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SUSY Measurements w i th ATLAS: Hadron ic Signatures and Focus Point

SUSY Measurements w i th ATLAS: Hadron ic Signatures and Focus Point. Outline. Tommaso Lari Università and INFN Milano On Behalf of the ATLAS Collaborat ion. Reconstruct ion of glu i no , r ight-handed squar ks and 3 rd generat ion squar k s for some low-mass mSUGRA benchmar k po i nts

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SUSY Measurements w i th ATLAS: Hadron ic Signatures and Focus Point

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  1. SUSY Measurements with ATLAS:Hadronic Signatures and Focus Point Outline Tommaso Lari Università and INFN Milano On Behalf of the ATLAS Collaboration • Reconstruction of gluino, right-handed squarks and 3rd generation squarks • for some low-mass mSUGRA benchmark points • First study of gluino decays in the focus-point region

  2. Bulk and Focus Point regions tanb=10 A0=0 m>0 mt=175 GeV Green: Regions of mSUGRA parameter space that give an acceptably low density of relic neutralinos 1st part of the talk Bulk low-mass:Several well-studied benchmark points 2nd part of the talk Focus Point: Studies started more recently. M1/2(GeV) Coannihilation Focus Point Bulk M0(GeV) H. Baer and C. Balazs, arXiv:hep-ph/0303114 T. Lari SUSY measurements with ATLAS: hadronic signatures

  3. Possible SUSY timeline • Phase 1- Discovery: See excess of events with large missing energy, make sure they are from New Physics • Phase 2 - First SUSY masses: Reconstruction of leptonic decays, combine lepton with jets • G. Comune’s talk • Phase 3 - More SUSY masses: Combine with b-jets and reconstructed tops. Purely hadronic final states. • This talk T. Lari SUSY measurements with ATLAS: hadronic signatures

  4. p p ~ c01 ~ ~ ~ q ~ c02 l g q q l l lq edge llq edge 1% error (100 fb1) 1% error (100 fb-1) Phase 2: a typical decay chain Other possibilities: c02 → c01 l+l- c02→ c01 h→ c01bb ~ ~ ~ ~ ~ The invariant mass of each combination has a minimum or a maximum which provides one constraint on the masses of c01 c02l q ~ ~ ~ ~ LHCC Point 5 ATLAS TDR ATLAS TDR ATLAS TDR ATLAS TDR llq threshold ll edge T. Lari SUSY measurements with ATLAS: hadronic signatures

  5. Sparticle Expected precision (100 fb-1) qL 3% 02 6% lR 9% 01 12% ~ ~ ~ ~ Model-independent masses • Combine measurements from edges from different jet/lepton combinations to obtain ‘model-independent’ mass measurements. ~ ~ c01 lR ~ ~ ~ ATLAS ~ ~ ~ c02 qL T. Lari SUSY measurements with ATLAS: hadronic signatures

  6. Going up the decay chain ~ • Once the mass of the c01 is known, it is possible to get the momentum of the c02 using the approximate relation p(c02) = ( 1-m(c01)/m(ll) ) pll valid for lepton pairs with invariant mass near the edge. • The c02 can be combined with b-jets to reconstruct the gluino mass peak: g → bb → bbc02 ~ ~ ~ ~ ~ ~ ~ Example: SPS1a B.K.Gjelsten et al., ATL-PHYS-2004-007 M0 = 100 GeV M1/2 = 250 GeV Tan b = 10 A = -100 GeV m > 0 ~ M(g) = 611 GeV M(b1) = 515 GeV M(b2) = 539 GeV M(c02) = 177 GeV ~ ~ ~ ATLAS - ATL-PHYS-2004-007 T. Lari SUSY measurements with ATLAS: hadronic signatures

  7. Gluino and sbottom reconstruction ATLAS - ATL-PHYS-2004-007 Good combinations. m(g) and m(b) correlated (Dominant error from c02 Momentum affects both) ~ ~ ~ ~ Bad c02 b combinations (b-jet is from gluino decay) T. Lari SUSY measurements with ATLAS: hadronic signatures

  8. Gluino mass reconstruction ATLAS ATL-PHYS-2004-007 ATLAS ATL-PHYS-2004-007 Reconstructed gluino mass. Width dominated byc02 momentum. Gluino mass as a function of the assumedc01 mass. ~ ~ ~ ~ m(g)-0.99m(c01) = (500.0 ± 6.4) GeV with 300 fb-1 Error is statistical plus 1% uncertainty on jet energy scale Central value 10 GeV lower than nominal because b-jet energy underestimated T. Lari SUSY measurements with ATLAS: hadronic signatures

