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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
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Long-Lived Gluinos and Stable Axinos.
1Department of Physics, The Ohio State University, 191 West Woodruff Avenue, Columbus, Ohio 43210, USA.
Physical Review Letters
|December 20, 2015
Summary
This study introduces long-lived gluinos in supersymmetric models, potentially lowering mass bounds to under 1000 GeV. Detecting decaying R hadrons offers the best limits, with axinos as dark matter candidates.
Area of Science:
- High Energy Physics
- Particle Physics
- Cosmology
Background:
- Supersymmetric (SUSY) models predict new particles, including gluinos.
- The properties and detection of long-lived particles are crucial for understanding beyond-the-Standard-Model physics.
- Previous constraints on gluino masses were significant.
Purpose of the Study:
- To present a novel scenario for "long-lived" gluinos in supersymmetric models.
- To explore reduced mass bounds for gluinos when they are the lightest ordinary supersymmetric particle (LOSP).
- To identify optimal detection strategies for these long-lived gluinos.
Main Methods:
- Investigating supersymmetric models where the gluino is the lightest ordinary supersymmetric particle (LOSP) and the axino is the lightest supersymmetric particle.
- Analyzing the impact of the axion decay constant (f_{a}) on gluino mass bounds.
- Simulating the detection of decaying R hadrons, specifically gluino decays to a gluon and axino in calorimeters.
Main Results:
- Gluino mass bounds can be reduced to below 1000 GeV for specific axion decay constant ranges (f_{a}<1×10^{10} GeV).
- Decaying R hadrons, with gluinos decaying into a gluon and axino, provide the most effective limits.
- The gluino LOSP scenario is viable in mirage mediation and general gauge-mediated SUSY breaking models.
Conclusions:
- The proposed scenario allows for lighter gluinos than previously constrained.
- Detecting decaying R hadrons is a promising experimental approach for discovering these particles.
- In this framework, axions or axinos emerge as viable dark matter candidates.
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