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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Main Authors: Mina Saeedhosseini, Ali Tofighi
Format: Article
Language:English
Published: Wiley 2017-01-01
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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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