Abstract

It is a distinct possibility that a Hidden Valley sector would have a spectrum of light particles consisting of both stable and unstable dark mesons. The simultaneous presence of these two types of particles can lead to novel mechanisms for generating the correct dark matter relic abundance, which in turn can reflect themselves into new exotic signatures at colliders. We study the viability of such sectors for various Hidden Valley models and map the valid parameter space to possible collider signatures. Mediators studied include various scalar bifundamentals and a heavy Z′. It is shown that in general bounds from direct and indirect detection can easily be avoided. In most of the allowed parameter space, the relic density is determined by stable mesons annihilating to unstable ones which in turn decay quickly to Standard Model particles. Dark mesons that decay mainly to heavier Standard Model fermions allow for more valid parameter space, though dark mesons are still allowed to decay exclusively to some of the lighter fermions. Possible exotic collider signatures include displaced vertices, emerging jets and semivisible jets.

Highlights

  • One interesting and understudied possibility is that dark matter consists of the stable dark mesons of a Hidden Valley sector [11] that contains unstable ones

  • In particular an increase in the sensitivity of indirect detection searches by a factor 10 would be able to probe a large region of the model of section 4.2 for dark pion masses below about 480 GeV and the Z model studied in this work for dark pions lighter than about 360 GeV.5

  • We studied Hidden Valley sectors whose spectra of light particles consist of both stable and unstable dark mesons

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Summary

General setup and overview of the mechanism

We begin by presenting the benchmark dark sector that will be used throughout the article and explain the mechanism that will lead to the correct dark matter relic abundance. Because of a suppression by a larger power of the number density, 3 → 2 processes are less important for the determination of the final dark matter relic abundance than the annihilation of two stable pions to two unstable ones. These subsequently decay to the Standard Model and are not replaced as inverse decay is not efficient in this regime. As λ continues to increase, it will eventually reach a point where the number densities of the πiu’s retain their equilibrium values until after the dark pions have decoupled from each other They are from left to right: codecaying dark matter, coupling-independent and standard thermal freeze-out

Overview of constraints
Direct detection
Indirect detection
Scalar mediators interacting only with down-type quarks
Multiple scalar mediators interacting only with down-type quarks
Z model
Additional comments
Conclusion
Lagrangian
Energy exchange
Boltzmann equation and approximations
Full Text
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