Strong Electroweak Phase Transition in a Model with Extended Scalar Sector
We consider an extension of the Standard Model (SM) with additional gauge singlets which exhibits a strong first-order phase transition. Due to this first-order phase transition in the early universe gravitational waves are produced. We estimate the contributions such as the sound wave, the bubble w...
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Wiley
2017-01-01
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Series: | Advances in High Energy Physics |
Online Access: | http://dx.doi.org/10.1155/2017/7638204 |
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author | Mina Saeedhosseini Ali Tofighi |
author_facet | Mina Saeedhosseini Ali Tofighi |
author_sort | Mina Saeedhosseini |
collection | DOAJ |
description | We consider an extension of the Standard Model (SM) with additional gauge singlets which exhibits a strong first-order phase transition. Due to this first-order phase transition in the early universe gravitational waves are produced. We estimate the contributions such as the sound wave, the bubble wall collision, and the plasma turbulence to the stochastic gravitational wave background, and we find that the strength at the peak frequency is large enough to be detected at future gravitational interferometers such as eLISA. Deviations in the various Higgs boson self-couplings are also evaluated. |
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id | doaj-art-e1c3dc4dc0d049f79fdce2ce30d636c3 |
institution | Kabale University |
issn | 1687-7357 1687-7365 |
language | English |
publishDate | 2017-01-01 |
publisher | Wiley |
record_format | Article |
series | Advances in High Energy Physics |
spelling | doaj-art-e1c3dc4dc0d049f79fdce2ce30d636c32025-02-03T01:03:03ZengWileyAdvances in High Energy Physics1687-73571687-73652017-01-01201710.1155/2017/76382047638204Strong Electroweak Phase Transition in a Model with Extended Scalar SectorMina Saeedhosseini0Ali Tofighi1Department of Physics, Faculty of Basic Sciences, University of Mazandaran, P.O. Box 47416-95447, Babolsar, IranDepartment of Physics, Faculty of Basic Sciences, University of Mazandaran, P.O. Box 47416-95447, Babolsar, IranWe consider an extension of the Standard Model (SM) with additional gauge singlets which exhibits a strong first-order phase transition. Due to this first-order phase transition in the early universe gravitational waves are produced. We estimate the contributions such as the sound wave, the bubble wall collision, and the plasma turbulence to the stochastic gravitational wave background, and we find that the strength at the peak frequency is large enough to be detected at future gravitational interferometers such as eLISA. Deviations in the various Higgs boson self-couplings are also evaluated.http://dx.doi.org/10.1155/2017/7638204 |
spellingShingle | Mina Saeedhosseini Ali Tofighi Strong Electroweak Phase Transition in a Model with Extended Scalar Sector Advances in High Energy Physics |
title | Strong Electroweak Phase Transition in a Model with Extended Scalar Sector |
title_full | Strong Electroweak Phase Transition in a Model with Extended Scalar Sector |
title_fullStr | Strong Electroweak Phase Transition in a Model with Extended Scalar Sector |
title_full_unstemmed | Strong Electroweak Phase Transition in a Model with Extended Scalar Sector |
title_short | Strong Electroweak Phase Transition in a Model with Extended Scalar Sector |
title_sort | strong electroweak phase transition in a model with extended scalar sector |
url | http://dx.doi.org/10.1155/2017/7638204 |
work_keys_str_mv | AT minasaeedhosseini strongelectroweakphasetransitioninamodelwithextendedscalarsector AT alitofighi strongelectroweakphasetransitioninamodelwithextendedscalarsector |