What the LHC Will Teach Us About Low Energy Supersymmetry Darin Acosta representing ATLAS & Outline Introduction to SUSY, LHC, and the Detectors Trigger strategies at start-up Inclusive squark/gluino searches SUSY Spectroscopy Î Di-lepton edges Î squark and gluino reconstruction Summary SUSY at the LHC, Aspen 2003 2 D. Acosta, University of Florida Minimal SuperSymmetry SUSY Î Symmetry between bosons and fermions ~, ~l q Î Squarks/sleptons: scalar counterparts to the fermions ~± , χ ~0 ~ χ ÎCharginos/neutralinos/gluinos: 1,2 1,2,3, 4 , g fermion counterparts to SM gauge bosons ÎAt least two Higgs doublets (5 scalars): h, H 0 , A, H ± Î Avoids fine-tuning of SM, can lead to GUTs MSSM Î Usually consider RP ≡ (-1)3(B-L)+2S conserved ⇒ LSP is stable Î 105 new parameters mSUGRA: Î Require SUSY to be a local symmetry Î Universal gravitational interactions break SUSY at scale F ~ (1011 GeV)2 Î 5 free parameters Îm0 : Common scalar mass Îm1/2 : Common gaugino mass ÎA0 : Common scalar trilinear coupling Îtan β : Ratio of v.e.v. of Higgs doublets ÎSign(µ) : sign of Higgsino mixing parameter d i d i d i ~f M a g~f > M aq~f > M a χ ~± ≈ M χ ~ 0 ≈ 2M χ ~0 Î Typically: M χ 1 2 1 SUSY at the LHC, Aspen 2003 3 D. Acosta, University of Florida Large Hadron Collider (LHC) CMS ATLAS R = 4.5 km E = 7 TeV Two proton rings housed in same tunnel as LEP Design luminosity: L = 1034 cm–2s–1 = 100 fb-1/year (Pile up: ~20 collisions/crossing) Start-up luminosity: L ~ 1033 cm–2s–1 = 10 fb-1/year Completion: mid 2007 SUSY at the LHC, Aspen 2003 4 D. Acosta, University of Florida mSUGRA Cross Sections @ LHC q~, g~ m1/2 (GeV) Total cross section 1400 1 fb 1200 1000 10 fb TH 800 100 fb 600 1 pb 400 10 pb 200 EX A0 = 0 , tan β = 35 , µ > 0 0 0 500 1000 1500 2000 m0 (GeV) Î Squark/gluino production dominates the total cross-section for low energy SUSY Î Cross sections don’t vary much with µ, tanβ SUSY at the LHC, Aspen 2003 5 D. Acosta, University of Florida Detectors Tile CAL toroids 4T solenoid ATLAS LAr CAL 2T solenoid TRT and Si tracker muon Cu/Scin HCAL PbWO4 ECAL Full Si tracker Compact Muon Solenoid (CMS) SUSY at the LHC, Aspen 2003 6 D. Acosta, University of Florida SUSY Signatures Complex squark/gluino decay chains Î Many high-ET jets Î Heavy-flavor (τ and b, especially at large tanβ) Î Leptons Î From sleptons, charginos, W/Z, and b-jets Î Missing transverse energy (MET) Î From LSP and neutrinos from taus, sneutrinos Example: m0 = 1000 GeV m1/2 = 500 GeV tan β = 35 µ>0 A0 = 0 CMS event simulation SUSY at the LHC, Aspen 2003 7 D. Acosta, University of Florida Trigger Challenge Reduce 40 MHz bx rate (1 GHz pp) → O(100 Hz) Î Inclusive Jet Rate (cone algorithm, R=0.5): Full GEANT-based detector simulation on QCD background CMS DAQ Technical Design Report CERN/LHCC 2002-26 High lumi Low lumi Î Expected MET