Abstract

Abstract We study a class of simplified dark matter models in which one dark matter particle couples with a mediator and a Standard Model fermion. In such models, collider and direct detection searches probe complimentary regions of parameter space. For Majorana dark matter, direct detection covers the region near mediator-dark matter degeneracy, while colliders probe regions with a large dark matter and mediator mass splitting. For Dirac and complex dark matter, direct detection is effective for the entire region above the mass threshold, but colliders provide a strong bound for dark matter lighter than a few GeV. We also point out that dedicated searches for signatures with two jets or a monojet not coming from initial state radiation, along missing transverse energy can cover the remaining parameter space for thermal relic dark matter.

Highlights

  • JHEP11(2013)171 detection experiments, but are still much below the center-of-mass energy, 8 TeV, of the latest run at the LHC

  • We study a class of simplified dark matter models in which one dark matter particle couples with a mediator and a Standard Model fermion

  • We study simplified dark matter models with SM fermions as the portal particle, which we call Fermion Portal (FP) dark matter

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Summary

Simplified dark matter model: fermion portal

If the dark matter sector interacts directly with a single fermion in the SM, two particles with different spins are required in the dark matter sector. Restricting to particles with a spin less than one, there are two general situations: fermionic dark matter with a color-triplet scalar partner or scalar dark matter with a color-triplet fermion partner. In the former case, we consider both Dirac and Majorana dark matter, while for the latter case we only consider a complex scalar dark matter and skip the real scalar dark matter case [6], which has a quark mass suppressed s-wave or a dwave or three-body suppressed annihilation rate and a velocity suppressed direct detection cross section if the quark masses are neglected. Some other studies for the spin-dependent direct detection and indirect detection signatures can be found in refs. [46, 47]

Relic abundance
Dark matter direct detection
Collider constraints
Estimated limits from monojet on t-change φ exchange
Limits from monojet on single φ productions
Discussion and conclusions
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