Abstract

We present simplified MSSM models for light neutralinos and charginos with realistic mass spectra and realistic gaugino-higgsino mixing, that can be used in experimental searches at the LHC. The formerly used naive approach of defining mass spectra and mixing matrix elements manually and independently of each other does not yield genuine MSSM benchmarks. We suggest the use of less simplified, but realistic MSSM models, whose mass spectra and mixing matrix elements are the result of a proper matrix diagonalisation. We propose a novel strategy targeting the design of such benchmark scenarios, accounting for user-defined constraints in terms of masses and particle mixing. We apply it to the higgsino case and implement a scan in the four relevant underlying parameters {mu , tan beta , M_{1}, M_{2}} for a given set of light neutralino and chargino masses. We define a measure for the quality of the obtained benchmarks, that also includes criteria to assess the higgsino content of the resulting charginos and neutralinos. We finally discuss the distribution of the resulting models in the MSSM parameter space as well as their implications for supersymmetric dark matter phenomenology.

Highlights

  • Standard Model, feature gauge coupling unification at high energy and generally include a natural explanation for the presence of dark matter in the universe

  • We present simplified Minimal Supersymmetric Standard Model (MSSM) models for light neutralinos and charginos with realistic mass spectra and realistic gaugino-higgsino mixing, that can be used in experimental searches at the LHC

  • The simplified model that we investigate in this work takes the gaugino-higgsino sector from the MSSM in all its complexity, as it is defined by supersymmetry and gauge invariance

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Summary

Introduction

Standard Model, feature gauge coupling unification at high energy and generally include a natural explanation for the presence of dark matter in the universe. When one targets next-to-minimal simplified models where a mass splitting between the second-lightest state and its neighbours is introduced, some amount of mixing between the different gaugino and higgsino fields must be included in order to maintain viability with respect to the initial MSSM motivation This concerns in particular identities guaranteed by gauge invariance and/or supersymmetry that could be violated when one tweaks by hand masses and mixing matrix elements, like in the above-mentioned wino set of simplified models. We define a strategy to efficiently scan this four-dimensional parameter space for given sets of light neutralino and chargino masses, that allows to maximise the gaugino or higgsino content, couplings to certain sparticles etc This procedure allows to find approximate solutions for simplified MSSM models that have a realistic and properly defined gauginohiggsino sector in contrast to many of the overly simplified models studied so far.

Theoretical definitions with
Symmetry transformations
Mass spectra and gaugino-higgsino content
Parameter space exploration
Benchmark selection
Generalisation
Case study
Definition of the simplified model
Quality of the scan
MSSM scenarios
The Higgs-stop sector
Q 3 and
Implications on dark matter
Findings
Conclusion

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