Rate: Recon. MET (hi lumi) Recon. MET (low lumi) Gen. MET (hi lumi) Gen MET (low lumi) Requiring a rate to tape of a ~few Hz implies an inclusive single jet threshold of 400–600GeV, and an inclusive MET threshold of 100–200 GeV Reconstructed MET rate below 100 GeV mainly from calorimeter energy resolution SUSY at the LHC, Aspen 2003 8 D. Acosta, University of Florida SUSY Trigger Exercise (CMS) Î Consider several points in the m0-m1/2 plane near the Tevatron reach (most difficult for LHC) (1 day of running) Î Consider points with and without Rp conservation ~0 → 3j χ Î For Rp choose most difficult case: 1 Î Run full GEANT-based detector simulation on SUSY signals and SM backgrounds to evaluate trigger performance Î Optimize efficiency for a rate to tape O(10 Hz) SUSY at the LHC, Aspen 2003 9 D. Acosta, University of Florida Example Trigger Strategy (CMS) Low luminosity case, L = 2×1033 cm-2s-1 Possible triggers at Level-2 (looser requirements at Level-1): Î 1 jet ET>180 GeV & MET>120 GeV Î 4 jets ET>110 GeV (values at 95% gen. effic.) Overall efficiencies to pass both trigger levels for the SUSY points are: Î ε=0.63, 0.63, 0.37, 0.43, 0.38, 0.23 4 5 6 4R 2nd jet 5R 6R With RP 1st jet Background rate of ~12Hz dominated by QCD More exclusive triggers involving angular correlations among objects can be added to further improve efficiency Trigger becomes more efficient at high luminosity since one expects to explore higher masses SUSY at the LHC, Aspen 2003 10 D. Acosta, University of Florida Lepton and Photon Triggers Differential Rate ( Hz/GeV/c 2 ) Anticipated thresholds by ATLAS and CMS for an initial luminosity of L = 2×1033 cm-2s-1 Î 1e: PT > 25 GeV Î 2e: PT > 15 GeV Î 1µ: PT > 20 GeV Î 2µ: PT > 10 GeV Î 1τ: PT > 85 GeV Î 2τ: PT > 60 GeV Î 1γ: PT > 60–80 GeV Î 2γ: PT > 20–40 GeV 10 L = 2x10 33 1 Minimum Bias Z/ γ* → µ + X 10 10 10 10 CMS tt→ µ+X -1 -2 -3 -4 0 20 40 60 80 100 120 140 160 180 200 2 µµ M inv ( GeV /c ) Di-muon invariant mass at Level-3 Sufficient handle on muon trigger rate: SUSY at the LHC, Aspen 2003 11 D. Acosta, University of Florida Fast Simulation Full simulation of signals and backgrounds like that shown for trigger exercise is too CPU intensive for complete SUSY reach determination Î Require O(108) events, but full GEANT simulation takes tens of minutes per event Î Use physics generators + parameterized detector performance ATLFAST: Î Tracks (µ): ∆PT/PT = 0.4PT ⊕ 1% (PT in TeV) Î EM resolution: σ/E ~ 10%/√E ⊕ 0.3% (E in GeV) Î Jet resolution: σ/E ~ 60%/√E ⊕ 2% (E in GeV) CMSJET: Î Tracks (µ): ∆PT/PT = 0.15PT ⊕ 0.5% (PT in TeV) Î EM resolution: σ/E ~ 5%/√E ⊕ 0.5% (E in GeV) Î Jet resolution: σ/E ~ 100%/√E ⊕ 5% (E in GeV) SUSY at the LHC, Aspen 2003 12 D. Acosta, University of Florida ~ g ~ Search Inclusive q, Counting excess events over SM background Î