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14-18 November, PrahaECFA/DESY Linear Collider Workshop 1 TRILINEAR GAUGE COUPLINGS AT PHOTON COLLIDER - e mode DESY - Zeuthen Klaus Mönig and Jadranka Sekaric
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ECFA/DESY Linear Collider Workshop2 14-18 November, Praha INTRODUCTION 1. signal to background separation study (e W, hadronic decay channel) (e W, hadronic decay channel) 2. observables sensitive to trilinear gauge couplings - higher order radiative corrections : g W /16 2 ~ 10 -3, (3-6) - same order deviations of the TGCs might arise if the SM is the low energy limit of a larger theory test of EW theory, probe of some possible extensions new physics beyond the SM manifest itself : - new particles produced at a collider - precision measurements of deviations from its SM values (anomalous TGC) 3. preliminary fitting results of parameters and (two methods)
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ECFA/DESY Linear Collider Workshop3 14-18 November, Praha EVENT SELECTION TOOLS: PYTHIA event generator SIMDET V3 detector simulation sample of 10 5 mixed signal and background events, generated with PYTHIA at E CM = 450 GeV, variable photon energy spectrum, without beam polarization and anomalous couplings response of a detector simulated with SIMDET V3 (acceptance effects) W reconstructed from hadronic decays (W qq (2jets))
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ECFA/DESY Linear Collider Workshop4 14-18 November, Praha e e e Z°Z° W e e W ee q q qq breamstrahlung q e W t-channel Channel’s contribution: e eZ 0 s-channel t-channel exchange dominates (for the signal) t-channel exchange dominates (for the signal) e e e W s-channel
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ECFA/DESY Linear Collider Workshop5 14-18 November, Praha high W production cross-section (~ pb) allows us to efficiently separate signal from background ( e e W eZ 0 eqq (QED) qq ) Applied cuts: acc. detector angle - 7° acc. detector angle - 7° number of energy flow objects* number of energy flow objects* W energy W energy W mass W mass NEFO EWEW * electrons, photons, muons, charged and neutral hadrons and unresolved clusters that deposited energy in the calorimeters
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ECFA/DESY Linear Collider Workshop6 14-18 November, Praha e e W e qq e eZ 0 eqq qq High efficiency with low background MWMW θ°θ°
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ECFA/DESY Linear Collider Workshop7 14-18 November, Praha SENSITIVE OBSERVABLES total and differential production cross-section sensitive to anomalous coupling W production angle (polar angle - cosθ) W decay angle (between the quark and the total momentum of quark pair – cosθ 1 ) e z x y q q e W 11
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ECFA/DESY Linear Collider Workshop8 14-18 November, Praha TOOLS analytic formula for total (differential) cross- section (A. Denner, A.Dittmaier, Nucl.Phys. B398 (1993)239 helicity amplitudes for different initial photon and final W states (E.Yehudai, Phys.Rev. D11(44)1991)) differential cross-section distribution over the decay angle (Bilenky at al.,Nuc.Phys. B(409) (1993)22 WHIZARD Monte Carlo tree–level generator (W.Kilian,University of Karlsruhe)
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ECFA/DESY Linear Collider Workshop9 14-18 November, Praha 1.Analytic formula DCS in presence of anomalous coupling for J = ± 1 state normalized to its SM value DCS for J = ±1 state in SM
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ECFA/DESY Linear Collider Workshop10 14-18 November, Praha W’s polarization fraction as a function of coupling parameter deviation W’s polarization fraction as a function of coupling parameter deviation - production of longitudinal Ws for J = -1 suppressed in SM
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ECFA/DESY Linear Collider Workshop11 14-18 November, Praha Deviation effects of W L ’s in presence of anomalous coupling
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ECFA/DESY Linear Collider Workshop12 14-18 November, Praha 2D acceptance function
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ECFA/DESY Linear Collider Workshop13 14-18 November, Praha Fitting results of the fit of and for ± 1 photon polarization state – single and two parameter fit for real (e ) mode Fitting results of the fit of and for ± 1 photon polarization state – single and two parameter fit for real (e ) mode REAL MODE 1 par. fit E CM = 450 GeV, L = 110 fb -1 J = +1J = -1 LL 1%0.1%accur.1%0.1%accur. ·10 -3 3.41.00.59.71.10.5 ·10 -3 1.61.5 4.64.43.8 2 par. fit ·10 -3 5.11.10.59.71.10.6 ·10 -3 2.31.6 4.6 REAL MODE - pure e -mode, known beam directions
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ECFA/DESY Linear Collider Workshop14 14-18 November, Praha Fitting results of the fit of and for ± 1 photon polarization state – single and two parameter fit for parasitic (e ) mode Fitting results of the fit of and for ± 1 photon polarization state – single and two parameter fit for parasitic (e ) mode 2 par. fit ·10 -3 8.51.10.59.71.10.6 ·10 -3 6.02.8 4.9 PARASITIC MODE 1 par. fit E CM = 450 GeV, L = 110 fb -1 J = +1J = -1 LL 1%0.1%accur.1%0.1%accur. ·10 -3 3.71.00.59.71.10.5 ·10 -3 2.6 2.44.94.74.0 PARASITIC MODE - running in -mode, could be considered as a background, unknown beam directions
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ECFA/DESY Linear Collider Workshop15 14-18 November, Praha 2.Reweighted events WHIZARD Monte Carlo generator for 10 5 (ūd) pairs at E CM = 450 GeV, fixed photon beam energy, polarized beams, anomalous couplings - N ev normalized to previous one matrix elements for different and values generated Monte Carlo events reweighted with function R( ) = 1 + A· + B· + C·( ) 2 + D·( ) 2 + E · 2D cross-section distributions over cosθ and cosθ1 are fitted
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ECFA/DESY Linear Collider Workshop16 14-18 November, Praha - single parameter fit - two parameter fit REAL MODE E CM = 450 GeV, L = 110 fb -1 J = +1J = -1 LL 1%0.1%accur.1%0.1%accur. ·10 -3 2.490.980.432.220.950.41 ·10 -3 0.58 0.79 0.78 ·10 -3 2.741.000.432.170.950.41 ·10 -3 0.640.59 0.79 - agreement within 10% with previous results for and more sensitive in determination – differs for a factor ~3 (‘better’) – still not understood - single and two parameter fit in a good agreement
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ECFA/DESY Linear Collider Workshop17 14-18 November, Praha comparison of the single parameter fit for e , comparison of the single parameter fit for e , -, and e - e + - colliders E e = 450 GeV L=110 fb -1 E = 400 GeV L=110 fb -1 E ee = 500 GeV L=500 fb -1 LL 0.1% ·10 -4 10 / 9.86.73.1 ·10 -4 15 / 5.86.04.3
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ECFA/DESY Linear Collider Workshop18 14-18 November, Praha SUMMARY e W production in e collider at high energies is sensitive process to the possible scenario of EWSB efficient signal to background separation sensitivity to WW only! - , ~ 10 -3 agreement in determination for two different fitting procedures FUTURE PLANS low energy qq background not included yet signal to bck by WHIZARD (implantation of variable energy spectrum for photon beam) fitting procedure with variable energy spectrum
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