Abstract
We consider a minimal natural supersymmetric model based on an extra dimension with supersymmetry breaking provided by the Scherk-Schwarz mechanism. The lightest supersymmetric particle is a neutral, quasi-Dirac Higgsino and, unlike in previous studies, we assume that all Standard Model fields are propagating in the bulk. The resulting setup is minimal, as neither extra matter, effective operators, nor extra $U(1)$ groups are needed in order to be viable. The model has three free parameters which are fixed by the Higgsino mass -- set to the range 1.1-1.2 TeV so it can play the role of Dark Matter, and by the requirements of correct electroweak breaking and the mass of the Higgs. After imposing the previous conditions we find a benchmark scenario that passes all experimental constrains with an allowed range for the supersymmetric parameters. In particular we have found gluinos in the range 2.0-2.1 TeV mass, electroweakinos and sleptons almost degenerate in the range 1.7-1.9 TeV and squarks degenerate in the range 1.9-2.0 TeV. The best discovery prospects are: i.) gluino detection at the high luminosity LHC ($\gtrsim 3\, \text{ab}^{-1}$), and ii.) Higgsino detection at next-generation dark matter direct detection experiments. The model is natural, as the fine-tuning for the fixed values of the parameters is moderate mainly because supersymmetry breaking parameters contribute linearly to the Higgs mass parameter, rather than quadratically as in most models.
Highlights
In spite of its experimental elusiveness, low-scale supersymmetry still remains as the most complete and best motivated beyond the Standard Model (BSM) theory.1 On top of solving the naturalness problem, supersymmetric theories with R parity conservation have naturally candidates for thermal dark matter (DM), the neutralinos
The lightest supersymmetric particle is a neutral, quasi-Dirac Higgsino and, unlike in previous studies, we assume that all Standard Model fields are propagating in the bulk
The model has three free parameters which are fixed by the Higgsino mass—set to the range 1.1–1.2 TeV so it can play the role of dark matter, and by the requirements of correct electroweak breaking and the mass of the Higgs
Summary
In spite of its experimental elusiveness, low-scale supersymmetry still (arguably) remains as the most complete and best motivated beyond the Standard Model (BSM) theory. On top of solving the naturalness problem, supersymmetric theories with R parity conservation have naturally candidates for thermal dark matter (DM), the neutralinos. Unlike previous studies [12,13,14,15], the considered model is a 5D supersymmetric theory with all matter and gauge fields in the bulk It has three free parameters: the compactification scale 1=R, the supersymmetry breaking masses proportional to a real parameter qR and a supersymmetric mass in the Higgs sector proportional to another real parameter qH [12,13,14]. We find that for certain values of the parameters in the (qR, 1=R) plane, the (bulk propagating) stop sector is capable of radiatively triggering electroweak breaking—much as it happens in the minimal supersymmetric standard model (MSSM) for high-scale supersymmetry breaking—despite the fact our model has a low supersymmetry breaking scale.
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