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Updated: Dec 24, 2025

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Natural Twin Neutralino Dark Matter
Marcin Badziak1, Giovanni Grilli di Cortona1, Keisuke Harigaya2
1Institute of Theoretical Physics, Faculty of Physics, University of Warsaw, ul. Pasteura 5, PL-02-093 Warsaw, Poland.
Supersymmetric twin Higgs models offer a natural explanation for the electroweak scale and the lack of new particle discoveries at the Large Hadron Collider (LHC). These models also present a compelling dark matter candidate, a twin bino-like state, whose abundance matches observations without fine-tuning.
Area of Science:
- High Energy Physics
- Cosmology
- Particle Physics
Background:
- Supersymmetric twin Higgs models address the electroweak hierarchy problem and reconcile the absence of new particles at the LHC.
- These models introduce a mirror sector with identical gauge symmetries to the Standard Model.
Purpose of the Study:
- To investigate the potential of supersymmetric twin Higgs models to provide a natural dark matter candidate.
- To explore if a lightest supersymmetric particle (LSP) in the form of a twin bino-like state can explain the observed dark matter abundance.
Main Methods:
- Analysis of the freeze-out abundance of a twin bino-like lightest supersymmetric particle within the supersymmetric twin Higgs framework.
- Examination of the parameter space for consistency with dark matter observations and experimental constraints.
Main Results:
- The freeze-out abundance of a twin bino-like lightest supersymmetric particle naturally explains the observed dark matter abundance without requiring fine-tuning of the mass spectrum.
- A significant portion of the viable parameter space can be tested by future dark matter direct detection experiments and LHC searches for specific supersymmetric particles.
Conclusions:
- Supersymmetric twin Higgs models provide a compelling and natural dark matter solution.
- Future experimental searches at direct detection facilities and the LHC are crucial for probing these models and confirming the dark matter candidate.
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