Higgs instability and de Sitter radiation
If the Standard Model (SM) of elementary particle physics is assumed to hold good to arbitrarily high energies, then, for the best fit values of the parameters, the scalar potential of the Standard Model Higgs field turns negative at a high scale μinst. If the physics beyond the SM is such that it d...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2015-12-01
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| Series: | Physics Letters B |
| Subjects: | |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269315007789 |
| _version_ | 1818158736938631168 |
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| author | Gaurav Goswami Subhendra Mohanty |
| author_facet | Gaurav Goswami Subhendra Mohanty |
| author_sort | Gaurav Goswami |
| collection | DOAJ |
| description | If the Standard Model (SM) of elementary particle physics is assumed to hold good to arbitrarily high energies, then, for the best fit values of the parameters, the scalar potential of the Standard Model Higgs field turns negative at a high scale μinst. If the physics beyond the SM is such that it does not modify this feature of the Higgs potential and if the Hubble parameter during inflation (Hinf) is such that Hinf≫μinst, then, quantum fluctuations of the SM Higgs during inflation make it extremely unlikely that after inflation it will be found in the metastable vacuum at the weak scale. In this work, we assume that (i) during inflation, the SM Higgs is in Bunch–Davies vacuum state, and, (ii) the question about the stability of the effective potential must be answered in the frame of the freely falling observer (just like in Minkowski spacetime), and then use the well-known fact that the freely falling observer finds Bunch–Davies vacuum to be in thermal state to show that the probability to end up in the electroweak vacuum after inflation is reasonably high. |
| first_indexed | 2024-12-11T15:34:50Z |
| format | Article |
| id | doaj.art-91629bdad0f142d281f8119a8030b5f5 |
| institution | Directory Open Access Journal |
| issn | 0370-2693 1873-2445 |
| language | English |
| last_indexed | 2024-12-11T15:34:50Z |
| publishDate | 2015-12-01 |
| publisher | Elsevier |
| record_format | Article |
| series | Physics Letters B |
| spelling | doaj.art-91629bdad0f142d281f8119a8030b5f52022-12-22T00:59:58ZengElsevierPhysics Letters B0370-26931873-24452015-12-01751C11311810.1016/j.physletb.2015.10.027Higgs instability and de Sitter radiationGaurav Goswami0Subhendra Mohanty1Physical Research Laboratory, Navrangpura, Ahmedabad 380 009, IndiaPhysical Research Laboratory, Navrangpura, Ahmedabad 380 009, IndiaIf the Standard Model (SM) of elementary particle physics is assumed to hold good to arbitrarily high energies, then, for the best fit values of the parameters, the scalar potential of the Standard Model Higgs field turns negative at a high scale μinst. If the physics beyond the SM is such that it does not modify this feature of the Higgs potential and if the Hubble parameter during inflation (Hinf) is such that Hinf≫μinst, then, quantum fluctuations of the SM Higgs during inflation make it extremely unlikely that after inflation it will be found in the metastable vacuum at the weak scale. In this work, we assume that (i) during inflation, the SM Higgs is in Bunch–Davies vacuum state, and, (ii) the question about the stability of the effective potential must be answered in the frame of the freely falling observer (just like in Minkowski spacetime), and then use the well-known fact that the freely falling observer finds Bunch–Davies vacuum to be in thermal state to show that the probability to end up in the electroweak vacuum after inflation is reasonably high.http://www.sciencedirect.com/science/article/pii/S0370269315007789Physics beyond the Standard ModelHiggs vacuum instabilityInflationGibbons–Hawking temperature |
| spellingShingle | Gaurav Goswami Subhendra Mohanty Higgs instability and de Sitter radiation Physics Letters B Physics beyond the Standard Model Higgs vacuum instability Inflation Gibbons–Hawking temperature |
| title | Higgs instability and de Sitter radiation |
| title_full | Higgs instability and de Sitter radiation |
| title_fullStr | Higgs instability and de Sitter radiation |
| title_full_unstemmed | Higgs instability and de Sitter radiation |
| title_short | Higgs instability and de Sitter radiation |
| title_sort | higgs instability and de sitter radiation |
| topic | Physics beyond the Standard Model Higgs vacuum instability Inflation Gibbons–Hawking temperature |
| url | http://www.sciencedirect.com/science/article/pii/S0370269315007789 |
| work_keys_str_mv | AT gauravgoswami higgsinstabilityanddesitterradiation AT subhendramohanty higgsinstabilityanddesitterradiation |