  9. sbottom mass ~ ~ m(c02 bb) and m(c02 b) strongly correlated : use the difference ATLAS ATL-PHYS-2004-007 ATLAS ATL-PHYS-2004-007 300 fb-1 300 fb-1 ~ ~ With 300 fb-1 it should be possible to separate the b1 and b2 peaks ~ ~ ~ ~ m(g)-m(b1) = (103.3 ± 1.8) GeV m(g)-m(b2) = (70.6 ± 2.6) GeV With lower statistics only measure the average T. Lari SUSY measurements with ATLAS: hadronic signatures

  10. Right-handed squark ~ qR does not couple to Wino c01 is nearly a Bino c02 is nearly a Wino ~ ~ ~ qR → q c01 ~ ATLAS ATL-PHYS-2004-007 Combine the transverse momentum of two leading jets with missing transverse momentum as follows: 30 fb-1 ~ ~ Maximum of this variable is m(qR)-m(c01) ~ ~ m(qR)-m(c01) = (424.2 ± 10.9) GeV ~ ~ Note: can reconstruct lL→ l c01 with same technique ~ ~ m(lL)-m(c01) = (106.1 ± 1.6) GeV T. Lari SUSY measurements with ATLAS: hadronic signatures

  11. Purely hadronic final states ~ ~ ~ ~ ~ ~ Aim is to reconstruct g → tt1 → tbc±1 or g → bb → bt c±1 ~ ~ ~ ~ tb invariant mass has a maximum function of the masses of g, b(or t) andc±1 Two closely spaced edges from the two decays: can measure a weighed average. ATLAS • Selections: • - total jet energy and missing energy • 2 b-jets • lepton veto • 4 to 6 non-b jets Reconstruction: - m(jj) close to m(W) - m(jjb) close to m(t) - W-sidebands to estimate and subtract combinatorial background See J. Hisano et al., Phys. Rev. D68, 035007 for details T. Lari SUSY measurements with ATLAS: hadronic signatures

  12. Focus Point region Large scalar mass: heavy squarks and sleptons. Relatively low gaugino mass. Low m, large Higgsino/Bino mixing  low density of relic neutralinos, compatible with WMAP limits. The FP region has an high neutralino- nucleon cross section, so it will be probed by direct searches for dark matter. M1/2 (GeV) Focuspoint • Problems: • Very sensitive to top mass • Large discrepancies between SUSY mass • calculators Selected point for detailed study m0 = 3000 GeV M1/2 = 215 GeV Tanb = 10 A0 = 0 - m>0 M(top) = 175 GeV M0 (GeV) No EWSB solution T. Lari SUSY measurements with ATLAS: hadronic signatures

  13. Mass spectrum • Heavy squarks and leptons. • Heavy Higgs (except h) • Lighter gluino (640 GeV) decays into charginos and neutralinos ISAJET 7.69 T. Lari SUSY measurements with ATLAS: hadronic signatures

  14. Production x-Section Meff = Jet energy + ETmiss ~ ~ ATLAS ~ ~ ~ ~ • Neutralino/chargino production • abundant but without jet/missing • energy signature (mass similar or • lower than top mass). • Gluino pair production followed by • decay into chargino/neutralino is • dominant after cuts to reject SM • squarks still visible with • enough luminosity The gluino decays to chargino or neutralino via three-body decays: ~ ~ g→ cqq T. Lari SUSY measurements with ATLAS: hadronic signatures

  15. Dilepton analysis ~ ~ ~ ~ ~ ~ c02 → c01 ll c03 → c01 ll Direct three-body decay c0n → c01 ll Edge gives m(c0n)-m(c01) Z0→ ll ~ ~ ATLAS ATLAS 30 fb-1 30 fb-1 Combination with jets to reconstruct the gluino mass is under study. T. Lari SUSY measurements with ATLAS: hadronic signatures

  16. Gluino to chargino decay ~ ~ g → ctb Direct three-body decay: ATLAS 30 fb-1 ~ ~ m(g)-m(c1) = 530 GeV T. Lari SUSY measurements with ATLAS: hadronic signatures

  17. Conclusions • After the mass of the LSP has been measured with kinematic edges, the mass peaks of heavier particles can be reconstructed. • A detailed analysis has been performed for point SPS1a: a large number of SUSY masses can be measured with a precision of 5 to 12 GeV with a statistics of 300 fb-1. • The same reconstruction techniques can be used for other regions of parameter space. • Most studies done with fast simulation (parameterized detector response) so far. Analysis with detailed detector simulation has been started. • New regions of parameter space, guided by relic density constraints, are also an hot topic. A detailed characterization of the selected point in the focus point region is being made. T. Lari SUSY measurements with ATLAS: hadronic signatures

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