We study Dark Matter (DM) in the Exceptional Supersymmetric Standard Model (E6SSM). The model has both active and inert Higgs superfields and by imposing discrete symmetries one can generate two DM candidates. We show that the lightest higgsinos of the active and inert sectors give a viable setup for two-component DM. We also illustrate the scope of both direct and indirect detection experiments in extracting such a DM sector. Future experiments of the former kind have a good chance of finding the active component while the inert higgsino will be very hard to detect while those of the latter kind will have no sensitivity to either candidate.
I. INTRODUCTIONRecent Planck satellite observations of the fluctuations in the Cosmic Microwave Background (CMB) [1,2] confirmed that the largest part of our universe consists of invisible matter: Dark Matter (DM) for 26.8% and Dark Energy (DE) for 68.3% of it, while less than 5% of it is in the form of observable matter. Such a small part of visible matter is composed of (anti)quarks and (anti)leptons, in addition to gauge bosons. Therefore, it is not unrealistic to imagine that the DM sector is not minimal either and the assumption of multi-component DM is quite justified.In multi-component DM scenarios, we may have a combination of cold and warm DM that could explain the problem of small scale structure, where a discrepancy between collisionless cold DM and observational data was found [3]. Moreover, having multiple DM particles may provide interesting solutions for avoiding stringent constraints imposed nowadays from negative searches for DM at Direct Detection (DD) and Indirect Detection (ID) experiments and also at the Large Hadron Collider (LHC).A DM candidate is natural in the context of Supersymmetry (SUSY) with so-called R-parity conservation [4]. However, the minimal version of SUSY, the so-called Minimal Supersymmetric Standard Model (MSSM), contains only one DM candidate that has been widely studied in the literature. However, the combined LHC and relic abundance constraints rule out most of the MSSM parameter space except very narrow regions. Therefore, nonminimal SUSY models with a richer structure than the MSSM and hallmark signatures, such as the Exceptional Supersymmetry Standard Model (E 6 SSM) of Refs. [5][6][7], including in its constrained version [8][9][10][11], may provide new DM candidates that account for the observed relic density without a conflict with other experimental constraints. The E 6 SSM is a string inspired SUSY scenario with an E 6 gauge group. The E 6 gauge symmetry prevailing at the scale of a Grand Unification Theory (GUT) is then broken via1) N at lower energies. At such scales, wherein the E 6 SSM is essentially a Standard Model (SM) × U (1) N effective description from the viewpoint of a gauge theory, extra Right-Handed (RH) neutrinos are uncharged under U (1) N and can then acquire large intermediate scale Majorana masses leading to a Type-I see-saw mechanism to explain the small Left-Handed (LH) neutrino masses [12].In the E 6 SS...