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

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ID: 92653
2018
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Abstract
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.
Reference Key
baek2018darkjournal Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Baek, Seungwon;Yu, Chaehyun;
Journal journal of high energy physics
Year 2018
DOI
DOI not found
URL
http://link.springer.com/article/10.1007/JHEP11(2018)054
Keywords
chemistry physics education (general) special aspects of education mathematics electronic computers. computer science nuclear and particle physics. atomic energy. radioactivity

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