Mixed hidden sector-visible sector dark matter and observation of a CP odd Higgs boson at HL-LHC and HE-LHC

摘要

It is very likely that, similarly to the case of visible matter, dark matter (DM) is composed of more than one stable component. In this work, we investigate a two-component dark matter with one component from the visible sector and the other from the hidden sector. Specifically, we consider a U(1)_X hidden-sector extension of the minimal supersymmetric standard model with supergravity (MSSM/SUGRA), where we allow for kinetic and Stueckelberg mass mixing between the two Abelian U(1)'s, i.e., U(1)_X and U(1)_Y . We further assume that the hidden sector has chiral matter which leads to a Dirac fermion as a candidate for dark matter. The lightest neutralino in the visible sector and the Dirac fermion in the hidden sector then constitute the two components of dark matter. We investigate in particular MSSM/SUGRA models with radiative breaking occurring on the hyperbolic branch where the Higgs mixing parameter μ is small (the order of the electroweak scale), which leads to the lightest neutralino being dominantly a Higgsino. While dark matter constituted only of Higgsinos is significantly constrained by data on dark matter relic density and by limits on the spin-independent proton-DM scattering cross section, consistency with data can be achieved if only a fraction of the dark matter relic density is constituted of Higgsinos, with the rest coming from the hidden sector. An aspect of the proposed model is the prediction of a relatively light CP-odd Higgs A (as well as a CP-even H and a charged Higgs H~±) which is observable in the High-Luminosity and High-Energy Large Hadron Collider projects (HL-LHC and HE-LHC). We perform a detailed collider analysis search for the CP-odd Higgs using boosted decision trees in τ_h τ_h final states and compare the discovery potential at the HL-LHC and HE-LHC. We show that while several of the points among our benchmarks may be observable at the HL-LHC, all of them are visible at the HE-LHC with much lower integrated luminosities, thus