Abstract

Models where dark matter is a part of an electroweak multiplet feature charged particles with macroscopic lifetimes due to the charged-neutral mass split of the order of pion mass. At the Large Hadron Collider, the ATLAS and CMS experiments will identify these charged particles as disappearing tracks, since they decay into a massive invisible dark matter candidate and a very soft charged Standard-Model particle which fails to pass the reconstruction requirements. While ATLAS and CMS have focused on the supersymmetric versions of these scenarios, we have performed here the reinterpretation of the latest ATLAS disappearing track search for a suite of dark matter multiplets with different spins and electroweak quantum numbers. More concretely, we consider the cases of the inert Two Higgs Doublet model (i2HDM), of Minimal Fermion Dark Matter (MFDM) and of Vector Triplet Dark Matter (VTDM). Our procedure is validated by using the same wino and higgsino benchmark models employed by the ATLAS collaboration. We have found that with the disappearing track signature one can probe a vast portion of the parameter space, well beyond the reach of prompt missing energy searches (notably mono-jets). We provide tables with the upper-limits on the cross-section upper limits, and efficiencies in the lifetime - dark matter mass plane for all the models under consideration. Moreover we make the recasting code employed here publicly available, as part of the LLP Recasting Repository.

Highlights

  • The existence of Dark Matter (DM) has been established beyond any reasonable doubt by several independent cosmological observations

  • The Yþ are very soft and typically stopped by the magnetic field of the detector,2 leaving a short-track (Dþ) that “disappears” into missing transverse energy (D). This disappearing track (DT) signature which we explore in this paper is very powerful in probing DM scenarios which are compressed with ΔM ≃ mπ

  • In the Fig. (7c), we show, for the direct detection (DD) þ jet process with pTðjÞ > 100 GeV, the pT distribution of the charged dark particle at parton level normalized to the cross section, while in the Fig. (7d), we present this distribution convoluted with the experimental efficiency for the reconstruction of the charged track

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Summary

INTRODUCTION

The existence of Dark Matter (DM) has been established beyond any reasonable doubt by several independent cosmological observations. If DM is part of a weak multiplet, and there are no light Z0 resonances or other new particles playing the role of the mediators decaying into a DM pair (which could enhance DM mono-X signal), even the HL-LHC could probe DM mass only up to about 150–300 GeV, as shown, e.g., for the case of Higgsino DM in MSSM [3,4,5,6] This limitation motivates us to go beyond the mono-X signature. More detailed information on cross section upper limits and efficiencies, including the one for single and pair DÆ production can be found in LLP Recasting Repository

MODELS WITH DISAPPEARING TRACK SIGNATURES
The lifetime of charged LLPs and the effective W-pion mixing
Existing experimental studies
The event selection stage
The tracklet selection stage
Validation in the AMSB scenario
REINTERPRETATION FOR MINIMAL MODELS
Findings
CONCLUSIONS
Full Text
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