Discovery mode SUSY search at LHC Î Explicit sparticle reconstruction not done 6 Analyses: Î ETmiss: Î Ol: Î 1l: Î 2lOS: Î 2lSS: Î 3l: jets+MET, no lepton requirements no leptons 1 lepton 2 leptons, opposite sign 2 leptons, same sign 3 leptons CMS Study: Common cuts: Î MET>200 GeV, ≥2 jets, ETjet > 40 GeV, |η|<3 Lepton identification Î Electron: PT>20 GeV, isolated, |η|<2.4 Î Muon: PT>10 GeV, isolated or not, |η|<2.4 Vary cuts in 6 categories (~104 combinations) Î #Jets, MET, Jet ET, ∆φ(l,MET), Circ., µ Iso. Optimize S/√(S+B) in a counting experiment Î Probe 500 (m0, m1/2) points Î ~106 signal events, ~108 QCD, tt, W/Z+jets Plot 5σ sensitivity contours SUSY at the LHC, Aspen 2003 13 D. Acosta, University of Florida -1 1400 L dt = 100 fb A0 = 0 , tan β= 35 , µ > 0 ~ g(3000) miss ET 0l + 1l + 2l OS -1 (300 fb ) ) h(123 miss ET 1200 ISAJET 7.32 + CMSJET 4.5 m1/2 (GeV) ~ g ~ Reach CMS q, ~ g(2500) 0l 1l 1000 ~ ~ 25 q( q(2 0 ) 00 00) TH ~ g(2000) 2l OS 800 2l SS 3l ~ g(1500) 600 ~ q( ) 00 15 2 h =1 2 4 h = 0. ~ 400 g(1000) 0) 00 q(1 ~ 5 0.1 2 h = ~ ~ q(5 0 200 0) g(500) h(110) EX 0 0 500 1000 1500 2000 m0 ( GeV) Î Jets+MET search gives greatest sensitivity Î Opposite-sign leptons useful for sparticle recon. Nucl. Phys. B547 (1999) 60 SUSY at the LHC, Aspen 2003 14 D. Acosta, University of Florida m1/2 (GeV) Jets+MET Reach vs. Luminosity 1400 L dt = 1, 10, 100, 300 fb-1 A0 = 0 , tan β= 35 , µ > 0 ~ g(3000) miss ET miss ET 1200 CMS -1 (300 fb ) ) h(123 -1 (100 fb ) ~ g(2500) ~1 year @ L=1034 1000 ~ ~ 2 q( q(2 50 000 0) ) TH ~ g(2000) miss ET 800 -1 (10 fb ) ~1 year @ L=1033 ~ g(1500) 600 ~ miss 1 q( 0) 50 2 h =1 2 4 h = 0. ET -1 (1 fb ) ~1 month @L=1033 ~ 400 g(1000) 0) 00 ~ q(1 ~ 5 0.1 2 h = ~1 week @L=1033 200 ~ q(5 00) Tevatron reach < 0.5 TeV g(500) h(110) (but one year for sparticle 0 0 reconstruction) EX 500 1000 1500 2000 m0 ( GeV) Î Squarks/gluinos probed to ~1.5 TeV with 1 fb-1 Î Up to 2.5 TeV at design luminosity (100 fb-1) SUSY at the LHC, Aspen 2003 15 D. Acosta, University of Florida Other Parameter Choices ATLAS TDR 15 CERN/LHCC 99-15 L=10 fb–1 ~1 year @ L=1033 1l tan β = 10, µ < 0 0l 800 SS 600 3l OS 2l,0j 400 3l,0j 200 0 1l 0l 800 tan β = 10, µ > 0 3l SS 600 OS 400 2l,0j 3l,0j 200 0 0 500 1000 1500 2000 m0 (GeV) Î Similar cuts and optimization as for CMS study Î Sensitivity for lower tanβ also derived, but lower mass Higgs inconsistent with present limits SUSY at the LHC, Aspen 2003 16 D. Acosta, University of Florida R-Parity Violation Non-conservation of RP ≡ (-1)3(B-L)+2S leads to 3 new terms in SUSY superpotential: W = λ ijk Li L j Ekc + λ ijk ′ Qi L j Dkc + λ ijk ′′ Uic Lcj Dkc Choose most challenging of baryon number ~0 violation (last case): χ 1 → 3 j ATLAS Study of “Point 5” Î m0=100 GeV, m1/2=300 GeV, tanβ=2, µ>0, A0=300 Î MET is reduced, but still substantial