Abstract

In the mu nu SSM, the presence of R-parity violating couplings involving right-handed (RH) neutrinos solves simultaneously the mu - and nu -problems. We explore extensions of the mu nu SSM adding a U(1)' gauge group, which provides the RH neutrinos with a non-vanishing charge. In these models, dubbed Umu nu SSM, the anomaly cancellation conditions impose the presence of exotic quarks in the spectrum that are vector-like under the standard model (SM) gauge group: either three pairs SU(2) quark singlets, or a pair of quark singlets together with a pair of quark doublets. Several singlets under the SM group can also be present, with the U(1)' charges making distinctions among them, and therefore allowing different types of couplings. Some of these singlets dynamically generate Majorana masses for the RH neutrinos, and others can be candidates for dark matter. The useful characteristics of models with U(1)'s are also present in Umu nu SSM models: baryon-number-violating operators as well as explicit Majorana masses and mu terms are forbidden, and the domain wall problem is avoided. The phenomenology of Umu nu SSM models is very rich. We analyze the experimental constraints on their parameter space, specially on the mass and mixing of the new Z' boson. In addition to the exotic quarks, which can hadronize inside the detector or decay producing SM particles, the Umu nu SSM models can also have new signals such as decays of the Z' to sparticle pairs like right sneutrinos, charginos or neutralinos. Besides, Z' and Higgs mediated annihilations and interactions with the visible sector of WIMP dark matter particles, can also be present.

Highlights

  • Where the summation convention is implied on repeated indexes, with i, j, k = 1, 2, 3 the usual family indexes of the standard model (SM), and i = 1, ....nνc, with nνc the number of RH neutrinos

  • In order to study the phenomenology associated to superpotentials (11) and (12), it is enough to consider the simple case of no mixing between generations, as well as in the corresponding soft terms (49) and (51), respectively, and to assume that only one generation of sneutrinos and of a√dditional√singlets√under th√e SM gauge group get vacuum expectation values (VEVs): vL / 2, vR/ 2, vS/ 2, vN / 2

  • Rb = RbSM [1 − 1.81δcbL + 0.33δcbR − 0.42δccL + 0.19δccR], Once we have shown in the previous section that UμνSSM models are phenomenologically viable, with reasonable lower bounds on the Z mass that depend on the parameter space analyzed, let us discuss other type of signals that could be relevant for its detection

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Summary

The superpotential of UμνSSM models

There, apart from the exotic quarks, only two RH neutrinos are present In these cases, since in UμνSSM models the couplings κi j νkc are forbidden, the useful outcome of the μνSSM where Majorana masses are dynamically generated cannot be obtained. Once the Ssuperfields are present, we will show that it is helpful for the anomaly cancellation conditions to be fulfilled, to allow the presence of other singlets under the SM gauge group Nwith different U (1) charges. They can be used as an additional source of masses for the Sfields. This implies that a given solution for the U (1) charges of a given number of fields applies for other constructions with the number of fields related by Eq (45)

Building UμνSSM models
The scalar potential
Masses and mass mixings
Present bounds
Constraints from the LHC
Indirect limits
Conclusions
Full Text
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