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Updated: Mar 30, 2026

Setting Limits on Supersymmetry Using Simplified Models
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Supersymmetric dark matter after LHC run 1.

E A Bagnaschi1, O Buchmueller2, R Cavanaugh3

  • 1DESY, Notkestraße 85, 22607 Hamburg, Germany.

The European Physical Journal. C, Particles and Fields
|November 7, 2015
PubMed
Summary

Different mechanisms explain dark matter (DM) relic density within the Minimal Supersymmetric Standard Model (MSSM). Future LHC and direct detection experiments will probe these DM mechanisms, complementing each other in exploring parameter space.

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Area of Science:

  • Particle Physics
  • Cosmology
  • Astrophysics
  • Supersymmetry (SUSY) Phenomenology

Background:

  • The lightest neutralino, a potential dark matter (DM) particle, must satisfy relic density constraints within the Minimal Supersymmetric Standard Model (MSSM).
  • Various mechanisms, including coannihilation, resonant annihilation, and focus-point enhancements, influence the neutralino's relic density across different MSSM parameter spaces.

Purpose of the Study:

  • To analyze how future Large Hadron Collider (LHC) and direct dark matter detection experiments can probe diverse DM mechanisms within specific MSSM scenarios.
  • To investigate the complementary roles of collider and direct detection searches in exploring the parameter space of constrained models (CMSSM, NUHM1, NUHM2) and a more general scenario (pMSSM10).

Main Methods:

  • Examination of different DM production mechanisms: coannihilation (e.g., with stau, stop, chargino), resonant annihilation (via Higgs bosons H/A, h, or Z boson), and focus-point region enhancement.
  • Analysis of MSSM scenarios including CMSSM, NUHM1, NUHM2, and pMSSM10.
  • Assessment of the reach of future LHC searches (e.g., for specific event signatures and long-lived particles) and direct DM detection experiments (e.g., LZ, Darwin).

Main Results:

  • For CMSSM, NUHM1, and NUHM2, the LHC can largely probe [Formula: see text] coannihilation regions via specific event searches and long-lived charged particle detection.
  • The H/A funnel, focus-point, and [Formula: see text] coannihilation regions in CMSSM, NUHM1, and NUHM2 are largely accessible to LZ and Darwin direct detection experiments.
  • In the pMSSM10 scenario, [Formula: see text] coannihilation is the dominant DM mechanism, with parts of its parameter space accessible to the LHC and a larger portion to future direct DM searches.

Conclusions:

  • Future LHC and direct DM detection experiments offer complementary probes of various dark matter mechanisms within different MSSM frameworks.
  • The combined power of collider and direct detection searches is crucial for a comprehensive exploration of the supersymmetric parameter space and its implications for dark matter.
  • Specific experimental strategies, like searching for [Formula: see text] events at the LHC or utilizing direct detection experiments like LZ and Darwin, are vital for testing distinct DM scenarios.