak Phase Transitions in Einstein’s Static Universe |
| title_sort | electroweak phase transitions in einstein s static universe |
| url | http://dx.doi.org/10.1155/2018/4653202 |
| work_keys_str_mv | AT mgogberashvili electroweakphasetransitionsineinsteinsstaticuniverse |