Physics Impact of Detector Performance Tim Barklow SLAC March 18, 2005 1 Outline • General Considerations – – – – Vertex Detector Tracker Calorimeter Far forward detector • Examples of parametric physics studies – Calorimeter DEjet – Tracker Dpt • Summary 2 Vertex Detector • Classic application of b,c tagging to Higgs branching ratios. • But there’s more: – vertex charge • top, W helicity • qq asymmetries t tagging • stau analyses • Higgs tau BR • b jets with several n’s bb t t gg cc W W *Talk by Chris Damerell 21Mar2005 M (GeV) 3H Vertex Detector – tau tagging example e e nn tt is an important strong symmetry breaking signal (WW tt ). The large e e e e tt background can be mostly supressed by vetoing the forward e and requiring unbalanced p t . But there remains a seemingly irreducible background from e e e e tt e e bbW W where one of the b quarks undergoes the decay b ct n t c n tn t , ce n en tn t , etc. b t decays have at least 2 n 's Tau tagging could reduce this background (and help b jet energy flow analysis in general). 4 Tracker pt 2 t p • Momentum resolution set by recoil mass analysis of ZH l l X • K S0 , 0 reconstruction and long-lived new particles (GMSB SUSY) • Multiple scattering effects • Forward tracking • Measurement of Ecm, differential luminosity and polarization using physics events pt 2 t p 2 105 8 105 Recoil Mass (GeV) 5 Calorimeter • Separate hadronically decaying W’s from Z’s in reactions where kinematic fits won’t work: e e nn W W , nn ZZ sE/E = 0.6/E e e 1 1 10 10W W e e 20 20 10 10 ZZ • Help solve combinatoric problem in reactions with 4 or more jets e e ZH qqWW * qqqqln e e ZHH qqbbbb sE/E = 0.3/E 6 Far Forward Detector • Electron veto down to 3.2 mrad in presence of very large e e pair background • Useful in general to suppress ff backround. Takes on added importance given that the SUSY parameter space consistent with Dark Matter density includes region with nearly degenerate 10 , t • Crossing angle implications. t signal after 3.2 mrad e veto 7 Far Forward Detector cross 20 mrad M/Mstau (%) cross 0 Rel. stau mass error increases from 0.14% to 0.22% with 20 mrad cross angle 8 Signal significance at s = 500 GeV for e e ZHH qqbbbb C. Castanier et al. hep-ex/0101028 Error on BR( H WW *) from measurement of e e ZH qqWW * qqqqln at s 360 GeV, L=500 fb 1 J.-C. Brient, LC-PHSM-2004-001 9 e e ZH qqbb Reconstructed Mbb E jet E jet 4C Fitted Mbb 0.3 0.5 Mbb (GeV) 0.4 E jet E jet 0.6 Mbb (GeV) 0.4 0.3 0.5 Mbb (GeV) 0.6 Mbb (GeV) 10 e e ZH qqbb E jet E jet 0.3 DM h 42 MeV E jet E jet 0.4 DM h 46 MeV s 350 GeV L 500 fb 1 Mbb (GeV) Mbb (GeV) E jet E jet 0.5 DM h 48 MeV Mbb (GeV) E jet E jet 0.6 DM h 50 MeV Mbb (GeV) 11 e e ZH qqbb s 350 GeV L 500 fb 1 DM h (MeV) E jet E jet 1 2 (GeV ) 12 Simdet Fast MC with this parameterization of pt resolution in place of Simdet’s emulation of LDC: a 2.1105 pt pt2 b 1.0 103 p=3 GeV pt pt2 a b pt sin SiD Detector Resolution p=20 GeV p=100 GeV p=20 GeV, SIMDET LDC log10 (1 cos ) log10 (1 cos ) 13 e e ZH X a 2.0 105 a 1.0 105 b 1.0 103 b 1.0 103 DM h 103 MeV DM h 85 MeV s 350 GeV L 500 fb 1 pt b a 2 pt pt sin Recoil Mass (GeV) Recoil Mass (GeV) a 4.0 105 a 8.0 105 b 1.0 103 b 1.0 103 