Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model

Abstract We propose a new physics model which has a cold dark matter candidate and can explain the b → sμ + μ − anomaly at the same time. Our model includes a scalar quark q ˜ $$ \tilde{q} $$ and a scalar lepton ℓ ˜ $$ \tilde{\ell} $$ which are SU(2) L -doublet as well as a Dirac fermion N which is...

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Main Authors: Seungwon Baek, Chaehyun Yu
Format: Article
Language:English
Published: SpringerOpen 2018-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP11(2018)054
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spelling doaj-00252e86de97429db45c7633d252a7222020-11-25T02:02:27ZengSpringerOpenJournal of High Energy Physics1029-84792018-11-0120181112610.1007/JHEP11(2018)054Dark matter for b → sμ + μ − anomaly in a gauged U(1) X modelSeungwon Baek0Chaehyun Yu1Department of Physics, Korea UniversityDepartment of Physics, Korea UniversityAbstract We propose a new physics model which has a cold dark matter candidate and can explain the b → sμ + μ − anomaly at the same time. Our model includes a scalar quark q ˜ $$ \tilde{q} $$ and a scalar lepton ℓ ˜ $$ \tilde{\ell} $$ which are SU(2) L -doublet as well as a Dirac fermion N which is SU(2) L -singlet. The new particles are charged under a gauged U(1) X group which is spontaneously broken to a discrete Z 2 symmetry by a dark scalar S. The remnant Z 2 symmetry stabilizes the dark matter. Box diagrams with q ˜ $$ \tilde{q} $$ , ℓ ˜ $$ \tilde{\ell} $$ , and N running inside the loop can generate the correct Wilson coefficients C 9 μ  = − C 10 μ to accommodate the b → sμ + μ − anomaly while avoiding constraints such as B s − B ¯ s $$ {B}_s-{\overline{B}}_s $$ mixing. The dark matter annihilation into a second generation lepton pair via t-channel ℓ ˜ $$ \tilde{\ell} $$ -exchanging process plays an important role in producing the current dark matter relic abundance of the universe, showing a strong interplay between the flavor and dark matter physics. We also discuss dark-gauge-interaction-dominated and Higgs-portal-dominated scenarios for dark matter physics.http://link.springer.com/article/10.1007/JHEP11(2018)054Beyond Standard ModelHeavy Quark Physics
collection DOAJ
language English
format Article
sources DOAJ
author Seungwon Baek
Chaehyun Yu
spellingShingle Seungwon Baek
Chaehyun Yu
Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model
Journal of High Energy Physics
Beyond Standard Model
Heavy Quark Physics
author_facet Seungwon Baek
Chaehyun Yu
author_sort Seungwon Baek
title Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model
title_short Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model
title_full Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model
title_fullStr Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model
title_full_unstemmed Dark matter for b → sμ + μ − anomaly in a gauged U(1) X model
title_sort dark matter for b → sμ + μ − anomaly in a gauged u(1) x model
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-11-01
description Abstract We propose a new physics model which has a cold dark matter candidate and can explain the b → sμ + μ − anomaly at the same time. Our model includes a scalar quark q ˜ $$ \tilde{q} $$ and a scalar lepton ℓ ˜ $$ \tilde{\ell} $$ which are SU(2) L -doublet as well as a Dirac fermion N which is SU(2) L -singlet. The new particles are charged under a gauged U(1) X group which is spontaneously broken to a discrete Z 2 symmetry by a dark scalar S. The remnant Z 2 symmetry stabilizes the dark matter. Box diagrams with q ˜ $$ \tilde{q} $$ , ℓ ˜ $$ \tilde{\ell} $$ , and N running inside the loop can generate the correct Wilson coefficients C 9 μ  = − C 10 μ to accommodate the b → sμ + μ − anomaly while avoiding constraints such as B s − B ¯ s $$ {B}_s-{\overline{B}}_s $$ mixing. The dark matter annihilation into a second generation lepton pair via t-channel ℓ ˜ $$ \tilde{\ell} $$ -exchanging process plays an important role in producing the current dark matter relic abundance of the universe, showing a strong interplay between the flavor and dark matter physics. We also discuss dark-gauge-interaction-dominated and Higgs-portal-dominated scenarios for dark matter physics.
topic Beyond Standard Model
Heavy Quark Physics
url http://link.springer.com/article/10.1007/JHEP11(2018)054
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