NLO electroweak corrections in general scalar singlet models

Abstract If no new physics signals are found, in the coming years, at the Large Hadron Collider Run-2, an increase in precision of the Higgs couplings measurements will shift the discussion to the effects of higher order corrections. In Beyond the Standard Model (BSM) theories this may become the on...

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Main Authors: Raul Costa, Marco O. P. Sampaio, Rui Santos
Format: Article
Language:English
Published: SpringerOpen 2017-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP07(2017)081
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spelling doaj-8464d22c740f466b97193312ec1b401a2020-11-24T21:09:58ZengSpringerOpenJournal of High Energy Physics1029-84792017-07-012017713810.1007/JHEP07(2017)081NLO electroweak corrections in general scalar singlet modelsRaul Costa0Marco O. P. Sampaio1Rui Santos2CERNDepartamento de Física da Universidade de Aveiro and CIDMA (Center for Research & Development in Mathematics and Applications)Instituto Superior de Engenharia de Lisboa — ISELAbstract If no new physics signals are found, in the coming years, at the Large Hadron Collider Run-2, an increase in precision of the Higgs couplings measurements will shift the discussion to the effects of higher order corrections. In Beyond the Standard Model (BSM) theories this may become the only tool to probe new physics. Extensions of the Standard Model (SM) with several scalar singlets may address several of its problems, namely to explain dark matter, the matter-antimatter asymmetry, or to improve the stability of the SM up to the Planck scale. In this work we propose a general framework to calculate one loop-corrections to the propagators and to the scalar field vacuum expectation values of BSM models with an arbitrary number of scalar singlets. We then apply our method to a real and to a complex scalar singlet models. We assess the importance of the one-loop radiative corrections first by computing them for a tree level mixing sum constraint, and then for the main Higgs production process gg → H. We conclude that, for the currently allowed parameter space of these models, the corrections can be at most a few percent. Notably, a non-zero correction can survive when dark matter is present, in the SM-like limit of the Higgs couplings to other SM particles.http://link.springer.com/article/10.1007/JHEP07(2017)081Beyond Standard ModelHiggs PhysicsSpontaneous Symmetry Breaking
collection DOAJ
language English
format Article
sources DOAJ
author Raul Costa
Marco O. P. Sampaio
Rui Santos
spellingShingle Raul Costa
Marco O. P. Sampaio
Rui Santos
NLO electroweak corrections in general scalar singlet models
Journal of High Energy Physics
Beyond Standard Model
Higgs Physics
Spontaneous Symmetry Breaking
author_facet Raul Costa
Marco O. P. Sampaio
Rui Santos
author_sort Raul Costa
title NLO electroweak corrections in general scalar singlet models
title_short NLO electroweak corrections in general scalar singlet models
title_full NLO electroweak corrections in general scalar singlet models
title_fullStr NLO electroweak corrections in general scalar singlet models
title_full_unstemmed NLO electroweak corrections in general scalar singlet models
title_sort nlo electroweak corrections in general scalar singlet models
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2017-07-01
description Abstract If no new physics signals are found, in the coming years, at the Large Hadron Collider Run-2, an increase in precision of the Higgs couplings measurements will shift the discussion to the effects of higher order corrections. In Beyond the Standard Model (BSM) theories this may become the only tool to probe new physics. Extensions of the Standard Model (SM) with several scalar singlets may address several of its problems, namely to explain dark matter, the matter-antimatter asymmetry, or to improve the stability of the SM up to the Planck scale. In this work we propose a general framework to calculate one loop-corrections to the propagators and to the scalar field vacuum expectation values of BSM models with an arbitrary number of scalar singlets. We then apply our method to a real and to a complex scalar singlet models. We assess the importance of the one-loop radiative corrections first by computing them for a tree level mixing sum constraint, and then for the main Higgs production process gg → H. We conclude that, for the currently allowed parameter space of these models, the corrections can be at most a few percent. Notably, a non-zero correction can survive when dark matter is present, in the SM-like limit of the Higgs couplings to other SM particles.
topic Beyond Standard Model
Higgs Physics
Spontaneous Symmetry Breaking
url http://link.springer.com/article/10.1007/JHEP07(2017)081
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