Abstract

We study the dark matter phenomenology of Standard Model extensions addressing the reported anomaly in the R_K observable at one-loop. The article covers the case of fermionic singlet DM coupling leptophilically, quarkphilically or amphiphilically to the SM. The setup utilizes a large coupling of the new particle content to the second lepton generation to explain the R_K anomaly, which in return tends to diminish the dark matter relic density. Further, dark matter direct detection experiments provide stringent bounds even in cases where the dark matter candidate only contributes a small fraction of the observed dark matter energy density. In fact, direct detection rules out all considered models as an explanation for the R_K anomaly in the case of Dirac dark matter. Conversely, for Majorana dark matter, the R_K anomaly can be addressed in agreement with direct detection in coannihilation scenarios. For leptophilic dark matter this region only exists for M_text {DM} lesssim 1000 , mathrm {GeV} and dark matter is underabundant. Quarkphilic and amphiphilic scenarios even provide narrow regions of parameter space where the observed relic density can be reproduced while offering an explanation to R_K in agreement with direct detection experiments.

Highlights

  • [2] or gravitational lensing effects [3], provide strong evidence for the existence of dark matter (DM)

  • In addition to the scenarios presented in this article, we have studied an examplatory case for each model class allowing for a non-degenerate, non-DM dark sector

  • For quarkphilic and leptophilic scenarios, only coannihilating scenarios are affected by a non-degenerate, non-DM dark sector, while amphiphilic models can be affected in both setups

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Summary

Introduction

[2] or gravitational lensing effects [3], provide strong evidence for the existence of (particle) DM. This setup requires a relatively large coupling of the new particles to the second lepton generation to explain the RK anomaly, since, in comparison to tree-level realizations, the one-loop suppression has to be compensated and, the coupling to quarks is constrained by B0B0 mixing This in turn can lead to an underpopulated dark sector, as the strong coupling to the second lepton generation tends to delay the DM freeze-out. We discuss the implications of the models on the relic density and direct detection experiments, where we provide a summary of our analysis strategy for our numerical analysis The results of this analysis for each model are presented in Sect.

Setup and classification
Constraints on new Yukawa couplings
Constraints on parameters from the scalar potential
Dark matter phenomenology
Relic density
Direct detection
Fermionic DM χ and scalar mediator A
N μ2χ N λ2χs m
Fermionic DM χ and vector mediator Vμ
Twist-2 contributions to the SI DM-nucleon cross section
Indirect detection
Results of the numerical analysis
Dirac DM
Majorana DM
Collider constraints
Summary and conclusions

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