Feebly coupled vector boson dark matter in effective theory

Abstract A model of dark matter (DM) that communicates with the Standard Model (SM) exclusively through suppressed dimension five operator is discussed. The SM is augmented with a symmetry U(1) X ⊗ Z 2, where U(1) X is gauged and broken spontaneously by a very heavy decoupled scalar. The massive U(1...

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Main Authors: Basabendu Barman, Subhaditya Bhattacharya, Bohdan Grzadkowski
Format: Article
Language:English
Published: SpringerOpen 2020-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2020)162
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spelling doaj-0453014bf79e4fd0bc17b0faefbd06ce2020-12-27T12:02:48ZengSpringerOpenJournal of High Energy Physics1029-84792020-12-0120201214110.1007/JHEP12(2020)162Feebly coupled vector boson dark matter in effective theoryBasabendu Barman0Subhaditya Bhattacharya1Bohdan Grzadkowski2Department of Physics, Indian Institute of Technology GuwahatiDepartment of Physics, Indian Institute of Technology GuwahatiFaculty of Physics, University of WarsawAbstract A model of dark matter (DM) that communicates with the Standard Model (SM) exclusively through suppressed dimension five operator is discussed. The SM is augmented with a symmetry U(1) X ⊗ Z 2, where U(1) X is gauged and broken spontaneously by a very heavy decoupled scalar. The massive U(1) X vector boson (X μ ) is stabilized being odd under unbroken Z 2 and therefore may contribute as the DM component of the universe. Dark sector field strength tensor X μν couples to the SM hypercharge tensor B μν via the presence of a heavier Z 2 odd real scalar Φ, i.e. 1/Λ X μν B μν Φ, with Λ being a scale of new physics. The freeze-in production of the vector boson dark matter feebly coupled to the SM is advocated in this analysis. Limitations of the so-called UV freeze-in mechanism that emerge when the maximum reheat temperature T RH drops down close to the scale of DM mass are discussed. The parameter space of the model consistent with the observed DM abundance is determined. The model easily and naturally avoids both direct and indirect DM searches. Possibility for detection at the Large Hadron Collider (LHC) is also considered. A Stueckelberg formulation of the model is derived.https://doi.org/10.1007/JHEP12(2020)162Beyond Standard ModelCosmology of Theories beyond the SMEffective Field TheoriesHiggs Physics
collection DOAJ
language English
format Article
sources DOAJ
author Basabendu Barman
Subhaditya Bhattacharya
Bohdan Grzadkowski
spellingShingle Basabendu Barman
Subhaditya Bhattacharya
Bohdan Grzadkowski
Feebly coupled vector boson dark matter in effective theory
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
Effective Field Theories
Higgs Physics
author_facet Basabendu Barman
Subhaditya Bhattacharya
Bohdan Grzadkowski
author_sort Basabendu Barman
title Feebly coupled vector boson dark matter in effective theory
title_short Feebly coupled vector boson dark matter in effective theory
title_full Feebly coupled vector boson dark matter in effective theory
title_fullStr Feebly coupled vector boson dark matter in effective theory
title_full_unstemmed Feebly coupled vector boson dark matter in effective theory
title_sort feebly coupled vector boson dark matter in effective theory
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2020-12-01
description Abstract A model of dark matter (DM) that communicates with the Standard Model (SM) exclusively through suppressed dimension five operator is discussed. The SM is augmented with a symmetry U(1) X ⊗ Z 2, where U(1) X is gauged and broken spontaneously by a very heavy decoupled scalar. The massive U(1) X vector boson (X μ ) is stabilized being odd under unbroken Z 2 and therefore may contribute as the DM component of the universe. Dark sector field strength tensor X μν couples to the SM hypercharge tensor B μν via the presence of a heavier Z 2 odd real scalar Φ, i.e. 1/Λ X μν B μν Φ, with Λ being a scale of new physics. The freeze-in production of the vector boson dark matter feebly coupled to the SM is advocated in this analysis. Limitations of the so-called UV freeze-in mechanism that emerge when the maximum reheat temperature T RH drops down close to the scale of DM mass are discussed. The parameter space of the model consistent with the observed DM abundance is determined. The model easily and naturally avoids both direct and indirect DM searches. Possibility for detection at the Large Hadron Collider (LHC) is also considered. A Stueckelberg formulation of the model is derived.
topic Beyond Standard Model
Cosmology of Theories beyond the SM
Effective Field Theories
Higgs Physics
url https://doi.org/10.1007/JHEP12(2020)162
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