LHC and SUSY Aug 2010 results, implications for string theory

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SUMMARY

The LHC has effectively ruled out significant portions of the supersymmetry (SUSY) parameter space, particularly concerning gluinos with masses exceeding 205 GeV, as detailed in the ATLAS results published on August 2, 2010. The findings indicate that if SUSY gluinos were detected, it would significantly bolster string theory and supergravity models beyond the Standard Model. Current limits suggest that gluinos may extend up to approximately 295 GeV, surpassing the Tevatron's capabilities. The implications of these results are critical for ongoing research in high energy physics and dark matter detection.

PREREQUISITES
  • Understanding of LHC experimental methodologies
  • Familiarity with supersymmetry (SUSY) concepts
  • Knowledge of high energy physics phenomenology
  • Basic principles of dark matter detection techniques
NEXT STEPS
  • Review the ATLAS results on SUSY searches in detail
  • Explore the implications of gluino mass limits on string theory
  • Investigate the role of dark matter detectors like CDMS II in SUSY research
  • Study the differences between MSSM, NMSSM, and nMSSM models
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Physicists, researchers in high energy physics, and anyone involved in theoretical physics, particularly those focused on supersymmetry and its implications for dark matter and string theory.

ensabah6
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LHC thus far has ruled out some of the SUSY parameter space over and above Tev, esp gluinos above a certain mass.

So LHC has offered some useful research into SUSY. Were SUSY gluinos detected it would be a huge boost to strings/Supergravity Beyond the Standard Model

http://arxiv.org/abs/1008.0407

High Energy Physics - Phenomenology
Title: It's On: Early Interpretations of ATLAS Results in Jets and Missing Energy Searches
Authors: Daniele S. M. Alves, Eder Izaguirre, Jay G. Wacker
(Submitted on 2 Aug 2010)

Abstract: The first search for supersymmetry from ATLAS with 70/nb of integrated luminosity sets new limits on colored particles that decay into jets plus missing transverse energy. For gluinos that decay directly or through a one step cascade into the LSP and two jets, these limits translate into a bound of m_g > 205 GeV, regardless of the mass of the LSP. In some cases the limits extend up to m_g ~= 295 GeV, already surpassing the Tevatron's reach for compressed supersymmetry spectra.

Comments: 5 pages, 3 figures, 1 table
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Experiment (hep-ex)
Cite as: arXiv:1008.0407v1 [hep-ph]LHC is not only experimental search for SUSY, dark matter detectors also weigh inhttp://arxiv.org/abs/1005.0761
SUSY dark matter in light of CDMS II results: a comparative study for different models
Authors: Junjie Cao, Ken-ichi Hikasa, Wenyu Wang, Jin Min Yang, Li-Xin Yu
(Submitted on 5 May 2010)

Abstract: We perform a comparative study of the neutralino dark matter scattering on nucleon in three popular supersymmetric models: the minimal (MSSM), the next-to-minimal (NMSSM) and the nearly minimal (nMSSM). First, we give the predictions of the elastic cross section by scanning over the parameter space allowed by various direct and indirect constraints, which are from the measurement of the cosmic dark matter relic density, the collider search for Higgs boson and sparticles, the precision electroweak measurements and the muon anomalous magnetic moment. Then we demonstrate the property of the allowed parameter space with/without the new limits from CDMS II. We obtain the following observations: (i) For each model the new CDMS limits can exclude a large part of the parameter space allowed by current collider constraints; (ii) The property of the allowed parameter space is similar for MSSM and NMSSM, but quite different for nMSSM; (iii) The future SuperCDMS can cover most part of the allowed parameter space for each model.
 
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ensabah6 said:
The first search for supersymmetry from ATLAS with 70/nb of integrated luminosity
Still no sign of supersymmetry, now with a million times more integrated luminosity and higher energy. If it exist it must be at higher energies or have a really weak coupling to our matter.
 

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