Î Number of jets increases Î Leptons from neutralino decays 0.16 0.14 3 10 0.12 Probability Events/10 GeV/30 fb -1 Should still be able to explore much of the parameter space as with mSUGRA 2 10 0.10 0.08 0.06 0.04 0.02 10 0 0 200 400 600 800 1000 ETmiss (GeV) Figure 20-85 E Tmiss distribution for SUGRA Point 5 in the case of R-parity conservation (shaded histogram) and R-parity violation (empty histogram). SUSY at the LHC, Aspen 2003 17 0 2 4 6 8 10 12 14 16 18 20 Njet Figure 20-86 Total jet multiplicity ( p Tjet > 15GeV ) distribution for R-parity conservation (shaded) and Rparity violation at SUGRA Point 5. The jets are reconstructed using a topological algorithm based on joining neighbouring cells. D. Acosta, University of Florida Exclusive Di-Lepton Reconstruction Measure invariant mass distribution of same flavor leptons as evidence for ~0 → χ ~ 0 l + l − or χ ~ 0 → ~l + l − → χ 2 1 2 OS ~ 0l+l− χ 1 ~ 0 can be produced via Drell-Yan χ ~±χ ~0, χ 2 1 2 ~, g~ but more prevalent in cascade decays of q Endpoint in mass spectrum exhibits sharp edge: ~0 → χ ~ 0l+ l− χ 2 1 SUSY e+e− + µ+µ− SM background Events/4 GeV/30 fb −1 ATLAS “Point 4”: m0=800GeV m1/2=200GeV tanβ=10 µ>0 A0=0 L=30 fb–1 M( l+l−) (GeV) This point selected by: Some Z0 from other gauginos SM background is small Î Two OS leptons (e,µ), PT>(20,10) GeV, |η|<2.5 Î MET>200 GeV, 4 jets: PT1>100 GeV, PT234>50 GeV d i d i c hie c h d ii c h max ~0 − m χ ~0 =m χ 3-body decay endpoint: mll 2 1 2-body: m max = m 2 χ ~ 0 − m 2 ~l m 2 ~l − m 2 χ ~ 0 / m ~l ll 2 1 e d i SUSY at the LHC, Aspen 2003 18 D. Acosta, University of Florida Evolution of Di-Lepton Edges 104 m0 = 90 GeV, m1/2 = 220 GeV m~ χ2o = 164 GeV, me~R= 129 GeV m~ τ1 = 128 GeV 103 Events / 4 GeV m0 = 100 GeV, m1/2 = 190 GeV µ>0, A0 = 0 tanβ = 2 ~0 χ 2 103 m~ χ2o = 140 GeV, me~R= 132 GeV mτ1 = 124 GeV ~ eRe / ~ µR µ ee,µµ ee,µµ ~0 χ 2 ~ ~ eRe / µRµ ~0 ~ χ τ1 τ 2 102 5 fb-1 102 µ>0, A0 = 0 tanβ = 10 5 fb-1 eµ eµ 10 10 SM SM 1 0 1 100 200 + M(I I ) (GeV) 103 300 100 200 M(I+I-) (GeV) 0 103 m0 = 90 GeV, m1/2 = 220 GeV µ>0, A0 = 0 tanβ = 20 m~ χ20 = 167 GeV, me~R= 132 GeV m~ τ1 = 103 GeV ee,µµ 102 300 m0 = 100 GeV, m1/2 = 190 GeV µ>0, A0 = 0 tanβ = 25 102 m~ χ20 = 141 GeV, me~R= 132 GeV mτ1 = 91 GeV eµ 5 fb-1 5 fb-1 ee,µµ eµ SM 1 0 SM 1 100 200 300 D_D_2017c 10 10 0 M(I+I-) (GeV) 100 200 M(I+I-) (GeV) 300 Î SUSY may reveal itself early through peculiarities in the the di-lepton spectra Î Structures tend to be less evident with ~0 → χ ~ 0τ +τ − dominates increasing tanβ, where χ 2 1 SUSY at the LHC, Aspen 2003 19 D. Acosta, University of Florida Di-Tau Edge Reconstruction ATLAS Physics TDR study (Full GEANT simulation) to select hadronic tau decays Î Select narrow isolated jets: Rjet=0.2, Riso=0.4 Î Require 0.8 GeV < Mjet < 3.6 GeV Î Biased against 1-prong decays, but