Abstract

We consider renormalizable theories such that the scattering of dark matter off leptons arises at tree level, but scattering off nuclei only arises at loop. In this framework, the various dark matter candidates can be classified by their spins and by the forms of their interactions with leptons. We determine the corrections to the anomalous magnetic moment of the muon that arise from these interactions. We then consider the implications of these results for a set of simplified models of leptophilic dark matter. When a dark matter candidate reduces the existing tension between the standard model prediction of the anomalous magnetic moment and the experimental measurement, the region of parameter space favored to completely remove the discrepancy is highlighted. Conversely, when agreement is worsened, we place limits on the parameters of the corresponding simplified model. These bounds and favored regions are compared against the experimental constraints on the simplified model from direct detection and from collider searches. Although these constraints are severe, we find there do exist limited regions of parameter space in these simple theories that can explain the observed anomaly in the muon magnetic moment while remaining consistent with all experimental bounds.

Highlights

  • The standard model (SM) of particle physics is in very good agreement with experiment [1]

  • These include theories where dark matter (DM) is composed of WIMPs, particles of weak scale mass that survive as thermal relics [5, 6], and some models of Asymmetric Dark Matter [7,8,9,10,11,12,13,14,15,16,17]

  • We focus on renormalizable theories where the scattering of DM off leptons arises at tree level, but DM scattering off nuclei only arises at loop

Read more

Summary

Introduction

The standard model (SM) of particle physics is in very good agreement with experiment [1]. If this observed anomaly is a consequence of new physics, a very interesting possibility is that it is associated with the interactions of leptons with DM. We do not take into account limits on the parameter space that arise from the relic abundance, since these bounds tend to be more model dependent, and are less robust than the constraints we consider. These constraints do not apply to scenarios where the dark matter is non-thermal or asymmetric.

Contributions to aμ
Charged mediator diagrams
Neutral mediator diagrams
Limits from direct detection
Self-conjugate particles
Dirac fermion DM
Neutral vector mediator
Limits
Collider constraints
Compositeness bounds from LEP
Resonant production at LEP
Light neutral mediators
Monophoton searches at LEP
Collider limits on charged mediators
Analysis of simplified models
Charged mediator
Neutral spin-0 mediator
Charged spin-0 mediator
Charged spin-1 mediator
Neutral spin-1 mediator
Findings
Conclusions
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.