The B anomalies, the U 1 leptoquark and dark matter

Abstract The present-day B-anomalies involving b → sμ + μ − or b → cτ − ν ¯ $$ \overline{\nu} $$ transitions can all be explained with the addition of a vector U 1 leptoquark with a mass of M U 1 $$ {M}_{U_1} $$ ≳ 1.8 TeV. In the scalar singlet dark matter model (SSDMM), the DM is a scalar S that co...

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Main Authors: Geneviève Bélanger, Jacky Kumar, David London, Alexander Pukhov
Format: Article
Language:English
Published: SpringerOpen 2023-01-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP01(2023)041
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author Geneviève Bélanger
Jacky Kumar
David London
Alexander Pukhov
author_facet Geneviève Bélanger
Jacky Kumar
David London
Alexander Pukhov
author_sort Geneviève Bélanger
collection DOAJ
description Abstract The present-day B-anomalies involving b → sμ + μ − or b → cτ − ν ¯ $$ \overline{\nu} $$ transitions can all be explained with the addition of a vector U 1 leptoquark with a mass of M U 1 $$ {M}_{U_1} $$ ≳ 1.8 TeV. In the scalar singlet dark matter model (SSDMM), the DM is a scalar S that couples to the Higgs via λ hS S 2 |H| 2. We update the fit to the data and find that the SSDMM is now viable only for M S ≳ 1.6 TeV. In this paper, we assume that the DM also couples to the U 1 via λ U 1 S S 2 U 1 μ † U 1 μ $$ {\lambda}_{U_1S}{S}^2{U}_{1\mu}^{\dagger }{U}_1^{\mu } $$ . In addition to leading to DM annihilation via SS → U 1 U ¯ 1 $$ {U}_1{\overline{U}}_1 $$ , this coupling generates SSgg and SSγγ couplings at one loop. Although naively divergent, these loop diagrams can be calculated under the assumption that the U 1 is a gauge boson of a group broken at the TeV scale. With this DM-U 1 coupling term, there are additional contributions to the various DM observables (relic density, direct and indirect detection). We find that the constraints on the SSDMM are relaxed for both heavy DM (M S ≳ M U 1 $$ {M}_{U_1} $$ ) and light DM (M S < M U 1 $$ {M}_{U_1} $$ ).
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spelling doaj.art-4be5983575474194bbefa63f0e0489d32023-04-30T11:03:49ZengSpringerOpenJournal of High Energy Physics1029-84792023-01-012023112010.1007/JHEP01(2023)041The B anomalies, the U 1 leptoquark and dark matterGeneviève Bélanger0Jacky Kumar1David London2Alexander Pukhov3LAPTh, CNRS, USMBPhysique des Particules, Université de MontréalPhysique des Particules, Université de MontréalSkobeltsyn Institute of Nuclear Physics, Moscow State UniversityAbstract The present-day B-anomalies involving b → sμ + μ − or b → cτ − ν ¯ $$ \overline{\nu} $$ transitions can all be explained with the addition of a vector U 1 leptoquark with a mass of M U 1 $$ {M}_{U_1} $$ ≳ 1.8 TeV. In the scalar singlet dark matter model (SSDMM), the DM is a scalar S that couples to the Higgs via λ hS S 2 |H| 2. We update the fit to the data and find that the SSDMM is now viable only for M S ≳ 1.6 TeV. In this paper, we assume that the DM also couples to the U 1 via λ U 1 S S 2 U 1 μ † U 1 μ $$ {\lambda}_{U_1S}{S}^2{U}_{1\mu}^{\dagger }{U}_1^{\mu } $$ . In addition to leading to DM annihilation via SS → U 1 U ¯ 1 $$ {U}_1{\overline{U}}_1 $$ , this coupling generates SSgg and SSγγ couplings at one loop. Although naively divergent, these loop diagrams can be calculated under the assumption that the U 1 is a gauge boson of a group broken at the TeV scale. With this DM-U 1 coupling term, there are additional contributions to the various DM observables (relic density, direct and indirect detection). We find that the constraints on the SSDMM are relaxed for both heavy DM (M S ≳ M U 1 $$ {M}_{U_1} $$ ) and light DM (M S < M U 1 $$ {M}_{U_1} $$ ).https://doi.org/10.1007/JHEP01(2023)041Particle Nature of Dark MatterSemi-Leptonic DecaysSpecific BSM Phenomenology
spellingShingle Geneviève Bélanger
Jacky Kumar
David London
Alexander Pukhov
The B anomalies, the U 1 leptoquark and dark matter
Journal of High Energy Physics
Particle Nature of Dark Matter
Semi-Leptonic Decays
Specific BSM Phenomenology
title The B anomalies, the U 1 leptoquark and dark matter
title_full The B anomalies, the U 1 leptoquark and dark matter
title_fullStr The B anomalies, the U 1 leptoquark and dark matter
title_full_unstemmed The B anomalies, the U 1 leptoquark and dark matter
title_short The B anomalies, the U 1 leptoquark and dark matter
title_sort b anomalies the u 1 leptoquark and dark matter
topic Particle Nature of Dark Matter
Semi-Leptonic Decays
Specific BSM Phenomenology
url https://doi.org/10.1007/JHEP01(2023)041
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