improves Mττ resolution (less neutrino momentum) Î Di-tau efficiency is 41% Î Mvis = 0.66 Mττ Additional event selection cuts Î 4 jets: ET1 > 100 GeV, ET2-4 > 50 GeV, Î MET>100 GeV, no e,µ leptons with pT>20 GeV ATLAS “Point 6”: m0=200GeV m1/2=200GeV tanβ=45 µ<0 A0=0 d Real τ from SUSY L=30 fb–1 Events/2.4 GeV/10 fb-1 i ~ 0 → ττ ~ = 99.9% BR χ 2 Fake τ from SUSY SM background 1000 500 0 0 25 50 75 Mττ (GeV) SUSY at the LHC, Aspen 2003 100 20 Mvis = 40 GeV Expected edge = 60 GeV D. Acosta, University of Florida Exclusive Sparticle Reconstruction Completely reconstruct a SUSY decay chain: p l b m ~ χ 20 ~ g ~± l ~ b p ATLAS Study ~ χ10 l± b ~ q ~~, qq ~~, gg ~~ dominate) ( qg Î “Point 3” of Physics TDR Îm0=200 GeV, m1/2=100 GeV, tanβ=2, µ<0, A0=0 CMS Study [Chiorboli] Î Investigate Points B & G of “Proposed Post-LEP Benchmarks for SUSY” (hep-ph/0106204) ÎB: m0=100 GeV, m1/2=250 GeV, tanβ=10, µ>0, A0=0 – σTOT(SUSY) = 58 pb ÎG: m0=120 GeV, m1/2=375 GeV, tanβ=20, µ>0, A0=0 – σTOT(SUSY) = 6.0 pb Î ISASUGRA→PYTHIA→CMSJET SUSY at the LHC, Aspen 2003 21 D. Acosta, University of Florida Di-Lepton Edge Reconstruction p l b ~ χ 20 ~ g ~± l ~ b BR=16% l± b ~ q p ~ χ10 m ~ 0 (tanβ not too large) Start with reconstructing χ 2 900 800 Point B Events / 2 GeV Events / 3 GeV Î Two OS isolated leptons, PT>15 GeV, |η|<2.4 Î MET>150 GeV, E(ll)>100 GeV SUSY - tt 700 Subtract opposite flavors Edge= 79±2 GeV 50 Z + jet 600 40 L=10 fb–1 CMS 500 400 30 300 20 200 10 100 0 0 25 50 75 100 125 150 175 200 0 M(e e )+M(µ µ ) (GeV) + - + - 0 20 40 60 80 100 120 140 160 180 200 M(e+e-)+M(µ+µ-)-M(e+µ-)-M(µ+e-) (GeV) Select 15 GeV window around di-lepton endpoint ~0 ~0 Î χ 1 at rest in χ 2 rest frame d i IJ pvdl l i d iK ~ from di - lepton endpoint and Can estimate md χ i ~ ≈ 2m χ md χ i d ~ i Point B: 174 GeV, F d i GH ~0 m χ 1 v ~0 p χ2 = 1+ m l+l− + − 0 1 0 2 0 1 but analysis not too sensitive to details SUSY at the LHC, Aspen 2003 22 D. Acosta, University of Florida ~ b Reconstruction p b ~ χ 20 ~ g ~± l ~ b p ~ χ10 lm l± b ~ q BR ~ 5% Add most energetic b-jet to reconstruct b Î Eb-jet>250 GeV, |η|<2.4 Î b-jet: ≥2 tracks with IP significance > 3σ Require Î MET>150 GeV Î E(ll)>100 GeV Point B Events / 28 GeV Result of fit: ~ = 500±7 GeV M(b) σM = 42 GeV 35 30 - tt P1 P2 P3 P4 P5 P6 P7 P8 L=10 fb–1 CMS 25 20 Generated masses: ~ ) = 496 GeV M(b ID Entries Mean RMS SUSY 103 291 504.6 152.8 25.38 / 20 0.3074E-13 -0.1512E+16 0.2550E+13 0.2699E+11 -0.6571E-02 25.57 500.1 42.22 15 10 L ~ M(bR) = 524 GeV 5 0 0 200 σ × BR dominates SUSY at the LHC, Aspen 2003 23 400 600 800 M( 1000 0 2 b) (GeV) Mass (GeV) D. Acosta, University of Florida ~ g Reconstruction p b ~ χ 20 ~ g ~± l ~ b l± BR ~ 1% b ~ q p ~ χ10 lm Add another b-jet closest in φ to reconstruct g~ ~ & 400 GeV < M b < 600 GeV Events / 28 GeV ch Result of fit: ~ M(g) = 594±7 GeV σM = 42 GeV SUSY 30 203 153 626.7 91.15 12.39 / 10 0.1430E-12 0.1678E+15 -0.5078E+14 0.1170E+12 -0.9486E-02 19.45 593.5 42.37 ID Entries Mean RMS 35 - tt P1 P2 P3 P4 P5 P6 P7 P8 CMS L=10 fb–1 Point B 25 20 15 10 Generated mass: ~ = 595 GeV M(g) 5 0 af ch 200 300 400 500 d i 30 Entries 124 8.681 / 7 -0.2030E-09 -0.2055E+09 0.1989E+08 -0.1692E+08 -0.2288E-01 27.32 92.41 16.91 P1 P2 P3 P4 P5 P6 P7 P8 25 SUSY - tt Expect 87 GeV 10 900 0 2 1000 b b) (GeV) Mass (GeV) ATLAS Point 3 20 15 800 20000 Events/4 GeV/10 fb-1 Events / 15 GeV Point B CMS 700 M( ~0 : ~ − m b~ is independent of m χ Îm g 1 35 600 Expect 20 GeV 15000 10000 5000 5 0 0 50 100 150 200 M( 250 0 2 b b) - M( 0 300 0 2 b) (GeV) Mass (GeV) SUSY at the LHC, Aspen 2003 24 0 20 40 60 M(χ2bb)-M(χ2b) GeV 80 D. Acosta, University of Florida 100 ~ q Reconstruction BR ~ 5% q Same di-lepton edge selection as before Two jets with pT>20 GeV, |η|<2.4 MET > 100 GeV Veto all b-jets Î Track with second largest IP significance < 2σ Î Helps reject sbottom and stop decays Less luminosity required (1 fb-1) Result of fit: ~ M(q) = 536±10 GeV σM = 60 GeV CMS L=1 fb–1 Point B Generated masses: ~ ) = 543 GeV M(q L ~ M(qR) = 537 GeV Mass (GeV) SUSY at the LHC, Aspen 2003 25 D. Acosta, University of Florida Point G Reconstruction Cross section 10× smaller Smaller branching ratios Require 300 fb-1 >1 year @ 1034 Î Eb-jet>350 GeV, MET>350 GeV ID Entries Mean RMS 14 P1 P2 P3 P4 P5 P6 P7 P8 12 10 8 Result of fit: ~ M(b) = 720 ±26 GeV σM = 81 GeV 101 89 739.9 206.3 10.13 / 9 0.3413E-12 0.3982E+14 -0.9041E+12 0.2531E+10 -0.5623E-02 9.488 719.7 81.06 Generated masses: ~ M(bL) = 702 GeV ~ M(bR) = 748 GeV 6 4 2 0 400 600 800 1000 1200 Result of fit: ~ M(g) = 850±40 GeV σM = 130 GeV gluino 1400 M( 0 2 b) (GeV) Events / 60 GeV Events / 60 GeV sbottom ID Entries Mean RMS 25 P1 P2 P3 P4 P5 P6 P7 P8 20 15 201 112 898.4 141.6 9.009 / 4 0.6774E-13 0.3944E+16 -0.7096E+14 0.1002E+12 -0.6384E-02 13.08 852.7 130.6 10 Generated mass: ~ = 860 GeV M(g) 5 0 400 600 800 1000 M( SUSY at the LHC, Aspen 2003 26 1200 0 2 1400 b b) (GeV) D. Acosta, University of Florida Can mSUGRA Escape LHC? M.Battaglia et al., Eur.Phys.J. C22 (2001) 535 (hep-ph/0106204) proposed several SUSY benchmark points in the post-LEP era Two of them would lead to sparticles beyond the reach of the LHC except for a light Higgs Î squark/gluino masses > 2.5 TeV But most other points covered well X Sparticles reconstructed in 10 fb-1 X Di-lepton Sparticles reconstructed edge not observable in 300 fb-1 If SUSY exists, prospects at LHC look favorable SUSY at the LHC, Aspen 2003 27 D. Acosta, University of Florida LHC Summary Discovery of SUSY, if it exists, is almost assured at the LHC Î Inclusive mSUGRA squark/gluino discovery reach to 1.5 TeV with 1 fb–1, 2.5 TeV with 100 fb–1 Î