DM h 153 MeV DM h 273 MeV Recoil Mass (GeV) Recoil Mass (GeV)14 e e ZH X a 2.0 105 a 2.0 105 b 1.0 103 b 0.5 103 DM h 103 MeV DM h 96 MeV s 350 GeV L 500 fb 1 pt b a 2 pt pt sin Recoil Mass (GeV) Recoil Mass (GeV) a 2.0 105 a 2.0 105 b 2.0 103 b 4.0 103 DM h 124 MeV DM h 188 MeV Recoil Mass (GeV) Recoil Mass (GeV) 15 e e ZH X s 350 GeV L 500 fb 1 DM h vs a DM h vs b DM h (MeV) pt pt2 a b pt sin a 105 or b 103 16 e e R R pt 2 t p a a 2 105 a 4 105 Muon Energy (GeV) DM 34 MeV M R 224 GeV b pt sin Fit for M s 500 GeV L 500 fb 1 only a 1105 b 1 103 b 0.5 103 a 8 105 b 2 103 b 4 103 Muon Energy (GeV) Muon Energy (GeV) Muon Energy (GeV) No dependence on a or b in the range 1.0 105 a 8.0 105 , 0.5 103 b 4.0 10 3 17 Branching Ratio of H CC e e ZH l l X * Talk by Haijun Yang in TRK session 20Mar2005 DBr/Br ~ 39% (120GeV), 64% (140GeV) for Zl+l-, 1000 fb-1 18 Beam Energy Profiles Before Collision s Ecm 0.1% Ebeam (GeV) E beam (incoming) 250 GeV After Collision bias 50 ppm < E CM < 250 ppm B 4.3% Lumi Weighted B 1.6% Ebeam (GeV) Ebeam (GeV) Center of Mass Energy Error Requirements • Top mass: • Higgs mass: • Giga-Z program: 200 ppm (35 Mev) 200 ppm (60 MeV for 120 GeV Higgs) 50 ppm 19 Reconstructed E cm using Z events and measured angles. Z + s 350 GeV L 100 fb 1 DEcm = 47 MeV * Talk by Klaus Moenig in MDI session 20Mar2005 Ecm (GeV) 20 The momentum resolution is set by Higgs recoil mass measurement in e e ZH H In the reaction e e Z we know the mass of the photon. Why not invert the problem and use the excellent momentum resolution to solve for s instead of the mass of the system opposite ? 21 Reconstructed E cm & M Z using Z events and measured momenta & angles. Z + DE cm = 2 GeV DE cm = 2 GeV Ecm (GeV) M (GeV) 22 Reconstructed E cm & M Z using Z events and measured momenta & angles. Z + Trk mom scale factor = 0.996 Trk mom scale factor = 1.004 Ecm (GeV) M (GeV) 23 Lumi 100 fb1 E cm 350 GeV E Z = Measured E cm assuming Z boson recoil against single photon E = Measured E cm using full energy e e measured var a b E Z ang only DE cm (GeV) DE cm (GeV) DE cm (GeV) DE cm (ppm) E cm stat sys(E scale) total total .0473 0 .0473 135 E Z |p| & ang 2 105 1103 .0085 .0206 .0223 64 E Z |p| & ang 2 105 .5 10 3 .0054 .0124 .0135 39 E Z |p| & ang 34 105 4 103 .0375 .0313 .0488 139 2 105 1103 .0056 .0124 .0136 39 E |p| & ang 24 Ecm Resolution in MeV vs a or b DE vs a angles only DEZ vs b e e DEZ vs a DE vs b DE SIMDET LDC DEZ SIMDET LDC pt pt2 a b pt sin a 105 or b 103 25 Ecm Resolution in MeV vs a or b angles only e e DEZ vs b DE vs b DE vs a DEZ vs a DE SIMDET LDC DEZ SIMDET LDC pt pt2 a b pt sin a 105 or b 103 26 Simdet Fast MC with this parameterization of pt resolution in place of Simdet’s emulation of LDC: a 2.1105 pt pt2 b 1.0 103 p=3 GeV pt pt2 a b pt sin SiD Detector Resolution p=20 GeV p=100 GeV p=20 GeV, SIMDET LDC log10 (1 cos ) log10 (1 cos ) 27 Summary • Current detector designs appear well matched to envisioned physics program • Choices will have to be made as realitities of detector engineering and cost are confronted – physics benchmark studies will play a crucial role. The examples of parametric studies shown here are just the beginning. 28