1 / 23

…AT THE LHC

DARK MATTER …. …AT THE LHC. Alan Barr University of Oxford. On behalf of the ATLAS and CMS collaborations. PASCOS 2009 DESY 9 July 2009.

natan
Télécharger la présentation

…AT THE LHC

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. DARK MATTER … …AT THE LHC Alan BarrUniversity of Oxford On behalf of the ATLAS and CMScollaborations PASCOS 2009 DESY 9 July 2009

  2. You may have noticed there is a new collider starting operation

  3. 1/α +SUSY Log10 (μ / GeV) The value of prejudice rapidly decreasing stop higgs higgs Motivation

  4. Proton-proton controlled environment up to 14 TeV 109 collisions/second ~ decade operation The machine … ATLAS CMS 26.659 km circumference 9300 magnets Four experiments(two general purpose)

  5. Segment of 4π detector

  6. CMS Beam splash2008-09-10

  7. Events… From Steve Meyers More info: http://indico.cern.ch/conferenceDisplay.py?confId=62277

  8. Complete “event” Decay part Time heavyexotic lighterexotic standard Time = exotic = standard Dark Matter … Z2 ? Production part standard • Events build from blobs with 2 “exotic legs” • A pair of cascade decays results • Complicated end result 2 exotics Time Candidates include: {Supersymmetry, UED, Little Higgs}+ appropriate parity

  9. Example SUSY search Mass (GeV) Missing energy + Jets • Assume R-parity • Look for: • Jets from squark & gluino decays • Leptons from gaugino & slepton decays • Missing energy from (stable) LSPs “Typical” SUSY spectrum

  10. Prospino Cross-sections etc “Rediscover” Lower backgrounds WW ZZ “Discover” Higher backgrounds

  11. Caveats • Current public results mostly: • √S = 14 TeV • ∫L ≥ 1 fb-1 • no pile-up† • Initial conditions will be different • Work in progress for smaller √S, ∫L • 10 TeV • 10-100 pb-1 †some CMS physics TDR results include 5 pile-up events

  12. Signal BG Example 4 jet + pT distribution Typical search: inclusive distributions • Jet pT > {100, 50,50,50} GeV • pT > 100 GeV • pT > 0.2 meff • ST > 0.2 • Δφ(pT,j) > 0.2j = {1,2,3} • No e or μ • meff > 800 GeV

  13. Statistics limited Also use: W (μ) + jet γ + jet R: Z -> ννB: EstimatedR: Estimated • Measure in Z -> μμ • Use in Z -> νν Standard Model backgrounds

  14. W, t backgrounds Good match to “true” background Search region Control Region These are examples onlyLots of detail about Z, top, QCD, detectorBGs in further reading

  15. Multiple channels for discovery 1 fb-1, 14 TeV 1 fb-1, 14 TeV Systematics include BG determination Different final states accessible Below the lines = discovered

  16. SUS-08-001 Measuring masses • Large literature exists • Practical methods will be put to the test mll = ½ mllmax (1 – cos θ) • l+l- : pT > 10 GeV, |η|<2.4 • 3 jets |η|<3 ET>120,80,30 GeV • pTmiss > 200 GeV

  17. “Predict” relic density of observed LSPs Caveats: lifetimes beyond detector? optimistic case (light sparticles) many annihilation modes need to be checked Dark matter relic density? f f PoleselloTovey Drees, Kim, Nojiri hep-ph/0007202 Polesello, Tovey hep-ph/0403047 (cMSSM) Nojiri, Polesello, Tovey hep-ph/0512204 (MSSM) Moulin et al. arXiv:0712.3151 (Focus point)

  18. To find out more… CMSCERN-LHCC-2006-021J.Phys.G34:995-1579,2007 ATLASCERN-OPEN-2008-020arXiv:0901.0512 • New results will appear at: • https://twiki.cern.ch/twiki/bin/view/CMS/PhysicsResults • https://twiki.cern.ch/twiki/bin/view/Atlas/AtlasResults • Results for EPS and summer conferences in progress

  19. Conclusions

  20. Extras

  21. Et(miss) Lesson from the Tevatron Importance of detailed detector understanding • Simulation shows events with large fake missing energy • Vital to remove these in missing energy tails • Large effort in physics commissioning

  22. Neutralino spin from angles in decay chains ~ l+ _ q q θ ~ l- Spin measurements… Slepton spin from angles in Drell-Yan production

More Related