Difficult part will be untangling decay chains and measuring mass relations Possibility to reconstruct squark/gluino/neutralino decays in mSUGRA for several prototype analyses Î Mass resolution <10% under some assumptions Î Generally require tanβ<35 Î Generally require much more data (years) Trigger strategies identified for efficient coverage Many more exhaustive SUSY studies at the LHC experiments are available: Î ATLAS TDR 15 CERN/LHCC 99-15 Î CMS Note 1998/006 Looking forward to studying SUSY spectroscopy before the end of the decade ! SUSY at the LHC, Aspen 2003 28 D. Acosta, University of Florida Minimal GMSB Gauge Mediated Symmetry Breaking Î Uses SM gauge interactions instead of gravity to break SUSY Î Solves FCNC problem Î SUSY breaking scale much less than mSUGRA scale √F << 1011 GeV Î Particles get mass from SM gauge interactions at a messenger scale Mm ~ O(1000 TeV) << MPl Î n = number of SU(5) messenger fields Λ = F / Mm ~ 100 TeV ~ G is LSP ( m << 1 GeV) ~ ~0 → G γ ( n = 1, low tan β ) NLSP: χ 1 ~ ~ l → Gl (n > 1, high tan β ) Î NLSP lifetime: F 100 GeVIJ FG F IJ cτ ~ 1.3 mG H M K H 1000 TeVK 5 4 NLSP Î cτ >> detector size Î slepton ( ~ τ ) is a long-lived heavy lepton (like µ) Î neutralino leads to MET, like MSSM Î cτ ~ detector size Î Measure NLSP lifetime Î Estimate F Î cτ << detector size Î radiative decay with γ SUSY at the LHC, Aspen 2003 29 D. Acosta, University of Florida ~ GMSB Heavy Lepton (τ) Search 1/β Use drift-tube muon systems of ATLAS and CMS to measure time-of-flight for heavy leptons 2 (σ ~ 1ns) 1.8 1.6 1.4 1.2 1 0.8 0.6 0 200 400 600 800 1000 1200 1400 momentum (GeV) Î Measure 1/β and p ⇒ reconstruct mass particles / 20 GeV CMS: Î Require 2 “muons” with PT>45 GeV, M>97 GeV Î |η|<1 for CMS drift-tube system Î Can measure stau mass from 90–700 GeV: n=3, tanβ=45, CMS CR 1999/019 ATLAS Λ=50-300 TeV, 70 114GeV; L=1/fb; eff=5% M/Λ=200 60 50 303GeV; L=10/fb; eff=15% 40 30 636GeV; L=100/fb; eff=26% 20 10 0 0 100 200 300 400 500 600 700 800 900 1000 reconstructed mass (GeV) SUSY at the LHC, Aspen 2003 30 D. Acosta, University of Florida ~ GMSB N1 Lifetime Measurement ~ Look for N1 decays inside detectors: 1) Electromagnetic showers not pointing to vertex ATLAS vertex resolution for H→γγ Events/0.2cm Î Use fine angular resolution from LAr EM calorimeter (ATLAS) and PbWO4 crystals (CMS) 300 σ =1.33 cm 200 100 Î ATLAS: if no non-pointing γ’s in 30 fb-1 ⇒ cτ > 100km 0 -10 -5 0 5 10 z cal o-ztrue (cm) (Λ=90 TeV, M = 500 TeV, n=1) 2) Showers in muon system Î Identify showers with high hit multiplicity σ+(cτ)/cτ CMS: Overall sensitivity to measure cτ: L=143/fb; effkin=10% 10 m(N1)=291GeV ECAL counting 1 µ CAL counting ECAL/µ CAL ECAL impact µ -1 CAL slope COMBINED 10 10 -2 10 -1 SUSY at the LHC, Aspen 2003 1 10 31 10 2 10 3 cτ (m) D. Acosta, University of Florida