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SUSY at LEP2 (third generation and ewinos)
LEP2, data What were we searching for? What have we learned from not finding anything.. MSSM with neutralino LSP MSSM + 4 more constraints "mSUGRA" or " CMSSM" MSSM + (1 -2) more constraints (MSSM +)
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The MSSM tan v2/v1
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Mass relations in MSSM+
Gauge unification and ..... Sfermion unification Gauginos and squarks are related now, we can use charginos to set a limit on squarks and sleptons, and sleptons to set limits on charginos Mixing -> mass splitting for stop and , sbottom and stau A - /tan , A - tantan t b
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Backup * ALEPH Collaboration, "Search for scalar quarks in e+e- collisions at sqrt(s) up to 209 GeV", Phys. Lett. B537 (2002) 5-20; * DELPHI Collaboration, " Searches for supersymmetric particles in e+e- collisions up to 208 GeV and interpretation o f the results within the MSSM", Eur. Phys. J. C31 (2003) ; * L3 Collaboration, "Search for Scalar Leptons and Scalar Quarks at LEP", Phys. Lett. B580 (2004) 37-49; * OPAL Collaboration, "Search for Scalar Top and Scalar Bottom Quarks at LEP" Phys. Lett. B545 (2002)
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Backup slides Centre-of-Mass Energy ALEPH DELPHI L3 OPAL
191.6 GeV 195.6 GeV 199.6 GeV 201.6 GeV 205 GeV 206.6 GeV 208.1 GeV
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e e mass of the selectron neutralino mass Searches for sleptons e
R,L l Produced in the same way as leptons. x-section depends on mass and "handness". For selectron t-channel diagram introduces model dependence due to the neutralino mass and coupling. To be conservative we consider usually right-handed sleptons-smaller coupling e R,L / l e e R,L R,L low visibility of the final state if selectron mass close to the neutralino mass-> small e e large WW with W->e background mass of the selectron neutralino mass
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Background and signal x-sections
Background depends on M(SP)-M(LSP) two-photon for low M, four-fermion for high M "2 photon" Signal x-sections similar to the corresponding SM x-sections, due to same couplings WW Wino Wino ZZ Zino Zino (if selectron light) Higgsino Zino
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