Conformal vector dark matter and strongly first-order electroweak phase transition
Abstract We study a conformal version of the Standard Model (SM), which apart from SM sector, containing a U D (1) dark sector with a vector dark matter candidate and a scalar field (scalon). In this model the dark sector couples to the SM sector via a Higgs portal. The theory is scale-invariant in...
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Online Access: | http://link.springer.com/article/10.1007/JHEP03(2019)181 |
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doaj-6cf40d25390246bdb0c500cb2928a44d2020-11-25T02:04:21ZengSpringerOpenJournal of High Energy Physics1029-84792019-03-012019312510.1007/JHEP03(2019)181Conformal vector dark matter and strongly first-order electroweak phase transitionSeyed Yaser Ayazi0Ahmad Mohamadnejad1Physics Department, Semnan UniversityYoung Researchers and Elite Club, Islamshahr Branch, Islamic Azad UniversityAbstract We study a conformal version of the Standard Model (SM), which apart from SM sector, containing a U D (1) dark sector with a vector dark matter candidate and a scalar field (scalon). In this model the dark sector couples to the SM sector via a Higgs portal. The theory is scale-invariant in lowest order, therefore the spontaneous symmetry breaking of scale invariance entails the existence of a scalar particle, scalon, with vanishing zeroth-order mass. However, one-loop corrections break scale invariance, so they give mass to the scalon. Because of the scale invariance, our model is subjected to constraints which remove many of the free parameters. We put constraints to the two remaining parameters from the Higgs searches at the LHC, dark matter relic density and dark matter direct detection limits by PandaX-II. The viable mass region for dark matter is about 1–2 TeV. We also obtain the finite temperature one-loop effective potential of the model and demonstrate that finite temperature effects, for the parameter space constrained by dark matter relic density, induce a strongly first-order electroweak phase transition.http://link.springer.com/article/10.1007/JHEP03(2019)181Beyond Standard ModelCosmology of Theories beyond the SM |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Seyed Yaser Ayazi Ahmad Mohamadnejad |
spellingShingle |
Seyed Yaser Ayazi Ahmad Mohamadnejad Conformal vector dark matter and strongly first-order electroweak phase transition Journal of High Energy Physics Beyond Standard Model Cosmology of Theories beyond the SM |
author_facet |
Seyed Yaser Ayazi Ahmad Mohamadnejad |
author_sort |
Seyed Yaser Ayazi |
title |
Conformal vector dark matter and strongly first-order electroweak phase transition |
title_short |
Conformal vector dark matter and strongly first-order electroweak phase transition |
title_full |
Conformal vector dark matter and strongly first-order electroweak phase transition |
title_fullStr |
Conformal vector dark matter and strongly first-order electroweak phase transition |
title_full_unstemmed |
Conformal vector dark matter and strongly first-order electroweak phase transition |
title_sort |
conformal vector dark matter and strongly first-order electroweak phase transition |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2019-03-01 |
description |
Abstract We study a conformal version of the Standard Model (SM), which apart from SM sector, containing a U D (1) dark sector with a vector dark matter candidate and a scalar field (scalon). In this model the dark sector couples to the SM sector via a Higgs portal. The theory is scale-invariant in lowest order, therefore the spontaneous symmetry breaking of scale invariance entails the existence of a scalar particle, scalon, with vanishing zeroth-order mass. However, one-loop corrections break scale invariance, so they give mass to the scalon. Because of the scale invariance, our model is subjected to constraints which remove many of the free parameters. We put constraints to the two remaining parameters from the Higgs searches at the LHC, dark matter relic density and dark matter direct detection limits by PandaX-II. The viable mass region for dark matter is about 1–2 TeV. We also obtain the finite temperature one-loop effective potential of the model and demonstrate that finite temperature effects, for the parameter space constrained by dark matter relic density, induce a strongly first-order electroweak phase transition. |
topic |
Beyond Standard Model Cosmology of Theories beyond the SM |
url |
http://link.springer.com/article/10.1007/JHEP03(2019)181 |
work_keys_str_mv |
AT seyedyaserayazi conformalvectordarkmatterandstronglyfirstorderelectroweakphasetransition AT ahmadmohamadnejad conformalvectordarkmatterandstronglyfirstorderelectroweakphasetransition |
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1724942811562770432 |