Abstract
We investigate a so-called 331 extension of the Standard Model gauge sector which accommodates neutrino masses and where the lightest of the new neutral fermions in the theory is a viable particle dark matter candidate. In this model, processes mediated by the additional $Z^{\prime}$ gauge boson set both the dark matter relic abundance and the scattering cross section off of nuclei. We calculate with unprecedented accuracy the dark matter relic density, including the important effect of coannihilation across the heavy fermion sector, and show that indeed the candidate particle has the potential of having the observed dark matter density. We find that the recent LUX results put very stringent bounds on the mass of the extra gauge boson, $M_{Z^{\prime}} \gtrsim 2$~TeV, independently of the dark matter mass. We also comment on regime where our bounds on the $Z^{\prime}$ mass may apply to generic 331-like models, and on implications for LHC phenomenology.
Highlights
Dimensions [5,6,7,8], Little Higgs Models [9,10], 331 models [11,12,13,14], and minimal extensions of the Standard Model (SM) [15]
We focus on the dark matter phenomenology of a special class of theories, the so-called 331 models, whose phenomenology has been studied in great detail from various particle physics standpoints, but not as far as dark matter searches are concerned
S1 and S2 are new scalars particles added to the SM and have masses proportional to the scale of symmetry breaking of the model vχ, while H is identified with the SM Higgs boson.√The vev v which appears in Eq (12) must be equal to 246/ 2 GeV, in order to reproduce the masses of the Z and W bosons
Summary
Dimensions [5,6,7,8], Little Higgs Models [9,10], 331 models [11,12,13,14], and minimal extensions of the SM [15]. In the present study we accurately calculate the dark matter thermal relic density, including new processes that have never been included in this context before (namely, coannihilation in the heavy fermion sector) and we derive stringent bounds on the mass of the Z gauge boson by comparing the predicted scattering cross section off of nuclei with the most current limits from LUX [76] and XENON100 [77] These bounds we discuss here apply, up to some extent, to other extensions of the so called minimal 331 models in the sense that singlet neutral fermions are the most natural dark matter candidates in those models.
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