Abstract
The idea that dark matter forms part of a larger dark sector is very intriguing, given the high degree of complexity of the visible sector. In this paper, we discuss lepton jets as a promising signature of an extended dark sector. As a simple toy model, we consider an $\mathcal{O}(\text{GeV})$ DM fermion coupled to a new $U(1)'$ gauge boson (dark photon) with a mass of order GeV and kinetically mixed with the Standard Model photon. Dark matter production at the LHC in this model is typically accompanied by collinear radiation of dark photons whose decay products can form lepton jets. We analyze the dynamics of collinear dark photon emission both analytically and numerically. In particular, we derive the dark photon energy spectrum using recursive analytic expressions, using Monte Carlo simulations in Pythia, and using an inverse Mellin transform to obtain the spectrum from its moments. In the second part of the paper, we simulate the expected lepton jet signatures from radiating dark matter at the LHC, carefully taking into account the various dark photon decay modes and allowing for both prompt and displaced decays. Using these simulations, we recast two existing ATLAS lepton jet searches to significantly restrict the parameter space of extended dark sector models, and we compute the expected sensitivity of future LHC searches.
Highlights
Large class of more complicated scenarios, to which our conclusions can be applied as well
We have studied the possibility of revealing the properties of a dark sector of particle physics by using final state radiation from dark matter produced at the LHC
While our conclusions apply to a very large class of extended dark sector models, we have worked in the framework of a toy model where fermionic dark matter particles χ are charged under a new dark sector gauge group U(1) and coupled to the SM through a heavy mediator
Summary
The results of this paper can be applied to any model in which a 10 GeV DM particle interacts with a new 10 GeV gauge boson, as long as the typical energy at which DM particles are produced at the LHC is much higher than their masses. To illustrate our main points, we will use a specific toy model of radiating DM, in which the dark sector consists of a fermionic DM particle χ and a massive U(1) gauge boson A. The coupling strength between χ and A is described by a dark fine structure constant αA ≡ gA2 /(4π). The dark photon A is kinetically mixed with the SM photon. The Lagrangian for the dark sector is
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